2. Filter & explore results

The querying functions presented in the previous section return a PANDAS DataFrame that can be used to further narrow down your search. This section presents some examples of how you can further filter and explore the results of your queries:

Load libraries & create a query

To explore these options, we will first query the archive using one of the methods presented in the previous section and use the results in the remainder of this tutorial.

[1]:
import alminer

observations = alminer.keysearch({'science_keyword':['Galaxy chemistry']},
                                 print_targets=False)
================================
alminer.keysearch results
================================
--------------------------------
Number of projects = 47
Number of observations = 339
Number of unique subbands = 1162
Total number of subbands = 1361
Total number of targets with ALMA data = 63
--------------------------------

2.1 Explore results

You can simply display the DataFrame table returned by the query functions using the name you gave it (in this case observations), but often there are limits to how many rows and columns are presented. With the alminer.explore function, you can control whether or not you want to display all rows (allrows=True/False) and/or all columns (allcols=True/False). By default, only the 18 most useful columns are shown and the number of rows is truncated.

Example 2.1.1: View the queried observations as a table (shortened)

[2]:
alminer.explore(observations)
[2]:
Obs project_code ALMA_source_name RAJ2000 DEJ2000 ang_res_arcsec min_freq_GHz max_freq_GHz central_freq_GHz bandwidth_GHz freq_res_kHz vel_res_kms LAS_arcsec FoV_arcsec cont_sens_bandwidth line_sens_10kms line_sens_native MOUS_id
0 1 2011.0.00268.S LESS J0332-2756 53.122042 -27.938694 1.167 239.50 241.37 240.43 1.875 976.56 1.213 8.943 23.564 79.299 1708.54 111.94 uid://A002/X303d22/X7b
1 2 2011.0.00268.S LESS J0332-2756 53.122042 -27.938694 1.167 252.85 254.73 253.79 1.875 976.56 1.149 8.943 23.564 79.299 1675.07 112.74 uid://A002/X303d22/X7b
2 3 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 105.07 106.95 106.01 1.878 976.56 2.737 12.937 58.774 29.824 1370.09 59.71 uid://A002/X36d874/X80
3 4 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 283.51 285.39 284.45 1.874 976.56 1.026 3.448 20.113 60.429 1673.64 119.28 uid://A002/X36d874/X7a
4 5 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 281.64 283.51 282.57 1.874 976.56 1.033 3.448 20.113 60.429 1677.23 119.14 uid://A002/X36d874/X7a
5 6 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 103.20 105.08 104.14 1.878 976.56 2.786 12.937 58.774 29.824 1381.77 59.69 uid://A002/X36d874/X80
6 7 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 259.58 261.47 260.52 1.894 976.56 1.120 5.088 23.118 74.597 2278.21 154.60 uid://A002/X36d874/X7c
7 8 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 292.55 294.43 293.49 1.880 976.56 0.994 4.104 19.504 68.197 1867.41 134.98 uid://A002/X36d874/X7e
8 9 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 91.20 93.08 92.14 1.878 976.56 3.145 12.937 58.774 29.824 1500.60 61.02 uid://A002/X36d874/X80
9 10 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 256.63 258.53 257.58 1.894 976.56 1.132 5.088 23.118 74.597 2189.73 147.77 uid://A002/X36d874/X7c
10 11 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 244.13 246.02 245.08 1.893 976.56 1.190 5.088 23.118 74.597 2229.45 146.80 uid://A002/X36d874/X7c
11 12 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 295.51 297.38 296.45 1.874 976.56 0.984 3.448 20.113 60.429 1735.78 126.28 uid://A002/X36d874/X7a
12 13 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 293.63 295.51 294.57 1.874 976.56 0.991 3.448 20.113 60.429 1655.25 120.04 uid://A002/X36d874/X7a
13 14 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 242.31 244.20 243.25 1.894 976.56 1.199 5.088 23.118 74.597 2229.83 146.24 uid://A002/X36d874/X7c
14 15 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 304.55 306.43 305.49 1.880 976.56 0.955 4.104 19.504 68.197 1868.50 137.78 uid://A002/X36d874/X7e
15 16 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 93.07 94.95 94.01 1.878 976.56 3.083 12.937 58.774 29.824 1440.54 59.16 uid://A002/X36d874/X80
16 17 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 290.68 292.56 291.62 1.880 976.56 1.001 4.104 19.504 68.197 1903.65 137.16 uid://A002/X36d874/X7e
17 18 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 302.68 304.56 303.62 1.880 976.56 0.961 4.104 19.504 68.197 1848.24 135.87 uid://A002/X36d874/X7e
18 19 2011.0.00820.S ngc4418 186.727617 -0.877642 0.665 261.72 263.60 262.66 1.874 976.56 1.111 8.262 22.748 191.363 5507.00 377.20 uid://A002/X314ea1/X1fa
19 20 2011.0.00820.S ngc4418 186.727617 -0.877642 1.355 97.88 99.75 98.82 1.875 976.56 2.935 9.305 63.355 60.616 2862.27 120.59 uid://A002/X327408/X100
20 21 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 251.60 253.47 252.54 1.874 976.56 1.155 8.158 22.463 184.788 5492.90 368.94 uid://A002/X314ea1/X1ee
21 22 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 266.60 268.47 267.53 1.874 976.56 1.090 8.158 22.463 184.788 5382.61 372.08 uid://A002/X314ea1/X1ee
22 23 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 249.97 251.85 250.91 1.874 976.56 1.162 8.158 22.463 184.788 5505.70 368.62 uid://A002/X314ea1/X1ee
23 24 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 264.97 266.85 265.91 1.874 976.56 1.097 8.158 22.463 184.788 5393.90 371.73 uid://A002/X314ea1/X1ee
24 25 2011.0.00820.S ngc4418 186.727617 -0.877642 0.665 246.72 248.60 247.66 1.874 976.56 1.178 8.262 22.748 191.363 5623.83 374.09 uid://A002/X314ea1/X1fa
... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...
1336 1337 2018.1.01395.S NGC_253 11.888058 -25.288800 0.019 235.98 237.85 236.91 1.874 1128.91 1.434 0.500 25.549 12.404 382.31 24.78 uid://A001/X133d/X3025
1337 1338 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 108.29 110.16 109.23 1.873 1938.48 5.366 24.940 55.903 10.485 468.79 20.59 uid://A001/X1465/X389c
1338 1339 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 91.70 93.57 92.63 1.873 1938.48 6.210 27.132 59.612 10.282 508.68 20.77 uid://A001/X1465/X3888
1339 1340 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 97.97 99.84 98.90 1.873 1938.48 5.820 24.940 55.903 10.485 507.47 21.40 uid://A001/X1465/X389c
1340 1341 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 96.28 98.15 97.21 1.873 1938.48 5.920 24.940 55.903 10.485 511.67 21.39 uid://A001/X1465/X389c
1341 1342 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 108.87 110.74 109.80 1.873 1938.48 5.338 22.321 55.608 18.936 799.25 35.19 uid://A001/X1465/X388c
1342 1343 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 110.76 112.63 111.69 1.873 1938.48 5.247 22.321 55.608 18.936 792.83 35.21 uid://A001/X1465/X388c
1343 1344 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 98.49 100.36 99.42 1.873 1938.48 5.791 22.321 55.608 18.936 976.30 41.27 uid://A001/X1465/X388c
1344 1345 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 96.80 98.67 97.73 1.873 1938.48 5.890 22.321 55.608 18.936 984.33 41.26 uid://A001/X1465/X388c
1345 1346 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 103.38 105.26 104.32 1.873 1938.48 5.621 20.838 59.730 9.858 461.89 19.82 uid://A001/X1465/X3890
1346 1347 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 101.58 103.45 102.51 1.873 1938.48 5.721 20.838 59.730 9.858 459.66 19.55 uid://A001/X1465/X3890
1347 1348 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 91.51 93.39 92.45 1.873 1938.48 6.223 20.838 59.730 9.858 480.47 19.59 uid://A001/X1465/X3890
1348 1349 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 89.72 91.59 90.65 1.873 1938.48 6.345 20.838 59.730 9.858 494.60 19.97 uid://A001/X1465/X3890
1349 1350 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 89.43 91.30 90.36 1.873 1938.48 6.364 27.048 59.922 9.343 466.81 18.82 uid://A001/X1465/X3898
1350 1351 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 101.78 103.65 102.72 1.873 1938.48 5.710 27.132 59.612 10.282 475.79 20.26 uid://A001/X1465/X3888
1351 1352 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 108.65 110.52 109.59 1.873 1938.48 5.349 21.118 55.719 21.996 960.67 42.25 uid://A001/X1465/X3894
1352 1353 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 110.54 112.42 111.48 1.873 1938.48 5.257 21.118 55.719 21.996 1131.63 50.21 uid://A001/X1465/X3894
1353 1354 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 98.29 100.16 99.23 1.873 1938.48 5.802 21.118 55.719 21.996 1007.18 42.54 uid://A001/X1465/X3894
1354 1355 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 103.05 104.92 103.99 1.873 1938.48 5.639 27.048 59.922 9.343 436.95 18.72 uid://A001/X1465/X3898
1355 1356 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 91.20 93.07 92.13 1.873 1938.48 6.243 27.048 59.922 9.343 459.55 18.71 uid://A001/X1465/X3898
1356 1357 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 101.24 103.11 102.18 1.873 1938.48 5.740 27.048 59.922 9.343 437.00 18.56 uid://A001/X1465/X3898
1357 1358 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 96.60 98.47 97.53 1.873 1938.48 5.902 21.118 55.719 21.996 1015.52 42.52 uid://A001/X1465/X3894
1358 1359 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 103.59 105.46 104.52 1.873 1938.48 5.610 27.132 59.612 10.282 478.30 20.54 uid://A001/X1465/X3888
1359 1360 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 89.90 91.77 90.84 1.873 1938.48 6.332 27.132 59.612 10.282 513.50 20.76 uid://A001/X1465/X3888
1360 1361 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 110.17 112.05 111.11 1.873 1938.48 5.274 24.940 55.903 10.485 465.01 20.60 uid://A001/X1465/X389c

