J/AJ/155/180    A catalog of cool dwarf targets for the TESS   (Muirhead+, 2018)

A catalog of cool dwarf targets for the Transiting Exoplanet Survey Satellite. Muirhead P.S., Dressing C.D., Mann A.W., Rojas-Ayala B., Lepine S., Paegert M., De Lee N., Oelkers R. <Astron. J., 155, 180-180 (2018)> =2018AJ....155..180M 2018AJ....155..180M (SIMBAD/NED BibCode)
ADC_Keywords: Stars, dwarfs ; Stars, late-type ; Stars, K-type ; Stars, M-type ; Photometry, ultraviolet ; Photometry, UBVRIJKLMNH ; Photometry, SDSS ; Proper motions ; Stars, distances Keywords: planetary systems - stars: fundamental parameters - stars: late-type - stars: low-mass Abstract: We present a catalog of cool dwarf targets (V-J>2.7, Teff~<4000 K) and their stellar properties for the upcoming Transiting Exoplanet Survey Satellite (TESS), for the purpose of determining which cool dwarfs should be observed using two minute observations. TESS has the opportunity to search tens of thousands of nearby, cool, late K- and M-type dwarfs for transiting exoplanets, an order of magnitude more than current or previous transiting exoplanet surveys, such as Kepler, K2, and ground-based programs. This necessitates a new approach to choosing cool dwarf targets. Cool dwarfs are chosen by collating parallax and proper motion catalogs from the literature and subjecting them to a variety of selection criteria. We calculate stellar parameters and TESS magnitudes using the best possible relations from the literature while maintaining uniformity of methods for the sake of reproducibility. We estimate the expected planet yield from TESS observations using statistical results from the Kepler mission, and use these results to choose the best targets for two minute observations, optimizing for small planets for which masses can conceivably be measured using follow-up Doppler spectroscopy by current and future Doppler spectrometers. The catalog is available in machine readable format and is incorporated into the TESS Input Catalog and TESS Candidate Target List until a more complete and accurate cool dwarf catalog identified by ESA's Gaia mission can be incorporated. Description: In this paper, we describe a catalog of cool dwarfs for two minute TESS observations using archival parallaxes where available, or proper motion observations from the SUPERBLINK program (Lepine & Gaidos 2011, J/AJ/142/138), in combination with a variety of photometric catalogs. As a base catalog for determining cool dwarfs for TESS observations, we therefore adopted the SUPERBLINK catalog as the primary source of targets. Although SUPERBLINK already lists 2MASS magnitudes for most objects, we independently cross-matched the catalog again with 2MASS in order to obtain the 2MASS photometric flags. SUPERBLINK contains Tycho-2 V-band magnitudes where available (Hog et al. 2000, Cat. I/259). More recent visible magnitudes are available from the American Association Variable Star Observers Photometric All-sky Survey (APASS, Henden & Munari 2014CoSka..43..518H 2014CoSka..43..518H) catalog. APASS contains Landolt B and V magnitudes, and SDSS-like g', r' and i' magnitudes for roughly 2.5 million stars. We therefore cross-matched SUPERBLINK with APASS in addition to 2MASS. Cross-matching between the three catalogs was performed using a PostgreSQL database maintained at Vanderbilt University for the purpose of determining the TESS Input Catalog and the Candidate Target List (TIC and CTL; Stassun et al. 2018AJ....156..102S 2018AJ....156..102S) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 611 1140225 The cool dwarf catalog -------------------------------------------------------------------------------- See