/ftp/cats/J_AJ/130/1324



==========================================================================
J/AJ/130/1324    Faint emission-line galaxies at z<=1.6      (Drozdovsky+, 2005)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table2.dat
==========================================================================
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/AJ/130/1324
==========================================================================

drwxr-xr-x 78 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 09:35 [TAR file] -rw-r--r-- 1 cats archive 469 Jun 15 2006 .message -rw-r--r-- 1 cats archive 6241 Jun 15 2006 ReadMe -rw-r--r-- 1 cats archive 681 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2759 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 145050 Feb 8 2006 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/130/1324 Faint emission-line galaxies at z<=1.6 (Drozdovsky+, 2005) ================================================================================ The Hubble Space Telescope ACS grism parallel survey. II. First results and a catalog of faint emission-line galaxies at z<=1.6. Drozdovsky I., Yan L., Chen H.-W., Stern D., Kennicutt R.JR, Spinrad H., Dawson S. <Astron. J., 130, 1324-1336 (2005)> =2005AJ....130.1324D ================================================================================ ADC_Keywords: Galaxy catalogs ; Photometry, HST ; Redshifts Keywords: catalogs - galaxies: high-redshift - surveys Abstract: We present the first results from the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) Grism Parallel Survey, a large program obtaining deep, slitless ACS grism (R 100) spectroscopy of high-latitude HST parallel fields. We identify 601 compact emission-line galaxies at z<=1.6, reaching emission lines to a flux limit of > 5x10^-18^ergs/cm^2^/s (3sigma). We determine redshifts by cross-correlation of the target spectra with template spectra, followed by visual inspection. We measure star formation rates from the observed [OII]lambda3727, [OIII]lambda5007, and Halpha line fluxes.

© UDS/CNRS

Contact