J/A+A/533/A119 GOODS-Herschel North and South catalogs (Elbaz+, 2011)
GOODS-Herschel: an infrared main sequence for star-forming galaxies.
Elbaz D., Dickinson M., Hwang H.S., Diaz-santos T., Magdis G., Magnelli B.,
Le Borgne D., Galliano F., Pannella M., Chanial P., Armus L.,
Charmandaris V., Daddi E., Aussel H., Popesso P., Kartaltepe J.,
Altieri B., Valtchanov I., Coia D., Dannerbauer H., Dasyra K., Leiton R.,
Mazzarella J., Alexander D.M., Buat V., Burgarella D., Chary R.-R.,
Gilli R., Ivison R.J., Juneau S., Le Floc'h E., Lutz D., Morrison G.E.,
Mullaney J.R., Murphy E., Pope A., Scott D., Brodwin M., Calzetti D.,
Cesarsky C., Charlot S., Dole H., Eisenhardt P., Ferguson H.C.,
Foerster Schreiber N., Frayer D., Giavalisco M., Huynh M., Koekemoer A.M.,
Papovich C., Reddy N., Surace C., Teplitz H., Yun M.S., Wilson G.
<Astron. Astrophys., 533, A119 (2011)>
=2011A&A...533A.119E 2011A&A...533A.119E
ADC_Keywords: Surveys ; Galaxies, IR ; Galaxy catalogs ; Photometry, infrared
Keywords: galaxies: active - infrared: galaxies - galaxies: evolution -
galaxies: starburst
Abstract:
We present the deepest 100 to 500µm far-infrared observations
obtained with the Herschel Space Observatory as part of the
GOODS-Herschel key program, and examine the infrared (IR) 3-500µm
spectral energy distributions (SEDs) of galaxies at 0<z<2.5,
supplemented by a local reference sample from IRAS, ISO, Spitzer, and
AKARI data. We determine the projected star formation densities of
local galaxies from their radio and mid-IR continuum sizes.
Description:
The sample of high-redshift galaxies analyzed here consists of
galaxies observed in the two Great Observatories Origins Deep Survey
(GOODS) fields in the Northern and Southern hemispheres. Observations
with the Herschel Space Observatory were obtained as part of the open
time key program GOODS-Herschel (PI Elbaz), for a total time of
361.3h. PACS observations at 100 and 160um cover the whole
GOODS-north field of 10'x16' and part of GOODS-south, i.e., 10'x10'
(but reaching the largest depths over ∼64arcmin2). When considering
the total observing times of 124h in GOODS-N and 206.3h in GOODS-S
(including 2.6 and 5h of overheads), the PACS GOODS-Herschel
observations reach a total integration time per sky position of 2.4h
in GOODS-N and of 15.1h in GOODS-S, i.e., 6.3 times longer. Due to the
larger beam size and observing configuration, the SPIRE observations
of GOODS-N cover a field of 900 arcmin2, hence largely encompassing
the central 10'x16', for a total observing time of 31.1h and an
integration time per sky position of 16.8h.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
ghn.dat 740 2710 GOODS-HERSCHEL North catalog
ghs.dat 535 2531 GOODS-HERSCHEL Sourth catalog
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See also:
II/261 : GOODS initial results (Giavalisco+, 2004)
VII/246 : GOODS Morphological Catalog (Bundy+, 2005)
VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)
J/AJ/127/3121 : TKRS catalog of GOODS-North Field (Wirth+, 2004)
J/ApJ/653/1027 : TKRS/GOODS-N Field galaxies (Weiner+, 2006)
J/A+A/511/A50 : JHks of GOODS-South field (Retzlaff+, 2010)
J/A+A/449/951 : GOODS-MUSIC sample: multicolour catalog (Grazian+, 2006)
J/A+A/454/423 : GOODS-South Field VLT/FORS2 redshifts. II (Vanzella+, 2006)
J/A+A/478/83 : GOODS-South Field VLT/FORS2 redshifts. III (Vanzella+, 2008)
J/ApJ/666/863 : GOODS MIPS early-type galaxies (Van Der Wel+, 2007)
J/A+A/504/751 : GOODS-MUSIC catalog updated version (Santini+, 2009)
J/A+A/528/A35 : Infrared luminosity in GOODS fields (Magnelli+, 2011)
J/ApJS/187/251 : Ultradeep Ks imaging in the GOODS-N (Wang+, 2010)
J/AJ/141/1 : Spitzer observations of GOODS fields (Teplitz+, 2011)
J/MNRAS/417/2239 : SPIRE (f250um>17.4mJy) GOODS-N galaxies (Symeonidis+, 2011)
J/PASP/122/261 : Herschel Reference Survey Sample (Boselli+, 2010)
Byte-by-byte Description of file: ghn.dat
