J/A+A/566/A130 Rotation and variability of substellar objects (Crossfield, 2014)

Doppler imaging of exoplanets and brown dwarfs. Crossfield I.J.M. <Astron. Astrophys. 566, A130 (2014)> =2014A&A...566A.130C 2014A&A...566A.130C
ADC_Keywords: Stars, variable - Rotational velocities Keywords: instrumentation: spectrographs - techniques: spectroscopic - catalogs - planets and satellites: atmospheres - brown dwarfs - stars: imaging Abstract: Doppler Imaging produces 2D global maps of rotating objects using high-dispersion spectroscopy. When applied to brown dwarfs and extrasolar planets, this technique can constrain global atmospheric dynamics and/or magnetic effects on these objects in un- precedented detail. I present the first quantitative assessment of the prospects for Doppler Imaging of substellar objects with current facilities and with future giant ground-based telescopes. Observations will have the greatest sensitivity in K band, but the H and L bands will also be useful for these purposes. To assess the number and availability of targets, I also present a compilation of all measurements of photometric variability, rotation period (P), and projected rotational velocity (vsini) for brown dwarfs and exoplanets. Several bright objects are already accessible to Doppler Imaging with currently available instruments. With the development of giant ground-based telescopes, Doppler Imaging will become feasible for many dozens of brown dwarfs and for the few brightest directly imaged extrasolar planets (such as beta Pic b). The present set of measurements of P, vsini, and variability are incomplete for many objects, and the sample is strongly biased toward early-type objects (<L5). Thus, surveys to measure these quantities for later-type objects will be especially helpful in expanding the sample of candidates for global weather monitoring via Doppler Imaging. Description: Measurements of variability, projected rotational velocities (vsini), and rotation periods for brown dwarfs and exoplanets compiled from the literature. Also included are information on spectral type, binarity, youth, near-infrared photometry (2MASS JHKs). References are included for all reported values. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file rotation.dat 246 347 Variability and rotation measurements rotation.fits 2880 75 FITS version of the table refs.dat 148 171 References -------------------------------------------------------------------------------- See also: J/PAZh/27/403 : CCD R photometry in the UMa supercluster (Kopylova+, 2001) Byte-by-byte Description of file: rotation.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 26 A26 --- Name Name of brown dwarf or exoplanet 28- 29 I2 h RAh Right ascension (J2000) 31- 32 I2 min RAm Right ascension (J2000) 34- 39 F6.3 s RAs Right ascension (J2000) 41 A1 --- DE- Declination sign (J2000) 42- 43 I2 deg DEd Declination (J2000) 45- 46 I2 arcmin DEm Declination (J2000) 48- 52 F5.2 arcsec DEs Declination (J2000) 54 I1 --- fy [0/1] Flag for youth; 1 if young 56 I1 --- fb [1]? Flag for binarity; 1 if a binary 58- 65 F8.5 arcsec Sep [0/22]? Separation of binary components 67- 76 A10 --- r_Sep Reference for multiplicity (in refs.dat file) 78- 82 F5.2 km/s vsini [0/86]? Projected rotational velocity 84- 88 F5.2 km/s e_vsini ? rms uncertainty on vsini 90- 91 I2 km/s B_vsini ?=- Upper limit for vsini 93-110 A18 --- r_vsini Reference for vsini (in refs.dat file) 112 A1 --- l_Per Limit flag on Per 113-119 F7.3 h Per [1.4/114]? Period 121-129 A9 --- r_Per Period reference (in refs.dat file) 131-136 F6.4 --- Var [0/1]? Variability 138-153 A16 --- n_Var Bandpass of variability measurement 155-171 A17 --- r_Var Variability reference (in refs.dat file) 173-180 A8 --- SpT Spectral type 182-186 F5.2 --- SpT.N ?=- Numerical spectral type (M0=0, L0=10) 188-200 A13 --- n_SpT Note on Spectral type from DwarfArchives.org 202-207 A6 --- r_SpT Reference for SpType (in refs.dat file) 209-214 F6.3 mag Jmag 2MASS J-band NIR flux 216-220 F5.3 mag e_Jmag rms uncertainty on Jmag 222-227 F6.3 mag Hmag 2MASS H-band NIR flux 229-233 F5.3 mag e_Hmag rms uncertainty on Hmag 235-240 F6.3 mag Ksmag 2MASS Ks-band NIR flux 242-246 F5.3 mag e_Ksmag rms uncertainty on Ksmag -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference number 5- 23 A19 --- BibCode BibCode 25- 55 A31 --- Aut Author's name 57-148 A92 --- Com Comments -------------------------------------------------------------------------------- Acknowledgements: Ian Crossfield, ianc(at)lpl.arizona.edu
(End) Ian Crossfield [MPIA, Germany], Patricia Vannier [CDS] 06-Jun-2014
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