J/ApJ/848/34 CATalog of Stellar Unified Properties (Hinkel+, 2017)
A CATalog of Stellar Unified Properties (CATSUP) for 951 FGK-Stars within 30 pc.
Hinkel N.R., Mamajek E.E., Turnbull M.C., Osby E., Shkolnik E.L.,
Smith G.H., Klimasewski A., Somers G., Desch S.J.
<Astrophys. J., 848, 34-34 (2017)>
=2017ApJ...848...34H 2017ApJ...848...34H (SIMBAD/NED BibCode)
ADC_Keywords: Stars, nearby ; X-ray sources ; Radio sources ;
Photometry, ultraviolet ; Abundances ; Space velocities
Keywords: catalogs - solar neighborhood - stars: abundances -
stars: fundamental parameters - ultraviolet: stars - X-rays: stars
Abstract:
Almost every star in our Galaxy is likely to harbor a terrestrial
planet, but accurate measurements of an exoplanet's mass and radius
demand accurate knowledge of the properties of its host star. The
imminent TESS and CHEOPS missions are slated to discover thousands of
new exoplanets. Along with WFIRST, which will directly image nearby
planets, these surveys make urgent the need to better characterize
stars in the nearby solar neighborhood (<30pc). We have compiled the
CATalog of Stellar Unified Properties (CATSUP) for 951 stars,
including such data as: Gaia astrometry; multiplicity within stellar
systems; stellar elemental abundance measurements; standardized
spectral types; CaII H and K stellar activity indices; GALEX NUV and
FUV photometry; and X-ray fluxes and luminosities from ROSAT, XMM, and
Chandra. We use this data-rich catalog to find correlations,
especially between stellar emission indices, colors, and galactic
velocity. Additionally, we demonstrate that thick-disk stars in the
sample are generally older, have lower activity, and have higher
velocities normal to the galactic plane. We anticipate that CATSUP
will be useful for discerning other trends among stars within the
nearby solar neighborhood, for comparing thin-disk versus thick-disk
stars, for comparing stars with and without planets, and for finding
correlations between chemical and kinematic properties.
Description:
We have assembled a data set of stellar properties for 951 FGK-type
stars within 30pc of the Sun. Beginning with the Gaia (Cat. I/337)
TGAS subset of astrometric data, we have combined information
regarding multiplicity within stellar systems (ExoCat, Gray et al.,
2003, Cat. J/AJ/126/2048; 2006, Cat. J/AJ/132/161; Valenti & Fischer
2005, Cat. J/ApJS/159/141; Takeda et al. 2007, Cat. J/PASJ/59/1127),
stellar abundance measurements (Hypatia, Hinkel et al. 2014, Cat.
J/AJ/148/54; 2016ApJS..226....4H 2016ApJS..226....4H), standardized spectral types, Ca II
H and K stellar activity indices, NUV and FUV photometry from GALEX
(Cat. II/312), and X-ray fluxes and luminosities from ROSAT (Cat.
IX/10), XMM (Cat. IX/50), and Chandra (Cat. IX/45). The aim of this
project was to collate a wide variety of data for nearby stars such
that they could be more easily characterized. The information
available in CATSUP can be utilized for the direct sample or act as a
proxy for similar stars, in order to better understand the overall
trends within solar neighborhood stars, as well as stars that host
exoplanets. CATSUP was compiled in anticipation of upcoming exoplanet
surveys such as TESS, CHEOPS, and WFIRST.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table3.dat 543 951 Catalog of Stellar Unified Properties
