J/A+A/476/151 SWIRE ELAIS-S1 IR-peak galaxy IR fluxes (Berta+, 2007)
The contribution of very massive high-redshift SWIRE galaxies to the stellar
mass function.
Berta S., Lonsdale C.J., Polletta M., Savage R.S., Franceschini A.,
Buttery H., Cimatti A., Dias J., Feruglio C., Fiore F., Held E.V.,
La Franca F., Maiolino R., Marconi A., Matute I., Oliver S.J.,
Ricciardelli E., Rubele S., Sacchi N., Shupe D., Surace J.
<Astron. Astrophys. 476, 151 (2007)>
=2007A&A...476..151B 2007A&A...476..151B
ADC_Keywords: Galaxies, IR ; Photometry, infrared
Keywords: galaxies: evolution - galaxies: luminosity function, mass function -
galaxies high-redshift - galaxies: fundamental parameters -
galaxies: statistics - infrared: galaxies
Description:
Main data on the IR-peakers sample in the SWIRE ELAIS-S1 field. For
each IR-peak galaxy, we report R band magnitude (AB units, from the
ESIS survey, Berta et al., 2006A&A...451..881B 2006A&A...451..881B), Spitzer SWIRE fluxes
(Lonsdale et al., 2003PASP..115..897L 2003PASP..115..897L, 2004ApJS..154...54L 2004ApJS..154...54L),
photometric redshift (based on Hyper-z fit, Bolzonella et al.,
2000A&A...363..476B 2000A&A...363..476B), the stellar mass and its minimal-maximal range.
The stellar mass estimate is based on mixed stellar population (MSP)
synthesis (Berta et al., 2004A&A...418..913B 2004A&A...418..913B). The minimal and maximal
stellar masses are obtained by exploring the SFH-extinction parameter
space with the Adaptive Simulated Annealing algorithm (Ingber et al.,
2001, http://www.ingber.com/asa01_lecture.pdf). See the paper
associated to these data for more details.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table.dat 134 326 Properties of IR-peakers in the Spitzer/SWIRE
ELAIS-S1 survey
--------------------------------------------------------------------------------
See also:
J/MNRAS/351/1290 : ELAIS: final band-merged catalogue (Rowan-Robinson+, 2004)
J/AJ/127/3075 : ELAIS-S1 sample mid-infrared population (La Franca+, 2004)
J/MNRAS/305/297 : ISO ELAIS 1.4GHz survey (Gruppioni+, 1999)
J/A+A/457/501 : XMM-Newton survey of the ELAIS-S1 field (Puccetti+, 2006)
Byte-by-byte Description of file: table.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 I6 --- Seq ID number
8- 16 F9.5 deg RAdeg Right ascension (J2000)
17- 25 F9.5 deg DEdeg Declination (J2000)
27- 31 F5.2 mag Rcmag ?=24.50 Cousins R magnitude, in AB system
33- 37 F5.2 mag e_Rcmag ?=99.99 uncertainty on Rcmag
39- 44 F6.2 uJy S3.6um 3.6um flux
46- 49 F4.2 uJy e_S3.6um 3.6um flux uncertainty
51- 56 F6.2 uJy S4.5um 4.5um flux
58- 61 F4.2 uJy e_S4.5um 4.5um flux uncertainty
63- 68 F6.2 uJy S5.8um 5.8um flux
70- 73 F4.2 uJy e_S5.8um 5.8um flux uncertainty
75- 80 F6.2 uJy S8um ?=28.80 8.0um flux
82- 86 F5.2 uJy e_S8um ?=28.80 8.0um flux uncertainty
88- 94 F7.2 uJy S24um ?=250.00 24um flux
96-101 F6.2 uJy e_S24um ?=250.00 24um flux uncertainty
103-107 F5.3 --- zphot Photometric redshift
109-116 E8.3 solMass Mass Stellar mass, best fit
118-125 E8.3 solMass Mmin Stellar mass, minimal
127-134 E8.3 solMass Mmax Stellar mass, maximal
--------------------------------------------------------------------------------
Acknowledgements:
Stefano Berta, ste_atreb(at)yahoo.it
History:
* 13-Sep-2007: Original position, without positions
* 16-Apr-2008: Addition of position, supplied by the author.
(End) Stefano Berta [MPE], Patricia Vannier [CDS] 13-Sep-2007