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 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 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. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file main.htm 958 125 The electronic paper (copy of the original atlas) table1.dat 50 128 List of the blue plates table2.dat 50 149 List of the infrared plates table3.dat 88 210 Principal elements of the variables in the field of M16-M17 charts/* . 10 Finding charts graphs/* . 189 Images of the light curves tables/* . 3 Original tables -------------------------------------------------------------------------------- See also: B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013) http://astrowww.phys.uniroma1.it/nesci/MIRA/All/main.htm : Original atlas Byte-by-byte Description of file: table1.dat table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Tel [12CJI] Telescope used (1) 3- 7 I5 --- ID Plate ID 9- 18 A10 "YYYY.MM.DD" Date Observation date 20- 29 F10.4 d JD Observation date (JD-2400000) 31- 32 I2 min texp Exposure time 34- 45 A12 --- Em/Filter Plate, emulsion and filter 47- 50 A4 --- Obs Observer code (2) -------------------------------------------------------------------------------- Note (1): The following telescope codes are used: 1 = Asiago Astrophysical observatory- Schmidt 50/40 2 = Asiago Astrophysical observatory- Schmidt 90/65 C = Catania Astrophysical observatory- Schmidt 61/41 J = UKSTU blue plate I = UKSTU infra-red plate Note (2): Observers are abbreviated as follows: B = Assia Blaghikh Br = Roberto Burchi C = Salvatore Cristaldi F = Aldo Frigo M = Paolo Maffei Mt = Aldo Martini N = Giuliano Natali P = Valerio Pertile R = Lucio Rossi IR = Italo Rigoni; S = Antonello Satta Sc = Vincenzo Stancanelli T = Luciano Traverso V = Roberto Viotti -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- --- [M] 2- 4 I03 --- Seq [1/208]? (empty for previously known stars) 9- 17 A9 --- Name Variable star name 25- 26 I2 h RAh ? Right Ascension B1950 (hours) 28- 29 I2 min RAm ? Right Ascension B1950 (minutes) 31- 32 I2 s RAs ? Right Ascension B1950 (seconds) 34 A1 --- DE- ? Declination B1950 (sign) 35- 36 I2 deg DEd ? Declination B1950 (degrees) 38- 41 F4.1 arcmin DEm ? Declination B1950 (minutes) 45 A1 --- f_bmax [B] specifies that bmax and bmin are also observed in B-band 46- 50 F5.2 mag bmax ? I-band magnitude at maximum brightness 53 A1 --- l_bmin [<] indicates bmin is a lower value of magnitude 54- 58 F5.2 mag bmin ? I-band magnitude at minimum brightness 62- 66 A5 --- Vt Variable type (includes : for uncertain values) 70- 74 F5.1 d Per ? Period 75- 76 A2 --- u_Per [: ] Uncertainty flag on Per 78- 82 I5 d T0 ? Epoch of maximum brightness (JD-2400000) 83- 84 A2 --- u_T0 [: ] Uncertainty flag on T0 86- 88 I3 --- Nobs ? Number of observations -------------------------------------------------------------------------------- History: * 02-Jul-2013: Copied from http://astrowww.phys.uniroma1.it/nesci/MIRA/All/ * 30-Sep-2013: two incorrect names have been corrected, in the table3 and the light curves: - M023 corrected from V3954 into V3945 Sgr - M113 corrected from NSV 10732 into NSV 10752 (=V5536 Sgr) * 18-Nov-2013: the positions of V3917 Sgr (=V404 Ser) and HH Ser were corrected (from Prof. Roberto Nesci) Acknowledgements: The material was kindly supplied by Roberto Nesci; the digitization was made by Alessandro Nesci.
(End) Francois Ochsenbein [CDS] 02-Jul-2013
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