J/AcA/67/297    OGLE Galactic center Cepheids and RR Lyrae   (Soszynski+, 2017)
The OGLE Collection of Variable Stars.
Classical, Type II, and Anomalous Cepheids toward the Galactic Center.
    Soszynski I., Udalski A., Szymanski M.K., Wyrzykowski L., Ulaczyk K.,
    Poleski R., Pietrukowicz P., Kozlowski S., Skowron D.M., Skowron J.,
    Mroz P., Pawlak M., Rybicki K., Jacyszyn-Dobrzeniecka A.
   <Acta Astron. 67, 297-316 (2017)>
   =2017AcA....67..297S 2017AcA....67..297S    (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Milky Way ; Stars, variable
Keywords: stars: variables: Cepheids - stars: variables: RR Lyrae -
          stars: oscillations - Galaxy: center - Catalogs
Abstract:
    We present a collection of classical, type II, and anomalous Cepheids
    detected in the OGLE fields toward the Galactic center. The sample
    contains 87 classical Cepheids pulsating in one, two or three radial
    modes, 924 type II Cepheids divided into BL Her, W Vir, peculiar W
    Vir, and RV Tau stars, and 20 anomalous Cepheids - first such
    objects found in the Galactic bulge. Additionally, we upgrade the OGLE
    Collection of RR Lyr stars in the Galactic bulge by adding 828 newly
    identified variables. For all Cepheids and RR Lyr stars, we publish
    time-series VI photometry obtained during the OGLE-IV project, from
    2010 through 2017.
    We discuss basic properties of our classical pulsators: their spatial
    distribution, light curve morphology, period-luminosity relations,
    and position in the Petersen diagram. We present the most interesting
    individual objects in our collection: a type II Cepheid with
    additional eclipsing modulation, W Vir stars with the period
    doubling effect and the RVb phenomenon, a mode-switching RR Lyr star,
    and a triple-mode anomalous RRd star.
Description:
    The OGLE-IV data set used in this investigation was obtained between
    March 2010 and August 2017 with the 1.3-m Warsaw telescope located at
    Las Campanas Observatory, Chile (operated by the Carnegie Institution
    for Science). A mosaic camera composed of 32 CCD chips with
    Johnson-Cousins VI filters was used, providing a field of view of
    1.4 square degrees with a pixel scale of 0.26". Details of the
    instrument can be found in Udalski et al. (2015AcA....65....1U 2015AcA....65....1U).
    In total, 121 OGLE-IV fields toward the Galactic center were searched
    for classical pulsating stars.
File Summary:
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 FileName     Lrecl  Records   Explanations
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ReadMe           80        .   This file
table1.dat       36       32   Reclassified stars from the OGLE-III Catalog
                                of Variable Stars in the Galactic bulge
ident.dat       133    40112   Identification of stars
cep.dat         236       87   Parameters of Cepheids (fundamental-mode F,
                                first-overtone 1O, double-mode F/1O,
                                double-mode 1O/2O and triple-mode 1O/2O/3O)
t2cep.dat       113      924   Parameters of type II Cepheids
acep.dat        113       27   Parameters of fundamental-mode (F) and
                                first-overtone (F/1O) anomalous Cepheids
rrlyr.dat       181    39074   Parameters of RRab, RRc, RRd and aRRd  stars
remarks.dat      92      163   Remarks
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See also:
       II/323 : OGLE-III Bulge Photometric Catalog (Szymanski+ 2011)
 J/AcA/63/115 : OGLE-III Galactic disk eclipsing binaries (Pietrukowicz+, 2013)
