2014ApJ...791...34N


Query : 2014ApJ...791...34N

2014ApJ...791...34N - Astrophys. J., 791, 34 (2014/August-2)

Star formation and black hole growth at z ≃ 4.8.

NETZER H., MOR R., TRAKHTENBROT B., SHEMMER O. and LIRA P.

Abstract (from CDS):

We report Herschel/SPIRE, Spitzer and Wide-field Infrared Survey Explorer observations of 44 z ≃ 4.8 optically selected active galactic nuclei (AGNs). This flux-limited sample contains the highest mass black holes (BHs) at this redshift. Ten of the objects were detected by Herschel and five show emission that is not clearly associated with the AGNs. The star formation (SF) luminosity (LSF) obtained by fitting the spectral energy distribution (SED) with standard SF templates, taking into account AGN contribution, is in the range 1046.62-1047.21 erg/s corresponding to SF rates of 1090-4240 M☉/yr. Fitting with very luminous submillimeter galaxy SEDs gives SF rates that are smaller by 0.05 dex when using all bands and 0.1 dex when ignoring the 250 µm band. A 40 K graybody fits to only the 500 µm fluxes reduce LSF by about a factor of two. A stacking analysis of 29 undetected sources gives significant signals in all three bands. A SF template fit indicates LSF= 1046.19–46.23 erg/s depending on the assumed AGN contribution. A 40 K fit to the stacked 500 µm flux gives LSF= 1045.95 erg/s. The mean BH mass (MBH) and AGN luminosity (LAGN) of the detected sources are significantly higher than those of the undetected ones. The spectral differences are seen all the way from UV to far infrared wavelengths. The mean optical-UV spectra are similar to those predicted for thin accretion disks around BHs with similar masses and accretion rates. We suggest two alternative explanations to the correlation of LSF, LAGN and MBH, one involving no AGN feedback and the second involving moderate feedback that affects, but does not totally quench, SF in three-quarters of the sources. We compare our LSFand LAGNto lower redshift samples and show a new correlation between LSFand MBH. We also examine several rather speculative ideas about the host galaxy properties including the possibility that the detected sources are above the SF mass sequence (MS) at z ≃ 4.8, perhaps in mergers, and most of the undetected sources are on the MS.

Abstract Copyright: ∼

Journal keyword(s): galaxies: active - galaxies: star formation - quasars: general