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See also:
I/337 : Gaia DR1 (Gaia Collaboration, 2016)
Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 6 I6 --- HIP ? Hipparcos name
10- 15 I6 --- HD ? Henry-Draper catalog name
17- 27 A11 --- TYC Tycho name
29- 36 F8.4 deg RAdeg Right Ascension, decimal degrees (J2000)
38- 45 F8.4 deg DEdeg Declination, decimal degrees (J2000)
47- 53 F7.3 pc X Cartesian, geocentric x-coordinate from the
Sun, in pc (1)
55- 61 F7.3 pc Y Cartesian, geocentric y-coordinate from the
Sun, in pc (1)
63- 69 F7.3 pc Z Cartesian, geocentric z-coordinate from the
Sun, in pc (1)
71- 76 F6.3 pc Dist Distance in pc from Gaia
78- 83 F6.1 km/s UVel ?=9999.0 Component of space velocity, km/s,
positive toward the Galactic anticenter,
radial
85- 90 F6.1 km/s VVel ?=9999.0 Component of space velocity, km/s,
positive in the direction of Galactic
rotation
92- 97 F6.1 km/s WVel ?=9999.0 Component of space velocity, km/s,
positive toward the North Galactic Pole
99-105 F7.2 K Teff ?=99.99 stellar effective temperature, in K
107-112 A6 --- r_Teff Reference source for Teff (2)
114-118 F5.2 [cm/s2] logg ?=99.99 surface gravity of the star
120-125 A6 --- r_logg Reference source for surface gravity (2)
127-131 A5 --- Disk Likely origin within the disk, thin,
thick, based on kinematics
133-135 A3 --- Planet Flag as to whether a planet is known
to orbit the star (3)
137-141 F5.2 mag Bmag ?=99.99 B magnitude (4)
143-147 F5.2 mag Vmag ?=99.99 V magnitude (4)
149-153 F5.2 mag B-V ?=99.99 B-V color index (4)
157 I1 --- Single [0/1] a true single star, true=1
159-160 A2 --- Comp Component identifier (5)
163-168 I6 --- HIP2 ? Component HIP number, if known (5)
170-186 A17 --- SpType Spectral type
188-206 A19 --- r_SpType ADS bibcode for spectral type source
207 A1 --- f_SpType Spectral type flag (6)
209-214 F6.3 [-] logRHK ?=99.99 Average of logR'HK Ca II HK emission
indices derived from literature sources
216-217 I2 --- o_logRHK ?=0 number of sources compiled for logRHK
222-226 F5.2 [-] FeH ?=99.99 [Fe/H] abundance in dex
228-232 F5.2 [-] spFeH ?=99.99 Spread in FeH
234-238 F5.2 [-] CH ?=99.99 [CH/H] abundance in dex
240-244 F5.2 [-] spCH ?=99.99 Spread in CH
246-250 F5.2 [-] OH ?=99.99 [O/H] abundance in dex
252-256 F5.2 [-] spOH ?=99.99 Spread in OH
258-262 F5.2 [-] NaH ?=99.99 [Na/H] abundance in dex
264-268 F5.2 [-] spNaH ?=99.99 Spread in NaH
270-274 F5.2 [-] MgH ?=99.99 [Mg/H] abundance in dex
276-280 F5.2 [-] spMgH ?=99.99 Spread in MgH
282-286 F5.2 [-] AlH ?=99.99 [Al/H] abundance in dex
288-292 F5.2 [-] spAlH ?=99.99 Spread in AlH
294-298 F5.2 [-] SiH ?=99.99 [Si/H] abundance in dex
300-304 F5.2 [-] spSiH ?=99.99 Spread in SiH
306-310 F5.2 [-] CaH ?=99.99 [Ca/H] abundance in dex
312-316 F5.2 [-] spCaH ?=99.99 Spread in CaH
318-322 F5.2 [-] TiH ?=99.99 [Ti/H] abundance in dex
324-328 F5.2 [-] spTiH ?=99.99 Spread in TiH
330-334 F5.2 [-] VH ?=99.99 [V/H] abundance in dex
336-340 F5.2 [-] spVH ?=99.99 Spread in VH
342-346 F5.2 [-] CrH ?=99.99 [Cr/H] abundance in dex
348-352 F5.2 [-] spCrH ?=99.99 Spread in CrH
354-358 F5.2 [-] MnH ?=99.99 [Mn/H] abundance in dex
360-364 F5.2 [-] spMnH ?=99.99 Spread in MnH
366-370 F5.2 [-] CoH ?=99.99 [Co/H] abundance in dex
372-376 F5.2 [-] spCoH ?=99.99 Spread in CoH
378-382 F5.2 [-] NiH ?=99.99 [Ni/H] abundance in dex
384-388 F5.2 [-] spNiH ?=99.99 Spread in NiH
