J/ApJS/244/30 Spitzer catalog of Herschel star-forming galaxies (Ma+, 2019)
Spitzer catalog of Herschel-selected ultrared dusty star-forming galaxies.
Ma J., Cooray A., Nayyeri H., Brown A., Ghotbi N., Ivison R., Oteo I.,
Duivenvoorden S., Greenslade J., Clements D., Wardlow J., Battisti A.,
da Cunha E., Ashby M.L.N., Perez-Fournon I., Riechers D., Oliver S.,
Eales S., Negrello M., Dye S., Dunne L., Omont A., Scott D., Cox P.,
Serjeant S., Maddox S., Valiante E.
<Astrophys. J. Suppl. ser., 244, 30 (2019)>
=2019ApJS..244...30M 2019ApJS..244...30M
ADC_Keywords: Galaxies, IR; Redshifts; Gravitational lensing; Interferometry;
Photometry, infrared; Millimetric/submm sources
Keywords: High-redshift galaxies ; Starburst galaxies
Abstract:
The largest Herschel extragalactic surveys, H-ATLAS and HerMES, have
selected a sample of "ultrared" dusty star-forming galaxies (DSFGs)
with rising SPIRE flux densities (S500>S350>S250; the so-called
"500µm risers") as an efficient way for identifying DSFGs at higher
redshift (z>4). In this paper, we present a large Spitzer follow-up
program of 300 Herschel ultrared DSFGs. We have obtained
high-resolution Atacama Large Millimeter/submillimeter Array, Northern
Extended Millimeter Array, and SMA data for 63 of them, which allow us
to securely identify the Spitzer/IRAC counterparts and classify them
as gravitationally lensed or unlensed. Within the 63 ultrared sources
with high-resolution data, ∼65% appear to be unlensed and ∼27% are
resolved into multiple components. We focus on analyzing the unlensed
sample by directly performing multiwavelength spectral energy
distribution modeling to derive their physical properties and compare
with the more numerous z∼2 DSFG population. The ultrared sample has a
median redshift of 3.3, stellar mass of 3.7x1011M☉, star
formation rate (SFR) of 730M☉/yr, total dust luminosity of
9.0x1012L☉, dust mass of 2.8x109M☉, and V-band
extinction of 4.0, which are all higher than those of the ALESS DSFGs.
Based on the space density, SFR density, and stellar mass density
estimates, we conclude that our ultrared sample cannot account for the
majority of the star-forming progenitors of the massive, quiescent
galaxies found in infrared surveys. Our sample contains the rarer,
intrinsically most dusty, luminous, and massive galaxies in the early
universe that will help us understand the physical drivers of extreme
star formation.
Description:
The H-ATLAS observations were performed in the parallel mode with both
SPIRE and PACS. The survey covers three equatorial fields at right
ascensions of 9, 12, and 15hr (namely the GAMA09, GAMA12, and GAMA15
fields), the North Galactic Pole (NGP) field in the north, and the
South Galactic Pole (SGP) field in the south. The total survey area is
about 600deg2. The detailed descriptions of the H-ATLAS observations
and source extraction can be found in Valiante+ (2016, J/MNRAS/462/3146),
Ivison+ (2016, J/ApJ/832/78), and Maddox+ (2018, J/ApJS/236/30).
The HeLMS field covers an effective area of ∼274deg2 of the
equatorial region spanning 23h14m<RA_J2000<1h16m and
-9°<DEJ2000<+9°. The observations were conducted with the
SPIRE instrument. See Asboth+ (2016, J/MNRAS/462/1989) and
Duivenvoorden+ (2018, J/MNRAS/477/1099) for more information on the
HeLMS observations.
A total of 300 Herschel ultrared sources were followed up by the
Spitzer snapshot imaging program PID 13042 (PI: A. Cooray) using IRAC.
For the H-ATLAS ultrared DSFGs, Ivison+ (2016, J/ApJ/832/78) obtained
850um continuum imaging with SCUBA-2 and/or 870um continuum imaging
with LABOCA.
