J/MNRAS/459/1626 HST Frontier Fields Herschel sources (Rawle+, 2016)
A complete census of Herschel-detected infrared sources within the
HST Frontier Fields.
Rawle T.D., Altieri B., Egami E., Perez-Gonzalez P.G., Boone F.,
Clement B., Ivison R.J., Richard J., Rujopakarn W., Valtchanov I.,
Walth G., Weiner B.J., Blain A.W., Dessauges-Zavadsky M., Kneib J.-P.,
Lutz D., Rodighiero G., Schaerer D., Smail I.
<Mon. Not. R. Astron. Soc., 459, 1626-1645 (2016)>
=2016MNRAS.459.1626R 2016MNRAS.459.1626R (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, IR ; Photometry, infrared ;
Photometry, millimetric/submm
Keywords: galaxies: star formation - infrared: galaxies -
submillimetre: galaxies
Abstract:
We present a complete census of all Herschel-detected sources within
the six massive lensing clusters of the HST Frontier Fields (HFF). We
provide a robust legacy catalogue of 263 sources with Herschel fluxes,
primarily based on imaging from the Herschel Lensing Survey and
PEP/HerMES Key Programmes. We optimally combine Herschel, Spitzer and
WISE infrared (IR) photometry with data from HST, VLA and ground-based
observatories, identifying counterparts to gain source redshifts. For
each Herschel-detected source we also present magnification factor
(µ), intrinsic IR luminosity and characteristic dust temperature,
providing a comprehensive view of dust-obscured star formation within
the HFF. We demonstrate the utility of our catalogues through an
exploratory overview of the magnified population, including more than
20 background sub-LIRGs unreachable by Herschel without the assistance
gravitational lensing.
Description:
We present a complete census of the 263 Herschel-detected sources
within the HST Frontier Fields, including 163 lensed sources located
behind the clusters. Our primary aim is to provide a robust legacy
catalogue of the Herschel fluxes, which we combine with archival data
from Spitzer and WISE to produce IR SEDs.
We optimally combine the IR photometry with data from HST, VLA and
ground-based observatories in order to identify optical counterparts
and gain source redshifts.
Each cluster is observed in two distinct regions, referred to as the
central and parallel footprints.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table4.dat 92 263 Observed PACS and SPIRE fluxes for Herschel-detected
sources within the HST Frontier Fields
table6.dat 105 263 *Optical counterparts for Herschel-detected sources
within HFF
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Note on table6.dat: Derived properties account for magnification (µ).
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See also:
VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)
J/A+A/543/A161 : Submillimetre obs. of 323 HRS nearby galaxies (Ciesla+, 2012)
J/MNRAS/444/268 : HST Frontier Fields clusters (Richard+, 2014)
Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
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1- 3 A3 --- --- [HLS]
4- 19 A16 --- HLS Herschel ID (JHHMMSS.s+DDMMSS)
21 A1 --- n_HLS [PS] Herschel ID derived from PACS (P) or
SPIRE (S) catalogue position
23- 28 A6 --- Field Field
30 A1 --- n_Field [CP] central (C) or parallel (P) region
32- 35 F4.1 mJy S70 ?=- Flux density at 70um
37- 39 F3.1 mJy e_S70 ?=- rms uncertainty on S70
42- 45 F4.1 mJy S100 ?=- Flux density at 100um
47- 49 F3.1 mJy e_S100 ?=- rms uncertainty on S100
51- 55 F5.1 mJy S160 ?=- Flux density at 160um
57- 59 F3.1 mJy e_S160 ?=- rms uncertainty on S160
61- 65 F5.1 mJy S250 ?=- Flux density at 250um
67- 70 F4.1 mJy e_S250 ?=- rms uncertainty on S250