390-394 F5.2 mag FUVmag ?=99.99 GALEX/FUV magnitude, AB mag
396-400 F5.2 mag e_FUVmag ?=99.99 Uncertainty in FUVmag
402-406 F5.2 mag NUVmag ?=99.99 GALEX/NUV magnitude, AB mag
408-412 F5.2 mag e_NUVmag ?=99.99 Uncertainty in NUVmag
414 A1 --- l_FUVflux Lower limit flag on FUVflux
416-423 F8.2 uJy FUVflux ?=99.99 GALEX/FUV flux, uJy
425-429 F5.2 uJy e_FUVflux ?=99.99 Uncertainty in FUVflux, uJy
431 A1 --- l_NUVflux Upper limit flag on NUVflux
433-440 F8.2 uJy NUVflux ?=99.99 GALEX/NUV flux, uJy
442-447 F6.2 uJy e_NUVflux ?=99.99 Uncertainty in NUVflux, uJy
449-453 F5.2 [-] logRx ?=99.99 fractional X-ray luminosity, log
455-459 F5.2 [Lsun] logLsun ?=99.99 log(L/Lsun), bolometric luminosity (7)
461-468 E8.2 W Lbol ?=9.99e+01 bolometric luminosity, watts
470-475 F6.2 [mW/m2] fROSAT ?=99.99 ROSAT X-ray flux, log10, erg/s/cm2
477-481 F5.2 [mW/m2] fsROSAT ?=99.99 ROSAT X-ray surface flux,
log10, erg/s/cm2
483-487 F5.2 [10-7W] LROSAT ?=99.99 ROSAT X-ray luminosity, log10, erg/s
489-493 F5.2 [-] RxROSAT ?=99.99 RxROSAT ROSAT Rx = Lx/Lbol, log10
495-500 F6.2 [mW/m2] fXMM ?=99.99 XMM X-ray flux, log10, erg/s/cm2
502-506 F5.2 [mW/m2] fsXMM ?=99.99 XMM X-ray surface flux,
log10, erg/s/cm2
508-512 F5.2 [10-7W] LXMM ?=99.99 XMM X-ray luminosity, log10, erg/s
514-518 F5.2 [-] RxXMM ?=99.99 XMM Rx = Lx/Lbol, log10
520-525 F6.2 [mW/m2] fChan ?=99.99 Chandra X-ray flux, log10, erg/s/cm2
527-531 F5.2 [mW/m2] fsChan ?=99.99 Chandra X-ray surface flux,
log10, erg/s/cm2
533-537 F5.2 [10-7W] LChan ?=99.99 Chandra X-ray luminosity, log10, erg/s
539-543 F5.2 [-] RxChan ?=99.99 Chandra Rx = Lx/Lbol, log10
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Note (1): Sun-centered system of locating objects in the solar system in
three-dimensions along the Cartesian X, Y and Z axes.
Note (2): Reference sources for Teff and logg as follows:
PASTEL = Soubiran et al. (2016A&A...591A.118S 2016A&A...591A.118S), and references therein;
Gray = Gray et al. (2003AJ....126.2048G 2003AJ....126.2048G, 2006AJ....132..161G 2006AJ....132..161G);
VF05 = Valenti & Fischer (2005ApJS..159..141V 2005ApJS..159..141V);
Takeda = Takeda et al. (2007PASJ...59.1127T 2007PASJ...59.1127T);
B-V = see paper;
V-K = see paper.
Note (3): Presence of a planet at the time of this publication, based on the
NASA Exoplanet Archive.
Note (4): B and V magnitudes take from the PASTEL catalog,
Soubiran et al. (2016A&A...591A.118S 2016A&A...591A.118S, Cat. B/pastel)
Note (5): If known to be a member of a multiple, to which component the HIP
number is referring (A, B, etc). If the HIP number includes more than
one star, either a known or suspected unresolved/very faint companion,
noted by a "+" symbol, e.g., A+. If more than one star in the system has
its own HIP number, the other associated HIP number is given in HIP2.
Note (6): An asterisk (*) indicates that the Houk spectral type was adjusted
to modern MK system (using Gray et al. 2003AJ....126.2048G 2003AJ....126.2048G,
2006AJ....132..161G 2006AJ....132..161G spectral types) following Pecaut & Mamajek
(2016MNRAS.461..794P 2016MNRAS.461..794P).
Note (7): Bolometric luminosities given in units of the IAU nominal solar
luminosity: LSun = 3.828E+26 W (Prsa et al. 2016AJ....152...41P 2016AJ....152...41P).
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Acknowledgements:
Natalie Hinkel, natalie.hinkel(at)gmail.com
(End) Patricia Vannier [CDS] 05-Dec-2017