A subset (21) of the H-ATLAS ultrared sources in
Ivison+ (2016, J/ApJ/832/78) was selected for continuum imaging with
NOEMA (PIs: R.J. Ivison, M. Krips; PIDs: W05A, X0C6, W15ET) at 1.3
and/or 3mm and ALMA (PI: A. Conley; PID: 2013.1.00499.S) at 3mm as
described in detail in Fudamoto+ (2017MNRAS.472.2028F 2017MNRAS.472.2028F).
Oteo+ (2017arXiv170904191O 2017arXiv170904191O) presented high-resolution (∼0.12") ALMA
continuum imaging at 870um (PI: R.J. Ivison; PIDs: 2013.1.00001.S,
2016.1.00139.S) for a sample of 44 equatorial and southern ultrared
sources from both the H-ATLAS and HerMES surveys. Thirty-one of them
are in our Spitzer sample.
Five HeLMS ultrared sources (HELMSRED1, 2, 4, 10, 13) were observed
with SMA at 1.1mm in the compact array configuration (PI: D. Clements;
PID: 2013A-S005). The details of the observations and data reduction
will be presented in J. Greenslade et al. (2019, in preparation).
Additional data with MUSIC/CSO (Sayers+ 2014SPIE.9153E..04S 2014SPIE.9153E..04S) and ACT
(Su+ 2017MNRAS.464..968S 2017MNRAS.464..968S) were obtained for five HeLMS sources
(HELMSRED1, 3, 4, 6, 7).
We analyze in this paper a total of 63 Herschel-selected ultrared
sources from H-ATLAS and HeLMS that have high-resolution positions
from various observations as described above. The positions and flux
densities of the high-resolution subsample are listed in Table 2.
For the ultrared sources that currently lack high-resolution
interferometry data, we use the SCUBA-2 or Herschel positions and
cross-match with IRAC sources. See section 3 for further explanations.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 267 300 Catalog of Herschel-selected ultrared sources
table2.dat 191 86 High-resolution sample followed up with ALMA,
NOEMA, and SMA
table3.dat 68 19 Spectroscopically confirmed Herschel-selected
ultrared dusty star-forming galaxies (DSFGs)
at z≥∼4.
table4.dat 125 79 Unlensed sample
table5.dat 177 48 Properties of the Herschel unlensed sample derived
from magphys+photo-z SED fitting
--------------------------------------------------------------------------------
See also:
II/329 : VIKING catalogue data release 1 (Edge+, 2013)
II/343 : VIKING catalogue data release 2 (Edge+, 2016)
VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)
VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)
VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)
V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)
J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)
J/MNRAS/380/199 : SCUBA Half-Degree Extragalactic Survey. III (Ivison+, 2007)
J/MNRAS/401/1521 : Stellar masses of Lyman break gal. at z∼3 (Magdis+, 2010)
J/ApJ/719/763 : Millimeter-wave sources in the SPT survey (Vieira+, 2010)
J/MNRAS/411/505 : Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)
J/ApJ/731/100 : 148GHz ACT extragalactic sources catalog (Marriage+, 2011)
J/ApJ/749/65 : H-ATLAS strongly lensed galaxies (Gonzalez-Nuevo+, 2012)
J/ApJ/761/140 : Spectroscopy of Herschel-SPIRE galaxies (Casey+, 2012)
J/A+A/559/A29 : BR 1202-0725 system in [CII] line (Carniani+, 2013)
