J/MNRAS/408/475     HATNet Pleiades Rotation Period Catalogue  (Hartman+, 2010)

A large sample of photometric rotation periods for FGK Pleiades stars. Hartman J.D., Bakos G.A., Kovacs G., Noyes R.W. <Mon. Not. R. Astron. Soc., 408, 475-489 (2010)> =2010MNRAS.408..475H 2010MNRAS.408..475H
ADC_Keywords: Clusters, open ; Stars, variable ; Photometry, UBV ; Photometry, infrared ; Rotational velocities Keywords: techniques: photometric - catalogues - stars: late-type - stars: rotation - starspots - open clusters and associations: individual: Pleiades Abstract: Using data from the Hungarian-made Automated Telescope Network (HATNet) survey for transiting exoplanets, we measure photometric rotation periods for 368 Pleiades stars with 0.4~<M~<1.3M. We detect periodic variability for 74 per cent of the cluster members in this mass range that are within our field-of-view, and 93 per cent of the members with 0.7~<M~<1.0M. This increases, by a factor of 5, the number of Pleiades members with measured periods. We compare these data to the rich sample of spectroscopically determined projected equatorial rotation velocities (vsini) available in the literature for this cluster. Included in our sample are 14 newly identified probable cluster members which have proper motions, photometry and rotation periods consistent with membership. Description: Photometric time-series observations of the Pleiades cluster were obtained between 2008 September 15 and 2009 March 16 using the identical HAT-9 and HAT-10 11-cm aperture robotic telescopes located at Mauna Kea Observatory (MKO) in Hawaii and at Fred L. Whipple Observatory (FLWO) in Arizona, respectively. This catalogue contains photometric rotation periods for stars in the Pleiades open cluster. Most of the periods were measured from light curves obtained with the Hungarian-made Automated Telescope Network (HATNet) of small aperture robotic telescopes located in Arizona and Hawaii. A handful of stars with periods from the literature that were not recovered with the HATNet data are also included in the catalogue. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file prd.dat 172 383 Catalogue of rotation periods knownprd.dat 45 94 Compilation of previously published periods memnovar.dat 133 120 Cluster Members without detected periods fieldprd.dat 76 1804 Non-cluster member periodic variables refs.dat 72 16 References -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) J/ApJS/172/663 : Infrared observations of the Pleiades (Stauffer+, 2007) Byte-by-byte Description of file: prd.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name HATNet Designation (HAT-NNN-NNNNNNN) 17- 25 F9.6 deg RAdeg Right Ascension J2000 (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 27- 35 F9.6 deg DEdeg Declination J2000 (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 37- 66 A30 --- OtherID *Other Designations 68- 78 F11.8 d Per *Rotation period 80- 90 F11.8 d e_Per ?=-9.99999999 Uncertainty on the rotation period from fitting a Gaussian function to the peak frequency in the power spectrum 92- 99 F8.5 d-1 fwidth ?=-9.99999 1-σ width of a Gaussian function fit to the peak in the power spectrum 101-112 A12 --- r_Per ? Other references for the period, in refs.dat file 114-120 F7.4 mag rAmp ?=-9.9999 Peak-to-peak amplitude in the Sloan r filter 122-126 F5.2 mag Bmag ?=-9.99 Magnitude (apparent) in B filter (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 128-132 F5.2 mas Vmag ?=-9.99 Magnitude (apparent) in V filter (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 134-139 F6.3 --- Kmag Magnitude (apparent) in K filter (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 141-145 F5.3 Msun Mass *Mass of the star 147-151 F5.3 Rsun Radius *Radius of the star 153 A1 --- l_vsini Upper or lower-limit flag on vsini 154-159 F6.2 km/s vsini ?