2009ApJS..182..628V

Query : 2009ApJS..182..628V

2009ApJS..182..628V - Astrophys. J., Suppl. Ser., 182, 628-666 (2009/June-0)

Spitzer quasar and ULIRG evolution study (QUEST). IV. Comparison of 1 Jy ultraluminous infrared galaxies with Palomar-Green quasars.

VEILLEUX S., RUPKE D.S.N., KIM D.-C., GENZEL R., STURM E., LUTZ D., CONTURSI A., SCHWEITZER M., TACCONI L.J., NETZER H., STERNBERG A., MIHOS J.C., BAKER A.J., MAZZARELLA J.M., LORD S., SANDERS D.B., STOCKTON A., JOSEPH R.D. and BARNES J.E.

Abstract (from CDS):

We report the results from a comprehensive study of 74 ultraluminous infrared galaxies (ULIRGs) and 34 Palomar-Green (PG) quasars within z ∼ 0.3 observed with the Spitzer Infrared Spectrograph (IRS). The contribution of nuclear activity to the bolometric luminosity in these systems is quantified using six independent methods that span a range in wavelength and give consistent results within ~±10%-15% on average. This agreement suggests that deeply buried active galactic nuclei (AGNs) invisible to Spitzer IRS but bright in the far-infrared are not common in this sample. The average derived AGN contribution in ULIRGs is ∼35%-40%, ranging from ∼15%-35% among "cool" (f 25/f60≤ 0.2) optically classified H II-like and LINER ULIRGs to ∼50 and ∼75% among warm Seyfert 2 and Seyfert 1 ULIRGs, respectively. This number exceeds ∼80% in PG QSOs. ULIRGs fall in one of three distinct AGN classes: (1) objects with small extinctions and large polycyclic aromatic hydrocarbon (PAH) equivalent widths are highly starburst-dominated; (2) systems with large extinctions and modest PAH equivalent widths have larger AGN contributions, but still tend to be starburst-dominated; and (3) ULIRGs with both small extinctions and small PAH equivalent widths host AGN that are at least as powerful as the starbursts. The AGN contributions in class 2 ULIRGs are more uncertain than in the other objects, and we cannot formally rule out the possibility that these objects represent a physically distinct type of ULIRGs. A morphological trend is seen along the sequence (1)-(2)-(3), in general agreement with the standard ULIRG-QSO evolution scenario and suggestive of a broad peak in extinction during the intermediate stages of merger evolution. However, the scatter in this sequence, including the presence of a significant number of AGN-dominated systems prior to coalescence and starburst-dominated but fully merged systems, implies that black hole accretion, in addition to depending on the merger phase, also has a strong chaotic/random component, as in local AGNs.

Abstract Copyright: ∼

Journal keyword(s): galaxies: active - galaxies: interactions - galaxies: Seyfert - galaxies: starburst - infrared: galaxies - quasars: general

VizieR on-line data: <Available at CDS (J/ApJS/182/628): table1.dat table2.dat table34.dat table5.dat table6.dat table7.dat table8.dat table12.dat table16.dat>

Errata: erratum vol. 213, art. 36 (2014)