J/ApJ/768/91 : ALMA observations of LESS submm galaxies (Hodge+, 2013)
J/ApJ/779/61 : SPT-SZ point sources at 95, 150 & 220GHz (Mocanu+, 2013)
J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)
J/MNRAS/439/1556 : ACT high significance 148 & 218GHz sources (Marsden+, 2014)
J/ApJ/788/125 : An ALMA survey of ECDFS submm galaxies (Simpson+, 2014)
J/ApJ/806/110 : ALESS survey: SMGs in the ECDF-S data (da Cunha+, 2015)
J/MNRAS/462/1989 : HerMES Large Mode Survey catalogue (Asboth+, 2016)
J/A+A/594/A26 : 2nd Planck Cat. of Compact Sources (PCCS2) (Planck+, 2016)
J/MNRAS/462/3146 : Herschel-ATLAS DR1 (HATLAS) (Valiante+, 2016)
J/ApJ/832/78 : SCUBA-2 & LABOCA obs. of HATLAS galaxies (Ivison+, 2016)
J/ApJ/840/78 : z survey of ALMA-identified SMGs in ECDFS (Danielson+, 2017)
J/A+A/614/A33 : 500µm-risers sources (Donevski+, 2018)
J/ApJS/236/30 : Herschel-ATLAS (H-ATLAS) DR2 (Maddox+, 2018)
J/MNRAS/477/1099 : SCUBA-2 850um obs. of Herschel gal. (Duivenvoorden+, 2018)
Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 A6 --- Survey [HATLAS/HerMES] "HATLAS" or "HerMES" survey (G1)
7- 22 A16 --- Name Herschel source name (JHHMMSS.s+DDMMSS)
24- 36 A13 --- ID Nickname or short name (G2)
38- 42 F5.3 --- z [2.7/9] Redshift
43 A1 --- n_z p=photometric or s=spectroscopic (1)
45- 46 A2 --- Lensed Lensed? (2)
48- 58 F11.7 deg RAIdeg ?=-99 Right Ascension,
Spitzer/IRAC counterpart (J2000)
60- 70 F11.7 deg DEIdeg ?=-99 Declination, Spitzer/IRAC
counterpart (J2000)
72- 77 F6.3 mag 3.6mag [14.9/24] Kron-like elliptical aperture
AB magnitude at 3.6um (MAG_AUTO3.6um)
79- 85 F7.3 mag e_3.6mag [0.02/2]?=-99 3.6mag uncertainty
(MAGERR_AUTO3.6um)
87- 92 F6.3 mag 4.5mag [15/24] Kron-like elliptical aperture
AB magnitude at 4.5um (MAG_AUTO4.5um)
94-100 F7.3 mag e_4.5mag [0.02/2]?=-99 4.5mag uncertainty
(MAGERR_AUTO4.5um)
102-110 E9.3 Jy S3.6um [8.8e-7/0.004] Spitzer/IRAC 3.6um flux density
112-120 E9.3 Jy e_S3.6um [1.5e-6/8.2e-5]?=-99 S3.6um uncertainty
122-130 E9.3 Jy S4.5um [9.8e-7/0.004] Spitzer/IRAC 4.5um flux density
132-140 E9.3 Jy e_S4.5um [1.7e-6/8.7e-5]?=-99 S4.5um uncertainty
142-151 F10.6 deg RAHdeg ?=-99 Herschel/SPIRE Right Ascension (J2000)
153-162 F10.6 deg DEHdeg ?=-99 Herschel/SPIRE Declination (J2000)
164-173 E10.3 Jy S250um [-0.008/0.2] Herschel/SPIRE 250um flux density
175-183 E9.3 Jy e_S250um [0.004/0.01] S250um uncertainty
185-193 E9.3 Jy S350um [0.008/0.2] Herschel/SPIRE 350um flux density
195-203 E9.3 Jy e_S350um [0.005/0.02] S350um uncertainty
205-213 E9.3 Jy S500um [0.02/0.2] Herschel/SPIRE 500um flux density
215-223 E9.3 Jy e_S500um [0.006/0.08] S500um uncertainty
225-235 F11.7 deg RASdeg ?=-99 SCUBA2 Right Ascension (J2000)
237-247 F11.7 deg DESdeg ?=-99 SCUBA2 Declination (J2000)
249-257 E9.3 Jy S850um [0.001/0.09]?=-99 SCUBA2/LABOCA 850/870um
flux density
259-267 E9.3 Jy e_S850um [0.001/0.02]?=-99 S850um uncertainty
--------------------------------------------------------------------------------
Note (1): Photometric redshift from FIR SED fitting -- 2 decimal points;
Ivison+ (2016, J/ApJ/832/78) and Duivenvoorden+ (2018, J/MNRAS/477/1099);
or spectroscopic redshift (3 decimal points; see Table 3).
