J/ApJ/708/717       Light curve templates of RR Lyrae stars       (Sesar+, 2010)

Light curve templates and Galactic distribution of RR Lyrae stars from Sloan Digital Sky Survey stripe 82. Sesar B., Ivezic Z., Grammer S.H., Morgan D.P., Becker A.C., Juric M., De Lee N., Annis J., Beers T.C., Fan X., Lupton R.H., Gunn J.E., Knapp G.R., Jiang L., Jester S., Johnston D.E., Lampeitl H. <Astrophys. J., 708, 717-741 (2010)> =2010ApJ...708..717S 2010ApJ...708..717S
ADC_Keywords: Photometry, SDSS ; Stars, variable ; Stars, halo Keywords: Galaxy: halo - Galaxy: stellar content - Galaxy: structure - methods: data analysis - stars: horizontal-branch - stars: statistics - stars: variables: other Abstract: We present an improved analysis of halo substructure traced by RR Lyrae stars in the Sloan Digital Sky Survey (SDSS) stripe 82 region. With the addition of SDSS-II data, a revised selection method based on new ugriz light curve templates results in a sample of 483 RR Lyrae stars that is essentially free of contamination. The main result from our first study persists: the spatial distribution of halo stars at galactocentric distances 5-100kpc is highly inhomogeneous. At least 20% of halo stars within 30kpc from the Galactic center can be statistically associated with substructure. We present strong direct evidence, based on both RR Lyrae stars and main-sequence stars, that the halo stellar number density profile significantly steepens beyond a Galactocentric distance of ∼30kpc, and a larger fraction of the stars are associated with substructure. By using a novel method that simultaneously combines data for RR Lyrae and main-sequence stars, and using photometric metallicity estimates for main-sequence stars derived from deep co-added u-band data, we measure the metallicity of the Sagittarius dSph tidal stream (trailing arm) toward RA∼2h-3h and DE∼0° to be 0.3dex higher ([Fe/H]=-1.2) than that of surrounding halo field stars. Description: We have combined SDSS-I imaging runs used in Sesar et al. (2007AJ....134.2236S 2007AJ....134.2236S) with recalibrated SDSS-II SN (Frieman et al. 2008AJ....135..338F 2008AJ....135..338F) imaging runs, and created a catalog with ∼4.4 million unique unresolved (point source) objects. Each object in the catalog was observed at least four times in the ugr bands. We selected 483 RR Lyrae stars in SDSS stripe 82. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 295 483 Light curve parameters for stripe 82 RR Lyrae stars table3.dat 115 483 Positions and derived parameters of stripe 82 RR Lyrae stars phot/* . 483 *Position and ugriz photometry for each star templ/* . 98 *Individual files for ugriz RR Lyrae template light curves -------------------------------------------------------------------------------- Notes on phot/*: This directory contains positions and ugriz photometry for 483 stripe 82 RR Lyrae stars. The filenames correspond to RR Lyrae ID numbers in Tables 2 and 3. Notes on templ/*: This directory contains ugriz RR Lyrae template light curves. The number in the filename corresponds to the template ID in Table 2 and the letter identifies the band. -------------------------------------------------------------------------------- See also: II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) J/A+A/526/A28 : SDSS-II supernovae NTT and NOT spectroscopy (Oestman+, 2011) J/ApJS/186/233 : Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010) J/AJ/130/1640 : Photometry of candidate RR Lyrae stars in the SDSS (Wu+, 2005) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- [SIG2010] RR Lyrae identification number 9- 10 A2 --- Type [abc ] RR Lyrae type 12- 25 F14.12 d Per Period 27- 40 F14.12 mag uAmp Best-fit template u band amplitude 42- 56 F15.12 mag umag1 Best-fit template u band maximum brightness (1) 58- 75 F18.12 d T0.u Best-fit template u band epoch of maximum brightness (MJD) 77- 79 I3 --- Tu Best-fit template