J/ApJ/838/122       Light curve analysis of 13 active stars       (Jetsu+, 2017)

General model for light curves of chromospherically active binary stars. Jetsu L., Henry G.W., Lehtinen J. <Astrophys. J. 838, 122 (2017)> =2017ApJ...838..122J 2017ApJ...838..122J (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Ephemerides ; Photometry Keywords: techniques: photometric - methods: data analysis - stars: binary - stars: activity Abstract: We present results from light curve fits to the photometry of 13 chromospherically active stars, covering the time evolution of the rotational phase of their primary light curve minimum and the light curve amplitude. Description: The data table contains estimates of the light curve minimum phases and amplitudes retrieved by the continuous period search analysis (Lehtinen et al., 2011A&A...527A.136L 2011A&A...527A.136L, Cat. J/A+A/527/A136). The results for different stars have been labeled according to the names of the stars. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 118 14 CABS Sample res.dat 73 815 Numerical results for the light curve fits lc/* . 14 Individual light curves -------------------------------------------------------------------------------- See also: J/A+A/527/A136 : HD 116956 V-band differential light curve (Lehtinen+, 2011) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Variable name 11- 19 A9 --- OName Variable other name 21- 29 A9 --- Comp Comparison star name 31- 40 A10 --- Date.Beg First observing date 42- 51 A10 --- Date.End Last observing date 53- 56 F4.1 yr DeltaT Time span 58- 61 I4 --- Nobs Number of observations 63- 71 F9.6 d Porb Orbital period 73- 80 F8.6 d e_Porb rms uncertainty on Porb 82- 91 F10.4 d t0 Epoch (HJD-2400000) 93 A1 --- n_t0 [abcde] Epoch type (1) 95-100 F6.4 --- e Eccentricity 102 I1 --- K [1/2] MLC order 104-108 F5.3 mag Amp Amplitude of variation 110-116 A7 --- FileName Name of the file with light curve data in subdirectory lc 118 A1 --- n_Name [n] n: no data in res.dat file for V478 Lyr -------------------------------------------------------------------------------- Note (1): Epoch types as follows: a = radial velocity maximum b = periastron c = cool in front d = primary in front e = primary behind -------------------------------------------------------------------------------- Byte-by-byte Description of file: res.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Name of the star 12- 21 F10.4 d t1 1st timepoint in dataset (1) 24- 33 F10.4 d tn Last timepoint in dataset (1) 36- 37 I2 --- n Number of observations in dataset 40- 49 F10.4 d tmin Epoch of the primary minimum (1) 52- 57 F6.4 d e_tmin Error of tmin 60- 65 F6.4 mag Amp Light curve amplitude 68- 73 F6.4 mag e_Amp Error of Amp -------------------------------------------------------------------------------- Note (1): All timepoints are Heliocentric Julian Dates given in format HJD-2400000. -------------------------------------------------------------------------------- Byte-by-byte Description of file: lc/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.4 d HJD Heliocentric Julian Date 14- 19 F6.3 mag DVmag Differential V band magnitude -------------------------------------------------------------------------------- Acknowledgements: Lauri Jetsu, lauri.jetsu(at)helsinki.fi
(End) Patricia Vannier [CDS] 04-Apr-2017
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