Note (2): Code as follows:
y = Lensed (73 occurrences),
n = unlensed (126 occurrences),
yn = both lensed and unlensed components (1 occurrence),
x = unknown (100 occurrences).
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 12 A12 --- ID Nickname or short name (G2)
13 A1 --- m_ID Multiple ID
15- 15 I1 --- HR [1/3] High-resolution data (Highres_data) (2)
17- 17 A1 --- Lensed Lensed? (3)
19- 29 F11.7 deg RAdeg Spitzer/IRAC counterpart right ascension (J2000)
31- 41 F11.7 deg DEdeg Spitzer/IRAC counterpart declination (J2000)
43- 48 F6.3 mag 3.6mag [14.9/23] Kron-like elliptical aperture
AB magnitude at 3.6um (MAG_AUTO3.6um)
50- 56 F7.3 mag e_3.6mag [0.02/1.1]?=-99 3.6mag uncertainty
(MAGERR_AUTO3.6um)
58- 63 F6.3 mag 4.5mag [15.5/23] Kron-like elliptical aperture AB
magnitude at 4.5um (MAG_AUTO4.5um)
65- 71 F7.3 mag e_4.5mag [0.03/1.1]?=-99 4.5mag uncertainty
(MAGERR_AUTO4.5um)
73- 81 E9.4 Jy S3.6um [2.5e-6/0.004] Spitzer/IRAC 3.6um flux density
83- 91 E9.4 Jy e_S3.6um [/9.2e-5]?=-99 S3.6um uncertainty
93-101 E9.4 Jy S4.5um [2.4e-6/0.003] Spitzer/IRAC 4.5um flux density
103-111 E9.4 Jy e_S4.5um [/7.2e-5]?=-99 S4.5um uncertainty
113-121 E9.4 Jy S250um [0.003/0.2] Herschel/SPIRE 250um flux density
123-131 E9.4 Jy e_S250um [0.002/0.02] S250um uncertainty
133-141 E9.4 Jy S350um [0.002/0.2] Herschel/SPIRE 350um flux density
143-151 E9.4 Jy e_S350um [0.001/0.02] S350um uncertainty
153-161 E9.4 Jy S500um [0.002/0.2] Herschel/SPIRE 500um flux density
163-171 E9.4 Jy e_S500um [0.002/0.03] S500um uncertainty
173-181 E9.4 Jy S850um [/0.09]?=-99 SCUBA2/LABOCA 850/870um flux density
183-191 E9.4 Jy e_S850um [/0.009]?=-99 S850um uncertainty
--------------------------------------------------------------------------------
Note (2): High-resolution data from facilities as follows:
1 = ALMA (75 occurrences);
2 = NOEMA (10 occurrences);
3 = SMA (1 occurrence).
Note (3): Lensed, unlensed, or unknown according to the high-resolution
interferometry data. Code as follows:
y = Lensed (22 occurrences),
n = unlensed (63 occurrences),
x = unknown (1 occurrence).
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 A6 --- Survey [HATLAS/HerMES/HLS ] "HATLAS", "HerMES" or
"HLS" survey (G1)
8- 23 A16 --- Name Herschel source name (JHHMMSS.s+DDMMSS)
25- 36 A12 --- ID Nickname or short name (G2)
38- 42 F5.3 --- zspec [3.79/6.4] Spectroscopic Redshift
44- 48 F5.1 10+13Lsun LIR [2/11]? Total IR Luminosity
50- 52 A3 --- Lensed Lensed?
54- 68 A15 --- Ref Reference(s) (1)
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Note (1): References as follows:
a = Fudamoto et al. (2017MNRAS.472.2028F 2017MNRAS.472.2028F);
b = Oteo et al. (2016ApJ...827...34O 2016ApJ...827...34O);
c = Oteo et al. (2018ApJ...856...72O 2018ApJ...856...72O);
d = Duivenvoorden et al. (2018, J/MNRAS/477/1099);
e = Asboth et al. (2016, J/MNRAS/462/1989)
f = Riechers et al. (2017ApJ...850....1R 2017ApJ...850....1R);
g = Zavala et al. (2018NatAs...2...56Z 2018NatAs...2...56Z);
h = Cox et al. (2011ApJ...740...63C 2011ApJ...740...63C);
i = Combes et al. (2012A&A...538L...4C 2012A&A...538L...4C);
j = Dowell et al. (2014ApJ...780...75D 2014ApJ...780...75D);
k = Riechers et al. (2013Natur.496..329R 2013Natur.496..329R);
l = Cooray et al. (2014ApJ...790...40C 2014ApJ...790...40C);
m = Wardlow et al. in prep.