Simbad objects: 112

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Number of rows : 112
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 89873 AGN 00 11 43.30008 -07 22 07.0644   18.41       ~ 64 0
2 IRAS 00182-7112 Sy2 00 20 34.72104 -70 55 26.2488     20.6     ~ 143 0
3 2MASX J00212652-0839261 LIN 00 21 26.5135306416 -08 39 25.967117268   18.37       ~ 124 1
4 LEDA 1790 Sy1 00 29 13.7012449608 +13 16 03.947778264   15.70 15.41     ~ 474 0
5 LEDA 165307 AGN 00 42 15.51192 -12 56 03.3108   19.45       ~ 86 0
6 IRAS 00456-2904 AGN 00 48 06.7010068082 -28 48 18.548437413   18.14       ~ 61 1
7 2MASS J00504031-2704390 LIN 00 50 40.31136 -27 04 39.0036   18.369   18.305   ~ 40 0
8 Mrk 1502 Sy1 00 53 34.9331107632 +12 41 35.929269132   14.41 14.03     ~ 1242 1
9 IRAS 01003-2238 Sy2 01 02 49.9920152640 -22 21 57.262136544   18.62 18.9 17.83   ~ 192 0
10 6dFGS gJ011907.7-082910 H2G 01 19 07.5686096832 -08 29 09.527103312   18.54       ~ 54 1
11 IRAS 01199-2307 AGN 01 22 20.8752532152 -22 52 05.252405952   18.04     17.33 ~ 53 0
12 LEDA 89903 AGN 01 32 21.39936 -07 29 08.3112   19.04       ~ 67 0
13 PSCz Q01355-1814 H2G 01 37 56.6 -17 59 25           ~ 33 0
14 LEDA 87896 AGN 01 51 51.4245944592 -18 30 46.601041068   18.77       ~ 41 1
15 Mrk 1014 Sy1 01 59 50.2534701768 +00 23 40.864244784   16.08 15.87     ~ 606 0
16 LEDA 7897 G 02 04 27.3254183088 -20 49 41.237644872   17.45       ~ 44 0
17 2MASX J03274981+1616594 LIN 03 27 49.81440 +16 16 59.4012       21.20   ~ 52 0
18 IRAS 03521+0028 AGN 03 54 42.14640 +00 37 03.3280           ~ 104 0
19 IRAS 04103-2838 LIN 04 12 19.4458581600 -28 30 24.933273876     16.9     ~ 75 0
20 6dFGS gJ043337.1-164331 LIN 04 33 37.05 -16 43 31.5   19.80   18.54   ~ 41 0
21 LEDA 2816449 Sy2 05 04 36.53952 -19 37 03.1332           ~ 39 1
22 IRAS 05189-2524 Sy2 05 21 01.3994605776 -25 21 45.321827832   15.47 14.75     ~ 545 0
23 IRAS 07598+6508 Sy1 08 04 30.4643108040 +64 59 52.789588188   14.3 15.5     ~ 242 0
24 2MASS J08105865+7602424 Sy1 08 10 58.6641543864 +76 02 42.450451260   15.03 14.71     ~ 508 0
25 MCG+13-07-002 Sy1 08 44 45.2999013720 +76 53 09.465739008     15.7     ~ 201 0
26 Ton 951 Sy1 08 47 42.4485615096 +34 45 04.482515304   14.83 14.50     ~ 487 0
27 IRAS 08572+3915 LIN 09 00 25.38288 +39 03 54.2988     16.66     ~ 450 1
28 IRAS 09039+0503 LIN 09 06 34.0537343016 +04 51 27.447987744           ~ 86 0
29 Ton 1057 Sy1 09 25 54.7145627448 +19 54 05.064888348   16.02 15.89     ~ 187 0
30 Z 289-11 Sy2 09 35 51.6045544584 +61 21 11.589382368   15.20 15.50     ~ 617 2
31 2MASX J09530021+8127282 LIN 09 53 00.34392 +81 27 28.7748           ~ 37 0
32 IRAS 09539+0857 Sy2 09 56 34.33800 +08 43 06.2472       20.90   ~ 63 0
33 PG 0953+414 Sy1 09 56 52.3931554992 +41 15 22.211247636 14.710 15.611 15.546 15.294 14.720 ~ 472 0
34 LEDA 29208 Sy1 10 04 20.1379926888 +05 13 00.400882728   16.73 16.55     ~ 260 1
35 4C 13.41 Sy1 10 07 26.0965408440 +12 48 56.184940764   15.81 15.68     ~ 418 2
36 LEDA 165552 LIN 10 12 16.7929453584 +46 49 43.491525384       22.20   ~ 46 0
37 2MASS J10214248+1306539 AGN 10 21 42.4964040120 +13 06 53.840159676           ~ 23 0