Simbad objects: 44

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Number of rows : 44
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 QSO J0007+0041 QSO 00 07 49.168 +00 41 19.61   25.36 23.11     ~ 31 0
2 QSO J0035+0040 QSO 00 35 25.2917898096 +00 40 02.807161536   24.03 22.48     ~ 36 0
3 QSO J0210-0018 QSO 02 10 43.1633481288 -00 18 18.444357900   23.49 21.97     ~ 69 0
4 QSO J0331-0741 QSO 03 31 19.6631898672 -07 41 43.170430344   25.87 22.92     ~ 41 0
5 SDSS J075907.58+180054.7 QSO 07 59 07.5819618072 +18 00 54.766391148   26.34 23.48     ~ 30 0
6 QSO J0800+3051 QSO 08 00 23.0206738560 +30 51 01.216318752   24.29 22.17     ~ 33 0
7 SDSS J080715.11+132805.1 QSO 08 07 15.1158011928 +13 28 05.183216076   24.94 22.83     ~ 27 0
8 [VV2006] J083920.6+352459 QSO 08 39 20.5358988240 +35 24 59.388807132   24.11 22.39     ~ 35 0
9 [VV2006] J085707.9+321031 QSO 08 57 07.9427028072 +32 10 31.978333488   24.88 22.39     ~ 29 0
10 [VV2006] J092303.5+024739 QSO 09 23 03.5323740816 +02 47 39.619054824   24.19 22.82     ~ 33 0
11 [VV2006] J093508.5+080114 QSO 09 35 08.5039480416 +08 01 14.516994072   23.65 22.37     ~ 32 0
12 [VV2006] J093523.3+411518 QSO 09 35 23.3232762432 +41 15 18.565026444   23.26 21.98     ~ 30 0
13 [VV2006] J094409.5+100656 QSO 09 44 09.5214922872 +10 06 56.679507576   23.96 22.34     ~ 32 0
14 [VV2006] J101759.7+032739 QSO 10 17 59.633 +03 27 39.91   25.01 23.35     ~ 22 0
15 [VV2006] J105919.2+023428 QSO 10 59 19.2185381400 +02 34 28.711427016   25.67 23.18     ~ 22 0
16 QSO J1100+1122 QSO 11 00 45.2300513352 +11 22 39.148223880   23.42 22.09     ~ 39 0
17 [VV2006] J111358.3+025333 QSO 11 13 58.3319783016 +02 53 33.727533108   25.14 23.12     ~ 23 0
18 [VV2006] J114448.6+055710 QSO 11 44 48.547 +05 57 09.78   25.87 23.60     ~ 24 0
19 [VV2006] J115158.2+030341 QSO 11 51 58.265 +03 03 41.84   25.56 23.74     ~ 30 0
20 [VV2006] J120256.4+072038 QSO 12 02 56.4451173408 +07 20 38.841471096   24.56 22.94     ~ 25 0
21 QSO J1235-0003 QSO 12 35 03.0467575584 -00 03 31.746486564   23.96 22.46     ~ 50 0
22 [VV2006] J130619.4+023658 QSO 13 06 19.3892431488 +02 36 58.913079084   24.28 22.55     ~ 33 0
23 [VV2006] J131737.2+110532 QSO 13 17 37.2720021216 +11 05 33.131190768   23.84 23.00     ~ 23 0
24 QSO J1321+0038 QSO 13 21 10.8210785904 +00 38 21.621816744   24.05 22.60     ~ 42 0
25 [VV2006] J132853.7-022441 QSO 13 28 53.6583045552 -02 24 41.789777940   24.38 22.67     ~ 29 0
26 [VV2006] J133125.6+025535 QSO 13 31 25.5741056616 +02 55 35.569194456   23.77 22.51     ~ 25 0
27 [VV2006] J134134.2+014157 QSO 13 41 34.1973615216 +01 41 57.671733516   23.52 21.74     ~ 41 0
28 [VV2006] J134546.9-015940 QSO 13 45 46.966 -01 59 40.38   23.42 22.23     ~ 31 0
29 [VV2006] J140404.7+031403 QSO 14 04 04.6523987088 +03 14 03.900360588   26.25 23.33     ~ 37 0
30 QSO J1433+0227 QSO 14 33 52.2087347832 +02 27 13.974100416   22.31 20.74     ~ 46 0
31 SDSS J143629.94+063508.0 QSO 14 36 29.9440699416 +06 35 08.013331212   25.68 23.38     ~ 25 0
32 QSO J1443+0605 QSO 14 43 52.945 +06 05 33.16   26.27 23.86     ~ 25 0
33 SDSS J144734.09+102513.1 QSO 14 47 34.099 +10 25 13.21   24.61 22.89     ~ 20 0
34 [VV2006] J151155.9+040802 QSO 15 11 55.9780096632 +04 08 03.053518224   24.38 22.65     ~ 37 0
35 QSO J1616+0501 QSO 16 16 22.1107195512 +05 01 27.718632228   23.50 21.80     ~ 24 0
36 SDSS J161931.58+123844.4 QSO 16 19 31.5904176312 +12 38 44.375043984   25.23 23.31     ~ 17 0
37 QSO J1654+2227 QSO 16 54 36.8596056120 +22 27 33.751477476   22.43 21.11     ~ 41 0
38 [VV2006] J205724.2-003019 QSO 20 57 24.1491890928 -00 30 18.755738244   22.51 21.14     ~ 35 0
39 QSO J2200+0017 QSO 22 00 08.6658519792 +00 17 44.881206144   24.25 22.24     ~ 44 0
40 SDSS J221705.71-001307.7 QSO 22 17 05.714 -00 13 07.64   25.37 22.1843   20.5616 ~ 25 0
41 [VV2006] J222050.8+001958 QSO 22 20 50.810 +00 19 59.16   24.30 22.0361 20.7650 20.2197 ~ 30 0
42 QSO J2225-0014 QSO 22 25 09.1923562032 -00 14 06.799695468   23.45 21.91     ~ 48 0
43 [VV2006] J224453.1+134631 QSO 22 44 53.068 +13 46 31.65   23.53 22.38     ~ 27 0
44 [VV2006] J235152.8+160048 QSO 23 51 52.8119641032 +16 00 48.980725956   24.04 22.45     ~ 25 0

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