1999A&A...341..348L

Query : 1999A&A...341..348L

1999A&A...341..348L - Astronomy and Astrophysics, volume 341348-354 (1999/1-2)

A survey of molecular gas content of galaxies at 0.08<z<1.06.

LO K.-Y., CHEN H.-W. and HO P.T.P.

Abstract (from CDS):

The study of high redshift galaxies has made tremendous progress in the last few years. In order to understand their evolution, it is important to probe the gas content of distant ``normal" galaxies beyond z∼0.3. We searched for CO emission from a sample of galaxies in the redshift range of 0.35 to 1.06. Given the current limited sensitivity, we can only place upper limits to the gas content of these progenitors to luminous field galaxies of ∼3x1011M☉. We also searched a sample of distant luminous IR galaxies and detected two new galaxies at z∼0.1. The upper limits to and the detection of CO emission from these distant galaxies are consistent with the suggested upper limit to galaxy masses of 1012M☉ posed by the cooling time argument.

Abstract Copyright: ∼

Journal keyword(s): submillimeter - galaxies: ISM - galaxies: evolution - ISM: molecules

CDS comments: U02, U05, U10 identified as IRAS 13153-1532, IRAS 14405+2634, IRAS 23220+2919

Simbad objects: 31

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Number of rows : 31
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 LEDA 2054727 G 00 41 04.2 +34 47 57           ~ 4 0
2 QSO B0109+2004 Bla 01 12 10.1908105872 +20 20 21.765069636     17 16.8   ~ 61 1
3 LAMOST J012343.44+354055.1 G 01 23 43.4455106184 +35 40 55.029467568           ~ 11 0
4 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
5 4C 13.14 Bla 02 31 45.89405619 +13 22 54.7162847   17.96 17.71 17.93   ~ 291 1
6 QSO B0235+1624 BLL 02 38 38.93010450 +16 36 59.2745528   16.46 15.50 15.92   ~ 1614 2
7 4C 05.19 QSO 04 14 37.76734974 +05 34 42.3295956   24.100 23.800 21.270   ~ 371 2
8 IRAS 04203+8120 G 04 29 42.1 +81 26 57           ~ 6 0
9 7C 082754.29+242103.00 Bla 08 30 52.08619250 +24 10 59.8202919   17.62 17.26 16.30   ~ 563 1
10 2MASX J09530021+8127282 LIN 09 53 00.34392 +81 27 28.7748           ~ 37 0
11 QSO J0957+5439 QSO 09 57 14.6711571816 +54 40 17.538366612   17.73 17.57     ~ 72 0
12 QSO B1019+309 QSO 10 22 30.2982157824 +30 41 05.119553544   17.0 17.47 17.0   ~ 103 1
13 [VV96] J102434.5+470911 Sy1 10 24 34.5 +47 09 11     20.5     ~ 489 0
14 QSO B1202-074 QSO 12 05 23.1360370080 -07 42 32.759842896     17.5     ~ 389 5
15 Z 294-4 Sy1 12 56 14.2341182928 +56 52 25.238373852   14.68 13.84     ~ 2096 3
16 IRAS 13153-1532 mul 13 17 59.2 -15 48 41           ~ 9 0
17 IRAS 13218+0552 Sy2 13 24 19.8862877976 +05 37 04.693531332   19.31 18.73 17.41   ~ 130 0
18 BRI B1335-0417 G 13 38 03.4151935680 -04 32 34.981751112   19.4       ~ 112 0
19 PB 1309 Sy1 14 04 38.7980689872 +43 27 07.452879120   16.12 15.76     ~ 134 0
20 QSO J1415+1129 QSO 14 15 46.25 +11 29 43.4   17.63 17.23     ~ 678 0
21 NVSS J144244+262134 rG 14 42 44.8293689256 +26 21 30.319683768   17.94       ~ 23 0
22 2MASX J15242648+0809082 rG 15 24 26.5043888448 +08 09 08.015998068   15       ~ 21 0
23 IRAS 16300+8407 FIR 16 22 47.6 +84 00 33           ~ 3 0
24 4C 23.43 Bla 16 24 39.0838297968 +23 45 12.223370412   17.91 17.47     ~ 343 1
25 QSO B1634+7037 QSO 16 34 28.9917184368 +70 31 32.393436960   14.90 14.66     ~ 273 0
26 6C 171301+501842 Sy2 17 14 14.758 +50 15 30.46   24.05   22.64   ~ 110 1
27 QSO J1824+1044 Bla 18 24 02.85524975 +10 44 23.7739493   17.66 17.27 16.71   ~ 182 1
28 2MASX J20044437+8354100 G 20 04 44.377 +83 54 10.00           ~ 1 0
29 [KE93] 90A G 20 05 04.2 +83 54 25           ~ 1 0
30 QSO B2128-123 BLL 21 31 35.2617909696 -12 07 04.795364172   16.33 16.11 15.87   ~ 470 1
31 IRAS 23220+2919 G 23 24 28.9 +29 35 49           ~ 11 0

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