J/MNRAS/427/3374 QUEST RR Lyrae Survey III. Low Galactic latitude (Mateu+, 2012)

The QUEST RR Lyrae Survey. III. The low Galactic latitude catalogue. Mateu C., Vivas A.K., Downes J.J., Briceno C., Zinn R., Cruz-Diaz G. <Mon. Not. R. Astron. Soc., 427, 3374-3395 (2012)> =2012MNRAS.427.3374M 2012MNRAS.427.3374M
ADC_Keywords: Stars, variable; Positional data; Stars, distances ; Photometry Keywords: astronomical data bases: miscellaneous - surveys - stars: variables: RR Lyrae - Galaxy: stellar content - Galaxy: structure 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 Jurgen Stock Schmidt telescope at the National Observatory of Venezuela. The survey spans an area of 476deg2 on the sky, with multi-epoch observations in the V, R and I photometric bands for 6.5x106 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=18.5mag, and I=18.0mag. 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 ≳95 and ∼85 per cent for RRab and RRc stars, respectively. Photometric metallicities were computed based on the light curves and individual extinctions calculated from minimum light colours for each RRab star. Distances were obtained with typical errors ∼7 per cent. The RR Lyrae survey simultaneously spans a large range of heliocentric distances 0.5≤Rhel(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. Description: The present survey spans a total area of 476 deg2 and makes use of archive observations obtained between late 1998 and mid-2008 with the QUEST camera and the 1.0/1.5-m Jurgen Stock Schmidt telescope at the NOV in Llano del Hato, Venezuela. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 65 1877 Magnitudes for second-order photometric standards table6.dat 107 163 Light-curve parameters for RRab stars table7.dat 107 47 Light curve parameters for RRc stars table8.dat 47 160 Distances, colour excesses and metallicities for RRab stars -------------------------------------------------------------------------------- See also: II/296 : QUEST1 variability survey (QVS). III. (Rengstorf+, 2009) J/AJ/127/1158 : QUEST RR Lyrae Survey first catalog (Vivas+, 2004) J/AJ/132/714 : QUEST RR Lyrae survey. II. Halo overdensities (Vivas+, 2006) J/AJ/136/1645 : Spectroscopy of bright QUEST RR Lyrae stars (Vivas+, 2008) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- --- [ss] 3- 6 I4 --- ssID [4000/5876] Star designation (ssNNNN) 8- 17 F10.6 deg RAdeg Right ascension (J2000) 19- 26 F8.5 deg DEdeg Declination (J2000) 28- 33 F6.3 mag Vmag V magnitude 35- 39 F5.3 mag e_Vmag rms uncertainty on Vmag 41- 46 F6.3 mag Rmag R magnitude 48- 52 F5.3 mag e_Rmag rms uncertainty on Rmag 54- 59 F6.3 mag Imag I magnitude 61- 65 F5.3 mag e_Imag rms uncertainty on Imag -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID [3/1158] Star sequential number 6- 15 F10.6 deg RAdeg Right ascension (J2000) 17- 25 F9.6 deg DEdeg Declination (J2000) 27- 29 I3 --- NV [0/128] Number of observation in V band 31- 32 I2 --- NR [0/88] Number of observation in R band 34- 36 I3 --- NI [0/119] Number of observation in I band 38- 45 F8.6 d Per [0.2/0.9] Period 47- 50 F4.2 mag Vamp ?=- Amplitude in V band 52- 55 F4.2 mag Ramp ?=- Amplitude in R band 57- 60 F4.2 mag Iamp ?=- Amplitude in I band 62- 74 F13.8 d T0 Time of maximum light (HJD-2450000) 76- 80 F5.2 mag ?=- Mean V magnitude 82- 85 F4.2 mag e_ ?=- rms uncertainty on 87- 91 F5.2 mag ?=- Mean R magnitude 93- 96 F4.2 mag e_ ?=- rms uncertainty on 98-102 F5.2 mag ?=- Mean I magnitude 104-107 F4.2 mag e_ ?=- rms uncertainty on -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID Star sequential number 6- 9 F4.2 mag E(B-V) B-V colour excess 11- 14 F4.1 [Sun] [Fe/H] Metallicity 16- 18 F3.1 [Sun] e_[Fe/H] rms uncertainty on [Fe/H] 20- 23 F4.1 kpc Rh Heliocentric distance 25- 28 F4.1 kpc e_Rh rms uncertainty on Rh 30- 34 F5.1 kpc z Height above the plane 36- 38 F3.1 kpc e_z rms uncertainty on z 40- 43 F4.1 kpc Rg Radial distance projected on the Galactic plane 45- 47 F3.1 kpc e_Rg rms uncertainty on R -------------------------------------------------------------------------------- History: From electronic version of the journal References: Vivas et al., Paper I 2004AJ....127.1158V 2004AJ....127.1158V, Cat. J/AJ/127/1158 Vivas & Zinn, Paper II 2006AJ....132..714V 2006AJ....132..714V, Cat. J/AJ/132/714
(End) Patricia Vannier [CDS] 06-Sep-2013
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line