2023MNRAS.521.5508H

Query : 2023MNRAS.521.5508H

2023MNRAS.521.5508H - Mon. Not. R. Astron. Soc., 521, 5508-5535 (2023/June-1)

Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71 Herschel targets.

HAGIMOTO M., BAKX T.J.L.C., SERJEANT S., BENDO G.J., URQUHART S.A., EALES S., HARRINGTON K.C., TAMURA Y., UMEHATA H., BERTA S., COORAY A.R., COX P., DE ZOTTI G., LEHNERT M.D., RIECHERS D.A., SCOTT D., TEMI P., VAN DER WERF P.P., YANG C., AMVROSIADIS A., ANDREANI P.M., BAKER A.J., BEELEN A., BORSATO E., BUAT V., BUTLER K.M., DANNERBAUER H., DUNNE L., DYE S., ENIA A.F.M., FAN L., GAVAZZI R., GONZALEZ-NUEVO J., HARRIS A.I., HERRERA C.N., HUGHES D.H., ISMAIL D., IVISON R.J., JONES B., KOHNO K., KRIPS M., LAGACHE G., MARCHETTI L., MASSARDI M., MESSIAS H., NEGRELLO M., NERI R., OMONT A., PEREZ-FOURNON I., SEDGWICK C., SMITH M.W.L., STANLEY F., VERMA A., VLAHAKIS C., WARD B., WEINER C., WEISS A. and YOUNG A.J.

Abstract (from CDS):

We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array. These lines include a total of 156 CO, [C I], and H2O emission lines. For 46 galaxies, we detect two transitions of CO lines, and for these galaxies we find gas properties similar to those of other dusty star-forming galaxy (DSFG) samples. A comparison to photodissociation models suggests that most of Herschel-selected galaxies have similar interstellar medium conditions as local infrared-luminous galaxies and high-redshift DSFGs, although with denser gas and more intense far-ultraviolet radiation fields than normal star-forming galaxies. The line luminosities agree with the luminosity scaling relations across five orders of magnitude, although the star formation and gas surface density distributions (i.e. Schmidt-Kennicutt relation) suggest a different star formation phase in our galaxies (and other DSFGs) compared to local and low-redshift gas-rich, normal star-forming systems. The gas-to-dust ratios of these galaxies are similar to Milky Way values, with no apparent redshift evolution. Four of 46 sources appear to have CO line ratios in excess of the expected maximum (thermalized) profile, suggesting a rare phase in the evolution of DSFGs. Finally, we create a deep stacked spectrum over a wide rest-frame frequency (220-890 GHz) that reveals faint transitions from HCN and CH, in line with previous stacking experiments.

Abstract Copyright: © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): galaxies: high-redshift - galaxies: ISM - infrared: galaxies - submillimetre: galaxies

Simbad objects: 51

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Number of rows : 51
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 HerBS 42 G 00 00 07.4 -33 40 59           ~ 11 0
2 HerBS 41 G 00 01 24.9 -35 42 12           ~ 11 0
3 H-ATLAS J000330.7-321136 G 00 03 30.7 -32 11 36           ~ 7 0
4 HerBS 117 G 00 08 06.80 -35 12 05.0           ~ 5 0
5 HerBS 106 G 00 18 02.16 -31 35 04.8           ~ 7 0
6 HerBS 22 G 00 26 24.8 -34 17 37           ~ 12 0
7 HerBS 24 G 00 47 36.0 -27 29 53           ~ 9 0
8 HerBS 57 G 00 48 53.2 -30 31 09           ~ 8 0
9 NAME SGP reg 00 51 26.275 -27 07 41.70           ~ 606 0
10 H-ATLAS J005132.0-302011 G 00 51 32.0 -30 20 11           ~ 7 0
11 H-ATLAS J005506.5-300027 G 00 55 06.5 -30 00 27           ~ 5 0
12 H-ATLAS J005629.6-311206 G 00 56 29.6 -31 12 06           ~ 5 0
13 H-ATLAS J005659.4-295039 G 00 56 59.4 -29 50 39           ~ 4 0
14 HerBS 60 G 00 57 24.2 -27 31 22           ~ 7 0
15 H-ATLAS J011014.5-314814 G 01 10 14.5 -31 48 14           ~ 6 0
16 HerBS 27 G 01 14 24.04 -33 36 13.7           ~ 7 0
17 H-ATLAS J012222.3-274456 G 01 22 22.3 -27 44 56           ~ 4 0
18 H-ATLAS J012335.1-314619 G 01 23 35.1 -31 46 18           ~ 7 0
19 HerBS 11 G 01 24 07.3 -28 14 34           ~ 11 0
20 HerBS 69 G 01 24 15.9 -31 05 00           ~ 7 0
21 HerBS 73 G 01 28 53.00 -33 27 19.3           ~ 6 0
22 HerBS 14 G 01 38 40.4 -28 18 55           ~ 9 0
23 H-ATLAS J013951.9-321446 G 01 39 51.9 -32 14 46           ~ 7 0
24 H-ATLAS J014313.2-332633 G 01 43 13.2 -33 26 33           ~ 6 0
25 H-ATLAS J014520.0-313835 G 01 45 20.0 -31 38 35           ~ 5 0
26 QSO J0831+5245 QSO 08 31 41.7108197808 +52 45 17.616994560   19.2   14.5 13.9 ~ 574 1
27 2MASX J13150638-5509225 Sy2 13 15 06.33480 -55 09 22.7736   17.3       ~ 172 0
28 QSO J1415+1129 QSO 14 15 46.25 +11 29 43.4   17.63 17.23     ~ 678 0
29 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
30 NGC 6240 Sy2 16 52 58.9 +02 24 03   14.31 13.37     ~ 1734 2
31 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
32 NAME Eyelash LeG 21 35 11.60 -01 02 52.0           ~ 245 0
33 H-ATLAS J223615.2-343301 G 22 36 15.2 -34 33 01           ~ 5 0
34 HerBS 111 G 22 39 42.44 -33 33 04.4           ~ 7 0
35 H-ATLAS J224920.6-332940 G 22 49 20.6 -33 29 40           ~ 6 0
36 H-ATLAS J225045.5-304719 G 22 50 45.5 -30 47 19           ~ 5 0
37 HerBS 47 G 22 52 50.7 -31 36 57           ~ 9 0
38 HerBS 189 G 22 56 00.69 -31 32 31.6           ~ 6 0
39 H-ATLAS J230538.5-312204 G 23 05 38.5 -31 22 04           ~ 7 0
40 HerBS 28 G 23 08 15.5 -34 38 01           ~ 10 0
41 H-ATLAS J231205.2-295027 G 23 12 05.2 -29 50 27           ~ 6 0
42 HerBS 18 G 23 24 19.8 -32 39 26           ~ 10 0
43 HerBS 37 G 23 26 23.0 -34 26 42           ~ 10 0
44 HerBS 39 G 23 29 00.6 -32 17 44           ~ 10 0
45 H-ATLAS J233024.1-325032 G 23 30 24.1 -32 50 32           ~ 4 0
46 H-ATLAS J233037.3-331218 G 23 30 37.3 -33 12 18           ~ 5 0
47 HerBS 21 G 23 44 18.1 -30 39 36           ~ 10 0
48 H-ATLAS J234750.5-352931 G 23 47 50.5 -35 29 31           ~ 8 0
49 H-ATLAS J235122.0-332902 G 23 51 22.0 -33 29 02           ~ 7 0
50 H-ATLAS J235324.7-331111 G 23 53 24.7 -33 11 11           ~ 8 0
51 HerBS 25 G 23 58 27.6 -32 32 44           ~ 10 0

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