u band ID number 81- 94 F14.12 mag gAmp Best-fit template g band amplitude 96-110 F15.12 mag gmag1 Best-fit template g band maximum brightness (1) 112-129 F18.12 d T0.g Best-fit template g band epoch of maximum brightness (MJD) 131-133 I3 --- Tg Best-fit template g band ID number 135-148 F14.12 mag rAmp Best-fit template r band amplitude 150-164 F15.12 mag rmag1 Best-fit template r band maximum brightness (1) 166-183 F18.12 d T0.r Best-fit template r band epoch of maximum brightness (MJD) 185-187 I3 --- Tr Best-fit template r band ID number 189-202 F14.12 mag iAmp Best-fit template i band amplitude 204-218 F15.12 mag imag1 Best-fit template i band maximum brightness (1) 220-237 F18.12 d T0.i Best-fit template i band epoch of maximum brightness (MJD) 239-241 I3 --- Ti Best-fit template i band ID number 243-256 F14.12 mag zAmp Best-fit template z band amplitude 258-272 F15.12 mag zmag1 Best-fit template z band maximum brightness (1) 274-291 F18.12 d T0.z Best-fit template z band epoch of maximum brightness (MJD) 293-295 I3 --- Tz Best-fit template z band ID number -------------------------------------------------------------------------------- Note (1): Corrected for the ISM extinction. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- [SIG2010] RR Lyrae identification number 9- 18 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 20- 28 F9.6 deg DEdeg Declination in decimal degrees (J2000) 30- 34 F5.3 mag Ar Schlegel et al. 1998ApJ...500..525S 1998ApJ...500..525S ISM extinction in r band 36- 41 F6.2 kpc Dist Heliocentric distance 43- 48 F6.2 kpc RGC Galactocentric distance 50- 55 F6.3 mag umag Flux-averaged u band magnitude (1) 57- 62 F6.3 mag gmag Flux-averaged g band magnitude (1) 64- 69 F6.3 mag rmag Flux-averaged r band magnitude (1) 71- 76 F6.3 mag imag Flux-averaged i band magnitude (1) 78- 83 F6.3 mag zmag Flux-averaged z band magnitude (1) 85- 90 F6.3 mag Vmag Flux-averaged V band magnitude (1) 92- 96 F5.3 mag u-g Median (u-g) color at minimum brightness (1) 98-102 F5.3 mag e_u-g Uncertainty in u-g 104-109 F6.3 mag g-r Median (g-r) color at minimum brightness (1) 111-115 F5.3 mag e_g-r Uncertainty in g-r -------------------------------------------------------------------------------- Note (1): Corrected for ISM extinction. -------------------------------------------------------------------------------- Byte-by-byte Description of files: phot/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.6 deg RAdeg [-51.99/59.25] Right Ascension in decimal degrees (J2000) 12- 20 F9.6 deg DEdeg Declination in decimal degrees (J2000) 22- 33 F12.6 d JDu Modified Julian date of u band observation 35- 41 F7.3 mag umag ?=-99.99 u band magnitude (1) 43- 49 F7.3 mag e_umag ?=-99 u band magnitude error 51- 62 F12.6 d JDg Modified Julian date of g band observation 64- 70 F7.3 mag gmag ?=-99.99 g band magnitude (1) 72- 78 F7.3 mag e_gmag ?=-99 g band magnitude error 80- 91 F12.6 d JDr Modified Julian date of r band observation 93- 99 F7.3 mag rmag ?=-99.99 r band magnitude (1) 101-107 F7.3 mag e_rmag ?=-99 r band magnitude error 109-120 F12.6 d JDi Modified Julian date of i band observation 122-128 F7.3 mag imag ?=-99.99 i band magnitude (1) 130-136 F7.3 mag e_imag ?=-99 i band magnitude error 138-149 F12.6 d JDz Modified Julian date of z band observation 151-157 F7.3 mag zmag ?=-99.99 z band magnitude (1) 159-165 F7.3 mag e_zmag ?=-99 z band magnitude error -------------------------------------------------------------------------------- Note (1): Not corrected for ISM extinction. -------------------------------------------------------------------------------- Byte-by-byte Description of files: templ/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 F5.3 --- phase Template light curve phase 7- 11 F5.3 --- value Template value -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 13-Feb-2012
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