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Bytes Format Units Label Explanations
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1- 7 A7 --- --- [GOODS_J]
8- 25 A18 --- GOODS IAU coded object identification,
GOODS_JHHMMSS.ss+DDMMSS.s
28- 31 I4 --- ID [1/2710] Sequential id specific to the catalogue
35- 57 E23.18 deg RAdeg Right Ascension (J2000)
60- 83 E24.18 deg DEdeg Declination (J2000)
86-100 E15.9 uJy F3.6 ?=-99. Spitzer/IRAC 3.6um flux density
103-117 E15.9 uJy e_F3.6 ?=-99. rms uncertainty on F3.6
124-125 I2 --- f_F3.6 IRAC 3.6um source extraction flag (G1)
128-142 E15.9 uJy F4.5 ?=-99. Spitzer/IRAC 4.5um flux density
145-159 E15.9 uJy e_F4.5 ?=-99. rms uncertainty on F4.5
166-167 I2 --- f_F4.5 IRAC 4.5um source extraction flag (G1)
170-184 E15.9 uJy F5.8 ?=-99. Spitzer/IRAC 5.8um flux density
187-201 E15.9 uJy e_F5.8 ?=-99. rms uncertainty on F5.8
208-209 I2 --- f_F5.8 IRAC 5.8um source extraction flag (G1)
212-226 E15.9 uJy F8.0 ?=-99. Spitzer/IRAC 8.0um flux density
229-243 E15.9 uJy e_F8.0 ?=-99. rms uncertainty on F8.0
250-251 I2 --- f_F8.0 IRAC 8.0um source extraction flag (G1)
255-268 E14.9 uJy F24 Spitzer/MIPS 24um flux density
272-285 E14.9 uJy e_F24 MIPS 24um flux error on residual map (G2)
288-302 E15.9 uJy eF24 ?=-99. MIPS 24um flux error on
Monte-Carlo simulations (G2)
306-319 E14.9 s/pix cov24 MIPS 24um coverage map value (G3)
322-336 E15.9 uJy F70 ?=-99. Spitzer/MIPS 70um flux density
340-353 E14.9 uJy e_F70 MIPS 70um flux error on residual map (G2)
356-370 E15.9 uJy eF70 ?=-99. MIPS 70um flux error on
Monte-Carlo simulations (G2)
374-387 E14.9 s/pix cov70 Spitzer/MIPS 70um coverage map value (G3)
390-404 E15.9 uJy F100 ?=-99. Herschel/PACS 100um flux density
407-421 E15.9 uJy e_F100 ?=-99. PACS 100um flux error on residual map (G2)
424-438 E15.9 uJy eF100 ?=-99. PACS 100um flux error on
Monte-Carlo simulations (G2)
442-456 E15.9 --- cov100 PACS 100um coverage map value (G4)
458-472 E15.9 uJy F160 ?=-99. Herschel/PACS 160um flux density
475-489 E15.9 uJy e_F160 ?=-99. PACS 160um flux error on residual map (G2)
492-506 E15.9 uJy eF160 ?=-99. PACS 160um flux error on
Monte-Carlo simulations (G2)
510-523 E14.9 --- cov160 PACS 160um coverage map value (G4)
526-540 E15.9 uJy F250 ?=-99. Herschel/SPIRE 250um flux density
544-557 E14.9 uJy e_F250 SPIRE 250um flux error on residual map (G2)
560-574 E15.9 uJy eF250 ?=-99. SPIRE 250um flux error on
Monte-Carlo simulations (G2)
578-591 E14.9 --- cov250 SPIRE 250um coverage map value (G4)
594-608 E15.9 uJy F350 ?=-99. Herschel/SPIRE 350um flux density
612-625 E14.9 uJy e_F350 SPIRE 350um flux error on residual map (G2)
628-642 E15.9 uJy eF350 ?=-99. SPIRE 350um flux error on
Monte-Carlo simulations (G2)
646-659 E14.9 --- cov350 SPIRE 350um coverage map value (G4)
662-676 E15.9 uJy F500 ?=-99. Herschel/SPIRE 500um flux density
680-693 E14.9 uJy e_F500 SPIRE 500um flux error on residual map (G2)
696-710 E15.9 uJy eF500 ?=-99. SPIRE 500um flux error on
Monte-Carlo simulations (G2)
714-727 E14.9 --- cov500 SPIRE 500um coverage map value (G4)
735-740 I6 --- Clean Index (CLEAN_INDEX) measuring flux contamination
from nearby sources (G5)
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Byte-by-byte Description of file: ghs.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- --- [GOODS_J]
8- 25 A18 --- GOODS IAU coded object identification,
GOODS_JHHMMSS.ss+DDMMSS.s
28- 31 I4 --- ID [1/2531] Sequential id specific to the catalogue
35- 57 E23.18 deg RAdeg Right Ascension (J2000)
60- 83 E24.18 deg DEdeg Declination (J2000)
86-100 E15.9 uJy F3.6 ?=-99. Spitzer/IRAC 3.6um flux density
103-117 E15.9 uJy e_F3.6 ?=-99. rms uncertainty on F3.6
124-125 I2 --- f_F3.6 IRAC 3.6um source extraction flag (G1)
128-142 E15.9 uJy F4.5 ?=-99. Spitzer/IRAC 4.5um flux density
145-159 E15.9 uJy e_F4.5 ?=-99. rms uncertainty on F4.5
166-167 I2 --- f_F4.5 IRAC 4.5um source extraction flag (G1)
170-184 E15.9 uJy F5.8 ?=-99. Spitzer/IRAC 5.8um flux density
