/ftp/cats/J_AN/326/321



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J/AN/326/321  Absolute magnitudes for late-type dwarfs    (Bilir+, 2005)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/AN/326/321
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drwxr-xr-x 4 cats root 55 Jan 29 2012 [Up] drwxr-xr-x 2 cats root 4096 Dec 15 2013 [TAR file] -rw-r--r-- 1 cats archive 460 Nov 28 2007 .message -rw-r--r-- 1 cats archive 3800 Nov 28 2007 ReadMe -rw-r--r-- 1 cats archive 608 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 3109 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 42425 Jul 15 2005 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AN/326/321 Absolute magnitudes for late-type dwarfs (Bilir+, 2005) ================================================================================ Absolute magnitudes for late-type dwarf stars for Sloan photometry. Bilir S., Karaali S., Tuncel S. <Astronomische Nachrichten, 326, 321-331 (2005)> =2005AN....326..321B ================================================================================ ADC_Keywords: Stars, late-type ; Photometry, ugriz ; Photometry, UBVRI ; Photometry, Cousins ; Magnitudes, absolute Keywords: techniques: Sloan photometry - stars: distances - stars: luminosity function Abstract: We present a new formula for absolute magnitude determination for late-type dwarf stars as a function of (g-r) and (r-i) for Sloan photometry (as defined by Abazajian et al., 2003AJ....126.2081A). The absolute magnitudes estimated by this approach are brighter than those estimated by colour-magnitude diagrams, and they reduce the luminosity function rather close to the luminosity function of Hipparcos.

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