This work = This work (Ma et al. 2019ApJS..244...30M 2019ApJS..244...30M).
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Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 12 A12 --- ID Nickname or short name (G2)
13 A1 --- m_ID Multiple ID
15- 19 F5.3 --- zFIR [2.8/4.9]? FIR photometric redshift or
spectroscopic redshift (1)
20 A1 --- n_zFIR p: photometric redshift (1)
22- 25 F4.2 --- E_zFIR [0.06/0.8]? Upper uncertainty on zFIR
27- 30 F4.2 --- e_zFIR [0.1/0.8]? Lower uncertainty on zFIR
32- 35 F4.2 --- zMAGPHYS [1.8/5.6] MAGPHYS derived redshift (2)
37- 40 F4.2 --- E_zMAGPHYS [0.7/1.7] Upper uncertainty on zMAGPHYS
42- 45 F4.2 --- e_zMAGPHYS [0.5/1.6] Lower uncertainty on zMAGPHYS
47- 47 A1 --- l_S3.6um 3 sigma upper limit flag on S3.6
49- 53 F5.2 uJy S3.6um [2.5/76] Spitzer/IRAC 3.6um flux density
55- 59 F5.2 uJy e_S3.6um [2/13.3]? S3.6um uncertainty
61- 61 A1 --- l_S4.5um 3 sigma upper limit flag on S4.5
63- 67 F5.2 uJy S4.5um [2.4/69.6] Spitzer/IRAC 4.5um flux density
69- 73 F5.2 uJy e_S4.5um [1.5/12.7]? S4.5um uncertainty
75- 79 F5.2 mJy S250um [3/55.4] Deblended Herschel/SPIRE 250um
flux density (3)
81- 84 F4.1 mJy e_S250um [2.3/11.3] S250um uncertainty
86- 89 F4.1 mJy S350um [2.7/87.6] Deblended Herschel/SPIRE 350um
flux density (3)
91- 94 F4.1 mJy e_S350um [2.5/15] S350 uncertainty
96- 99 F4.1 mJy S500um [5.2/97.2] Deblended Herschel/SPIRE 500um
flux density 500um (3)
101-104 F4.1 mJy e_S500um [1/22.3] S500um uncertainty
106-109 F4.1 mJy S850um [1.2/64.1]? Deblended SCUBA2 850um
flux density (3)
111-114 F4.1 mJy e_S850um [0.2/11]? S850um uncertainty
116-120 F5.2 mJy S870um [0.8/47.7]? ALMA 870um flux density (4)
122-125 F4.2 mJy e_S870um [0.1/3.1]? S870um uncertainty
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Note (1): zFIR is the photometric redshift derived from FIR SED fitting by
Ivison+ (2016, J/ApJ/832/78) and Duivenvoorden+ (2018, J/MNRAS/477/1099).
We list the spectroscopic redshift (three decimals) instead of
zFIR whenever available.
Note (2): zMAGPHYS is the photometric redshift derived from
magphys+photo-z SED fitting in Section 4.
Note (3): The deblended SPIRE and SCUBA-2/LABOCA flux densities for the
individual components are described in Section 3.
Note (4): The ALMA flux densities are from Oteo+ (2017, arXiv:1709.04191) and
this work.