38 IRAS 10190+1322 PaG 10 21 42.718 +13 06 55.36           ~ 88 0
39 2MASS J10214273+1306556 LIN 10 21 42.8040022344 +13 06 55.957660596   17.51       ~ 87 0
40 IRAS 10378+1109 Sy1 10 40 29.1640944744 +10 53 18.202070076   17.79 17.18     ~ 115 1
41 LEDA 32516 LIN 10 51 03.67 -15 03 19.8           ~ 47 0
42 IRAS 10565+2448 LIN 10 59 18.12811 +24 32 34.7357   15.7       ~ 302 0
43 LEDA 125693 LIN 11 12 03.37008 -02 54 22.7232   17.45 17.40     ~ 113 1
44 IRAS 11119+3257 Sy1 11 14 38.8902542640 +32 41 33.483258276   19.22 17.96     ~ 165 0
45 Ton 1388 Sy1 11 19 08.6786220240 +21 19 17.987085948   14.91 14.80     ~ 492 0
46 IC 2746 Sy2 11 21 47.1179115936 +11 44 18.909849876   15.38 14.93     ~ 234 0
47 Mrk 1298 Sy1 11 29 16.7288400936 -04 24 07.246460520   14.97 14.61     ~ 224 1
48 IRAS 11506+1331 rG 11 53 14.22000 +13 14 27.6400   17.77       ~ 67 0
49 LEDA 1888605 LIN 12 00 46.8386541480 +30 04 14.151358452           ~ 38 0
50 IRAS 12018+1941 Sy2 12 04 24.5432777064 +19 25 09.773024772           ~ 89 0
51 IRAS 12032+1707 LIN 12 05 47.7089284392 +16 51 08.355094704   18.758   17.327   ~ 68 0
52 LEDA 90164 Sy2 12 09 45.1187842872 -05 01 13.431047484   17.52 17.8 16.56   ~ 114 1
53 IRAS 12112+0305 PaG 12 13 45.98880 +02 48 39.9600           ~ 373 0
54 [CGM90] IRAS 12112+0305 NE rG 12 13 46.10735 +02 48 41.4959           ~ 369 0
55 PB 3894 Sy1 12 14 17.6738687784 +14 03 13.182723144   14.46 14.19     ~ 873 0
56 2MASX J12151913-1429422 LIN 12 15 19.134 -14 29 42.23           ~ 43 0
57 NGC 4355 Sy2 12 26 54.6206739120 -00 52 39.421212996   14.21 13.37     ~ 527 2
58 3C 273 BLL 12 29 06.6998257176 +02 03 08.597629980   13.05 14.830 14.11   ~ 6022 1
59 Z 99-79 Sy1 12 32 03.6223710000 +20 09 29.495834136   15.57 15.30     ~ 526 0
60 LBQS 1244+0238 Sy1 12 46 35.2527826632 +02 22 08.782546368   16.57 16.37     ~ 313 0
61 Z 294-4 Sy1 12 56 14.2341182928 +56 52 25.238373852   14.68 13.84     ~ 2096 3
62 QSO J1305-1033 Bla 13 05 33.0150535680 -10 33 19.430383680   15.18 15.23 14.46   ~ 624 1
63 LEDA 45656 Sy1 13 09 47.0031619008 +08 19 48.212362524   16.04 15.89     ~ 412 0
64 Ton 1565 Bla 13 12 17.7526981968 +35 15 21.086467128   15.45 15.64 14.2   ~ 292 1
65 IRAS 13218+0552 Sy2 13 24 19.8862877976 +05 37 04.693531332   19.31 18.73 17.41   ~ 130 0
66 2MASS J13362231-2627338 LIN 13 36 22.31064 -26 27 33.8832   17.93   16.90 16.27 ~ 41 1
67 IRAS 13342+3932 Sy2 13 36 24.0619427808 +39 17 31.105014396     17.76     ~ 96 0
68 Z 271-60 Sy2 13 44 42.1883001099 +55 53 13.596220922   15.68 14.91     ~ 958 3
69 PKS 1345+12 Sy2 13 47 33.36161873 +12 17 24.2398927   19.28 18.44 15.718   ~ 652 2
70 2MASX J13481941-3012017 Sy2 13 48 19.4115734304 -30 12 01.486438740   18.86 17.71     ~ 33 0
71 2XMM J135315.8+634546 Sy1 13 53 15.8311116864 +63 45 45.683126676   14.54 14.28     ~ 404 1
72 IRAS 14070+0525 Sy2 14 09 31.26096 +05 11 31.3548     17.00     ~ 78 0
73 LEDA 50824 Sy1 14 13 48.3306274368 +44 00 14.003371296   14.99 14.99     ~ 402 0
74 IRAS 14197+0812 LIN 14 22 11.6354625144 +07 59 28.013201808           ~ 33 0
