J/ApJS/150/1        VV29 and NGC 4676 HST photometry         (Benitez+, 2004)

Faint galaxies in Deep Advanced Camera for Surveys observations. Benitez N., Ford H., Bouwens R., Menanteau F., Blakeslee J., Gronwall C., Illingworth G., Meurer G., Broadhurst T.J., Clampin M., Franx M., Hartig G.F., Magee D., Sirianni M., Ardila D.R., Bartko F., Brown R.A., Burrows C.J., Cheng E.S., Cross N.J.G., Feldman P.D., Golimowski D.A., Infante L., Kimble R.A., Krist J.E., Lesser M.P., Levay Z., Martel A.R., Miley G.K., Postman M., Rosati P., Sparks W.B., Tran H.D., Tsvetanov Z.I., White R.L., Zheng W. <Astrophys. J. Suppl. Ser., 150, 1 (2004)> =2004ApJS..150....1B 2004ApJS..150....1B (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, photometry ; Redshifts Keywords: galaxies: evolution - galaxies: fundamental parameters - galaxies: high-redshift - galaxies: photometry - techniques: photometric Abstract: We present the analysis of the faint galaxy population in the Advanced Camera for Surveys (ACS) Early Release Observation fields VV 29 (UGC 10214) and NGC 4676. These observations cover a total area of 26.3arcmin2 and have depths close to that of the Hubble Deep Fields in the deepest part of the VV 29 image, with 10σ detection limits for point sources of 27.8, 27.6, and 27.2 AB magnitudes in the gF475W, VF606W, and IF814W bands, respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4a.dat 84 5712 Redshift catalog in the VV 29 field table4b.dat 144 5712 Photometric catalog in the VV 29 field table5a.dat 84 3254 Redshift catalog in the NGC 4676 field table5b.dat 144 3254 Photometric catalog in the NGC 4676 field -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4a.dat table5a.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID SExtractor identification number (G1) 6- 7 I2 h RAh Hour of Right Ascension (J2000) 9- 10 I2 min RAm Minute of Right Ascension (J2000) 12- 16 F5.2 s RAs Second of Right Ascension (J2000) 17 A1 --- DE- Sign of Declination (J2000) 18- 19 I2 deg DEd Degree of Declination (J2000) 21- 22 I2 arcmin DEm Arcminute of Declination (J2000) 24- 27 F4.1 arcsec DEs Arcsecond of Declination (J2000) 29- 34 F6.1 pix Xpix X pixel coordinate 36- 41 F6.1 pix Ypix Y pixel coordinate 43- 46 F4.2 --- B-z Bayesian photometric redshift 48- 51 F4.2 --- B-zmin The 95% lower confidence redshift interval 53- 56 F4.2 --- B-zmax The 95% upper confidence redshift interval 58- 61 F4.2 --- B-Type Bayesian spectral type (1) 63- 68 F6.4 --- B-Odds Bayesian odds (2) 70- 73 F4.2 --- ML-z Maximum likelihood redshift 75- 78 F4.2 --- ML-Type Maximum likelihood spectral type (1) 80- 84 F5.2 --- ML-chi2 The χ2 for best maximum likelihood fit -------------------------------------------------------------------------------- Note (1): the types are: El(1), Sbc(2), Scd(3), Im(4), SB3(5), and SB2(6). Note (2): It is the integral of the redshift probability distribution in a region of about 0.2(1+zB). If close to 1, it means that the redshift probability is narrow and has a single peak. Very low values of the odds indicate that the color/magnitude information is almost useless to estimate the redshift. Photometric redshifts with values <0.9 are unreliable. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4b.dat table5b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID SExtractor identification number (G1) 6- 7 I2 h RAh Hour of Right Ascension (J2000) 9- 10 I2 min RAm Minute of Right Ascension (J2000) 12- 16 F5.2 s RAs Second of Right Ascension (J2000) 17 A1 --- DE- Sign of Declination (J2000) 18- 19 I2 deg DEd Degree of Declination (J2000) 21- 22 I2 arcmin DEm Arcminute of Declination (J2000) 24- 27 F4.1 arcsec DEs Arcsecond of Declination (J2000) 29- 34 F6.1 pix Xpix X pixel coordinate 36- 41 F6.1 pix Ypix Y pixel coordinate 43- 48 F6.2 mag gauto ?=99 F475W band SExtractor MAG_AUTO AB magnitude 52- 55 F4.2 mag e_gauto Error in gauto 57- 62 F6.2 mag Vauto ?=99 F606W band SExtractor MAG_AUTO AB magnitude 66- 69 F4.2 mag e_Vauto Error in Vauto 71- 76 F6.2 mag Iauto ?=99 F814W band SExtractor MAG_AUTO AB magnitude 80- 83 F4.2 mag e_Iauto Error in Iauto 85- 90 F6.2 mag giso ?=99 F475W band SExtractor MAG_ISO AB magnitude 94- 97 F4.2 mag e_giso Error in giso 99-104 F6.2 mag Viso ?=99 F606W band SExtractor MAG_ISO AB magnitude 108-111 F4.2 mag e_Viso Error in Viso 113-118 F6.2 mag Iiso ?=99 F814W band SExtractor MAG_ISO AB magnitude 122-125 F4.2 mag e_Iiso Error in Iiso 127-133 F7.2 pix FWHM SExtractor Full Width at Half Maximum (1) 135-138 F4.2 --- Class SExtractor star/galaxy classification (2) 140-142 I3 --- SExFlag SExtractor detection flag 144 I1 --- MFlag Mask flag (3) -------------------------------------------------------------------------------- Note (1): Where scale = 0.05 arcsec/pixel. Note (2): We consider as stars or point sources all objects which have a value of this parameter ≥0.94, and set all their photometric redshift parameters to zero. Note (3): Mask flags are: 1 = masked out due to being close to bright objects; 0 = not masked. -------------------------------------------------------------------------------- Global notes: Note (G1): in Simbad, the designations are: In table4.dat, [BFB2004] VV 29 NNNN In table5.dat, [BFB2004] NGC 4676 NNNN -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 23-Jan-2004
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