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Byte-by-byte Description of file: table5.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 12 A12 --- ID Nickname or short name (G2)
13 A1 --- m_ID Multiple ID
15- 18 F4.2 --- b_zphot [0/3.8] log, 16th percentile,
photometric redshift (2)
20- 24 F5.3 --- zphot [1.9/5.1] log, median
photometric redshift (2)
26- 29 F4.2 --- B_zphot [0/6.5] log, 84th percentile,
photometric redshift (2)
31- 35 F5.2 [Msun] b_logM* [10.3/11.6] log, 16th percentile,
stellar mass (2)
37- 41 F5.2 [Msun] logM* [10.7/12] log, median stellar
mass (2)
43- 47 F5.2 [Msun] B_logM* [11/12.3] log, 84th percentile,
stellar mass (2)
49- 52 F4.2 [Msun/yr] b_logSFR [1/3.3] log, 16th percentile,
current SFR (2)(3)
54- 57 F4.2 [Msun/yr] logSFR [1.7/3.4] log, median current star
formation rate (2)(3)
59- 62 F4.2 [Msun/yr] B_logSFR [2.2/3.7] log, 84th percentile,
current SFR (2)(3)
64- 68 F5.2 [yr-1] b_logsSFR [-10/-8.6] log, 16th percentile,
specific SFR (2)
70- 74 F5.2 [yr-1] logsSFR [-9.2/-8.3] log, median specific
star formation rate (2)
76- 80 F5.2 [yr-1] B_logsSFR [-8.6/-7.9] log, 84th percentile,
specific SFR (2)
82- 85 F4.2 [yr] b_logAge [7.9/8.5] log, 16th percentile, age (2)
87- 90 F4.2 [yr] logAge [8.3/9] log, median mass-weighted
stellar population age (2)
92- 95 F4.2 [yr] B_logAge [8.5/9.3] log, 84th percentile, age (2)
97-101 F5.2 [Msun/Lsun] b_logM*/LH [-0.4/0.5] log, 16th percentile,
mass-luminosity ratio (2)
103-107 F5.2 [Msun/Lsun] logM*/LH [-0.2/1] log, median stellar
mass to H-band luminosity ratio (2)
109-112 F4.2 [Msun/Lsun] B_logM*/LH [0.1/1.6] log, 84th percentile,
mass-luminosity ratio (2)
114-117 F4.2 mag b_Av [0.5/5.5] 16th percentile,
V-band extinction (2)
119-122 F4.2 mag Av [1/7.5] median V-band extinction (2)
124-127 F4.2 mag B_Av [1.7/10] 84th percentile,
V-band extinction (2)
129-133 F5.2 [Lsun] b_logLdust [11.4/13.4] log, 16th percentile,
dust luminosity (2)
135-139 F5.2 [Lsun] logLdust [11.9/13.5] log, median total dust
luminosity = IR luminosity (2)
141-145 F5.2 [Lsun] B_logLdust [12.3/13.7] log, 84th percentile,
dust luminosity (2)
147-150 F4.1 K b_Tdust [27.9/37] 16th percentile, dust
temperature (2)
152-155 F4.1 K Tdust [32.5/46] median luminosity-weighted
dust temperature (2)
157-160 F4.1 K B_Tdust [41.4/56.5] 84th percentile, dust
temperature (2)
162-165 F4.2 [Msun] b_logMdust [7.5/10] log, 16th percentile,
dust mass (2)
167-171 F5.2 [Msun] logMdust [8.1/10] log, median dust mass (2)
173-177 F5.2 [Msun] B_logMdust [8.5/10.1] log, 84th percentile,
dust mass (2)
--------------------------------------------------------------------------------
Note (2): The median values and 16th-84th percentile ranges are determined
from the stacked posterior probability distributions.
Note (3): Current SFR defined as the average of the star formation history
over the last 10 Myr.
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Global notes:
Note (G1): Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS;
Valiante+ 2016, J/MNRAS/462/3146 ; Ivison+ 2016, J/ApJ/832/78 and
Maddox+ 2018, J/ApJS/236/30); <H-ATLAS JHHMMSS.s+DDMMSS> in Simbad ;
HerMES Large Mode Survey (HeLMS; Asboth+ 2016, J/MNRAS/462/1989
(<[ACS2016] HELMS RED NNN> for Simbad) and
Duivenvoorden+ 2018, J/MNRAS/477/1099).
Note (G2): Nickname or short name in Ivison+ (2016, J/ApJ/832/78) and
Duivenvoorden+ (2018, J/MNRAS/477/1099)
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History:
From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 24-Feb-2020