also: I/259 : The Tycho-2 Catalogue (Hog+ 2000) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/337 : Gaia DR1 (Gaia Collaboration, 2016) II/336 : AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016) J/ApJS/94/749 : RI photometry of cool dwarfs (Kirkpatrick+ 1994) J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005) J/AJ/142/138 : All-sky catalog of bright M dwarfs (Lepine+, 2011) J/ApJ/779/188 : Spectra of nearby late K and M Kepler stars (Mann+, 2013) J/ApJ/800/85 : Teff, radii and luminosities of cool dwarfs (Newton+, 2015) J/ApJ/809/77 : Transiting Exoplanet Survey Satellite (TESS) (Sullivan+, 2015) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 I10 --- TMCNTR [2546/1340033412] Parameter used for cross-matching catalogs 12- 19 F8.4 deg RAdeg Right Ascension in decimal degrees (J2000) 21- 28 F8.4 deg DEdeg Declination in decimal degrees (J2000) 30- 35 F6.3 mag Vmag [1.35/20.92] V band magnitude 37- 42 F6.3 mag e_Vmag [-0.263/3.481] Uncertainty in Vmag 44- 49 A6 --- f_Vmag Flag indicating source for Vmag (apass, tycho or sblink) 51- 56 F6.3 mag TESSmag [-0.383/23.446]? TESS magnitude 58- 62 F5.3 mag e_TESSmag [0/6.677]? Uncertainty in TESSmag 64- 76 A13 --- f_TESSmag Flag indicating method for determining TESSmag (1) 78- 81 I4 K Teff [2500/4243]? Effective temperature 83- 86 I4 K e_Teff [60/7055]? Uncertainty in Teff 88- 94 A7 --- f_Teff Flag indicating method for determining Teff (2) 96-100 F5.3 Rsun R* [0.112/0.727] Stellar radius 102-106 F5.3 Rsun e_R* [0.003/3.633] Uncertainty in R* 108-116 A9 --- f_R* Flag indicating method for determining R* (3) 118-122 F5.3 Msun M* [0.078/0.718] Stellar mass 124-128 F5.3 Msun e_M* [0.001/4.505] Uncertainty in M* 130-140 A11 --- f_M* Flag indicating method for determining M* (4) 142-148 I7 --- SblinkPK [1/2704782] Parameter used for cross-matching catalogs 150-165 A16 --- Sblink Superblink star designation (PM IHHMMm+DDMMWw) 167-172 I6 --- HIP [112/120005]? Hipparcos catalog number 174-177 I4 --- TYC1 [4/9536]? Tycho-2 catalog number 1 179-182 I4 --- TYC2 [2/5848]? Tycho-2 catalog number 2 184 I1 --- TYC3 [1/3]? Tycho-2 catalog number 3 186-197 F12.8 deg RAGdeg ? GAIA-revised Right Ascension in decimal degrees (J2000) 199-210 F12.8 deg DEGdeg ? GAIA-revised Declination in decimal degrees (J2000) 212-218 F7.5 arcsec/yr pm [0/8.65115] GAIA-revised total proper motion 220-227 F8.5 arcsec/yr pmRA [-4.02083/6.49529] GAIA-revised proper motion in RA 229-236 F8.5 arcsec/yr pmDE [-5.71434/1.85853] GAIA-revised proper motion in DE 238-247 F10.6 deg RAOdeg Original Right Ascension in decimal degrees (J2000) 249-258 F10.6 deg DEOdeg Original Declination in decimal degrees (J2000) 260-265 F6.3 arcsec/yr pmO [0.006/10.358] Original total proper motion 267-272 F6.3 arcsec/yr pmRAO [-4.411/6.767] Original proper motion in RA 274-279 F6.3 arcsec/yr pmDEO [-5.731/10.327] Original proper motion in DE 281-286 F6.4 ct/s FX [0/3.91]? X-ray flux from ROSAT 288-292 F5.2 mag FUV [13.38/26.19]? Far-UV magnitude from GALEX 294-298 F5.2 mag NUV [13.72/26.65]? Near-UV magnitude from GALEX 300-304 F5.2 mag BTmag [0/22.23]? Tycho-2 BT magnitude 306-310 F5.2 mag VTmag [0/14.87]? Tycho-2 VT magnitude 312-317 F6.3 mag Gmag [5.866/21.172]? GAIA G magnitude 319-322 F4.1 mag BJmag [0/24.7]? Photographic blue (IIIaJ) magnitude 324-327 F4.1 mag RFmag [0/24.9]? Photographic red (IIIaF) magnitude 329-332 F4.1 mag INmag [0/20]? Photographic infrared (IVN) magnitude 334-338 F5.2 mag Jmag [-1.45/17.49]? 2MASS infrared J magnitude 340-344 F5.2 mag Hmag [-1.89/27.77]? 2MASS infrared H magnitude 346-350 F5.2 mag Ksmag [-2.01/17.22]? 