72- 76 F5.1 mJy S350 ?=- Flux density at 350um
78- 81 F4.1 mJy e_S350 ?=- rms uncertainty on S350
84- 87 F4.1 mJy S500 ?=- Flux density at 500um
89- 92 F4.1 mJy e_S500 ?=- rms uncertainty on S500
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Byte-by-byte Description of file: table6.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 A3 --- --- [HLS]
4- 19 A16 --- HLS Herschel ID (JHHMMSS.s+DDMMSS)
21- 26 A6 --- Field Field
28 A1 --- n_Field [CP] central (C) or parallel (P) region
30- 39 F10.6 deg RAdeg Optical/NIR/radio counterpart
right ascension (J2000) (1)
41- 50 F10.6 deg DEdeg Optical/NIR/radio counterpart
declination (J2000) (1)
52 A1 --- r_Pos [VHOIWPS] Position reference (2)
54 A1 --- l_z [~] Limit flag on z
55- 59 F5.3 --- z Counterpart spectroscopic, optical
photometric or IR estimated redshift
61- 62 I2 --- r_z [1/24] Reference for redshift (3)
64- 68 F5.2 --- mu ?=- Magnification
70 I1 --- r_mu [1/3]? Reference for mu (4)
72- 76 F5.2 [Lsun] logLIR IR luminosity from the best-fitting
rie09-556 template
78- 81 F4.2 [Lsun] e_logLIR rms uncertainty on logLIR
83- 87 F5.1 Msun/yr SFRIR IR star formation rate from the best-fitting
rie09-556 template
89- 93 F5.1 Msun/yr e_SFRIR rms uncertainty on SFRIR
95- 98 F4.1 K Tdust Characteristic dust temperature of the
best-fitting single-temperature modified
blackbody
100-103 F4.1 K e_Tdust rms uncertainty on Tdust
105 I1 --- AGN [0/1] 1 for non-negligible contribution to
LIR from the AGN component (5)
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Note (1): Counterpart RA and Dec, from the most accurate available position
Note (2): Position reference as follows:
V = VLA
H = HST
O = [ground-based] optical
I = IRAC
W = WISE
P = PACS
S = SPIRE
Note (3): Redshift references as follows:
1 = Owers et al. (2011, Cat. J/ApJ/728/27)
2 = zphotFIR_
3 = Couch et al (1998, Cat. J/ApJ/497/188)
4 = Rawle et al. (2014MNRAS.442..196R 2014MNRAS.442..196R)
5 = Wang et al. (2015, Cat. J/ApJ/811/29)
6 = Busarello et al. (2002, Cat. J/A+A/389/787)
7 = Braglia et al. (2009, cat. J/A+A/500/947)
8 = Wold et al. (2012, Cat. J/ApJ/811/29)
9 = HST GRISM
10 = Bamford (2005, Cat. J/MNRAS/361/109)
11 = Ivison et al. (1998MNRAS.298..583I 1998MNRAS.298..583I)
12 = Soucail et al. (1988A&A...191L..19S 1988A&A...191L..19S)
13 = Henry & Lavery et al. (1987ApJ...323..473H 1987ApJ...323..473H)
14 = Soucail et al. (1999A&A...343L..70S 1999A&A...343L..70S)
15 = Magellan/IMACS
16 = CLASH HST photo-z
17 = CLASH Subraru photo-z, Umetsu et al. (2014ApJ...795..163U 2014ApJ...795..163U)
18 = Balestra (2013, Cat. J/A+A/559/A9)
19 = Ebeling et al. (2014, Cat. J/ApJS/211/21)
20 = LBT/MODS
21 = Smith et al. (2009ApJ...701..163S 2009ApJ...701..163S)
22 = Walth et al. (in preparation)
23 = Gomez et al. (2012AJ....144...79G 2012AJ....144...79G)
24 = Karman et al. (2015A&A...574A..11K 2015A&A...574A..11K)
Note (4): Reference for magnification as follows:
1 = CATS models (Jullo & Kneib 2009MNRAS.395.1549H 2009MNRAS.395.1549H;
Jauzac et al. 2012MNRAS.426.3369J 2012MNRAS.426.3369J; Richard et al. 2014,
Cat. J/MNRAS/444/268; Jauzac et al. 2014, Cat. J/MNRAS/443/1549)
3 = SaWLens wide-field method Merten et al. (2009A&A...500..681M 2009A&A...500..681M,
2011MNRAS.417..333M 2011MNRAS.417..333M)
blank for foreground and cluster sources
Note (5): Flag for alternate IR SED fit using SF+AGN model, effectively
correcting LIR and SFRIR for AGN contamination (see Section 4.4.4)
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History:
From electronic version of the journal
(End) Patricia Vannier [CDS] 28-Jul-2017