/ftp/cats/II/320



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II/320              Variable stars in the M16-M17 field       (Maffei+ 1999)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat table2.dat table3.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/320
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 7 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 479 Dec 19 2022 .message drwxr-xr-x 2 cats archive 256 Jul 2 2013 Charts drwxr-xr-x 3 cats archive 8192 Sep 29 2013 Graphs -r--r--r-- 1 cats archive 6219 Nov 18 2013 ReadMe drwxr-xr-x 2 cats archive 76 Sep 29 2013 Tables -rw-r--r-- 1 cats archive 403 Jan 25 2019 +footg5.gif -rw-r--r-- 1 cats archive 2232 Jan 25 2019 +footg8.gif drwxr-xr-x 2 cats archive 256 Jul 2 2013 charts drwxr-xr-x 3 cats archive 8192 Sep 29 2013 graphs -r--r--r-- 1 cats archive 14008 Sep 11 2013 main.htm -r--r--r-- 1 cats archive 6179 Sep 11 2013 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 7189 Sep 11 2013 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 18218 Nov 18 2013 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 76 Sep 29 2013 tables
Beginning of ReadMe : II/320 Variable stars in the M16-M17 field (Maffei+ 1999) ================================================================================ Variable stars in the M16-M17 field: list, finding charts and Atlas of 176 Mira/SR light curves Maffei P., Tosti G. <Perugia University Observatory (1999) > =2013yCat.2320....0M ================================================================================ ADC_Keywords: Stars, variable ; Clusters, open ; Photometry, photographic Description: The original work was published as a paper book by the Perugia University in 1999. Before that, only the variable stars list (coordinates, classifications, periods, epochs, magnitude ranges) was published (P. Maffei, 1975IBVS..985....1M) The photographic material was discontinuously collected with the two Schmidt telescopes of the Asiago Observatory and with the Schmidt telescope of the Catania Astrophysical Observatory in the years 1961 to 1991. 103a-O without or with filter GG13 and hypersensitized with NH3 or pre-flashed I-N+RG5 were used. Date, JD, exposure time, emulsion/filter combination and the observer for each plate are listed in Table 1 and Table 2. The variable search was carried out with the blink microscope plate comparator of the Asiago Observatory. Details about the history and the reduction of the observational material are given in the "main.htm" file; the digitization was made by Alessandro Nesci.