J/MNRAS/406/1318    Lensed-arc statistics of galaxy clusters (Horesh+, 2010)

The lensing efficiencies of MACS X-ray-selected versus RCS optically selected galaxy clusters. Horesh A., Maoz D., Ebeling H., Seidel G., Bartelmann M. <Mon. Not. R. Astron. Soc., 406, 1318-1336 (2010)> =2010MNRAS.406.1318H 2010MNRAS.406.1318H
ADC_Keywords: Clusters, galaxy ; X-ray sources ; Redshifts ; Photometry, HST Keywords: galaxies: clusters: general - gravitational lensing: strong Abstract: The statistics of strongly lensed arcs in samples of galaxy clusters provide information on cluster structure that is complementary to that from individual clusters. However, samples of clusters that have been analysed to date have been either small, heterogeneous or observed with limited angular resolution. We measure the lensed-arc statistics of 97 clusters imaged at high angular resolution with the Hubble Space Telescope, identifying lensed arcs using two automated arc-detection algorithms. The sample includes similar numbers of X-ray-selected [MAssive Cluster Survey (MACS)] and optically selected [Red-Sequence Cluster Survey (RCS)] clusters, and spans cluster redshifts in the range 0.2<z<1. We compile a catalogue of 42 arcs in the X-ray-selected subsample and seven arcs in the optical subsample. All but five of these arcs are reported here for the first time. Description: We have compiled from the HST archive a sample of clusters observed with the Advanced Camera for Surveys (ACS). Here we use images of 35 MACS clusters observed with the ACS (GO-09722, GO-10491, GO-10875, PI Ebeling). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 55 23 *MACS low-redshift (0.3≤z<0.5) sample table2.dat 64 12 *MACS medium-redshift (0.5≤z<0.7) sample table3.dat 54 18 *RCS low-redshift (0.3≤z<0.5) sample table4.dat 54 18 *RCS medium-redshift (0.5≤z<0.7) sample table5.dat 47 16 *RCS high-redshift (0.7≤z≤1) sample table6.dat 52 49 Detected arcs and properties -------------------------------------------------------------------------------- Note on table1.dat, table2.dat: MACS = MAssive Cluster Survey Note on table3.dat, table4.dat, table5.dat: RCS = Red-Sequence Cluster Survey -------------------------------------------------------------------------------- See also: J/MNRAS/339/913 : Two distant massive clusters of galaxies (Edge+, 2003) J/ApJS/157/1 : Red-Sequence Cluster Survey (Gladders+, 2005) J/ApJS/158/161 : Photometric redshift catalog from the RCS (Hsieh+, 2005) Byte-by-byte Description of file: table[12].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [MACS] 5- 16 A12 --- MACS MACS name (JHHMM.m+DDMM) 18- 19 I2 h RAh Right ascension (J2000) 21- 22 I2 min RAm Right ascension (J2000) 24- 27 F4.1 s RAs Right ascension (J2000) 29 A1 --- DE- Declination sign (J2000) 30- 31 I2 deg DEd Declination (J2000) 33- 34 I2 arcmin DEm Declination (J2000) 36- 39 F4.1 arcsec DEs Declination (J2000) 41- 45 F5.3 --- z ?=- Redshift 47 I1 --- r_z Redshift reference (1) 49- 53 F5.2 mag F606W ?=- Brightest cluster galaxy F606W magnitude 55 A1 --- Arc [*] indicates arc in table6.dat 57- 60 F4.1 10+37W LX ? X-ray luminosity (0.1-2.4keV) (ref#7 only) 62- 64 F3.1 10+15Msun M200 ? Mass enclosed within r200 (2) -------------------------------------------------------------------------------- Note (1): References as follows: 1 = Ebeling et al. (in preparation) 2 = Stott et al. (2007ApJ...661...95S 2007ApJ...661...95S) 3 = Allen et al. (2008MNRAS.383..879A 2008MNRAS.383..879A) 4 = Edge et al. (2003, Cat. J/MNRAS/339/913) 5 = Balestra et al. (2007A&A...462..429B 2007A&A...462..429B) 6 = Smail et al. (2007ApJ...654L..33S 2007ApJ...654L..33S) 7 = Ebeling et al. (2007ApJ...661L..33E 2007ApJ...661L..33E), in table2 only Note (2): In table2 only. M200 is the mass enclosed within r200, the radius within which the average density is equal to 200 times the critical cosmological density at the observed redshift; M200 values are based on the LX-M200 relation of Reiprich & Boehringer (2002ApJ...567..716R 2002ApJ...567..716R). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table[345].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- --- [RCS] 4- 18 A15 --- RCS RCS name (HHMMSS+DDMM.m or HHMMSS.s+DDMMSS) 20- 21 I2 h RAh Right ascension (J2000) 23- 24 I2 min RAm Right ascension (J2000) 26- 29 F4.1 s RAs Right ascension (J2000) 31 A1 --- DE- Declination sign (J2000) 32- 33 I2 deg DEd Declination (J2000) 35- 36 I2 arcmin DEm Declination (J2000) 38- 41 F4.1 arcsec DEs Declination (J2000) 43- 47 F5.3 --- z Redshift 49- 52 F4.1 mag F814W ?=- Brightest cluster galaxy F814W magnitude 54 A1 --- Arc [*] indicates arc in table6.dat -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- Name Cluster name (MACS or RCS) 20- 21 A2 --- Arc Arc ID 22 A1 --- r_Arc [abc] Arc previously reported (1) 24- 27 F4.1 arcsec Length Arc length 29- 31 F3.1 arcsec Width Arc width 33- 37 F5.2 --- l/w Length-to-width ratio 39- 42 F4.1 mag F606W ? F606W magnitude 44- 47 F4.1 mag F814W ? F814W magnitude 49- 52 F4.1 arcsec Sep ?=- Radial separation from cluster centre -------------------------------------------------------------------------------- Note (1): Notes as follows: a = Arcs previously reported by Sand et al. (2005, Cat. J/ApJ/627/32) b = Arcs previously reported by Ebeling et al. (2009MNRAS.395.1213E 2009MNRAS.395.1213E) c = Arcs previously reported by Gladders et al. (2003ApJ...593...48G 2003ApJ...593...48G) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 25-Jan-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