187-201 E15.9 uJy e_F5.8 ?=-99. rms uncertainty on F5.8
208-209 I2 --- f_F5.8 IRAC 5.8um source extraction flag (G1)
212-226 E15.9 uJy F8.0 ?=-99. Spitzer/IRAC 8.0um flux density
229-243 E15.9 uJy e_F8.0 ?=-99. rms uncertainty on F8.0
250-251 I2 --- f_F8.0 IRAC 8.0um source extraction flag (G1)
255-268 E14.9 uJy F24 Spitzer/MIPS 24um flux density
272-285 E14.9 uJy e_F24 MIPS 24um flux error on residual map (G2)
288-302 E15.9 uJy eF24 ?=-99. MIPS 24um flux error on
Monte-Carlo simulations (G2)
306-319 E14.9 s/pix cov24 MIPS 24um coverage map value (G3)
322-336 E15.9 uJy F70 ?=-99. Spitzer/MIPS 70um flux density
340-353 E14.9 uJy e_F70 MIPS 70um flux error on residual map (G2)
356-370 E15.9 uJy eF70 ?=-99. MIPS 70um flux error on
Monte-Carlo simulations (G2)
374-387 E14.9 s/pix cov70 MIPS 70um coverage map value (G3)
390-404 E15.9 uJy F100 ?=-99. Herschel/PACS 100um flux density
407-421 E15.9 uJy e_F100 ?=-99. PACS 100um flux error on residual map (G2)
424-438 E15.9 uJy eF100 ?=-99. PACS 100um flux error on
Monte-Carlo simulations (G2)
442-456 E15.9 --- cov100 PACS 100um coverage map value (G4)
458-472 E15.9 uJy F160 ?=-99. Herschel/PACS 160um flux density
475-489 E15.9 uJy e_F160 ?=-99. PACS 160um flux error on residual map (G2)
492-506 E15.9 uJy eF160 ?=-99. PACS 160um flux error on
Monte-Carlo simulations (G2)
510-523 E14.9 --- cov160 PACS 160um coverage map value (G4)
530-535 I6 --- Clean Index (CLEAN_INDEX) measuring flux contamination
from nearby sources (G5)
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Global notes:
Note (G1): The IRAC source extraction flag come from the IRAC flag maps as
described in the GOODS project DR1 documentation. It's a composite flag
based on the binary values:
0 = >50% of the modal exposure time
1 = <50% of the modal exposure time
2 = <20% of the modal exposure time
16 = Region with significant residual muxbleed
64 = No data (zero retained exposure time)
These values will often appear in combination. For example, regions
with <20% of the modal exposure time (flag value 2) also have <50% of
the modal exposure time (flag value 1). Therefore, those sources will
have flag values of 2+1=3. Regions with no data will have flag values
64+2+1=67. Regions with residual muxbleed (flag 16) and also <50%
modal exposure time (flag 1) will have flag 16+1=17.
Note (G2): Please, read the GOODS-Herschel release document for a complete
description of the two noise estimations: e_FNNN (errNNN_ima) based on the
residual map and eFNNN (errNNN_sim) based on Monte-Carlo simulations. In
particular, to be conservative, users should always use the highest
uncertainty but not the quadratic combination of both since they are not
independent. Also, the Monte-Carlo simulations were made on regions with
relatively homogeneous exposure time; therefore, uncertainties derived
from these simulations are not suitable and hence not provided for
sources situated outside these homogeneous exposure time regions.
Note (G3): the coverage map for MIPS is the time spent per pixel.
Note (G4): the coverage map for PACS and SPIRE is proportional to the time
spent per pixel (s/pix). It corresponds to the number of detector
pixels that have contributed to the value of the pixel in the final
projected image. Because Herschel scans the sky at constant speed,
this number of 'detector pixels' is proportional to the exposure time
in seconds/'projected image pixels'.
Note (G5): Measure of the flux contamination by nearby sources, computed as
CLEAN_INDEX = Neib24 + Neib100x10 + Neib160x102 + Neib250x103 +
Neib350x104 + Neib500x105
where Neib24 (resp. Neib100, Neib160, ...) is the number of bright neighbours
(see the GOODS-Herschel release document) at 24um (resp. 100um 160um, ...).
On GOODS-South, it is assumed that Neib250 = Neib350 = Neib500 = 0.
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History:
Copied at http://hedam.lam.fr/GOODS-Herschel/
(End) Patricia Vannier [CDS] 02-Oct-2013