1361 rows × 18 columns

Example 2.1.2: View the queried observations as a table and show all columns

[3]:
alminer.explore(observations, allcols=True, allrows=False)
# you can also set allrows=True to see all rows in the table
# but this may be slow for very large queries
[3]:
Obs project_code ALMA_source_name RAJ2000 DEJ2000 ang_res_arcsec min_freq_GHz max_freq_GHz central_freq_GHz bandwidth_GHz freq_res_kHz vel_res_kms LAS_arcsec FoV_arcsec cont_sens_bandwidth line_sens_10kms line_sens_native MOUS_id access_url access_format proposal_id data_rights gal_longitude gal_latitude obs_publisher_did obs_collection facility_name instrument_name obs_id dataproduct_type calib_level target_name s_ra s_dec s_fov s_region s_resolution t_min t_max t_exptime t_resolution em_min em_max em_res_power pol_states o_ucd band_list em_resolution authors pub_abstract publication_year proposal_abstract schedblock_name proposal_authors sensitivity_10kms cont_sensitivity_bandwidth pwv group_ous_uid member_ous_uid asdm_uid obs_title type scan_intent science_observation spatial_scale_max bandwidth antenna_arrays is_mosaic obs_release_date spatial_resolution frequency_support frequency velocity_resolution obs_creator_name pub_title first_author qa2_passed bib_reference science_keyword scientific_category lastModified
0 1 2011.0.00268.S LESS J0332-2756 53.122042 -27.938694 1.167 239.50 241.37 240.43 1.875 976.56 1.213 8.943 23.564 79.299 1708.54 111.94 uid://A002/X303d22/X7b http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00268.S Public 223.796062 -54.451922 ADS/JAO.ALMA#2011.0.00268.S ALMA JAO ALMA uid://A002/X303d22/X7b cube 2 LESS J0332-2756 53.122042 -27.938694 0.006546 Circle ICRS 53.122042 -27.938694 0.003273 1.167248 55936.913188 55939.193372 4536.000 4536.000 0.001242 0.001252 247134.408560 /XX/YY/ phot.flux.density;phys.polarization 6 2.928016e+14 Leon, S.; Cortes, P.C.; Guerard, M.; Villard, ... Aims: We aim at analyzing the (sub-)millimeter... 2012 Metallicity of galaxies and its redshift evolu... LESS J0332-2756 De Breuck, Carlos; Hatsukade, Bunyo; Maiolino,... 1.708538 0.079299 1.422843 uid://A002/X303d22/X7b uid://A002/X36a70f/X318 Metallicity of a Submillimeter Galaxy at z=5 S TARGET WVR T 8.943092 1.875000e+09 A002:PM02 A004:DV04 A009:DA43 A011:DV12 A013:D... F 2013-02-09T01:45:00.000 1.167248 [239.50..241.37GHz,976.56kHz,1.7mJy/beam@10km/... 247.112856 1149.468553 Nagao, Tohru ALMA reveals a chemically evolved submillimete... Leon, S. Nagao, T. Ono, Yoshiaki T 2012A&A...542L..34N 2014ApJ...795....5O 2016A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
1 2 2011.0.00268.S LESS J0332-2756 53.122042 -27.938694 1.167 252.85 254.73 253.79 1.875 976.56 1.149 8.943 23.564 79.299 1675.07 112.74 uid://A002/X303d22/X7b http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00268.S Public 223.796062 -54.451922 ADS/JAO.ALMA#2011.0.00268.S ALMA JAO ALMA uid://A002/X303d22/X7b cube 2 LESS J0332-2756 53.122042 -27.938694 0.006546 Circle ICRS 53.122042 -27.938694 0.003273 1.167248 55936.913188 55939.193372 4536.000 4536.000 0.001177 0.001186 260809.621360 /XX/YY/ phot.flux.density;phys.polarization 6 2.928016e+14 Leon, S.; Cortes, P.C.; Guerard, M.; Villard, ... Aims: We aim at analyzing the (sub-)millimeter... 2012 Metallicity of galaxies and its redshift evolu... LESS J0332-2756 De Breuck, Carlos; Hatsukade, Bunyo; Maiolino,... 1.675071 0.079299 1.422843 uid://A002/X303d22/X7b uid://A002/X36a70f/X318 Metallicity of a Submillimeter Galaxy at z=5 S TARGET WVR T 8.943092 1.875000e+09 A002:PM02 A004:DV04 A009:DA43 A011:DV12 A013:D... F 2013-02-09T01:45:00.000 1.167248 [239.50..241.37GHz,976.56kHz,1.7mJy/beam@10km/... 247.112856 1149.468553 Nagao, Tohru ALMA reveals a chemically evolved submillimete... Leon, S. Nagao, T. Ono, Yoshiaki T 2012A&A...542L..34N 2014ApJ...795....5O 2016A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
2 3 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 105.07 106.95 106.01 1.878 976.56 2.737 12.937 58.774 29.824 1370.09 59.71 uid://A002/X36d874/X80 http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X80 cube 2 PKS1830-211 278.416330 -21.061080 0.016326 Circle ICRS 278.416330 -21.061080 0.008163 1.331051 56069.374548 56093.397660 3719.520 3719.520 0.002803 0.002853 109524.742000 /XX/YY/ phot.flux.density;phys.polarization 3 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_HCOplus_b3_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.370093 0.029824 0.923567 uid://A002/X36d874/X80 uid://A002/X411025/X441 A survey of strong absorption lines at z=0.89 ... S TARGET T 12.936728 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-10T14:47:51.000 1.331051 [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... 99.075504 2737.212182 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
3 4 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 283.51 285.39 284.45 1.874 976.56 1.026 3.448 20.113 60.429 1673.64 119.28 uid://A002/X36d874/X7a http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7a cube 2 PKS1830-211 278.416330 -21.061080 0.005587 Circle ICRS 278.416330 -21.061080 0.002793 0.454758 56028.238332 56028.363572 3144.960 3144.960 0.001050 0.001057 292274.950000 /XX/YY/ phot.flux.density;phys.polarization 7 2.927253e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CH_and_H2O_b7_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.673643 0.060429 0.703871 uid://A002/X36d874/X7a uid://A002/X3cb0a0/X9e8 A survey of strong absorption lines at z=0.89 ... S TARGET T 3.448268 1.875000e+09 A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... F 2013-05-22T07:31:59.000 0.454758 [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... 289.509775 984.336598 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
4 5 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 281.64 283.51 282.57 1.874 976.56 1.033 3.448 20.113 60.429 1677.23 119.14 uid://A002/X36d874/X7a http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7a cube 2 PKS1830-211 278.416330 -21.061080 0.005587 Circle ICRS 278.416330 -21.061080 0.002793 0.454758 56028.238332 56028.363572 3144.960 3144.960 0.001057 0.001064 290354.950000 /XX/YY/ phot.flux.density;phys.polarization 7 2.927253e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CH_and_H2O_b7_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.677226 0.060429 0.703871 uid://A002/X36d874/X7a uid://A002/X3cb0a0/X9e8 A survey of strong absorption lines at z=0.89 ... S TARGET T 3.448268 1.875000e+09 A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... F 2013-05-22T07:31:59.000 0.454758 [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... 289.509775 984.336598 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
5 6 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 103.20 105.08 104.14 1.878 976.56 2.786 12.937 58.774 29.824 1381.77 59.69 uid://A002/X36d874/X80 http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X80 cube 2 PKS1830-211 278.416330 -21.061080 0.016326 Circle ICRS 278.416330 -21.061080 0.008163 1.331051 56069.374548 56093.397660 3719.520 3719.520 0.002853 0.002905 107605.766000 /XX/YY/ phot.flux.density;phys.polarization 3 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_HCOplus_b3_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.381767 0.029824 0.923567 uid://A002/X36d874/X80 uid://A002/X411025/X441 A survey of strong absorption lines at z=0.89 ... S TARGET T 12.936728 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-10T14:47:51.000 1.331051 [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... 99.075504 2737.212182 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
6 7 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 259.58 261.47 260.52 1.894 976.56 1.120 5.088 23.118 74.597 2278.21 154.60 uid://A002/X36d874/X7c http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7c cube 2 PKS1830-211 278.416330 -21.061080 0.006422 Circle ICRS 278.416330 -21.061080 0.003211 0.562899 56026.250749 56093.330969 4838.400 4838.400 0.001147 0.001155 267762.499440 /XX/YY/ phot.flux.density;phys.polarization 6 2.927251e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830-211_CO4-3_b6_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 2.278214 0.074597 2.122151 uid://A002/X36d874/X7c uid://A002/X3ca066/Xa6f A survey of strong absorption lines at z=0.89 ... S TARGET T 5.088294 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-19T12:40:13.000 0.562899 [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... 251.884124 1119.620778 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
7 8 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 292.55 294.43 293.49 1.880 976.56 0.994 4.104 19.504 68.197 1867.41 134.98 uid://A002/X36d874/X7e http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7e cube 2 PKS1830-211 278.416330 -21.061080 0.005418 Circle ICRS 278.416330 -21.061080 0.002709 0.441708 56070.225109 56082.381661 6048.000 6048.000 0.001018 0.001025 301521.659760 /XX/YY/ phot.flux.density;phys.polarization 7 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CO5-4_b7_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.867413 0.068197 1.027013 uid://A002/X36d874/X7e uid://A002/X4122f3/X133 A survey of strong absorption lines at z=0.89 ... S TARGET T 4.104185 1.875000e+09 A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... F 2013-07-05T11:49:39.000 0.441708 [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... 298.550728 955.332153 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
