/ftp/cats/J_other/PASP/126/616



==========================================================================
J/PASP/126/616    Variable stars in Leo I dSph               (Stetson+, 2014)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat table2.dat table3.dat table4.dat table5.dat
==========================================================================
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/PASP/126/616
==========================================================================

drwxr-xr-x 9 cats archive 186 Sep 15 2017 [Up] drwxr-xr-x 4 cats archive 4096 May 26 2021 [TAR file] -rw-r--r-- 1 cats archive 508 Jan 6 2016 .message -r--r--r-- 1 cats archive 10459 Jan 6 2016 ReadMe -rw-r--r-- 1 cats archive 1013 Jan 6 2016 +footg5.gif -rw-r--r-- 1 cats archive 2988 Jan 6 2016 +footg8.gif -r--r--r-- 1 cats archive 3848 Dec 22 2014 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 15744 Jan 6 2016 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 5610 Nov 12 2014 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1558 Nov 12 2014 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 689 Nov 12 2014 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/PASP/126/616 Variable stars in Leo I dSph (Stetson+, 2014) ================================================================================ Homogeneous photometry. VI: Variable stars in the Leo I dwarf spheroidal galaxy. Stetson P.B., Fiorentino G., Bono G., Bernard E.J., Monelli M., Iannicola G., Gallart C., Ferraro I. <Publ. Astron. Soc. Pac., 126, 616-641 (2014)> =2014PASP..126..616S ================================================================================ ADC_Keywords: Galaxies, nearby ; Stars, variable ; Photometry, UBVRI Keywords: Stars Abstract: From archival ground-based images of the Leo I dwarf spheroidal galaxy, we have identified and characterized the pulsation properties of 164 candidate RR Lyrae variables and 55 candidate anomalous and/or short-period Cepheids. We have also identified 19 candidate long-period variable stars and 13 other candidate variables whose physical nature is unclear, but due to the limitations of our observational material we are unable to estimate reliable periods for them. Description: The observational material for this study consists of 1884 individual CCD images obtained on 48 nights during 32 observing runs. These data are contained within a much larger data collection ( 400000 images,  500 observing runs) compiled and maintained by the first author.

© Université de Strasbourg/CNRS

    • Contact