The IPHAS-POSS-I proper motion survey of the Galactic Plane
arXiv:0905.2594 · doi:10.1111/j.1365-2966.2009.15077.x
Abstract
We present a proper motion survey of the Galactic plane, using IPHAS data and POSS-I Schmidt plate data as a first epoch, that probes down to proper motions below 50 milliarcseconds per year. The IPHAS survey covers the northern plane () with CCD photometry in the , and H passbands. We examine roughly 1400 sq. deg. of the IPHAS survey area and draw up a catalogue containing 103058 objects with significant proper motions below 150 millarcseconds per year in the magnitude range 13.519. Our survey sample contains large samples of white dwarfs and subdwarfs which can be identified using a reduced proper motion diagram. We also found several objects with IPHAS colours suggesting H emission and significant proper motions. One is the known cataclysmic variable GD552; two are known DB white dwarfs and five others are found to be non-DA (DB and DC) white dwarfs, which were included in the H emission line catalogue due to their lack of absorption in the H narrow-band.
18 pages, 9 figures, MNRAS accepted, catalogue available at http://www.astro.ru.nl/~ndeacon/catalogues/
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Cited by in corpus (9)
- The Solar Neighborhood XXXV: Distances to 1404 M Dwarf Systems Within 25 pc in the Southern Sky
- The UV-Excess Survey of the Northern Galactic Plane (UVEX)
- The Most Massive White Dwarfs in the Solar Neighborhood
- A first catalogue of automatically selected UV-excess sources from the UVEX survey
- The Solar Neighborhood XXV: Discovery of New Proper Motion Stars with 0.40 "/yr > mu > 0.18 "/yr between Declinations -47 degrees and 00 degrees
- UCAC3 Proper Motion Survey. I. Discovery of New Proper Motion Stars in UCAC3 with 0.40 "/yr > mu >= 0.18 "/yr between Declinations -90 deg and -47 deg
- Spectroscopic follow-up of UV-excess objects selected from the UVEX survey
- UCAC3 Proper Motion Survey. II. Discovery Of New Proper Motion Stars In UCAC3 With 0.40" yr^-1 > mu >= 0.18" yr^-1 Between Declinations -47 deg and 00 deg
- UV-excess sources with a red/IR-counterpart: low-mass companions, debris disks and QSO selection