J/AJ/115/193        RR Lyrae V light curves                    (Layden, 1998)

RR Lyrae variables in the inner halo. I. Photometry. Layden A.C. <Astron. J. 115, 193 (1998)> =1998AJ....115..193L 1998AJ....115..193L (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Photometry, CCD Keywords: Galaxy: halo - Galaxy: stellar content - stars: distances - stars: Population II - stars: variables: other Abstract: I present V-band CCD photometry for a sample of 103 RR Lyrae variables selected from the General Catalogue of Variable Stars to lie in the inner halo of the Galaxy. I also describe a method for obtaining the mean apparent magnitude and the epoch at maximum light of an RR Lyrae star. The method requires as few as five photometric observations, and simulations demonstrate that the associated errors are relatively small. I employ this method to derive the mean magnitudes and maximum light epochs of the 103 RR Lyrae stars observed. These stars were selected, based on their Galactic coordinates and original photographic photometry, to lie near their orbital tangent points, thus providing a sample well suited for measuring the rotational kinematics of the inner halo. Using interstellar reddenings from the literature and the observed mean V magnitudes, I derive distances for these stars and show that their actual locations in the Galaxy are indeed suitable for use in a kinematic study, despite the large zero-point errors in the survey photographic photometry. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 44 915 Individual photometric observations table3.dat 82 106 Derived light-curve parameters table4.dat 40 51 Six light-curve templates -------------------------------------------------------------------------------- See also: II/214 : Combined General Catalogue of Variable Stars (Kholopov+ 1998) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Star Star name 11- 23 F13.5 d HJD Heliocentric Julian date of mid-observation 25- 29 F5.3 --- Phase Derive photometric phase 31- 36 F6.3 mag Vmag Johnson V magnitude 38- 42 F5.3 mag e_Vmag rms uncertainty on Vmag 44 I1 --- Run [1/8] Observing run number (1) -------------------------------------------------------------------------------- Note (1): 1: 1993 Jan 8-9 2: 1993 Apr 9-13 3: 1993 May 20-22, 26 4: 1993 Aug 6-8 5: 1993 Aug 28-31 6: 1993 Sep 28 7: 1993 Oct 27-29, Nov 2 8: 1994 June 17-20, 26-27 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Star Star name 11- 12 I2 h RAh Right ascension (J2000.0) 14- 15 I2 min RAm Right ascension (J2000.0) 17- 21 F5.2 s RAs Right ascension (J2000.0) 23 A1 --- DE- Declination sign (J2000.0) 24- 25 I2 deg DEd Declination (J2000.0) 27- 28 I2 arcmin DEm Declination (J2000.0) 30- 33 F4.1 arcsec DEs Declination (J2000.0) 35- 38 F4.2 mag AV Interstellar absorption in V band 40- 48 F9.7 d Per ? Adopted period 50- 51 I2 10-5d e_Per ? rms uncertainty on Per (99: e_Per>10-3d) 54 I1 --- n_Per [1/3]? Origin of the period (1) 56- 60 F5.2 mag <Vmag> ? Average V magnitude 62- 73 F12.4 d Emax ? Epoch (Julian date) at maximum light 75- 79 F5.3 d e_Emax ? rms uncertainty on Emax 81- 82 I2 --- Nobs ? Number of observations -------------------------------------------------------------------------------- Note (1): 1: PGCVS4 (Cat. II/214) was adopted for the star 2: the adopted period is at most a few percent away from PGCVS4 (Cat. II/214) 3: the adopted period is farther away from PGCVS4 (Cat. II/214), and hence more questionable -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 F4.2 --- Phase Phase 6- 10 F5.3 --- V1 Template 1 V magnitude 12- 16 F5.3 --- V2 Template 2 V magnitude 18- 22 F5.3 --- V3 Template 3 V magnitude 24- 28 F5.3 --- V4 Template 4 V magnitude 30- 34 F5.3 --- V5 Template 5 V magnitude 36- 40 F5.3 --- V6 Template 6 V magnitude -------------------------------------------------------------------------------- History: From AJ electronic version
(End) James Marcout, Patricia Bauer [CDS] 09-Mar-1999
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