/ftp/cats/aliases/K/./KISS_3_



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J/AJ/127/1943       KISS Halpha survey list 2                (Gronwall+, 2004)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table2.dat table4.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AJ/127/1943
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drwxr-xr-x 76 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 294 Apr 7 2023 [TAR file] -rw-r--r-- 1 cats archive 482 Dec 19 2022 .message -r--r--r-- 1 cats archive 7213 Feb 20 2005 ReadMe -rw-r--r-- 1 cats archive 657 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2631 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 72683 Jul 2 2004 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 20952 Oct 25 2004 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/127/1943 KISS Halpha survey list 2 (Gronwall+, 2004) ================================================================================ The KPNO International Spectroscopic Survey. IV. Halpha-selected survey list 2. Gronwall C., Salzer J.J., Sarajedini V.L., Jangren A., Chomiuk L., Moody J.W., Frattare L.M., Boroson T.A. <Astron. J., 127, 1943-1958 (2004)> =2004AJ....127.1943G ================================================================================ ADC_Keywords: Surveys ; Galaxies, Seyfert ; Photometry, H-alpha Keywords: galaxies: Seyfert - galaxies: starburst - surveys Abstract: The KPNO International Spectroscopic Survey (KISS) is an objective-prism survey for extragalactic emission-line objects. It combines many of the features of previous slitless spectroscopic surveys with the advantages of modern CCD detectors and is the first purely digital objective-prism survey for emission-line galaxies. Here we present the second list of emission-line galaxy candidates selected from our red spectral data, which cover the wavelength range 6400 to 7200AA. In most cases, the detected emission line is Halpha. The current survey list covers a 1.6deg-wide strip located at delta=43deg30'(B1950) and spans the right ascension range 11h55m to 16h15m. The survey strip runs through the center of the Bootes void and has enough depth to adequately sample the far side of the void. An area of 65.8deg^2^ is covered. A total of 1029 candidate emission-line objects have been selected for inclusion in the survey list (15.6deg^-2^). We tabulate accurate coordinates and photometry for each source, as well as estimates of the redshift and emission-line flux and equivalent width based on measurements of the digital objective-prism spectra. The properties of the KISS emission-line galaxies are examined using the available observational data. Although the current survey covers only a modest fraction of the total volume of the Bootes void, we catalog at least 12 objects that appear to be located within the void. Only one of these objects has been recognized previously as a void galaxy. Description: All survey data were acquired using the 0.61 m Burrell Schmidt telescope.