8 9 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 91.20 93.08 92.14 1.878 976.56 3.145 12.937 58.774 29.824 1500.60 61.02 uid://A002/X36d874/X80 http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X80 cube 2 PKS1830-211 278.416330 -21.061080 0.016326 Circle ICRS 278.416330 -21.061080 0.008163 1.331051 56069.374548 56093.397660 3719.520 3719.520 0.003221 0.003287 95317.766000 /XX/YY/ phot.flux.density;phys.polarization 3 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_HCOplus_b3_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.500603 0.029824 0.923567 uid://A002/X36d874/X80 uid://A002/X411025/X441 A survey of strong absorption lines at z=0.89 ... S TARGET T 12.936728 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-10T14:47:51.000 1.331051 [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... 99.075504 2737.212182 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
9 10 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 256.63 258.53 257.58 1.894 976.56 1.132 5.088 23.118 74.597 2189.73 147.77 uid://A002/X36d874/X7c http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7c cube 2 PKS1830-211 278.416330 -21.061080 0.006422 Circle ICRS 278.416330 -21.061080 0.003211 0.562899 56026.250749 56093.330969 4838.400 4838.400 0.001160 0.001168 264749.082480 /XX/YY/ phot.flux.density;phys.polarization 6 2.927251e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830-211_CO4-3_b6_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 2.189729 0.074597 2.122151 uid://A002/X36d874/X7c uid://A002/X3ca066/Xa6f A survey of strong absorption lines at z=0.89 ... S TARGET T 5.088294 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-19T12:40:13.000 0.562899 [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... 251.884124 1119.620778 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
10 11 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 244.13 246.02 245.08 1.893 976.56 1.190 5.088 23.118 74.597 2229.45 146.80 uid://A002/X36d874/X7c http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7c cube 2 PKS1830-211 278.416330 -21.061080 0.006422 Circle ICRS 278.416330 -21.061080 0.003211 0.562899 56026.250749 56093.330969 4838.400 4838.400 0.001219 0.001228 251943.624560 /XX/YY/ phot.flux.density;phys.polarization 6 2.927251e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830-211_CO4-3_b6_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 2.229454 0.074597 2.122151 uid://A002/X36d874/X7c uid://A002/X3ca066/Xa6f A survey of strong absorption lines at z=0.89 ... S TARGET T 5.088294 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-19T12:40:13.000 0.562899 [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... 251.884124 1119.620778 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
11 12 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 295.51 297.38 296.45 1.874 976.56 0.984 3.448 20.113 60.429 1735.78 126.28 uid://A002/X36d874/X7a http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7a cube 2 PKS1830-211 278.416330 -21.061080 0.005587 Circle ICRS 278.416330 -21.061080 0.002793 0.454758 56028.238332 56028.363572 3144.960 3144.960 0.001008 0.001014 304562.950000 /XX/YY/ phot.flux.density;phys.polarization 7 2.927253e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CH_and_H2O_b7_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.735785 0.060429 0.703871 uid://A002/X36d874/X7a uid://A002/X3cb0a0/X9e8 A survey of strong absorption lines at z=0.89 ... S TARGET T 3.448268 1.875000e+09 A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... F 2013-05-22T07:31:59.000 0.454758 [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... 289.509775 984.336598 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
12 13 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.455 293.63 295.51 294.57 1.874 976.56 0.991 3.448 20.113 60.429 1655.25 120.04 uid://A002/X36d874/X7a http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7a cube 2 PKS1830-211 278.416330 -21.061080 0.005587 Circle ICRS 278.416330 -21.061080 0.002793 0.454758 56028.238332 56028.363572 3144.960 3144.960 0.001014 0.001021 302642.950000 /XX/YY/ phot.flux.density;phys.polarization 7 2.927253e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CH_and_H2O_b7_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.655253 0.060429 0.703871 uid://A002/X36d874/X7a uid://A002/X3cb0a0/X9e8 A survey of strong absorption lines at z=0.89 ... S TARGET T 3.448268 1.875000e+09 A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... F 2013-05-22T07:31:59.000 0.454758 [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... 289.509775 984.336598 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
13 14 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.563 242.31 244.20 243.25 1.894 976.56 1.199 5.088 23.118 74.597 2229.83 146.24 uid://A002/X36d874/X7c http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7c cube 2 PKS1830-211 278.416330 -21.061080 0.006422 Circle ICRS 278.416330 -21.061080 0.003211 0.562899 56026.250749 56093.330969 4838.400 4838.400 0.001228 0.001237 250078.682480 /XX/YY/ phot.flux.density;phys.polarization 6 2.927251e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830-211_CO4-3_b6_run_x2 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 2.229828 0.074597 2.122151 uid://A002/X36d874/X7c uid://A002/X3ca066/Xa6f A survey of strong absorption lines at z=0.89 ... S TARGET T 5.088294 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-19T12:40:13.000 0.562899 [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... 251.884124 1119.620778 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
14 15 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 304.55 306.43 305.49 1.880 976.56 0.955 4.104 19.504 68.197 1868.50 137.78 uid://A002/X36d874/X7e http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7e cube 2 PKS1830-211 278.416330 -21.061080 0.005418 Circle ICRS 278.416330 -21.061080 0.002709 0.441708 56070.225109 56082.381661 6048.000 6048.000 0.000978 0.000984 313809.659760 /XX/YY/ phot.flux.density;phys.polarization 7 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CO5-4_b7_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.868498 0.068197 1.027013 uid://A002/X36d874/X7e uid://A002/X4122f3/X133 A survey of strong absorption lines at z=0.89 ... S TARGET T 4.104185 1.875000e+09 A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... F 2013-07-05T11:49:39.000 0.441708 [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... 298.550728 955.332153 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
15 16 2011.0.00405.S PKS1830-211 278.416330 -21.061080 1.331 93.07 94.95 94.01 1.878 976.56 3.083 12.937 58.774 29.824 1440.54 59.16 uid://A002/X36d874/X80 http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X80 cube 2 PKS1830-211 278.416330 -21.061080 0.016326 Circle ICRS 278.416330 -21.061080 0.008163 1.331051 56069.374548 56093.397660 3719.520 3719.520 0.003157 0.003221 97236.742000 /XX/YY/ phot.flux.density;phys.polarization 3 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_HCOplus_b3_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.440543 0.029824 0.923567 uid://A002/X36d874/X80 uid://A002/X411025/X441 A survey of strong absorption lines at z=0.89 ... S TARGET T 12.936728 1.875000e+09 A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... F 2013-10-10T14:47:51.000 1.331051 [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... 99.075504 2737.212182 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
16 17 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 290.68 292.56 291.62 1.880 976.56 1.001 4.104 19.504 68.197 1903.65 137.16 uid://A002/X36d874/X7e http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7e cube 2 PKS1830-211 278.416330 -21.061080 0.005418 Circle ICRS 278.416330 -21.061080 0.002709 0.441708 56070.225109 56082.381661 6048.000 6048.000 0.001025 0.001031 299601.659760 /XX/YY/ phot.flux.density;phys.polarization 7 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CO5-4_b7_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.903645 0.068197 1.027013 uid://A002/X36d874/X7e uid://A002/X4122f3/X133 A survey of strong absorption lines at z=0.89 ... S TARGET T 4.104185 1.875000e+09 A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... F 2013-07-05T11:49:39.000 0.441708 [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... 298.550728 955.332153 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
17 18 2011.0.00405.S PKS1830-211 278.416330 -21.061080 0.442 302.68 304.56 303.62 1.880 976.56 0.961 4.104 19.504 68.197 1848.24 135.87 uid://A002/X36d874/X7e http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00405.S Public 12.165817 -5.711677 ADS/JAO.ALMA#2011.0.00405.S ALMA JAO ALMA uid://A002/X36d874/X7e cube 2 PKS1830-211 278.416330 -21.061080 0.005418 Circle ICRS 278.416330 -21.061080 0.002709 0.441708 56070.225109 56082.381661 6048.000 6048.000 0.000984 0.000990 311889.659760 /XX/YY/ phot.flux.density;phys.polarization 7 2.927369e+14 Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... A limit on a possible cosmological variation o... 2013 The z=0.89 (sub)mm molecular absorber toward t... PKS1830_CO5-4_b7_run_x3 Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... 1.848243 0.068197 1.027013 uid://A002/X36d874/X7e uid://A002/X4122f3/X133 A survey of strong absorption lines at z=0.89 ... S TARGET T 4.104185 1.875000e+09 A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... F 2013-07-05T11:49:39.000 0.441708 [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... 298.550728 955.332153 Muller, Sebastien A strong magnetic field in the jet base of a s... Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... T 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... Galaxy structure & evolution, Galaxy chemistry Galaxy evolution 2021-06-16T16:46:50.431
