J/MNRAS/466/163     Candidate Halpha sources in GBS              (Wevers+, 2017)
Candidate Halpha emission and absorption line sources in the
Galactic Bulge Survey.
    Wevers T., Jonker P.G., Nelemans G.,  Torres M.A.P., Groot P.J., Steeghs D.,
    Maccarone T.J., Hynes R.I., Heinke C., Britt C.
    <Mon. Not. R. Astron. Soc. 466, 163-173 (2017)>
    =2017MNRAS.466..163W 2017MNRAS.466..163W        (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Stars, emission ; Photometry, SDSS ; Photometry, H-alpha
Keywords: Galaxy: bulge - stars: emission line - cataclysmic variables -
          binaries: symbiotic - white dwarfs - galaxies: active
Abstract:
    We present a catalogue of candidate Halpha emission and absorption
    line sources and blue objects in the Galactic Bulge Survey (GBS)
    region. We use a point source catalogue of the GBS fields (two strips
    of (lxb)=(6°x1°) centred at b=1.5° above and below the
    Galactic centre), covering the magnitude range 16≥r'≥22.5. We
    utilize (r'-i', r'-Halpha) colour-colour diagrams to select Halpha
    emission and absorption line candidates, and also identify blue
    objects (compared to field stars) using the r'-i' colour index.
    We identify 1337 Halpha emission line candidates and 336 Halpha
    absorption line candidates. These catalogues likely contain a plethora
    of sources, ranging from active (binary) stars, early-type emission
    line objects, cataclysmic variables (CVs) and low-mass X-ray binaries
    (LMXBs) to background active galactic nuclei (AGN). The 389 blue
    objects we identify are likely systems containing a compact object,
    such as CVs, planetary nebulae and LMXBs. Hot subluminous dwarfs
    (sdO/B stars) are also expected to be found as blue outliers.
    Crossmatching our outliers with the GBS X-ray catalogue yields sixteen
    sources, including seven (magnetic) CVs and one qLMXB candidate among
    the emission line candidates, and one background AGN for the
    absorption line candidates. One of the blue outliers is a high state
    AM CVn system. Spectroscopic observations combined with the
    multi-wavelength coverage of this area, including X-ray, ultraviolet
    and (time-resolved) optical and infrared observations, can be used to
    further constrain the nature of individual sources.
Description:
    We use optical photometry in three filters (r', i' and Halpha to
    create (r'-i', r'-Halpha) colour-colour diagrams of point sources in
    the Galactic Bulge Survey Fields (Jonker et al., 2011, Cat.
    J/ApJS/194/18; 2014, Cat. J/ApJS/210/18; Wevers et al. 2016, Cat.
    J/MNRAS/458/4530).
    We identify 1337 emission line candidates, 336 absorption line
    candidates, and 389 blue outliers in the catalogue. These samples
    likely contain a plethora of sources, ranging from chromospherically
    active stars, subluminous hot dwarfs, white dwarfs, CVs, planetary
    nebulae, LMXBs and variable stars to background AGN.
File Summary:
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 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
absorber.dat      73      336   Absorption line sources
bluesrc.dat       73      389   Blue sources
emitters.dat      73     1337   Emission line sources
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See also:
 J/ApJS/194/18    : Galactic Bulge Survey: X-ray observations (Jonker+, 2011)
 J/ApJS/210/18    : X-ray survey of the Galactic Bulge (CXOGBS) (Jonker+, 2014)
 J/MNRAS/458/4530 : Chandra Galactic Bulge Survey (Wevers+, 2016)
Byte-by-byte Description of file: absorber.dat bluesrc.dat emitters.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  4  I4    ---     ID        Object number of the field on which the source
                                   was detected (1)
       6  I1    ---     CCD       [1/8] CCD number (i.e. detector) on which
                                   the source was detected (2)
   8- 17  F10.6 deg     RAdeg     Right ascension of the source (J2000)
  19- 28  F10.6 deg     DEdeg     Declination of the source (J2000)
  30- 34  F5.2  mag     r'mag     r'-band magnitude of the source in
                                   Vega magnitudes
  36- 39  F4.2  mag   e_r'mag     Measurement error of the r-band magnitude
  41- 45  F5.2  mag     i'mag     i'-band magnitude of the source in
                                   Vega magnitudes
  47- 50  F4.2  mag   e_i'mag     Measurement error of the i-band magnitude
  52- 56  F5.2  mag     Hamag     Halpha-band magnitude of the source in
                                   Vega magnitudes
  58- 61  F4.2  mag   e_Hamag     Measurement error of the Halpha-band magnitude
  63- 67  F5.2  mag     r'-i'     r'-i' colour index of the source
                                   (difference of r'mag and i'mag)
  69- 73  F5.2  mag     r'-Ha     r'-Halpha colour index of the source
                                   (difference of r'mag and Hamag)
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Note (1): can be used to trace back the image on which the source was found.
  Example: value 53 refers to npobj053catmercat.fits in the
  catalogue J/MNRAS/458/4530
  Example: value 118 refers to npobj118catmercat.fits in the
  catalogue J/MNRAS/458/4530
Note (2): can be used to trace back the image on which the source was found.
  Values range from 1-8, since there are 8 detectors in the instrument used.
  Example: value 3 refers to CCD 3 of the corresponding field of Column 1 in
  the fits catalogue files of catalogue J/MNRAS/458/4530.
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Acknowledgements:
   Thomas Wevers, t.wevers(at)astro.ru.nl
(End)                                        Patricia Vannier [CDS]  05-Jan-2017