The QUEST RR Lyrae Survey – III. The low Galactic latitude catalogue
dc.contributor.author | Mateu, C. | en_US |
dc.contributor.author | Vivas, A. K. | en_US |
dc.contributor.author | Downes, J. J. | en_US |
dc.contributor.author | Briceño, C. | en_US |
dc.contributor.author | Zinn, R. | en_US |
dc.contributor.author | Cruz‐diaz, G. | en_US |
dc.date.accessioned | 2013-01-03T19:46:52Z | |
dc.date.available | 2014-01-07T14:51:07Z | en_US |
dc.date.issued | 2012-12-21 | en_US |
dc.identifier.citation | Mateu, C.; Vivas, A. K.; Downes, J. J.; Briceño, C. ; Zinn, R.; Cruz‐diaz, G. (2012). "The QUEST RR Lyrae Survey â III. The low Galactic latitude catalogue." Monthly Notices of the Royal Astronomical Society 427(4): 3374-3395. <http://hdl.handle.net/2027.42/95669> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/95669 | |
dc.description.abstract | We present results for the QUEST RR Lyrae Survey at low Galactic latitude, conducted entirely with observations obtained with the QUEST mosaic camera and the 1.0/1.5‐m Jürgen Stock Schmidt telescope at the National Observatory of Venezuela. The survey spans an area of 476 deg 2 on the sky, with multi‐epoch observations in the V , R and I photometric bands for 6.5 × 10 6 stars in the Galactic latitude range −30° ≤ b ≤ +25°, in a direction close to the Galactic anticentre 190° ≤ l ≤ 230°. The variability survey has a typical number of 30 observations per object in V and I and ∼25 in R , with up to ∼120–150 epochs in V and I and up to ∼100 in R in the best sampled regions. The completeness magnitudes of the survey are V = R = 18.5 mag, and I = 18.0 mag. We identified 211 RR Lyrae stars, 160 bona fide stars of type ab and 51 candidates of type c , ours being the first deep RR Lyrae survey conducted at low Galactic latitude, in the Galactic disc. The completeness of the RR Lyrae survey was estimated in > rsim 95 and ∼85 per cent for RR ab and RR c stars, respectively. Photometric metallicities were computed based on the light curves and individual extinctions calculated from minimum light colours for each RR ab star. Distances were obtained with typical errors ∼ 7 per cent. The RR Lyrae survey simultaneously spans a large range of heliocentric distances 0.5 ≤ R hel (kpc) ≤ 40 and heights above the plane −15 ≤ z (kpc) ≤ +20, with well‐known completeness across the survey area, making it an ideal set for studying the structure of the Galactic thick disc. | en_US |
dc.publisher | Am. Inst. Phys. | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Surveys | en_US |
dc.subject.other | Astronomical Data Bases: Miscellaneous | en_US |
dc.subject.other | Stars: Variables: RR Lyrae | en_US |
dc.subject.other | Galaxy: Stellar Content | en_US |
dc.subject.other | Galaxy: Structure | en_US |
dc.title | The QUEST RR Lyrae Survey – III. The low Galactic latitude catalogue | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/95669/1/mnr21968.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2012.21968.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
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