18 19 2011.0.00820.S ngc4418 186.727617 -0.877642 0.665 261.72 263.60 262.66 1.874 976.56 1.111 8.262 22.748 191.363 5507.00 377.20 uid://A002/X314ea1/X1fa http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X314ea1/X1fa cube 2 ngc4418 186.727617 -0.877642 0.006319 Circle ICRS 186.727617 -0.877642 0.003159 0.664926 56293.314401 56293.327148 151.200 151.200 0.001137 0.001145 269951.750000 /XX/YY/ phot.flux.density;phys.polarization 6 2.927348e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B6 Setup 12 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 5.507000 0.191363 2.751811 uid://A002/X314ea1/X1fa uid://A002/X590461/X17e6 A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 8.261900 1.875000e+09 A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... F 2014-01-18T12:52:22.000 0.664926 [246.72..248.60GHz,976.56kHz,5.6mJy/beam@10km/... 255.972659 1103.737386 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
19 20 2011.0.00820.S ngc4418 186.727617 -0.877642 1.355 97.88 99.75 98.82 1.875 976.56 2.935 9.305 63.355 60.616 2862.27 120.59 uid://A002/X327408/X100 http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X327408/X100 cube 2 ngc4418 186.727617 -0.877642 0.017599 Circle ICRS 186.727617 -0.877642 0.008799 1.354752 56042.089628 56042.109167 332.640 332.640 0.003005 0.003063 102143.801200 /XX/YY/ phot.flux.density;phys.polarization 3 2.927779e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B3 Setup 1: Run x 1 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 2.862267 0.060616 2.623814 uid://A002/X327408/X100 uid://A002/X3e3a61/Xce A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 9.304600 1.875000e+09 A003:DA41 A021:DV08 A025:DV14 A045:DV11 A046:D... F 2013-06-15T09:26:34.000 1.354752 [84.07..85.94GHz,976.56kHz,3.2mJy/beam@10km/s,... 91.910024 2935.003931 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
20 21 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 251.60 253.47 252.54 1.874 976.56 1.155 8.158 22.463 184.788 5492.90 368.94 uid://A002/X314ea1/X1ee http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X314ea1/X1ee cube 2 ngc4418 186.727617 -0.877642 0.006240 Circle ICRS 186.727617 -0.877642 0.003120 0.656589 56293.474235 56293.487242 151.200 151.200 0.001183 0.001192 259583.750000 /XX/YY/ phot.flux.density;phys.polarization 6 2.927352e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B6 Setup 13 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 5.492896 0.184788 3.761806 uid://A002/X314ea1/X1ee uid://A002/X590461/X1b27 A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 8.158316 1.875000e+09 A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... F 2014-06-25T06:41:57.000 0.656589 [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... 259.222672 1090.377424 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
21 22 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 266.60 268.47 267.53 1.874 976.56 1.090 8.158 22.463 184.788 5382.61 372.08 uid://A002/X314ea1/X1ee http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X314ea1/X1ee cube 2 ngc4418 186.727617 -0.877642 0.006240 Circle ICRS 186.727617 -0.877642 0.003120 0.656589 56293.474235 56293.487242 151.200 151.200 0.001117 0.001125 274943.750000 /XX/YY/ phot.flux.density;phys.polarization 6 2.927352e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B6 Setup 13 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 5.382614 0.184788 3.761806 uid://A002/X314ea1/X1ee uid://A002/X590461/X1b27 A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 8.158316 1.875000e+09 A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... F 2014-06-25T06:41:57.000 0.656589 [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... 259.222672 1090.377424 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
22 23 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 249.97 251.85 250.91 1.874 976.56 1.162 8.158 22.463 184.788 5505.70 368.62 uid://A002/X314ea1/X1ee http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X314ea1/X1ee cube 2 ngc4418 186.727617 -0.877642 0.006240 Circle ICRS 186.727617 -0.877642 0.003120 0.656589 56293.474235 56293.487242 151.200 151.200 0.001190 0.001199 257919.750000 /XX/YY/ phot.flux.density;phys.polarization 6 2.927352e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B6 Setup 13 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 5.505704 0.184788 3.761806 uid://A002/X314ea1/X1ee uid://A002/X590461/X1b27 A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 8.158316 1.875000e+09 A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... F 2014-06-25T06:41:57.000 0.656589 [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... 259.222672 1090.377424 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
23 24 2011.0.00820.S ngc4418 186.727617 -0.877642 0.657 264.97 266.85 265.91 1.874 976.56 1.097 8.158 22.463 184.788 5393.90 371.73 uid://A002/X314ea1/X1ee http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X314ea1/X1ee cube 2 ngc4418 186.727617 -0.877642 0.006240 Circle ICRS 186.727617 -0.877642 0.003120 0.656589 56293.474235 56293.487242 151.200 151.200 0.001123 0.001131 273279.750000 /XX/YY/ phot.flux.density;phys.polarization 6 2.927352e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B6 Setup 13 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 5.393897 0.184788 3.761806 uid://A002/X314ea1/X1ee uid://A002/X590461/X1b27 A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 8.158316 1.875000e+09 A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... F 2014-06-25T06:41:57.000 0.656589 [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... 259.222672 1090.377424 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
24 25 2011.0.00820.S ngc4418 186.727617 -0.877642 0.665 246.72 248.60 247.66 1.874 976.56 1.178 8.262 22.748 191.363 5623.83 374.09 uid://A002/X314ea1/X1fa http://almascience.org/aq?member_ous_id=uid://... text/html 2011.0.00820.S Public 290.048542 61.379017 ADS/JAO.ALMA#2011.0.00820.S ALMA JAO ALMA uid://A002/X314ea1/X1fa cube 2 ngc4418 186.727617 -0.877642 0.006319 Circle ICRS 186.727617 -0.877642 0.003159 0.664926 56293.314401 56293.327148 151.200 151.200 0.001206 0.001215 254591.750000 /XX/YY/ phot.flux.density;phys.polarization 6 2.927348e+14 Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... Context. Extragalactic observations allow the ... 2015 A wide-band, high-quality, unbiased census of ... ngc4418 B6 Setup 12 Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... 5.623833 0.191363 2.751811 uid://A002/X314ea1/X1fa uid://A002/X590461/X17e6 A 170 GHz-wide Complete Spectral Scan of an IR... S TARGET T 8.261900 1.875000e+09 A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... F 2014-01-18T12:52:22.000 0.664926 [246.72..248.60GHz,976.56kHz,5.6mJy/beam@10km/... 255.972659 1103.737386 Costagliola, Francesco Abundance measurements of Titan's stratospheri... Costagliola, F. Thelen, Alexander E. T 2015A&A...582A..91C 2019Icar..319..417T Luminous and Ultra-Luminous Infra-Red Galaxies... Galaxy evolution 2021-06-16T16:46:50.431
... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...
1336 1337 2018.1.01395.S NGC_253 11.888058 -25.288800 0.019 235.98 237.85 236.91 1.874 1128.91 1.434 0.500 25.549 12.404 382.31 24.78 uid://A001/X133d/X3025 http://almascience.org/aq?member_ous_id=uid://... text/html 2018.1.01395.S Public 97.364395 -87.964503 ADS/JAO.ALMA#2018.1.01395.S ALMA JAO ALMA uid://A001/X133d/X3025 cube 2 NGC_253 11.888058 -25.288800 0.007097 Polygon ICRS 11.888794 -25.292286 11.887323 -2... 0.018645 58640.446034 58674.467208 16003.008 16003.008 0.001260 0.001270 209043.422558 /XX/YY/ phot.flux.density;phys.polarization 6 3.384169e+14 <NA> We have used 0.2" ALMA images of the HC3N vibr... NGC_253_a_06_TM1 Martin-Pintado, Jesus; Martin, Sergio; Gonzale... 0.382310 0.012404 0.911870 uid://A001/X133d/X3024 uid://A001/X133d/X3025 uid://A002/Xdd4cf3/X33a6 Witnessing the early stages of the formation o... S TARGET T 0.499517 1.875000e+09 A015:DA64 A058:DA41 A069:DV16 A074:DV09 A082:D... F 2021-02-12T18:33:55.000 0.018645 [217.98..219.85GHz,1128.91kHz,398.4uJy/beam@10... 227.913497 1434.115718 Rico Villas, Fernando T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1337 1338 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 108.29 110.16 109.23 1.873 1938.48 5.366 24.940 55.903 10.485 468.79 20.59 uid://A001/X1465/X389c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X389c cube 2 NGC4418 186.727617 -0.877642 0.015529 Polygon ICRS 186.727617 -0.869878 186.729072 -... 1.356746 58787.582055 58825.599964 4898.880 4898.880 0.002721 0.002768 55868.832936 /XX/YY/ phot.flux.density;phys.polarization 3 5.810830e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.468785 0.010485 2.368327 uid://A001/X1465/X389b uid://A001/X1465/X389c uid://A002/Xe2ada9/X15596 A decisive answer on the carbon isotopic ratio... S TARGET T 24.939648 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-17T19:10:59.000 1.356746 [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... 104.161888 5274.300699 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1338 1339 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 91.70 93.57 92.63 1.873 1938.48 6.210 27.132 59.612 10.282 508.68 20.77 uid://A001/X1465/X3888 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3888 cube 2 NGC4945 196.363663 -49.467900 0.016559 Polygon ICRS 196.371150 -49.461202 196.372949 ... 2.522933 58830.525869 58831.619778 10765.440 10765.440 0.003204 0.003269 48272.592043 /XX/YY/ phot.flux.density;phys.polarization 3 5.811169e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.508682 0.010282 3.740537 uid://A001/X1465/X3887 uid://A001/X1465/X3888 uid://A002/Xe50c9e/X11047 A decisive answer on the carbon isotopic ratio... S TARGET T 27.131876 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-06T23:21:24.000 2.522933 [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... 97.681492 5609.869359 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1339 1340 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 97.97 99.84 98.90 1.873 1938.48 5.820 24.940 55.903 10.485 507.47 21.40 uid://A001/X1465/X389c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X389c cube 2 NGC4418 186.727617 -0.877642 0.015529 Polygon ICRS 186.727617 -0.869878 186.729072 -... 