J/A+A/626/A119      EBLM J2349-32 photometry, RV and spectra       (Gill+, 2019)

The EBLM project. VI: Mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey. Gill S., Maxted P.F.L., Evans J.A., Evans D.F., Southworth J., Smalley B., Gary B.L., Anderson D.R., Bouchy F., Cameron A.C., Dominik M., Faedi F., Gillon M., Gomez Maqueo Chew L.Hebb Y., Hellier C., Jorgensen U.G., Longa-Pena P., Martin D.V., McCormac J., Pepe F.V., Pollaco D., Queloz D., Segransan D., Snodgrass C., Turner O.D., Triaud A.H.M., Udry S., West R.G. <Astron. Astrophys. 626, A119 (2019)> =2019A&A...626A.119G 2019A&A...626A.119G (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, eclipsing ; Radial velocities ; Photometry ; Spectra, optical Keywords: binaries: eclipsing; spectroscopic - stars: low-mass - stars: techniques: spectroscopic; photometry Abstract: Some M-dwarfs around F-/G-type stars have been measured to be hotter and larger than predicted by stellar evolution models. Inconsistencies between observations and models need to be addressed with more mass, radius, and luminosity measurements of low-mass stars to test and refine evolutionary models. Our aim is to measure the masses, radii and ages of the stars in five low-mass eclipsing binary systems discovered by the WASP survey. We used WASP photometry to establish eclipse-time ephemerides and to obtain initial estimates for the transit depth and width. Radial velocity measurements were simultaneously fitted with follow-up photometry to find the best-fitting orbital solution. This solution was combined with measurements of atmospheric parameters to interpolate evolutionary models and estimate the mass of the primary star, and the mass and radius of the M-dwarf companion. We assess how the best fitting orbital solution changes if an alternative limb-darkening law is used and quantify the systematic effects of unresolved companions. We also gauge how the best-fitting evolutionary model changes if different values are used for the mixing length parameter and helium enhancement. We report the mass and radius of five M-dwarfs and find little evidence of inflation with respect to evolutionary models. The primary stars in two systems are near the "blue hook" stage of their post sequence evolution, resulting in two possible solutions for mass and age. We find that choices in helium enhancement and mixing-length parameter can introduce an additional 3-5% uncertainty in measured M-dwarf mass. Unresolved companions can introduce an additional 3-8% uncertainty in the radius of an M-dwarf, while the choice of limb-darkening law can introduce up to an additional 2% uncertainty. The choices in orbital fitting and evolutionary models can introduce significant uncertainties in measurements of physical properties of such systems. Description: We used the SAAO 1-m telescope in Bessel I filter to observe J2349-32. Radial velocity measurements were obtained with CORALIE as part of the EBLM project. Objects: ------------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------------ 23 49 15.24 -32 46 17.5 EBLM J2349-32 = TYC 7519-142-1 ------------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 74 5 List of studied stars rv.dat 41 155 Radial velocities saao.dat 72 929 SAAO photometry ctio.dat 42 281 CTIO photometry hao.dat 46 1287 HAO photometry wasp.dat 88 47209 WASP photometry list.dat 168 17 List of fits spectra fits/* . 