J/ApJ/630/206       Hα data for 3 EDisCS galaxy clusters     (Finn+, 2005)

Hα-derived star formation rates for three z≃0.75 EDisCS galaxy clusters. Finn R.A., Zaritsky D., Mccarthy D.W.JR, Poggianti B., Rudnick G., Halliday C., Milvang-jensen B., Pello R., Simard L. <Astrophys. J., 630, 206-227 (2005)> =2005ApJ...630..206F 2005ApJ...630..206F (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Equivalent widths ; Photometry Keywords: galaxies: clusters: general - galaxies: evolution - galaxies: high-redshift - stars: formation Abstract: We present Hα-derived SFRs for three z∼0.75 galaxy clusters. Our 1σ flux limit corresponds to a star formation rate (SFR) of 0.10-0.24h-2100M_☉/yr, and our minimum reliable Hα+[NII] rest-frame equivalent width is 10Å. We show that H narrowband imaging is an efficient method for measuring star formation in distant clusters. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 98 41 Hα data for CL 1040-1155 galaxies table4.dat 98 71 Hα data for CL 1054-1245 galaxies table5.dat 98 147 Hα data for CL 1216-1201 galaxies -------------------------------------------------------------------------------- See also: J/ApJ/604/141 : Hα fluxes in Cl J0023+0423B galaxies (Finn+, 2004) J/ApJS/137/117 : Las Campanas Distant Cluster Survey (LCDCS) (Gonzales+, 2001) J/A+A/444/365 : ESO Distant Cluster Survey, EDisCS (White+, 2005) J/A+A/427/397 : Redshifts of 5 EDisCS galaxy clusters (Halliday+, 2004) Byte-by-byte Description of file: table3.dat table4.dat table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- EDCS Source name (HHMMSSs+DDMMSSs) (EDCS JHHMMSSs+DDMMSSs in Simbad) 17- 21 F5.1 arcsec oRA Right Ascension offset from brightest cluster galaxy 23- 27 F5.1 arcsec oDE Declination offset from brightest cluster galaxy 29- 33 F5.1 s-1 FHa Narrow-band Hα flux in ADU/s 35- 37 F3.1 s-1 e_FHa Error in FHa 39- 44 F6.1 s-1 FJ J-band flux (near-IR, 1.2µm) in ADU/s 46- 49 F4.1 s-1 e_FJ Error in FJ 51- 55 F5.2 mag Jmag SExtractor isophotal J-band magnitude 57- 60 F4.2 mag e_Jmag Error in Jmag 62- 66 F5.2 s-1 FCS Continuum-subtracted flux in ADU/s 68- 71 F4.2 s-1 e_FCS Error in FCS 73- 76 F4.1 --- SNR Signal-to-Noise ratio of continuum-subtracted flux 78- 82 F5.1 0.1nm EWHa Narrow-band Hα equivalent width in units of Angstroms 84- 87 F4.1 0.1nm e_EWHa Error in EW 89- 92 F4.1 solMass/yr SFR Star Formation Rate (1) 94- 96 F3.1 solMass/yr e_SFR Error in SFR (1) 98 I1 --- SF [0/1] Star-forming galaxy code (2) -------------------------------------------------------------------------------- Note (1): In units of h-2100solMass/yr. Note (2): Star-forming galaxy code, defined as follows: 1 = meets minimum continuum-subtracted flux and EW cuts; 0 = doesn't meet minimum continuum-subtracted flux and EW cuts. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 03-Jan-2006
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