1.356746 58787.582055 58825.599964 4898.880 4898.880 0.003003 0.003060 51508.746588 /XX/YY/ phot.flux.density;phys.polarization 3 5.810830e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.507473 0.010485 2.368327 uid://A001/X1465/X389b uid://A001/X1465/X389c uid://A002/Xe2ada9/X15596 A decisive answer on the carbon isotopic ratio... S TARGET T 24.939648 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-17T19:10:59.000 1.356746 [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... 104.161888 5274.300699 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1340 1341 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 96.28 98.15 97.21 1.873 1938.48 5.920 24.940 55.903 10.485 511.67 21.39 uid://A001/X1465/X389c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X389c cube 2 NGC4418 186.727617 -0.877642 0.015529 Polygon ICRS 186.727617 -0.869878 186.729072 -... 1.356746 58787.582055 58825.599964 4898.880 4898.880 0.003054 0.003114 50638.217620 /XX/YY/ phot.flux.density;phys.polarization 3 5.810830e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.511673 0.010485 2.368327 uid://A001/X1465/X389b uid://A001/X1465/X389c uid://A002/Xe2ada9/X15596 A decisive answer on the carbon isotopic ratio... S TARGET T 24.939648 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-17T19:10:59.000 1.356746 [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... 104.161888 5274.300699 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1341 1342 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 108.87 110.74 109.80 1.873 1938.48 5.338 22.321 55.608 18.936 799.25 35.19 uid://A001/X1465/X388c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X388c cube 2 NGC4945 196.363663 -49.467900 0.015447 Circle ICRS 196.363663 -49.467900 0.007723 2.309410 58803.513052 58803.528983 876.960 876.960 0.002707 0.002754 56162.029463 /XX/YY/ phot.flux.density;phys.polarization 3 5.811359e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.799253 0.018936 3.860288 uid://A001/X1465/X388b uid://A001/X1465/X388c uid://A002/Xe37224/X14cf9 A decisive answer on the carbon isotopic ratio... S TARGET T 22.320877 1.875000e+09 A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... F 2021-03-05T20:54:34.000 2.309410 [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... 104.713465 5246.997281 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1342 1343 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 110.76 112.63 111.69 1.873 1938.48 5.247 22.321 55.608 18.936 792.83 35.21 uid://A001/X1465/X388c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X388c cube 2 NGC4945 196.363663 -49.467900 0.015447 Circle ICRS 196.363663 -49.467900 0.007723 2.309410 58803.513052 58803.528983 876.960 876.960 0.002662 0.002707 57136.004067 /XX/YY/ phot.flux.density;phys.polarization 3 5.811359e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.792833 0.018936 3.860288 uid://A001/X1465/X388b uid://A001/X1465/X388c uid://A002/Xe37224/X14cf9 A decisive answer on the carbon isotopic ratio... S TARGET T 22.320877 1.875000e+09 A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... F 2021-03-05T20:54:34.000 2.309410 [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... 104.713465 5246.997281 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1343 1344 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 98.49 100.36 99.42 1.873 1938.48 5.791 22.321 55.608 18.936 976.30 41.27 uid://A001/X1465/X388c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X388c cube 2 NGC4945 196.363663 -49.467900 0.015447 Circle ICRS 196.363663 -49.467900 0.007723 2.309410 58803.513052 58803.528983 876.960 876.960 0.002987 0.003044 51772.734587 /XX/YY/ phot.flux.density;phys.polarization 3 5.811359e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.976296 0.018936 3.860288 uid://A001/X1465/X388b uid://A001/X1465/X388c uid://A002/Xe37224/X14cf9 A decisive answer on the carbon isotopic ratio... S TARGET T 22.320877 1.875000e+09 A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... F 2021-03-05T20:54:34.000 2.309410 [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... 104.713465 5246.997281 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1344 1345 2019.1.00130.S NGC4945 196.363663 -49.467900 2.309 96.80 98.67 97.73 1.873 1938.48 5.890 22.321 55.608 18.936 984.33 41.26 uid://A001/X1465/X388c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X388c cube 2 NGC4945 196.363663 -49.467900 0.015447 Circle ICRS 196.363663 -49.467900 0.007723 2.309410 58803.513052 58803.528983 876.960 876.960 0.003038 0.003097 50901.751170 /XX/YY/ phot.flux.density;phys.polarization 3 5.811359e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.984333 0.018936 3.860288 uid://A001/X1465/X388b uid://A001/X1465/X388c uid://A002/Xe37224/X14cf9 A decisive answer on the carbon isotopic ratio... S TARGET T 22.320877 1.875000e+09 A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... F 2021-03-05T20:54:34.000 2.309410 [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... 104.713465 5246.997281 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1345 1346 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 103.38 105.26 104.32 1.873 1938.48 5.621 20.838 59.730 9.858 461.89 19.82 uid://A001/X1465/X3890 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3890 cube 2 NGC1068 40.669879 -0.013289 0.016592 Polygon ICRS 40.669879 -0.021585 40.668325 -0.... 1.608789 58790.229826 58802.118198 9918.720 9918.720 0.002848 0.002900 53330.846587 /XX/YY/ phot.flux.density;phys.polarization 3 5.811652e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.461887 0.009858 2.751755 uid://A001/X1465/X388f uid://A001/X1465/X3890 uid://A002/Xe2eefc/X31df A decisive answer on the carbon isotopic ratio... S TARGET T 20.837939 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-10T20:24:07.000 1.608789 [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... 97.487731 5621.370692 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1346 1347 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 101.58 103.45 102.51 1.873 1938.48 5.721 20.838 59.730 9.858 459.66 19.55 uid://A001/X1465/X3890 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3890 cube 2 NGC1068 40.669879 -0.013289 0.016592 Polygon ICRS 40.669879 -0.021585 40.668325 -0.... 1.608789 58790.229826 58802.118198 9918.720 9918.720 0.002898 0.002951 52398.067385 /XX/YY/ phot.flux.density;phys.polarization 3 5.811652e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.459663 0.009858 2.751755 uid://A001/X1465/X388f uid://A001/X1465/X3890 uid://A002/Xe2eefc/X31df A decisive answer on the carbon isotopic ratio... S TARGET T 20.837939 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-10T20:24:07.000 1.608789 [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... 97.487731 5621.370692 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1347 1348 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 91.51 93.39 92.45 1.873 1938.48 6.223 20.838 59.730 9.858 480.47 19.59 uid://A001/X1465/X3890 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3890 cube 2 NGC1068 40.669879 -0.013289 0.016592 Polygon ICRS 40.669879 -0.021585 40.668325 -0.... 1.608789 58790.229826 58802.118198 9918.720 9918.720 0.003210 0.003276 48173.837781 /XX/YY/ phot.flux.density;phys.polarization 3 5.811652e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.480466 0.009858 2.751755 uid://A001/X1465/X388f uid://A001/X1465/X3890 uid://A002/Xe2eefc/X31df A decisive answer on the carbon isotopic ratio... S TARGET T 20.837939 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-10T20:24:07.000 1.608789 [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... 97.487731 5621.370692 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1348 1349 2019.1.00130.S NGC1068 40.669879 -0.013289 1.609 89.72 91.59 90.65 1.873 1938.48 6.345 20.838 59.730 9.858 494.60 19.97 uid://A001/X1465/X3890 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3890 cube 2 NGC1068 40.669879 -0.013289 0.016592 Polygon ICRS 40.669879 -0.021585 40.668325 -0.... 1.608789 58790.229826 58802.118198 9918.720 9918.720 0.003273 0.003342 47246.711574 /XX/YY/ phot.flux.density;phys.polarization 3 5.811652e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.494603 0.009858 2.751755 uid://A001/X1465/X388f uid://A001/X1465/X3890 uid://A002/Xe2eefc/X31df A decisive answer on the carbon isotopic ratio... S TARGET T 20.837939 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-10T20:24:07.000 1.608789 [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... 97.487731 5621.370692 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1349 1350 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 89.43 91.30 90.36 1.873 1938.48 6.364 27.048 59.922 9.343 466.81 18.82 uid://A001/X1465/X3898 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3898 cube 2 NGC4418 186.727617 -0.877642 0.016645 Polygon ICRS 186.727617 -0.869320 186.729177 -... 2.537301 58810.445022 58842.573071 16632.000 16632.000 0.003284 0.003352 47103.985999 /XX/YY/ phot.flux.density;phys.polarization 3 5.810791e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.466810 0.009343 2.977325 uid://A001/X1465/X3897 uid://A001/X1465/X3898 uid://A002/Xe3f5bb/X3259 A decisive answer on the carbon isotopic ratio... S TARGET T 27.047713 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-07T00:23:33.000 2.537301 [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... 97.175661 5638.752118 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1350 1351 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 101.78 103.65 102.72 1.873 1938.48 5.710 27.132 59.612 10.282 475.79 20.26 uid://A001/X1465/X3888 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3888 cube 2 NGC4945 196.363663 -49.467900 0.016559 Polygon ICRS 196.371150 -49.461202 196.372949 ... 