18 Individual fits spectra -------------------------------------------------------------------------------- See also: J/A+A/549/A18 : WASP-30 and J1219-39 light + velocity curves (Triaud+, 2013) J/A+A/572/A50 : J0113+31 light + velocity curves (Gomez Maqueo Chew+, 2014) J/A+A/604/L6 : EBLM J0555-57 photometry and RV (von Boetticher+, 2017) J/A+A/625/A150 : 10 very-low-mass stars photometry (von Boetticher+, 2019) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name 10- 11 I2 h RAh Right ascension (J2000) 13- 14 I2 min RAm Right ascension (J2000) 16- 20 F5.2 s RAs Right ascension (J2000) 22 A1 --- DE- Declination sign (J2000) 23- 24 I2 deg DEd Declination (J2000) 26- 27 I2 arcmin DEm Declination (J2000) 29- 32 F4.1 arcsec DEs Declination (J2000) 34- 38 F5.2 mag Vmag V magnitude 40- 52 A13 --- SName Simbad name 54- 55 A2 --- RV rv indicates radial velocity data in rv.dat file 57- 60 A4 --- SAAO saao indicates photometric data in saao.dat file 62- 65 A4 --- CTIO ctio indicates photometric data in ctio.dat file 67- 69 A3 --- HAO hao indicates photometric data in hao.dat file 71- 74 A4 --- WASP wasp indicates photometric data in wasp.dat file -------------------------------------------------------------------------------- Byte-by-byte Description of file: rv.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name 10- 21 F12.6 d BJD Barycentric Julian date 24- 33 F10.5 km/s RV Radial velocity 35- 41 F7.5 km/s e_RV rms uncertainty on radial velocity -------------------------------------------------------------------------------- Byte-by-byte Description of file: saao.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name 10 A1 --- Band [RI] SAAO observed band 12- 29 F18.10 d BJD Barycentric Julian date 31- 49 F19.16 mag mag SAAO 1m magnitude in Band 52- 72 F21.19 mag e_mag rms uncertainty on mag -------------------------------------------------------------------------------- Byte-by-byte Description of file: ctio.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name 10 A1 --- Band [griz] CTIO observed band 12- 22 F11.6 d BJD Barycentric Julian date 25- 32 F8.5 mag mag SAAO 1m magnitude in Band 36- 42 F7.5 mag e_mag rms uncertainty on mag -------------------------------------------------------------------------------- Byte-by-byte Description of file: hao.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name 10- 12 A3 --- Band [CBB gz ] HAO observed band 14- 23 F10.5 d BJD Barycentric Julian date 25- 31 F7.4 mag mag SAAO 1m magnitude in Band 33- 38 F6.4 mag e_mag rms uncertainty on mag 41- 46 F6.4 mag e_mag2 Second rms uncertainty on mag -------------------------------------------------------------------------------- Byte-by-byte Description of file: wasp.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name 10- 24 F15.7 d HJD Heliocentric Julian date, TDB 26- 40 F15.7 d JD Julian date, TDB 42- 56 F15.7 d BJD Barycentirc Julian date, TDB 58- 65 F8.5 mag mag WASP magnitude 67- 74 F8.6 mag e_mag rms uncertainty on WASP magnitude 76- 86 F11.9 --- Phase Phase 88 I1 --- Field [1/7] Field number -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.4 deg RAdeg Right Ascension of center (J2000) 9- 17 F9.5 deg DEdeg Declination of center (J2000) 19- 24 I6 --- Nx Number of pixels along X-axis 26- 44 A19 "datime" Obs.date Observation date 46- 52 F7.2 0.1nm blambda Lower value of wavelength interval 54- 60 F7.2 0.1nm Blambda Upper value of wavelength interval 62- 66 F5.3 0.1nm dlambda Wavelenght resolution 68- 71 I4 Kibyte size Size of FITS file 73-115 A43 --- FileName Name of FITS file, in subdirectory fits 116-168 A53 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Samuel Gill, samuel.gill(at)warwick.ac.uk References: Triaud et al., Paper I 2013A&A...549A..18T 2013A&A...549A..18T, Cat. J/A+A/549/A18 Gomez Maqueo Chew et al., Paper II 2014A&A...572A..50G 2014A&A...572A..50G, Cat. J/A+A/572/A50 von Boetticher et al., Paper III 2017A&A...604L...6V 2017A&A...604L...6V Triaud et al., Paper IV 2017A&A...608A.129T 2017A&A...608A.129T von Boetticher et al., Paper V 2019A&A...625A.150V 2019A&A...625A.150V, Cat. J/A+A/572/A50
(End) Patricia Vannier [CDS] 18-Jun-2019
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