J/AJ/142/107        Variable stars in NGC 1466               (Kuehn+, 2011)

Variable stars in Large Magellanic Cloud globular clusters. I. NGC 1466. Kuehn C.A., Smith H.A., Catelan M., Pritzl B.J., De Lee N., Borissova J. <Astron. J., 142, 107 (2011)> =2011AJ....142..107K 2011AJ....142..107K
ADC_Keywords: Magellanic Clouds ; Clusters, globular ; Stars, variable ; Photometry, UBV Keywords: Magellanic Clouds - stars: horizontal-branch - stars: variables: general - stars: variables: RR Lyrae Abstract: This is the first in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to better understand how the RR Lyrae stars in Oosterhoff-intermediate systems compare to those in Oosterhoff I/II systems. In this paper, we present the results of our new time-series BV photometric study of NGC 1466. A total of 62 variables were identified in the cluster, of which 16 are new discoveries. The variables include 30 RRab stars, 11 RRc stars, 8 RRd stars, 1 candidate RR Lyrae, 2 long-period variables, 1 potential anomalous Cepheid, and 9 variables of undetermined classification. We present photometric parameters for these variables. Description: A total of 40 V and 37 B images of NGC 1466 were obtained with the Southern Astrophysical Research (SOAR) telescope using the SOAR Optical Imager (SOI) in 2008 February and December. An additional 45 V and 43 B images were obtained using ANDICAM on the SMARTS 1.3m telescope operated by the SMARTS consortium6 from 2006 September to 2007 January. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 97 54 Photometric parameters for variables in NGC 1466, excluding RRd stars table3.dat 110 8 Photometric parameters for the RRd variables in NGC 1466 table2.dat 61 8160 Photometry of the variable stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name (V01 to V68) 5- 6 I2 h RAh Right ascension (J2000) 8- 9 I2 min RAm Right ascension (J2000) 11- 14 F4.1 s RAs Right ascension (J2000) 16 A1 --- DE- Declination sign (J2000) 17- 18 I2 deg DEd Declination (J2000) 20- 21 I2 arcmin DEm Declination (J2000) 23- 26 F4.1 arcsec DEs Declination (J2000) 28- 36 A9 --- Type Variable type (1) 38- 44 F7.5 d Per ? Period 46- 49 F4.2 mag Vamp ? Amplitude in V band 51- 54 F4.2 mag Bamp ? Amplitude in B band 56- 61 F6.3 mag <Vmag> ? Intensity-weighted V mean magnitude 63- 68 F6.3 mag <Bmag> ? Intensity-weighted B mean magnitude 70- 74 F5.3 mag <B-V> ? Magnitude-weighted B-V mean colour index 76- 84 A9 --- OName Other name(s) (G1) 86- 97 F12.4 d TMax ? Time of maximum light (HJD) -------------------------------------------------------------------------------- Note (1): The RRab stars that potentially exhibit the Blazhko effect are indicated as "RRab-BL," see Section 3.1 for further discussion on the detection of the Blazhko effect in the RRab stars in NGC 1466. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name (V01 to V68) 5- 6 I2 h RAh Right ascension (J2000) 8- 9 I2 min RAm Right ascension (J2000) 11- 14 F4.1 s RAs Right ascension (J2000) 16 A1 --- DE- Declination sign (J2000) 17- 18 I2 deg DEd Declination (J2000) 20- 21 I2 arcmin DEm Declination (J2000) 23- 26 F4.1 arcsec DEs Declination (J2000) 28- 30 A3 --- Type [RRd] Variable type 32- 37 F6.4 d P0 Fundamental mode period 39- 44 F6.4 d P1 First overtone period 46- 51 F6.4 d P1/P0 Period ratio, P1/P0 53- 56 F4.2 mag Vamp0 Fundamental mode amplitude in V band 58- 61 F4.2 mag Vamp1 First overtone amplitude in V band 63- 66 F4.2 mag Bamp0 Fundamental mode amplitude in B band 68- 71 F4.2 mag Bamp1 First overtone amplitude in B band 73- 78 F6.3 mag <Vmag> Intensity-weighted V mean magnitude 80- 85 F6.3 mag <Bmag> Intensity-weighted B mean magnitude 87- 91 F5.3 mag <B-V> Magnitude-weighted B-V mean colour index 93- 97 A5 --- OName Other name(s) (G1) 99-110 F12.4 d TMax Time of maximum light (HJD) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name (V01 to V68) 5 A1 --- Filter [BV] Filter 7- 20 F14.6 d HJD Heliocentric Julian Date 22- 26 F5.3 --- Phase ?=- Phase (1) 28- 33 F6.3 mag mag ? Magnitude in Filter (2) 35- 40 F6.4 mag e_mag ? Error in mag 41- 51 F11.3 --- dflux ? Differential flux in Filter (2) 53- 61 F9.4 --- e_dflux ? Error in dflux -------------------------------------------------------------------------------- Note (1): Computed such that maximum light occurs at phase 0. Note (2): Differential fluxes for V31, V51, V54, V60 and V67, magnitudes for the other variables. -------------------------------------------------------------------------------- Global notes: Note (G1): Other names from Walker, 1992AJ....104.1395W 1992AJ....104.1395W. In Simbad, WaNNN = Cl* NGC 1466 WALK NNNN and SNN = Cl* NGC 1466 S NN -------------------------------------------------------------------------------- History: From electronic version of the journal References: Kuehn et al., Paper II, 2012AJ....144..186K 2012AJ....144..186K, Cat. J/AJ/144/186 Kuehn et al., Paper III, 2013AJ....145..160K 2013AJ....145..160K, Cat. J/AJ/145/160
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 20-Nov-2012
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