J/ApJS/229/25 GOALS sample PACS and SPIRE fluxes (Chu+, 2017)
The Great Observatories All-Sky LIRG Survey:
Herschel image atlas and aperture photometry.
Chu J.K., Sanders D.B., Larson K.L., Mazzarella J.M., Howell J.H.,
Diaz-santos T., Xu K.C., Paladini R., Schulz B., Shupe D., Appleton P.,
Armus L., Billot N., Chan B.H.P., Evans A.S., Fadda D., Frayer D.T.,
Haan S., Ishida C.M., Iwasawa K., Kim D.-C., Lord S., Murphy E., Petric A.,
Privon G.C., Surace J.A., Treister E.
<Astrophys. J. Suppl. Ser., 229, 25-25 (2017)>
=2017ApJS..229...25C 2017ApJS..229...25C (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, IR ; Photometry, millimetric/submm
Keywords: atlases - galaxies: active - galaxies: interactions -
galaxies: starburst - galaxies: structure - infrared: galaxies
Abstract:
Far-infrared images and photometry are presented for 201 Luminous and
Ultraluminous Infrared Galaxies [LIRGs:
log(LIR/L☉)=11.00-11.99, ULIRGs:
log(LIR/L☉)=12.00-12.99], in the Great Observatories All-Sky
LIRG Survey (GOALS), based on observations with the Herschel Space
Observatory Photodetector Array Camera and Spectrometer (PACS) and the
Spectral and Photometric Imaging Receiver (SPIRE) instruments. The
image atlas displays each GOALS target in the three PACS bands (70,
100, and 160µm) and the three SPIRE bands (250, 350, and 500µm),
optimized to reveal structures at both high and low surface brightness
levels, with images scaled to simplify comparison of structures in the
same physical areas of ∼100x100kpc2. Flux densities of companion
galaxies in merging systems are provided where possible, depending on
their angular separation and the spatial resolution in each passband,
along with integrated system fluxes (sum of components). This data set
constitutes the imaging and photometric component of the GOALS
Herschel OT1 observing program, and is complementary to atlases
presented for the Hubble Space Telescope, Spitzer Space Telescope, and
Chandra X-ray Observatory. Collectively, these data will enable a wide
range of detailed studies of active galactic nucleus and starburst
activity within the most luminous infrared galaxies in the local
universe.
Description:
The IRAS RBGS contains 179 LIRGs (log(LIR/L☉)=11.0-11.99) and
22 ultra-luminous infrared galaxies (ULIRGs:
log(LIR/L☉)≥12.0); these 201 total objects comprise the GOALS
sample (Armus et al. 2009), a statistically complete flux-limited
sample of infrared-luminous galaxies in the local universe.
This paper presents imaging and photometry for all 201 LIRGs and LIRG
systems in the IRAS RBGS that were observed during our GOALS Herschel
OT1 program.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 99 209 Basic GOALS Data
table2.dat 161 209 Herschel Observtion Log
table3.dat 130 209 PACS and SPIRE Total Fluxes of GOALS Systems
table4.dat 188 372 PACS and SPIRE Total and Component Fluxes of
GOALS Systems
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 3 I3 --- Num Row reference number
5- 15 A11 --- IRAS IRAS identifier (1)
17 A1 --- f_IRAS [a] Flag on IRAS (2)
19- 45 A27 --- OName Common optical counterpart identifier(s)
47- 48 I2 h RAh Hour of Right Ascension (J2000) (3)
50- 51 I2 min RAm Minute of Right Ascension (J2000) (3)
53- 57 F5.2 s RAs Second of Right Ascension (J2000) (3)
59 A1 --- DE- Sign of the Declination (J2000) (3)
60- 61 I2 deg DEd Degree of Declination (J2000) (3)
63- 64 I2 arcmin DEm Arcminute of Declination (J2000) (3)
66- 69 F4.1 arcsec DEs Arcsecond of Declination (J2000) (3)
71- 75 F5.1 Mpc DA Angular diameter distance to galaxy (4)
77- 79 I3 kpc Size Map size used in atlas (5)
81- 87 F7.5 --- z NED non-relativistic spectroscopic redshift
89- 93 I5 km/s HRV Heliocentric velocity (6)
95- 99 F5.2 [Lsun] logLIR Log of infrared luminosity (6)
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Note (1): Ordered by ascending RA. Galaxies with the "F" prefix originate from
the IRAS Faint Source Catalog, and galaxies with no "F" prefix are
from the Point Source Catalog.
