J/MNRAS/414/2246    EROs in Groth Strip                      (Hempel+, 2011)

The morphologies and masses of extremely red galaxies in the Groth Strip. Hempel A., Cristobal-Hornillos D., Prieto M., Trujillo I., Balcells M., Lopez-Sanjuan C., Abreu D., Eliche-Moral M.C., Dominguez-Palmero L. <Mon. Not. R. Astron. Soc., 414, 2246-2264 (2011)> =2011MNRAS.414.2246H 2011MNRAS.414.2246H
ADC_Keywords: Infrared sources ; Galaxies, photometry ; Morphology Keywords: galaxies: evolution - galaxies: high-redshift - galaxies: photometry - galaxies: star formation - galaxies: stellar content - galaxies: structure Abstract: We present a new catalogue of EROs from the Groth Strip and study the relation between their morphology and mass. With a selection criterion F814W-Ks≥4 and Ks≤21.0 we find 102 EROs, over a survey area of 155 arcmin2, leading to a surface density of 0.66arcmin-2. The photometric data include U, B, F606W, F814W, J, Ks bands. Morphologies are based on a by eye classification and we distinguish between three basic classes: compact objects, targets with a disc and/or a bulge component and irregular or merger candidates. An additional group consists of the few objects which could not be classified. Description: We have selected a sample of extremely red galaxies (EROs) from the GOYA Survey (Balcells et al., 2002INGN....6...11B 2002INGN....6...11B). This is a combined Ks selected catalogue covering the Groth-Westphal strip (∼155arcmin2) in four optical bands, U, B, F606W and F814W, as well as J, Ks in the NIR. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 129 108 Summary of photometric, morphological and structural parameters tablea2.dat 76 108 Results of mass and age analysis -------------------------------------------------------------------------------- See also: J/ApJ/581/844 : Radio and Infrared observations of EROs (Smail+, 2002) J/MNRAS/330/1 : HST observations of Extremely Red Objects (Smith+, 2002) J/PASJ/55/1079 : BVRi'z'JHKs photometry of ERO objects (Miyazaki+, 2003) J/MNRAS/346/1125 : Faint Extremely Red Objects IK photometry (Gilbank+, 2003) J/A+A/432/69 : Extremely Red Objects XMM-Newton observations (Brusa+, 2005) J/ApJ/627/621 : Catalog of Extremely Red Objects (Sawicki+, 2005) J/MNRAS/361/525 : Las Campanas Infrared Survey. V. (Doherty+, 2005) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [ero_] 5- 22 A18 --- ero ero name (HHMMSS.ss+DDMMSS.s, J2000) (G1) 23 A1 --- n_ero [*#] DRG(*) or excluded object (#) (1) 25- 28 F4.2 --- zph Photometric redshift 30- 33 F4.2 --- e_zph rms uncertainty on zph 35- 36 A2 --- Class Visual classification (2) 38- 45 A8 --- Vote Security of the vote, Secure/Unsecure (3) 47- 51 F5.2 mag F814W Aperture magnitude F814W 53- 56 F4.2 mag e_F814W rms uncertainty on F814W 58- 62 F5.2 mag Ksmag Aperture magnitude Ks 64- 67 F4.2 mag e_Ksmag rms uncertainty on Ksmag 69- 72 F4.2 mag F814W-Ks F814W-Ks colour index 74- 78 F5.2 kpc ae Effective radius (half-light radius along semimajor axis) 80- 84 F5.2 kpc e_ae rms uncertainty on ae 86- 90 F5.2 --- n Sersic index 92- 98 F7.2 --- e_n rms uncertainty on n 100-103 F4.2 --- b/a Axial ratio 105-110 F6.2 --- e_b/a rms uncertainty on b/a 112-116 F5.2 mag F814WG GALFIT F814W magnitude 119-123 F5.2 mag e_F814WG ?=99.00 rms uncertainty on F814WG 125-129 F5.3 --- chi2G GALFIT χ2 value -------------------------------------------------------------------------------- Note (1): Individual notes as follows: * = object fulfil also the colour criteria for DRGs (distant red galaxy): J-K>2.3 # = object shows extremely low effective radii (reff≤0.01kpc) and was excluded from our final target list Note (2): Classification as follows: 1 = objects with very compact morphology, like expected for early-type galaxies 2a = objects with bulge and disc component (early-type discs) 2b = disc galaxies with no clear bulge component, including edge-on discs (late-type discs) 2c = extended objects with bulge and/or disc component, for which no clear classification as either class 2a or class 2b was possible 3 = irregular or merger candidates 4 = no clear classification at all Note (3): Each galaxy in our sample of 102 EROs was classified individually by four of the authors (A. Hempel, M. Prieto, I. Trujillo and M. Balcells). Sources for which at least three classifications agree are considered as 'secure'. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [ero_] 5- 22 A18 --- ero ero name (HHMMSS.ss+DDMMSS.s, J2000) (G1) 24 I1 --- zf [3/8]?=- Formation redshift 26- 29 F4.2 Gyr tau ?=- Exponential decay time 31- 33 F3.1 mag AV ?=- Optical depth 35- 39 F5.3 [-] Z ?=- Metallicity 41- 45 F5.2 Gpc DL Luminosity distance 47- 50 F4.2 Gpc E_DL Error on DL (upper limit) 52- 55 F4.2 Gpc e_DL Error on DL (lower limit) 57- 62 F6.3 10+10Msun Mtot ?=- Total stellar mass 64- 69 F6.3 10+8yr Age ?=- Age 71- 76 F6.2 --- chi2 ?=- χ2 value -------------------------------------------------------------------------------- Global notes: Note (G1): Sources identified as <[HCP2011] ero JHHMMSS.ss+DDMMSS.s> in Simbad -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 17-Feb-2012
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