2MASS infrared Ks magnitude 352-356 F5.2 mag umag [12.01/27.54]? SDSS u magnitude 358-362 F5.2 mag gmag [7.97/24.58]? SDSS g magnitude 364-368 F5.2 mag rmag [8.07/28.56]? SDSS r magnitude 370-374 F5.2 mag imag [7.11/28.35]? SDSS i magnitude 376-380 F5.2 mag zmag [8.13/23.1]? SDSS z magnitude 382-386 F5.2 mag VmagS [0/21.72]? SUPERBLINK estimated V magnitude 388-392 F5.2 mag V-J [-1.92/8.86]?=99.9 SUPERBLINK estimated V-J color 394-400 F7.5 arcsec Plxtr [0.001/0.7969]? Trigonometric parallax 402-408 F7.5 arcsec e_Plxtr [0.0001/0.047]? Error in Plxtr 410-413 A4 -- r_Plxtr Source of Plxtr 415-420 F6.4 arcsec Plxph [0.0001/0.8758]? Photometric parallax 422-427 F6.4 arcsec e_Plxph [0.0001/0.2627]? Error in Plxph 429-431 A3 -- r_Plxph Source of Plxph 433-436 F4.1 arcsec Dist [0.2/15]? GAIA close companion distance 438-441 F4.1 mag Cmag [0/11.8]? GAIA close companion magnitude 443-452 I10 --- 2MASSID [2546/1340033412] 2MASS Center Idenifying Number used for cross-matching catalogs 454-463 F10.6 deg RAAdeg ? APASS Right Ascension in decimal degrees (J2000) 465-469 F5.3 arcsec e_RAAdeg ? Uncertainty in RAAdeg 471-480 F10.6 deg DEAdeg ? APASS Declination in decimal degrees (J2000) 482-486 F5.3 arcsec e_DEAdeg ? Uncertainty in DEAdeg 488-490 I3 --- Nobs [2/369]? Number of APASS observed nights 492-495 I4 --- Nimg [2/2770]? Number of APASS images for this field 497-502 F6.3 mag VmagA [7.282/19.225]? Johnson APASS V-band magnitude 504-509 F6.3 mag B-V [-1.696/5.721]? APASS B-V color index 511-516 F6.3 mag BmagA [8.447/22.694]? Johnson APASS B-band magnitude 518-523 F6.3 mag gmagA [8.126/19.972]? APASS g'-band AB magnitude 525-530 F6.3 mag rmagA [7.316/18.202]? APASS r'-band AB magnitude 532-537 F6.3 mag imagA [6.636/20.479]? APASS i'-band AB magnitude 539-543 F5.3 mag e_VmagA [0.004/3.481]? Uncertainty in VmagA 545-549 F5.3 mag e_B-V [0.001/4.88]? Uncertainty in B-V 551-555 F5.3 mag e_BmagA [0.004/2.986]? Uncertainty in BmagA 557-561 F5.3 mag e_gmagA [0.004/2.486]? Uncertainty in gmagA 563-567 F5.3 mag e_rmagA [0.003/2.29]? Uncertainty in rmagA 569-573 F5.3 mag e_imagA [0.003/3.063]? Uncertainty in imagA 575-591 A17 --- 2MASS 2MASS source designation (HHMMSSss+DDMMSSs) 593-611 I19 --- Gaia ? Gaia source identifier -------------------------------------------------------------------------------- Note (1): The flag assigned to the TESS magnitude T can take one of five flags: fromapassik, fromsdssik, wmeanvkjhk, vk, or no_kmag. The first two use a combination of i band (from either APASS or SDSS, respectively) and 2MASS K band to determine T. The third uses a weighted mean between the V-K relation and the 2MASS only relation. The fourth uses only V-K, and the fifth indicates that the object does not have a reliable K-band magnitude, so a TESS magnitude could not be reliably determined. Note (2): The Teff flag is a combination of letters indicating which colors were used to determine the effective temperature. The combination can include rj, vj, and/or rz, each corresponding to the color used. The final Teff is the weighted average of all the color-Teff relations used. Note (3): The radius flag can take one of two strings: from_teff, indicating that it was determined from Teff or from_mk, indicating it was determined from the absolute K-band magnitude (Mann et al. 2015, J/ApJ/804/64). Note (4): The mass flag can take one of several strings: from_teff, frommkD00, indicating the Delfosse et al. (2000A&A...364..217D 2000A&A...364..217D) relations were used or frommkB16, indicating the Benedict et al. (2016, J/AJ/152/141) relations were used. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Tiphaine Pouvreau [CDS] 23-Nov-2018
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