2.522933 58830.525869 58831.619778 10765.440 10765.440 0.002892 0.002945 52507.569686 /XX/YY/ phot.flux.density;phys.polarization 3 5.811169e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.475794 0.010282 3.740537 uid://A001/X1465/X3887 uid://A001/X1465/X3888 uid://A002/Xe50c9e/X11047 A decisive answer on the carbon isotopic ratio... S TARGET T 27.131876 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-06T23:21:24.000 2.522933 [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... 97.681492 5609.869359 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1351 1352 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 108.65 110.52 109.59 1.873 1938.48 5.349 21.118 55.719 21.996 960.67 42.25 uid://A001/X1465/X3894 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3894 cube 2 NGC1068 40.669879 -0.013289 0.015477 Circle ICRS 40.669879 -0.013289 0.007739 2.246874 58803.153086 58803.168742 846.720 846.720 0.002712 0.002759 56045.630140 /XX/YY/ phot.flux.density;phys.polarization 3 5.811774e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.960667 0.021996 5.121032 uid://A001/X1465/X3893 uid://A001/X1465/X3894 uid://A002/Xe37224/X12917 A decisive answer on the carbon isotopic ratio... S TARGET T 21.118095 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-05T21:54:54.000 2.246874 [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... 104.505756 5257.484293 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1352 1353 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 110.54 112.42 111.48 1.873 1938.48 5.257 21.118 55.719 21.996 1131.63 50.21 uid://A001/X1465/X3894 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3894 cube 2 NGC1068 40.669879 -0.013289 0.015477 Circle ICRS 40.669879 -0.013289 0.007739 2.246874 58803.153086 58803.168742 846.720 846.720 0.002667 0.002712 57022.035883 /XX/YY/ phot.flux.density;phys.polarization 3 5.811774e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 1.131625 0.021996 5.121032 uid://A001/X1465/X3893 uid://A001/X1465/X3894 uid://A002/Xe37224/X12917 A decisive answer on the carbon isotopic ratio... S TARGET T 21.118095 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-05T21:54:54.000 2.246874 [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... 104.505756 5257.484293 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1353 1354 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 98.29 100.16 99.23 1.873 1938.48 5.802 21.118 55.719 21.996 1007.18 42.54 uid://A001/X1465/X3894 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3894 cube 2 NGC1068 40.669879 -0.013289 0.015477 Circle ICRS 40.669879 -0.013289 0.007739 2.246874 58803.153086 58803.168742 846.720 846.720 0.002993 0.003050 51667.340290 /XX/YY/ phot.flux.density;phys.polarization 3 5.811774e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 1.007181 0.021996 5.121032 uid://A001/X1465/X3893 uid://A001/X1465/X3894 uid://A002/Xe37224/X12917 A decisive answer on the carbon isotopic ratio... S TARGET T 21.118095 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-05T21:54:54.000 2.246874 [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... 104.505756 5257.484293 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1354 1355 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 103.05 104.92 103.99 1.873 1938.48 5.639 27.048 59.922 9.343 436.95 18.72 uid://A001/X1465/X3898 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3898 cube 2 NGC4418 186.727617 -0.877642 0.016645 Polygon ICRS 186.727617 -0.869320 186.729177 -... 2.537301 58810.445022 58842.573071 16632.000 16632.000 0.002857 0.002909 53166.454513 /XX/YY/ phot.flux.density;phys.polarization 3 5.810791e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.436953 0.009343 2.977325 uid://A001/X1465/X3897 uid://A001/X1465/X3898 uid://A002/Xe3f5bb/X3259 A decisive answer on the carbon isotopic ratio... S TARGET T 27.047713 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-07T00:23:33.000 2.537301 [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... 97.175661 5638.752118 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1355 1356 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 91.20 93.07 92.13 1.873 1938.48 6.243 27.048 59.922 9.343 459.55 18.71 uid://A001/X1465/X3898 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3898 cube 2 NGC4418 186.727617 -0.877642 0.016645 Polygon ICRS 186.727617 -0.869320 186.729177 -... 2.537301 58810.445022 58842.573071 16632.000 16632.000 0.003221 0.003287 48017.332095 /XX/YY/ phot.flux.density;phys.polarization 3 5.810791e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.459546 0.009343 2.977325 uid://A001/X1465/X3897 uid://A001/X1465/X3898 uid://A002/Xe3f5bb/X3259 A decisive answer on the carbon isotopic ratio... S TARGET T 27.047713 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-07T00:23:33.000 2.537301 [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... 97.175661 5638.752118 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1356 1357 2019.1.00130.S NGC4418 186.727617 -0.877642 2.537 101.24 103.11 102.18 1.873 1938.48 5.740 27.048 59.922 9.343 437.00 18.56 uid://A001/X1465/X3898 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3898 cube 2 NGC4418 186.727617 -0.877642 0.016645 Polygon ICRS 186.727617 -0.869320 186.729177 -... 2.537301 58810.445022 58842.573071 16632.000 16632.000 0.002907 0.002961 52231.920422 /XX/YY/ phot.flux.density;phys.polarization 3 5.810791e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.436998 0.009343 2.977325 uid://A001/X1465/X3897 uid://A001/X1465/X3898 uid://A002/Xe3f5bb/X3259 A decisive answer on the carbon isotopic ratio... S TARGET T 27.047713 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-07T00:23:33.000 2.537301 [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... 97.175661 5638.752118 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1357 1358 2019.1.00130.S NGC1068 40.669879 -0.013289 2.247 96.60 98.47 97.53 1.873 1938.48 5.902 21.118 55.719 21.996 1015.52 42.52 uid://A001/X1465/X3894 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 172.103977 -51.933584 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3894 cube 2 NGC1068 40.669879 -0.013289 0.015477 Circle ICRS 40.669879 -0.013289 0.007739 2.246874 58803.153086 58803.168742 846.720 846.720 0.003045 0.003104 50793.714099 /XX/YY/ phot.flux.density;phys.polarization 3 5.811774e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC1068_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 1.015517 0.021996 5.121032 uid://A001/X1465/X3893 uid://A001/X1465/X3894 uid://A002/Xe37224/X12917 A decisive answer on the carbon isotopic ratio... S TARGET T 21.118095 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-05T21:54:54.000 2.246874 [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... 104.505756 5257.484293 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1358 1359 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 103.59 105.46 104.52 1.873 1938.48 5.610 27.132 59.612 10.282 478.30 20.54 uid://A001/X1465/X3888 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3888 cube 2 NGC4945 196.363663 -49.467900 0.016559 Polygon ICRS 196.371150 -49.461202 196.372949 ... 2.522933 58830.525869 58831.619778 10765.440 10765.440 0.002843 0.002894 53440.185286 /XX/YY/ phot.flux.density;phys.polarization 3 5.811169e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.478302 0.010282 3.740537 uid://A001/X1465/X3887 uid://A001/X1465/X3888 uid://A002/Xe50c9e/X11047 A decisive answer on the carbon isotopic ratio... S TARGET T 27.131876 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-06T23:21:24.000 2.522933 [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... 97.681492 5609.869359 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1359 1360 2019.1.00130.S NGC4945 196.363663 -49.467900 2.523 89.90 91.77 90.84 1.873 1938.48 6.332 27.132 59.612 10.282 513.50 20.76 uid://A001/X1465/X3888 http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 305.271559 13.340115 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X3888 cube 2 NGC4945 196.363663 -49.467900 0.016559 Polygon ICRS 196.371150 -49.461202 196.372949 ... 2.522933 58830.525869 58831.619778 10765.440 10765.440 0.003267 0.003335 47345.641143 /XX/YY/ phot.flux.density;phys.polarization 3 5.811169e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4945_a_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.513502 0.010282 3.740537 uid://A001/X1465/X3887 uid://A001/X1465/X3888 uid://A002/Xe50c9e/X11047 A decisive answer on the carbon isotopic ratio... S TARGET T 27.131876 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-04-06T23:21:24.000 2.522933 [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... 97.681492 5609.869359 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431
1360 1361 2019.1.00130.S NGC4418 186.727617 -0.877642 1.357 110.17 112.05 111.11 1.873 1938.48 5.274 24.940 55.903 10.485 465.01 20.60 uid://A001/X1465/X389c http://almascience.org/aq?member_ous_id=uid://... text/html 2019.1.00130.S Public 290.048542 61.379017 ADS/JAO.ALMA#2019.1.00130.S ALMA JAO ALMA uid://A001/X1465/X389c cube 2 NGC4418 186.727617 -0.877642 0.015529 Polygon ICRS 186.727617 -0.869878 186.729072 -... 1.356746 58787.582055 58825.599964 4898.880 4898.880 0.002676 0.002721 56840.228703 /XX/YY/ phot.flux.density;phys.polarization 3 5.810830e+14 <NA> The 12C/13C isotopic ratio is a good tracer of... NGC4418_b_03_TM1 Krips, Melanie; Garcia-Burillo, Santiago; Mueh... 0.465008 0.010485 2.368327 uid://A001/X1465/X389b uid://A001/X1465/X389c uid://A002/Xe2ada9/X15596 A decisive answer on the carbon isotopic ratio... S TARGET T 24.939648 1.875000e+09 A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... F 2021-03-17T19:10:59.000 1.356746 [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... 104.161888 5274.300699 Martin, Sergio T Starbursts, star formation, Galaxy chemistry Active galaxies 2021-06-16T16:46:50.431