75 Mrk 1383 Sy1 14 29 06.5720038632 +01 17 06.155007252   15.21 14.87     ~ 494 0
76 LEDA 52270 Sy1 14 37 38.2867288488 -15 00 24.087592692   16.58 16.40     ~ 300 2
77 LEDA 52314 Sy1 14 38 16.1630434488 -06 58 20.662907124   16.13 16.01 15.5   ~ 133 0
78 Mrk 478 Sy1 14 42 07.4714418744 +35 26 22.938625500   14.91 14.58     ~ 567 1
79 2MASX J14510879+2709272 Sy1 14 51 08.7647938560 +27 09 26.962707132   15.01 15.01     ~ 239 0
80 IRAS 15001+1433 Sy2 15 02 31.9755844913 +14 21 34.926031528   20.69 20.13     ~ 68 0
81 Mrk 841 Sy1 15 04 01.1935384104 +10 26 15.780409692   14.50 14.27     ~ 701 0
82 2MASX J15155520-2009172 Sy2 15 15 55.1783451792 -20 09 16.916691024   18.34 17.1 17.16   ~ 55 0
83 IRAS 15206+3342 Sy2 15 22 38.104 +33 31 35.90           ~ 111 0
84 2MASX J15265942+3558372 LIN 15 26 59.44451 +35 58 37.0521   15.61       ~ 295 1
85 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
86 LEDA 90222 Sy1 15 48 56.8020209304 -04 59 33.598051584   16.4 16.40 16.85   ~ 106 0
87 LEDA 90237 LIN 16 11 40.4280459768 -01 47 06.566246232   16.6       ~ 95 0
88 Mrk 876 Sy1 16 13 57.1795021224 +65 43 09.952685328   16.03 15.49     ~ 620 0
89 LEDA 2817004 Sy2 16 18 09.4114 +01 39 20.951           ~ 44 1
90 Mrk 877 Sy1 16 20 11.2799789400 +17 24 27.515242152   15.79 15.39     ~ 286 0
91 QSO B1626+5529 Sy1 16 27 56.1123628752 +55 22 31.559061504   15.79 15.68     ~ 232 1
92 IRAS 16300+1558 Sy2 16 32 21.41352 +15 51 45.8280   18.72 18.06     ~ 64 0
93 IRAS 16334+4630 LIN 16 34 52.34448 +46 24 52.7796   17.66       ~ 52 1
94 NGC 6240 Sy2 16 52 58.9 +02 24 03   14.31 13.37     ~ 1734 2
95 IRAS 17002+5153 Sy1 17 01 24.8265469104 +51 49 20.447878836   15.49 15.12     ~ 401 0
96 IRAS 17068+4027 rG 17 08 31.9721059615 +40 23 28.300445082           ~ 52 0
97 2MASX J17185436+5441486 Sy2 17 18 54.4002 +54 41 48.289           ~ 84 1
98 LEDA 60189 LIN 17 23 21.96264 -00 17 00.8088   15.1       ~ 454 0
99 6dFGS gJ204418.2-164017 LIN 20 44 18.16392 -16 40 16.8132   18.02   17.04   ~ 100 0
100 LEDA 1049091 AGN 21 23 29.13960 -05 06 56.2392           ~ 37 1
101 LEDA 66703 Sy1 21 24 41.6403183696 -17 44 45.886080696   17.18 16.50 15.95   ~ 96 0
102 Mrk 1513 Sy1 21 32 27.8162556672 +10 08 19.252365396   14.92 14.64     ~ 651 0
103 2MASX J21354580-2332359 LIN 21 35 45.8178571488 -23 32 36.305302884           ~ 41 1
104 4C 31.63 BLL 22 03 14.9756830008 +31 45 38.269473228   15.85 15.58 14.33   ~ 523 1
105 Z 428-65 Sy1 22 17 12.2637639888 +14 14 20.917852980   15.02 14.66     ~ 371 0
106 LEDA 165898 AGN 22 23 28.88208 -27 00 03.1788   17.50       ~ 46 1
107 NAME South America rG 22 51 49.27872 -17 52 24.0600   16.97       ~ 348 3
108 4C 11.72 BLL 22 54 10.4214226080 +11 36 38.748083760   16.02 15.82     ~ 351 1
109 IRAS 23129+2548 LIN 23 15 21.39960 +26 04 32.2536           ~ 54 0
110 IRAS 23233+0946 LIN 23 25 56.1378291192 +10 02 49.715916252           ~ 61 0
111 4C -01.61 BLL 23 51 56.1224889360 -01 09 13.315371768   16.83 16.59     ~ 380 1
112 2MASS J23522592+2440165 Sy2 23 52 25.9250656752 +24 40 16.806785592     16.20     ~ 57 0

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