 J/AcA/63/135 : New OGLEIII dwarf novae in Galactic disk (Mroz+, 2013)
 J/AcA/63/379 : OGLE-III variable stars in Galactic disk area (Pietrukowicz+, 2
 J/AcA/64/177 : VI light curves of Galactic Bulge RR Lyrae (Soszynski+, 2014)
 J/AcA/66/433 : Gaia DR1 and OGLE variable stars (Udalski+, 2016)
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label     Explanations
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   1-  9  A9    ---     ---       [OGLE-BLG-]
  10- 20  A11   ---     Star      Star's ID (CEP-NNN T2CEP-NNN RRLYR-NNNNN) (G1)
  22- 36  A15   ---     Class     New classification
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Byte-by-byte Description of file: ident.dat
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   Bytes Format Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  5  A5    ---     Class    Classification (CEP T2CEP ACEP RRLYR)
   8- 16  A9    ---     ---      [OGLE-BLG- OGLE-GAL-]
  17- 27  A11   ---     Star     Star's ID (G1)
  29- 36  A8    ---     Mode     Mode(s) of pulsation for Cepheids or
                                  subtype of RR Lyrae (RRab, RRc, RRd, aRRd) (1)
  39- 40  I2    h       RAh      Right ascension (J2000.0)
  42- 43  I2    min     RAm      Right ascension (J2000.0)
  45- 49  F5.2  s       RAs      Right ascension (J2000.0)
      51  A1    ---     DE-      Declination sign (J2000.0)
  52- 53  I2    deg     DEd      Declination (J2000.0)
  55- 56  I2    arcmin  DEm      Declination (J2000.0)
  58- 61  F4.1  arcsec  DEs      Declination (J2000.0)
  64- 79  A16   ---     OGLE-IV  OGLE-IV ID
  81- 95  A15   ---     OGLE-III OGLE-III ID
  97-111  A15   ---     OGLE-II  OGLE-II ID
 113-133  A21   ---     OName    Other designation (from VSX)
--------------------------------------------------------------------------------
Note (1): Mode of pulsation as follows:
           F        = fundamental-mode F
           1O       = first-overtone 1O
           F/1O     = double-mode F/1O
           1O/2O    = double-mode 1O/20
           1O/2O/3O = triple-mode 10/20/30
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Byte-by-byte Description of file: cep.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     ---       [OGLE-BLG-]
  10- 16  A7    ---     Star      Star's ID (CEP-NNN) (G1)
  18- 23  A6    ---     Type      Cepheid Type
  25- 30  F6.3  mag     <Imag>    Intensity mean I-band magnitude
  32- 37  F6.3  mag     <Vmag>    ?=- Intensity mean V-band magnitude
  40- 49  F10.7 d       Per       Period or longest period for double-mode
  51- 59  F9.7  d     e_Per       Uncertainty of the longest period
  62- 71  F10.5 d       T0        Time of maximum brightness (HJD-2450000)
  74- 78  F5.3  mag     Iamp      I-band amplitude (maximum-minimum)
  81- 85  F5.3  ---     R21       Fourier coefficient R_21
  87- 91  F5.3  ---     phi21     ?=- Fourier coefficient phi_21
  94- 98  F5.3  ---     R31       Fourier coefficient R_31
 100-104  F5.3  ---     phi31     ?=- Fourier coefficient phi_31
 106-115  F10.7 d       PerM      ? Medium period for triple_mode
 117-125  F9.7  d     e_PerM      ? Uncertainty of the medium period
 128-137  F10.5 d       T0M       ? Time of maximum brightness (HJD-2450000)
 140-144  F5.3  mag     IampM     ? I-band amplitude (maximum-minimum)
 147-151  F5.3  ---     R21M      ? Fourier coefficient R21
 153-157  F5.3  ---     phi21M    ?=- Fourier coefficient phi21
 160-164  F5.3  ---     R31M      ? Fourier coefficient R31
 166-170  F5.3  ---     phi31M    ?=- Fourier coefficient phi31