1361 rows × 81 columns

2.2 Summarize results

The alminer.summary function will print a summary of the observations. This is done by default when the query is run, but it’s a useful function if the results are filtered further, as shown in the next section.

Example 2.2.1: print the summary of a given query result, including a list of unique ALMA target names

[4]:
alminer.summary(observations)
--------------------------------
Number of projects = 47
Number of observations = 339
Number of unique subbands = 1162
Total number of subbands = 1361
63 target(s) with ALMA data = ['LESS J0332-2756', 'PKS1830-211', 'ngc4418', 'NGC7469', 'NGC_1097', 'Arp220', 'NGC_5253', 'M83', 'NGC253', 'NGC1266', 'vv114', 'Mystery_Object', 'Sgr_A_star', 'SDSS_J080430.99+360718.1', 'ngc_3256', 'NGC_3256', 'NGC_55', 'ngc3256', 'NGC4418', 'NGC_3627_BE', 'circinus', 'IRAS_F16399-0937', 'ngc6240', 'ngc613', 'n613', 'ngc253', 'N159-E', 'N159-W', 'N159-W_south', 'm83', 'IRAS_13120-5453', 'ngc4945', 'HE1353-1917', 'HE0108-4743', 'HE1108-2813', 'HE1029-1831', 'HE0433-1028', 'Y052343.48-680033.9', 'Y045406.43-664601.4', 'Y045358.57-691106.7', 'Y051912.27-690907.2', 'Y045100.16-691934.4', 'Y052210.08-673459.6', 'Y052423.39-693904.7', 'ST6', 'Y051916.87-693757.5', 'Y054826.21-700850.2', 'Y050953.89-685336.7', 'Y052333.40-693712.1', 'Y053952.11-710930.7', 'Y045622.61-663656.9', 'Y054248.90-694446.3', 'Y054629.32-693514.2', 'Y051344.99-693510.6', 'Y050355.87-672045.1', 'Y044854.41-690948.3', 'ST10', 'ngc4526', 'Cloverleaf', 'ngc7465', 'NGC_253', 'NGC4945', 'NGC1068']
--------------------------------

Example 2.2.2: print the summary of a given query result WITHOUT the list of target names

For big tables, it is useful to avoid printing the list of target names in the summary. This can be done by setting print_targets=False.

[5]:
alminer.summary(observations, print_targets=False)
--------------------------------
Number of projects = 47
Number of observations = 339
Number of unique subbands = 1162
Total number of subbands = 1361
Total number of targets with ALMA data = 63
--------------------------------

2.3 Filter results

The search results can be further narrowed down by using PANDAS DataFrame functions. See also this introduction to data structures. For example, you can use your_query.columns to get a list of all columns in the DataFrame.

To get the description and units of any column use the function alminer.get_info(‘column_name’) where column_name is the name of the column.

Example 2.3.1: simple selection - observations with angular resolutions < 0.5”

Let’s first check what the description and units of ang_res_arcsec column are:

[6]:
alminer.get_info('ang_res_arcsec')
--------------------------------
Column: ang_res_arcsec
--------------------------------
Description: typical spatial resolution
Units: arcsec
--------------------------------

Now we can do the some further filtering, say to only keep observations with angular resolutions < 0.5”:

[7]:
selected = observations[observations['ang_res_arcsec'] < 0.5]

and print the summary:

[8]:
alminer.summary(selected, print_targets=False)
--------------------------------
Number of projects = 23
Number of observations = 121
Number of unique subbands = 367
Total number of subbands = 484
Total number of targets with ALMA data = 41
--------------------------------

Example 2.3.2: multiple selections - observations with angular resolution < 0.5” & velocity resolution < 1 km/s

[9]:
selected = observations[(observations['ang_res_arcsec'] < 0.5) &
                        (observations['vel_res_kms'] < 1.0)]
alminer.summary(selected, print_targets=False)
--------------------------------
Number of projects = 9
Number of observations = 48
Number of unique subbands = 65
Total number of subbands = 109
Total number of targets with ALMA data = 26
--------------------------------

Example 2.3.3: observations containing a given frequency

[10]:
freq = 220.5
selected = observations[(observations["min_freq_GHz"] < freq) &
                        (observations["max_freq_GHz"] > freq)]
alminer.summary(selected, print_targets=False)
--------------------------------
Number of projects = 6
Number of observations = 7
Number of unique subbands = 7
Total number of subbands = 7
Total number of targets with ALMA data = 5
--------------------------------

2.4 Line coverage

An alternative to the last example in the previous section is the alminer.line_coverage function which determines how many targets were observed at a given frequency with the option to include a redshift for the line of interest to be taken into account. Some notes: * Line frequencies should be given in GHz * Redshift is by default assumed to be 0 * The line_name keyword is the user’s defined name for the frquency provided

Example 2.4.1: search whether a given frequency is covered in the observations

[11]:
myline_obs = alminer.line_coverage(observations,
                                   line_freq=220.5,
                                   z=0,
                                   line_name="My favourite line",
                                   print_targets=True)
--------------------------------
Summary of 'My favourite line' observations at 220.5 GHz
--------------------------------
Number of projects = 6
Number of observations = 7
Number of unique subbands = 7
Total number of subbands = 7
5 target(s) with ALMA data = ['Arp220', 'ngc_3256', 'IRAS_13120-5453', 'ngc253', 'NGC_253']
--------------------------------

Example 2.4.2: search whether a given frequency is observed for a target at a given redshift

[12]:
myline_obs = alminer.line_coverage(observations,
                                   line_freq=400.0,
                                   z=0.5,
                                   line_name="My favourite line",
                                   print_targets=True)
--------------------------------
Summary of 'My favourite line' observations at 400.0 GHz (266.667 GHz at z=0.5)
--------------------------------
Number of projects = 8
Number of observations = 10
Number of unique subbands = 11
Total number of subbands = 11
6 target(s) with ALMA data = ['ngc4418', 'Arp220', 'ngc_3256', 'circinus', 'ngc4945', 'ngc253']
--------------------------------

2.5 Coverage of CO, 13CO, and C18O lines

The alminer.CO_lines function determines how many CO, 13CO, and C18O lines were observed in the provided DataFrame and returns a DataFrame containing all observations of these transitions.

