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J/ApJ/697/506     Mid-infrared galaxy luminosity function from AGN  (Dai+, 2009)

Mid-infrared galaxy luminosity functions from the AGN and galaxy evolution survey. Dai X., Assef R.J., Kochanek C.S., Brodwin M., Brown M.J.I., Caldwell N., Cool R.J., Dey A., Eisenhardt P., Eisenstein D., Gonzalez A.H., Jannuzi B.T., Jones C., Murray S.S., Stern D. <Astrophys. J., 697, 506-521 (2009)> =2009ApJ...697..506D
ADC_Keywords: Active gal. nuclei ; Photometry, infrared Keywords: galaxies: evolution - galaxies: luminosity function, mass function Abstract: We present galaxy luminosity functions at 3.6, 4.5, 5.8, and 8.0um measured by combining photometry from the IRAC Shallow Survey with redshifts from the AGN and Galaxy Evolution Survey (AGES) of the NOAO Deep Wide-Field Survey Bootes field. The well defined IRAC samples contain 3800-5800 galaxies for the 3.6-8.0um bands with spectroscopic redshifts and z<0.6. We obtained relatively complete luminosity functions in the local redshift bin of z<0.2 for all four IRAC channels that are well fitted by Schechter functions. Description: We measured the mid-IR galaxy LFs in the NDWFS Bootes field by combining IRAC photometry from the IRAC Shallow Survey and AGES redshifts. This field is also covered by multiwavelength data in the UV (GALEX; Martin et al. 2005ApJ...619L...1M), optical (NDWFS), z-band (zBootes; Cool 2007ApJS..169...21C), near-IR (NDWFS and FLAMEX; Elston et al., 2006, Cat. J/ApJ/639/816), and far-IR (24um; Soifer et al. 2004AAS...204.4805S), allowing us to use spectral energy distribution (SED) models to type the galaxies and make K-corrections. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 64 363 Binned SWML luminosity functions
See also: J/ApJ/314/493 : Boo Void survey (Kirshner+, 1987) J/A+A/535/A38 : NOAO Bootes field 153MHz observations (Intema+, 2011) J/AJ/123/1784 : 1.4 GHz imaging of the Bootes field (de Vries+, 2002) J/AJ/127/213 : LALA Bootes field X-ray source catalog (Wang+, 2004) J/AJ/130/923 : Faint radio sources in the NOAO Bootes field (Wrobel+, 2005) J/ApJ/634/L1 : 16µm sources in the NOAO Bootes field (Kasliwal+, 2005) J/ApJS/161/9 : X-ray survey of the NDWFS Bootes field (Kenter+, 2005) J/ApJ/641/140 : Optical counterparts in the NDWFS Bootes field (Brand+, 2006) J/AJ/136/2321 : Washington photometry of Bootes I stars (Hughes+, 2008) J/AJ/138/251 : Bright Galactic stars Spitzer 24um excess (Hovhannisyan+, 2009) Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 3 F3.1 um Band Filter band (3.6, 4.5, 5.8 or 8.0) 5- 9 A5 --- Type Galaxy type (All, Early or Late) 11- 16 F6.2 mag mag Galaxy absolute magnitude bin 18- 24 E7.2 Mpc-3/mag dN/dm1 ?=-9.9E+9 Luminosity function for z≤0.2 (1) 26- 32 E7.2 Mpc-3/mag e_dN/dm1 ?=-9.9E+9 Uncertainty in dN/dm1 (1) 34- 40 E7.2 Mpc-3/mag dN/dm2 ?=-9.9E+9 Luminosity function for 0.2≤z≤0.35 (1) 42- 48 E7.2 Mpc-3/mag e_dN/dm2 ?=-9.9E+9 Uncertainty in dN/dm2 (1) 50- 56 E7.2 Mpc-3/mag dN/dm3 ?=-9.9E+9 Luminosity function for 0.35≤z≤0.6 (1) 58- 64 E7.2 Mpc-3/mag e_dN/dm3 ?=-9.9E+9 Uncertainty in dN/dm3 (1)
Note (1): In units of h3/Mpc3/mag where H0=100h.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 01-Dec-2011
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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