J/ApJ/591/53        I photometry of Cl 0024+16               (Treu+, 2003)

A Wide-Field Hubble Space Telescope study of the cluster Cl 0024+16 at z = 0.4. I. Morphological distributions to 5 Mpc radius. Treu T., Ellis R.S., Kneib J.-P., Dressler A., Smail I., Czoske O., Oemler A., Natarajan P. <Astrophys. J. 591, 53 (2003)> =2003ApJ...591...53T 2003ApJ...591...53T
ADC_Keywords: Clusters, galaxy ; Galaxies, photometry Mission_Name: HST Keywords: galaxies: clusters: individual (Cl 0024+1654) - galaxies: evolution - galaxies: formation - galaxies: fundamental parameters - galaxies: high-redshift - galaxies: photometry Abstract: We describe a new wide-field Hubble Space Telescope survey of the galaxy cluster Cl 0024+16 (z∼0.4) consisting of a sparsely sampled mosaic of 39 Wide Field Planetary Camera 2 images that extends to a cluster radius of ∼5Mpc. Together with extensive ground-based spectroscopy taken from the literature, augmented with over a hundred newly determined redshifts, this unique data set enables us to examine environmental influences on the properties of cluster members from the inner core to well beyond the virial radius (∼1.7Mpc). We catalog photometric measures for 22000 objects to I≳25 and assign morphological types for 2181 to I=22.5, of which 195 are spectroscopically confirmed cluster members. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 131 22320 The catalog -------------------------------------------------------------------------------- See also: J/A+A/372/391 : Spectroscopic Survey of Cl 0024+1654 (Czoske+, 2001) Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- POS WFPC2 pointing, as identified in Table 2 (G1) 4 I1 --- Chip WFPC2 chip number (G1) 6- 8 I3 --- ID Running number within each chip (G1) 10- 16 F7.2 pix Xpix X-coordinate on the chip of the object baricenter 18- 24 F7.2 pix Ypix Y-coordinate on the chip of the object baricenter 28- 34 F7.5 deg RAdeg Right Ascension (J2000) in decimal degrees of the object baricenter 37- 45 F9.6 deg DEdeg Declination (J2000) in decimal degrees of the object baricenter 47- 54 F8.3 mag Imag ?=-999.999 SExtractor F814W band magnitude (1) 56- 63 F8.3 mag e_Imag ?=-999.999 Error in Imag (1) 65- 72 F8.3 mag I1mag ?=-999.999 SExtractor F814W band magnitude within 0.5'' diameter aperture (1) 74- 81 F8.3 mag e_I1mag ?=-999.999 Error in I1mag (1) 83- 90 F8.3 mag I2mag ?=-999.999 SExtractor F814W band magnitude within 1'' diameter aperture (1) 92- 99 F8.3 mag e_I2mag ?=-999.999 Error in I2mag (1) 101-104 F4.2 --- SClass [0,1] SExtractor stellar classification, (1 = star, 0 = galaxy) 106-107 I2 --- Type ? Morphological type by Richard S. Ellis 109-138 A30 --- Comm Comment by Richard S. Ellis -------------------------------------------------------------------------------- Note (1): All magnitudes are in the Vega system and corrected for galactic extinction, adopting E(B-V)=0.057 (Schlegel et al., 1998ApJ...500..525S 1998ApJ...500..525S). The value -999.999 indicates numerical problems in computing the quantity. -------------------------------------------------------------------------------- Global notes: Note (G1): Objects identified as [TEK2003] NN-N-NNN in Simbad -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 26-Sep-2003
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