 172-181  F10.7 d       PerS      ? Shortest period for double and
                                   triple mode
 183-191  F9.7  d     e_PerS      ? Uncertainty of the shortest period
 194-203  F10.5 d       T0S       ? Time of maximum brightness (HJD-2450000)
 206-210  F5.3  mag     IampS     ? I-band amplitude (maximum-minimum)
 213-217  F5.3  ---     R21S      ? Fourier coefficient R21
 219-223  F5.3  ---     phi21S    ?=- Fourier coefficient phi21
 226-230  F5.3  ---     R31S      ? Fourier coefficient R31
 232-236  F5.3  ---     phi31S    ?=- Fourier coefficient phi31
-------------------------------------------------------------------------------
Byte-by-byte Description of file: t2cep.dat acep.dat rrlyr.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     ---       [OGLE-BLG- OGLE-GAL-]
  10- 20  A11   ---     Star      Star's ID 
                                   (T2CEP-NNN, ACEP-NNN, RRLYR-NNNNN) (G1)
  22- 29  A8    ---     Type      Type of Cepheids or subtype of RR Lyrae (1)
  32- 37  F6.3  mag     <Imag>    Intensity mean I-band magnitude
  39- 44  F6.3  mag     <Vmag>    ?=- Intensity mean V-band magnitude
  47- 57  F11.8 d       Per       First-overtone period
  59- 68  F10.8 d     e_Per       Uncertainty of first-overtone period
  71- 80  F10.5 d       T0        Time of maximum brightness (HJD-2450000)
  83- 87  F5.3  mag     Iamp      I-band amplitude (maximum-minimum)
  90- 94  F5.3  ---     R21       Fourier coefficient R_21
  96-100  F5.3  ---     phi21     ?=- Fourier coefficient phi21
 103-107  F5.3  ---     R31       Fourier coefficient R31
 109-113  F5.3  ---     phi31     ?=- Fourier coefficient phi31
 116-125  F10.8 d       Per.0     ? Fundamental-mode period
 127-136  F10.8 d     e_Per.0     ? Uncertainty of fundamental-mode period
 139-148  F10.5 d       T0.0      ? Time of maximum brightness (HJD-2450000)
 151-155  F5.3  mag     Iamp.0    ? I-band amplitude (maximum-minimum)
 158-162  F5.3  ---     R21.0     ? R21 Fourier coefficient R21
 164-168  F5.3  ---     phi21.0   ?=- phi21 Fourier coefficient phi21
 171-175  F5.3  ---     R31.0     ? R31 Fourier coefficient R31
 177-181  F5.3  ---     phi31.0   ?=- phi31 Fourier coefficient phi31
--------------------------------------------------------------------------------
Note (1): Mode as follows:
   Type II = Type II Cepheid (t2cep.dat)
   F       = fundamental-mode anomalous Cepheid (acep.dat)
   1O      = first-overtone anomalous Cepheid (acep.dat)
   RRab    = RRab RR lyrae (rrlyr.dat)
   RRc     = RRc RR lyrae (rrlyr.dat)
   RRd     = RRd RR lyrae (rrlyr.dat)
   aRRd    = aRRd RR lyrae (rrlyr.dat)
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Byte-by-byte Description of file: remarks.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     ---       [OGLE-BLG- OGLE-GAL-]
  10- 20  A11   ---     Star      Star's ID (G1)
  22- 93  A72   ---     Rem       Remark
--------------------------------------------------------------------------------
Global notes:
Note (G1): Names as:
   CEP-NNN for Cepheids (OGLE-BLG-CEP-NNN)
   T2CEP-NNN for type II Cepheids (OGLE-BLG-T2CEP-NNN)
   ACEP-NNN for anomalous Cepheids (OGLE-GAL-ACEP-NNN)
   RRLYR-NNNNN for RR Lyrae (OGLE-BLG-RRLYR-NNNNN)
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History:
   Copied at:
   ftp://ftp.astrouw.edu.pl/ogle/ogle4/OCVS/blg/cep/
   ftp://ftp.astrouw.edu.pl/ogle/ogle4/OCVS/blg/t2cep/
   ftp://ftp.astrouw.edu.pl/ogle/ogle4/OCVS/gal/acep/
   ftp://ftp.astrouw.edu.pl/ogle/ogle4/OCVS/blg/rrlyr/
(End)                                      Patricia Vannier [CDS]    05-Sep-2018