Note (2): Falg as follows:
a = These are very widely separated galaxy pairs that required
two Herschel PACS observations.
Note (3): The Spitzer 8 micron centers of the system (see Mazzarella et al.
2017, in prep.).
Note (4): From Mazzarella et al. (2017, in prep.).
Note (5): Denoting the physical length of a side in each atlas image.
Note (6): From Armus et al. (2009PASP..121..559A 2009PASP..121..559A), which includes both
cosmological and non-cosmological effects. These values take into account
the effect of the local attractor to the DLs that one would normally obtain
from pure cosmological effects.
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Num Row reference number
5- 15 A11 --- IRAS IRAS identifier (1)
17 A1 --- f_IRAS [a] Flag on IRAS (2)
19- 45 A27 --- OName Common optical counterpart identifier(s)
47- 56 A10 --- Blue1 First PACS 70 micron observation ID
58 A1 --- f_Blue1 [e] Flag on Blue1 (3)
60- 69 A10 --- Blue2 Second PACS 70 micron observation ID
71 A1 --- f_Blue2 [e] Flag on Blue2 (3)
73- 82 A10 --- Green1 ? First PACS 100 micron observation ID
84 A1 --- f_Green1 [e] Flag on Green1 (3)
86- 95 A10 --- Green2 ? Second PACS 100 micron observation ID
97 A1 --- f_Green2 [e] Flag on Green2 (3)
99-102 I4 --- DurPACS Duration of each PACS scan and cross-scan
104 A1 --- f_DurPACS [b] Flag on DurPACS (4)
106-115 A10 "date" Blue.date PACS blue band observation date
117-126 A10 "date" Green.date PACS green band observation date
128 A1 --- f_Green.date [cd] Flag on Green.D (5)
130-131 I2 --- PACS-PI PACS Principal Investigator code (6)
133-142 I10 --- SPIRE ? SPIRE observation identifier (7)
144-147 I4 s DurSPIRE ? Duration of SPIRE observation
149-158 A10 "date" SPIRE.date SPIRE observation date
160-161 I2 --- SPIRE-PI ? SPIRE Principal Investigator code (6)
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Note (1): Ordered by ascending RA. Galaxies with the "F" prefix originate from
the IRAS Faint Source Catalog, and galaxies with no "F" prefix are
from the Point Source Catalog.
Note (2): Flag as follows:
a = These are very widely separated galaxy pairs that required
two Herschel PACS observations.
Note (3): Flag as follows:
e = Rescheduled to replace previous PACS observations:
1342245766 1342245767 1342245764 1342245765.
Note (4): Flag as follows:
b = Green 1 and Green 2 have durations of 65 sec., Blue 1 has a duration
of 141 sec. and Blue 2 has a duration of 153 sec.
Note (5): Flag as follows:
c = Green 2 was observed on 2012-04-24.
d = Green 2 was observed on 2012-03-29.
Note (6): Code as follows:
1 = OT1sanders1;
2 = KPGTesturm1;
3 = GT1msanchez2;
4 = KPOTpvanderw1;
5 = KPOTrkennicu1;
6 = OT1dfarrah1;
7 = GT1lspinogl2;
8 = cwilso01_1 (including KPGT);
9 = OT1mcluver2;
10 = KPGTsmadde011.
Note (7): Includes all three 250 micron, 350 micron, and 500 micron
observations. The scans and cross-scans for each target is
combined into one observation.