Example 2.5.1: search whether any CO, 13CO, and C18O lines were observed in the query results

[13]:
CO_obs = alminer.CO_lines(observations, print_targets=False)
--------------------------------
Summary of 'CO (1-0)' observations at 115.271 GHz
--------------------------------
Number of projects = 4
Number of observations = 5
Number of unique subbands = 4
Total number of subbands = 5
Total number of targets with ALMA data = 3
--------------------------------
--------------------------------
Summary of 'CO (2-1)' observations at 230.538 GHz
--------------------------------
Number of projects = 10
Number of observations = 13
Number of unique subbands = 13
Total number of subbands = 13
Total number of targets with ALMA data = 8
--------------------------------
--------------------------------
Summary of 'CO (3-2)' observations at 345.796 GHz
--------------------------------
Number of projects = 3
Number of observations = 5
Number of unique subbands = 5
Total number of subbands = 5
Total number of targets with ALMA data = 4
--------------------------------
--------------------------------
Summary of 'CO (4-3)' observations at 461.041 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'CO (5-4)' observations at 576.268 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'CO (6-5)' observations at 691.473 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'CO (7-6)' observations at 806.652 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'CO (8-7)' observations at 921.8 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of '13CO (1-0)' observations at 110.201 GHz
--------------------------------
Number of projects = 18
Number of observations = 23
Number of unique subbands = 23
Total number of subbands = 25
Total number of targets with ALMA data = 17
--------------------------------
--------------------------------
Summary of '13CO (2-1)' observations at 220.399 GHz
--------------------------------
Number of projects = 6
Number of observations = 7
Number of unique subbands = 7
Total number of subbands = 7
Total number of targets with ALMA data = 5
--------------------------------
--------------------------------
Summary of '13CO (3-2)' observations at 330.588 GHz
--------------------------------
Number of projects = 2
Number of observations = 5
Number of unique subbands = 5
Total number of subbands = 5
Total number of targets with ALMA data = 4
--------------------------------
--------------------------------
Summary of '13CO (4-3)' observations at 440.765 GHz
--------------------------------
Number of projects = 1
Number of observations = 1
Number of unique subbands = 1
Total number of subbands = 1
Total number of targets with ALMA data = 1
--------------------------------
--------------------------------
Summary of '13CO (5-4)' observations at 550.926 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of '13CO (6-5)' observations at 661.067 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of '13CO (7-6)' observations at 771.184 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of '13CO (8-7)' observations at 881.273 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'C18O (1-0)' observations at 109.782 GHz
--------------------------------
Number of projects = 19
Number of observations = 24
Number of unique subbands = 25
Total number of subbands = 27
Total number of targets with ALMA data = 18
--------------------------------
--------------------------------
Summary of 'C18O (2-1)' observations at 219.56 GHz
--------------------------------
Number of projects = 7
Number of observations = 9
Number of unique subbands = 12
Total number of subbands = 12
Total number of targets with ALMA data = 6
--------------------------------
--------------------------------
Summary of 'C18O (3-2)' observations at 329.331 GHz
--------------------------------
Number of projects = 2
Number of observations = 3
Number of unique subbands = 3
Total number of subbands = 3
Total number of targets with ALMA data = 2
--------------------------------
--------------------------------
Summary of 'C18O (4-3)' observations at 439.089 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'C18O (5-4)' observations at 548.831 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'C18O (6-5)' observations at 658.553 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'C18O (7-6)' observations at 768.252 GHz
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'C18O (8-7)' observations at 877.922 GHz
--------------------------------
No observations found.
--------------------------------

Example 2.5.2: search whether any redshifted CO, 13CO, and C18O lines were observed in the query results

[14]:
CO_obs = alminer.CO_lines(observations, z=1, print_targets=False)
--------------------------------
Summary of 'CO (1-0)' observations at 115.2712018 GHz (57.636 GHz at z=1)
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'CO (2-1)' observations at 230.538 GHz (115.269 GHz at z=1)
--------------------------------
Number of projects = 4
Number of observations = 5
Number of unique subbands = 4
Total number of subbands = 5
Total number of targets with ALMA data = 3
--------------------------------
--------------------------------
Summary of 'CO (3-2)' observations at 345.7959899 GHz (172.898 GHz at z=1)
--------------------------------
Number of projects = 2
Number of observations = 3
Number of unique subbands = 3
Total number of subbands = 3
Total number of targets with ALMA data = 2
--------------------------------
--------------------------------
Summary of 'CO (4-3)' observations at 461.0407682 GHz (230.52 GHz at z=1)
--------------------------------
Number of projects = 10
Number of observations = 13
Number of unique subbands = 13
Total number of subbands = 13
Total number of targets with ALMA data = 8
--------------------------------
--------------------------------
Summary of 'CO (5-4)' observations at 576.2679305 GHz (288.134 GHz at z=1)
--------------------------------
Number of projects = 3
Number of observations = 6
Number of unique subbands = 6
Total number of subbands = 6
Total number of targets with ALMA data = 3
--------------------------------
--------------------------------
Summary of 'CO (6-5)' observations at 691.4730763 GHz (345.737 GHz at z=1)
--------------------------------
Number of projects = 3
Number of observations = 5
Number of unique subbands = 5
Total number of subbands = 5
Total number of targets with ALMA data = 4
--------------------------------
--------------------------------
Summary of 'CO (7-6)' observations at 806.651806 GHz (403.326 GHz at z=1)
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of 'CO (8-7)' observations at 921.7997 GHz (460.9 GHz at z=1)
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of '13CO (1-0)' observations at 110.2013218 GHz (55.101 GHz at z=1)
--------------------------------
No observations found.
--------------------------------
--------------------------------
Summary of '13CO (2-1)' observations at 220.3986195 GHz (110.199 GHz at z=1)
--------------------------------
Number of projects = 18
Number of observations = 23
Number of unique subbands = 23
Total number of subbands = 25
Total number of targets with ALMA data = 17
--------------------------------
--------------------------------
Summary of '13CO (3-2)' observations at 330.5878671 GHz (165.294 GHz at z=1)
--------------------------------
Number of projects = 1
Number of observations = 2
Number of unique subbands = 2
Total number of subbands = 2
Total number of targets with ALMA data = 1
--------------------------------
--------------------------------
Summary of '13CO (4-3)' observations at 440.7651735 GHz (220.383 GHz at z=1)
--------------------------------
Number of projects = 6
Number of observations = 7
Number of unique subbands = 7
Total number of subbands = 7
Total number of targets with ALMA data = 5
--------------------------------
--------------------------------
Summary of '13CO (5-4)' observations at 550.9262851 GHz (275.463 GHz at z=1)
--------------------------------
Number of projects = 3
Number of observations = 4
Number of unique subbands = 4
Total number of subbands = 4
Total number of targets with ALMA data = 3
--------------------------------
--------------------------------
Summary of '13CO (6-5)' observations at 661.0672766 GHz (330.534 GHz at z=1)
--------------------------------
Number of projects = 2
Number of observations = 5
Number of unique subbands = 5
Total number of subbands = 5
Total number of targets with ALMA data = 4
--------------------------------
--------------------------------
Summary of '13CO (7-6)' observations at 771.184125 GHz (385.592 GHz at z=1)
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No observations found.
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Summary of '13CO (8-7)' observations at 881.272808 GHz (440.636 GHz at z=1)
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Number of projects = 1
Number of observations = 1
Number of unique subbands = 1
Total number of subbands = 1
Total number of targets with ALMA data = 1
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Summary of 'C18O (1-0)' observations at 109.7821734 GHz (54.891 GHz at z=1)
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No observations found.
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Summary of 'C18O (2-1)' observations at 219.5603541 GHz (109.78 GHz at z=1)
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Number of projects = 19
Number of observations = 24
Number of unique subbands = 25
Total number of subbands = 27
Total number of targets with ALMA data = 18
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Summary of 'C18O (3-2)' observations at 329.3305525 GHz (164.665 GHz at z=1)
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Number of projects = 1
Number of observations = 2
Number of unique subbands = 2
Total number of subbands = 2
Total number of targets with ALMA data = 1
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Summary of 'C18O (4-3)' observations at 439.0887658 GHz (219.544 GHz at z=1)
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Number of projects = 7
Number of observations = 9
Number of unique subbands = 12
Total number of subbands = 12
Total number of targets with ALMA data = 6
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Summary of 'C18O (5-4)' observations at 548.8310055 GHz (274.416 GHz at z=1)
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Number of projects = 2
Number of observations = 3
Number of unique subbands = 3
Total number of subbands = 3
Total number of targets with ALMA data = 2
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Summary of 'C18O (6-5)' observations at 658.5532782 GHz (329.277 GHz at z=1)
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Number of projects = 2
Number of observations = 3
Number of unique subbands = 3
Total number of subbands = 3
Total number of targets with ALMA data = 2
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Summary of 'C18O (7-6)' observations at 768.2515933 GHz (384.126 GHz at z=1)
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No observations found.
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Summary of 'C18O (8-7)' observations at 877.9219553 GHz (438.961 GHz at z=1)
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No observations found.
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