=-99.99 Projected equatorial rotation velocity 161-164 A4 --- r_vsini Reference for the vsini, in refs.dat file 166-172 A7 --- Bin *Note if the star is a known binary -------------------------------------------------------------------------------- Note on OtherID: These designations are taken from Stauffer et al., 2007, Cat. J/ApJS/172/663. Rows without an entry for this column are new candidate cluster members. Note on Per: The given period is derived from the HATNet light curves except for cases where e_Per, fwidth, or rAmp are NULL. In those cases no HATNet period is available, and the given period is taken from the first reference listed. Note on Mass and Radius: This is derived from the K magnitude and the YY2 isochrones, except for the 9 stars with periods taken from Scholz & Eisloeffel (2004A&A...421..259S 2004A&A...421..259S) for which the Baraffe 1998 (Cat. J/A+A/337/403) isochrones are used. Note on Bin: If this is not null the star is a known binary. The entry consists of two strings separated by a comma. The first string is either VB for a visual binary, or SB2 for a double-lined spectroscopic binary. The second string gives the reference for this determination. -------------------------------------------------------------------------------- Byte-by-byte Description of file: knownprd.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 30 A30 --- ID *Designation 32- 40 F9.6 d Per Rotation period 42- 45 A4 --- r_Per Reference for the period, in refs.dat file -------------------------------------------------------------------------------- Note on ID: These designations are taken from Stauffer et al., 2007, Cat. J/ApJS/172/663 -------------------------------------------------------------------------------- Byte-by-byte Description of file: memnovar.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name HATNet Designation (HAT-NNN-NNNNNNN) 17- 25 F9.6 deg RAdeg Right Ascension J2000 (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 27- 35 F9.6 deg DEdeg Declination J2000 (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 37- 67 A31 --- OtherID *Other Designations 69- 72 I4 --- Nobs Number of photometric observations 74- 81 F8.5 mag RMS rms of the light curve 83- 87 F5.2 mag Bmag ?=-9.99 Magnitude (apparent) in B filter (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 89- 93 F5.2 mas Vmag ?=-9.99 Magnitude (apparent) in V filter (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 95-100 F6.3 --- Kmag Magnitude (apparent) in K filter (from Stauffer et al., 2007, Cat. J/ApJS/172/663) 102-106 F5.3 Msun Mass *Mass of the star 108-112 F5.3 Rsun Radius *Radius of the star 114 A1 --- l_vsini Upper or lower-limit flag on vsini 115-120 F6.2 km/s vsini ?=-99.99 Projected equatorial rotation velocity 122-125 A4 --- r_vsini Reference for the vsini 127-133 A7 --- Bin *Note if the star is a known binary -------------------------------------------------------------------------------- Note on OtherID: Data are taken from Stauffer et al., 2007, Cat. J/ApJS/172/663. Note on Mass and Radius: This is derived from the K magnitude and the YY2 isochrones, except for the 9 stars with periods taken from Scholz & Eisloeffel (2004A&A...421..259S 2004A&A...421..259S) for which the Baraffe 1998 (Cat. J/A+A/337/403) isochrones are used. Note on Bin: If this is not null the star is a known binary. The entry consists of two strings separated by a comma. The first string is either VB for a visual binary, or SB2 for a double-lined spectroscopic binary. The second string gives the reference for this determination. -------------------------------------------------------------------------------- Byte-by-byte Description of file: fieldprd.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name HATNet Designation (HAT-NNN-NNNNNNN) 17- 25 F9.6 deg RAdeg Right Ascension J2000 (from 2MASS) 27- 35 F9.6 deg DEdeg Declination J2000 (from 2MASS) 37- 47 F11.8 d Per Period 49- 55 F7.4 mag rAmp Peak-to-peak amplitude in the Sloan r filter 57- 62 F6.3 --- Jmag ?=-9.999 Magnitude (apparent) in 2MASS J filter 64- 69 F6.3 --- Hmag ?=-9.999 Magnitude (apparent) in 2MASS H filter 71- 76 F6.3 --- Kmag ?=-9.999 Magnitude (apparent) in 2MASS K filter -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Ref Reference code 6- 24 A19 --- BibCode BibCode 26- 45 A20 --- Aut Author's name 47- 72 A26 --- Com Comments -------------------------------------------------------------------------------- Acknowledgements: Joel Hartman, jhartman(at)cfa.harvard.edu
(End) Joel Hartman [CfA], Patricia Vannier [CDS] 05-Apr-2011
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