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 3 I3 --- Num Row reference number
5- 15 A11 --- IRAS IRAS identifier (1)
17 A1 --- f_IRAS [ab] Flag on IRAS (2)
19- 45 A27 --- OName Common optical counterpart identifier(s)
47- 53 F7.3 Jy F70 PACS 70 micron band flux density
55- 60 F6.3 Jy e_F70 Uncertainty in F70
62- 68 F7.3 Jy F100 ? PACS 100 micron band flux density
70- 75 F6.3 Jy e_F100 ? Uncertainty in F100
77- 83 F7.3 Jy F160 PACS 160 micron band flux density
85- 90 F6.3 Jy e_F160 Uncertainty in F160
92- 98 F7.3 Jy F250 SPIRE 250 micron band flux density
100-104 F5.3 Jy e_F250 Uncertainty in F250
106-111 F6.3 Jy F350 SPIRE 350 micron band flux density
113-117 F5.3 Jy e_F350 Uncertainty in F350
119-124 F6.3 Jy F500 SPIRE 500 micron band flux density
126-130 F5.3 Jy e_F500 Uncertainty in F500
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Note (1): Ordered by ascending RA. Galaxies with the "F" prefix originate from
the IRAS Faint Source Catalog, and galaxies with no "F" prefix are
from the Point Source Catalog.
Note (2): Flag as follows:
a = These are very widely separated galaxy pairs that required
two Herschel PACS observations.
b = This is a triple system, however only two component galaxies are
visible in PACS due to its smaller field of view. The total flux for
this system does not include the third galaxy not visible in PACS.
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Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
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1- 3 I3 --- Num Row reference number
5- 15 A11 --- IRAS IRAS identifier (1)
17 A1 --- f_IRAS [a] Flag on IRAS (2)
19- 41 A23 --- OName Individual identifier
43- 44 I2 h RAh Hour of Right Ascension (J2000)
46- 47 I2 min RAm Minute of Right Ascension (J2000)
49- 53 F5.2 s RAs Second of Right Ascension (J2000)
55 A1 --- DE- Sign of the Declination (J2000)
56- 57 I2 deg DEd Degree of Declination (J2000)
59- 60 I2 arcmin DEm Arcminute of Declination (J2000)
62- 65 F4.1 arcsec DEs Arcsecond of Declination (J2000)
67- 69 I3 arcsec AngAp-P ? PACS aperture angular radius
71- 76 F6.3 kpc PhyAp-P ? PACS aperture physical radius
78- 84 F7.3 Jy F70 ? PACS 70 micron band flux density
86- 91 F6.3 Jy e_F70 ? Uncertainty in F70
93 A1 --- f_F70 [bc] Flag on F70 (3)
95-101 F7.3 Jy F100 ? PACS 100 micron band flux density
103-108 F6.3 Jy e_F100 ? Uncertainty in F100
110 A1 --- f_F100 [bc] Flag on F100 (3)
112-118 F7.3 Jy F160 ? PACS 160 micron band flux density
120-125 F6.3 Jy e_F160 ? Uncertainty in F160
127 A1 --- f_F160 [bc] Flag on F160 (3)
129-131 I3 arcsec AngAp ? SPIRE aperture angular radius
133-138 F6.3 kpc PhyAp ? SPIRE aperture physical radius
140-146 F7.3 Jy F250 ? SPIRE 250 mmicron band flux density
148-152 F5.3 Jy e_F250 ? Uncertainty in F250
154 A1 --- f_F250 Flag on F250 (3)
156-161 F6.3 Jy F350 ? SPIRE 350 mmicron band flux density
163-167 F5.3 Jy e_F350 ? Uncertainty in F350
169-171 A3 --- f_F350 Flag on F350 (3)
173-178 F6.3 Jy F500 ? SPIRE 500 mmicron band flux density
180-184 F5.3 Jy e_F500 ? Uncertainty in F500
186-188 A3 --- f_F500 Flag on F500 (3)
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Note (1): Ordered by ascending RA. Galaxies with the "F" prefix originate from
the IRAS Faint Source Catalog, and galaxies with no "F" prefix are
from the Point Source Catalog.
Note (2): Flag as follows:
a = These are very widely separated galaxy pairs that required
two Herschel PACS observations.
Note (3): Flag as follows:
b = This galaxy is part of a triple system, but is only visible in the
SPIRE images. The total flux for this system does not include
this galaxy.
c = These fluxes have an aperture correction factor applied.
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History:
From electronic version of the journal
(End) Patricia Vannier [CDS] 07-Jun-2017