J/ApJ/581/844       Radio and Infrared observations of EROs  (Smail+, 2002)

The diversity of Extremely Red Objects. Smail I., Owen F.N., Morrison G.E., Keel W.C., Ivison R.J., Ledlow M.J. <Astrophys. J., 581, 844-864 (2002)> =2002ApJ...581..844S 2002ApJ...581..844S
ADC_Keywords: Clusters, galaxy ; Infrared sources ; Photometry, infrared ; Radio sources Keywords: cosmology: observations - galaxies: clusters: individual (A851, Cl 0939+4713) - galaxies: evolution - galaxies: starburst - infrared: galaxies Abstract: We present the results from a sensitive multiwavelength analysis of the properties of extremely red objects (EROs). Our analysis employs deep RIzJHK photometry of an 8.5'x8.5' region to select a sample of 68 EROs with (R-K)≥5.3 and brighter than K=20.5 (5σ). We combine this photometric data set with an extremely deep 1.4GHz radio map of the field obtained from the VLA. This map reaches a 1σ limiting flux density of 3.5µJy , making it the deepest 1.4GHz map taken, and is sensitive enough to detect an active galaxy with L1.4≳1023W/Hz at z>1. Description: The radio image of A851 comprises a combination of A, B, C, and D configuration observations from the National Radio Astronomy Observatory's VLA taken at 1.4GHz between 1996 and 2000. Our primary near-infrared imaging data set comes from wide-field images in JHK taken with the KPNO 2.1 m telescope on the nights of 2001 January 4-11. On the nights of 1999 February 28, March 0102, and March 1516 we completed a K-band mosaic of 5x5 pointings using the UFTI imager on UKIRT On 2000 December 1112 we used the INGRID near-infrared imager in the WHT to obtain a J-band image of the cluster core. The optical imaging to complement our deep near-infrared data sets was obtained from three facilities. We have two wide-field imaging data sets of this region. The first comes from Suprime-Cam on Subaru (courtesy of T. Kodama) and consists of very deep RI imaging of a 27'x27' field centered on the cluster core, taken on the nights of 2001 January 21-22. We also have obtained similarly a wide-field KPNO 4m image in the z band, obtained on the night of 2001 January 25/26. Finally, an HST/WFPC2 mosaic of A851 has been observed in the F702W filter, but we will not use the HST imaging in our analysis. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 129 68 ERO Catalog -------------------------------------------------------------------------------- See also: J/MNRAS/330/1 : HST observations of Extremely Red Objects (Smith+, 2002) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- [SOM2002] Sequential number 6 A1 --- n_[SOM2002] [gh] Note on [SOM2002] (1) 8- 9 I2 h RAh Right ascension (J2000.0) 11- 12 I2 min RAm Right ascension (J2000.0) 14- 19 F6.3 s RAs Right ascension (J2000.0) 21 A1 --- DE- Declination sign (J2000.0) 22- 23 I2 deg DEd Declination (J2000.0) 25- 26 I2 arcmin DEm Declination (J2000.0) 28- 32 F5.2 arcsec DEs Declination (J2000.0) 34- 38 F5.2 mag Kmag Total K magnitude 40 A1 --- l_R-K Limit flag on R-K 41- 44 F4.2 mag R-K Aperture R-K colour index 46 A1 --- l_S1.4GHz Limit flag on S1.4GHz 47- 51 F5.1 uJy S1.4GHz Radio flux at 1.4GHz (or 3σ limit) 53 A1 --- l_Rapmag Limit flag on Rapmag 54- 58 F5.2 mag Rapmag 3" diameter aperture R magnitude 60- 62 F3.2 mag e_Rapmag ? rms uncertainty on Rapmag 64 A1 --- l_Iapmag Limit flag on Iapmag 65- 69 F5.2 mag Iapmag 3" diameter aperture I magnitude 71- 73 F3.2 mag e_Iapmag ? rms uncertainty on Iapmag 75 A1 --- l_Zapmag Limit flag on Zapmag 76- 80 F5.2 mag Zapmag 3" diameter aperture Z magnitude 82- 84 F3.2 mag e_Zapmag ? rms uncertainty on Zapmag 86 A1 --- l_Japmag Limit flag on Japmag 87- 91 F5.2 mag Japmag 3" diameter aperture J magnitude 93- 95 F3.2 mag e_Japmag ? rms uncertainty on Japmag 97 A1 --- l_Hapmag Limit flag on Hapmag 98-102 F5.2 mag Hapmag 3" diameter aperture H magnitude 104-106 F3.2 mag e_Hapmag ? rms uncertainty on Hapmag 108 A1 --- l_Kapmag Limit flag on Kapmag 109-113 F5.2 mag Kapmag 3" diameter aperture K magnitude 115-117 F3.2 mag e_Kapmag ? rms uncertainty on Kapmag 119 A1 --- SED [DEB] Best-fitting model SED (2) 121 A1 --- Morph1 [CIF] Visual morphology from high-resolution K-band imaging (3) 122 A1 --- n_Morph1 [def] Note on Morph1 (4) 123 A1 --- --- [/] 124 A1 --- Morph2 [CIF] Visual morphology from high-resolution R-band imaging (3) -------------------------------------------------------------------------------- Note (1): Individual notes: g: M star h: transient source Note (2): Best-fitting model SED: D: dusty E: evolved B: badly fitted Note (3): Morphology: C: compact/regular I: disky, disturbed or amorphous F: too faint to classify Note (4): Notes on morphology: d: SMM J09429+4658 (Smail et al., 1999MNRAS.308.1061S 1999MNRAS.308.1061S). e: ERO Cl 0939+4713 A (Persson et al. 1993, in The Evolution of Galaxies and Their Environments, NASA Tech. Report, ed. M. Shull & H. Thronson (Washington, DC: GPO), 78). f: ERO 333 (Smail et al., 1999ApJ...525..609S 1999ApJ...525..609S). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Bauer [CDS] 09-Feb-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