J/ApJ/893/27    TRENDS high-contrast imaging survey. VIII.    (Gonzales+, 2020)

The TRENDS high-contrast imaging survey. VIII. Compendium of benchmark objects. Gonzales E.J., Crepp J.R., Bechter E.B., Wood C.M., Johnson J.A., Montet B.T., Isaacson H., Howard A.W. <Astrophys. J., 893, 27 (2020)> =2020ApJ...893...27G 2020ApJ...893...27G
ADC_Keywords: Stars, double and multiple; Stars, masses; Infrared sources Keywords: Astrometric binary stars ; Binary stars ; Visual binary stars ; Spectroscopic binary stars ; Direct imaging ; Brown dwarfs ; Low mass stars ; Radial velocity ; M stars Abstract: The physical properties of faint stellar and substellar objects often rely on indirect, model-dependent estimates. For example, the masses of brown dwarfs are usually inferred using evolutionary models, which are age dependent and have yet to be properly calibrated. With the goal of identifying new benchmark objects to test low-mass stellar and substellar models, we have carried out a comprehensive adaptive optics survey as part of the TaRgetting bENchmark-objects with the Doppler Spectroscopy (TRENDS) high-contrast imaging program. Using legacy radial velocity measurements from the High Resolution Echelle Spectrometer at Keck, we have identified several dozen stars that show long-term Doppler accelerations. We present follow-up high-contrast observations from the campaign and report the discovery of 31 comoving companions, as well as 11 strong candidate companions, to solar-type stars with well-determined parallax and metallicity values. Benchmark objects of this nature lend themselves to orbit determinations, dynamical mass estimates, and independent compositional assessment. This compendium of benchmark objects will serve as a convenient test group to substantiate theoretical evolutionary and atmospheric models near the hydrogen fusing limit. Description: Targets were selected by analyzing legacy RV time series data obtained from the High Resolution Echelle Spectrometer (HIRES) at Keck. Complementary RV data was also obtained from the publicly available Lick-Carnegie Exoplanet Survey (Butler+ 2017, J/AJ/153/208). Standard observing methods used by the California Planet Search (CPS) program (Howard+ 2010ApJ...721.1467H 2010ApJ...721.1467H) were implemented for RV observations as has been done with previous TRENDS discoveries. See Section 3. Reconnaissance imaging observations span several observing seasons starting as early as 2010 May. Observations were obtained in natural guide star AO mode using NIRC2 (Instrument PI: Keith Matthews) on the Keck II telescope. See Section 4. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 72 39 TRENDS system parameters table7.dat 45 133 Adaptive optics imaging observations table8.dat 116 107 Astrometry and photometry: confirmed companions table9.dat 116 15 Astrometry and photometry: candidate companions -------------------------------------------------------------------------------- See also: I/259 : The Tycho-2 Catalogue (Hog+ 2000) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005) J/A+A/485/571 : Metallicities & activities of southern stars (Jenkins+, 2008) J/MNRAS/403/1949 : UBV(RcIc)JHK photometry of HIP nearby stars (Koen+, 2010) J/ApJ/725/331 : Astrometry in the Galactic Center (Yelda+, 2010) J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010) J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012) J/ApJS/201/19 : Hawaii Infrared Parallax Program. I. (Dupuy+, 2012) J/ApJ/753/156 : T/Y brown dwarfs with WISE photometry (Kirkpatrick+, 2012) J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013) J/ApJS/225/10 : Kinematic analysis of M7-L8 dwarfs (Faherty+, 2016) J/AJ/153/208 : LCES HIRES/Keck RV Exoplanet Survey (Butler+, 2017) J/ApJS/231/15 : Astrometric monitoring of ultracool dwarf bin. (Dupuy+, 2017) J/AJ/155/159 : RVs of the late-T dwarf GL 758 B host star (Bowler+, 2018) J/AJ/155/180 : A catalog of cool dwarf targets for the TESS (Muirhead+, 2018) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Target name 10- 11 I2 h RAh Gaia DR2 Hour of right ascension (J2000) 13- 14 I2 min RAm Gaia DR2 Minute of right ascension (J2000) 16- 20 F5.2 s RAs Gaia DR2 Second of right ascension (J2000) 22 A1 --- DE- Gaia DR2 Sign of declination (J2000) 23- 24 I2 deg DEd Gaia DR2 Degree of declination (J2000) 26- 27 I2 arcmin DEm Gaia DR2 Arcminute of declination (J2000) 29- 33 F5.2 arcsec DEs Gaia DR2 Arcsecond of declination (J2000) 35- 39 F5.2 mas plx [5.13/44.4] Gaia DR2 parallax 41- 44 F4.2 mas e_plx [0.02/1.37] plx uncertainty 46- 52 F7.2 mas/yr pmRA [-565/402] Gaia DR2 proper motion in right ascension direction (pmRA*cosDE) 54- 57 F4.2 mas/yr e_pmRA [0.04/1.5] pmRA uncertainty 59- 65 F7.2 mas/yr pmDE [-359/367] Gaia DR2 proper motion in declination direction 67- 70 F4.2 mas/yr e_pmDE [0.04/1.6] pmDE uncertainty 72 A1 --- Comp "c"=confirmed companion; otherwise candidate companions -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Target name 10- 12 A3 --- m_Name Component identifier 14- 20 F7.1 d JD [15342.1/17500.5]? Julian date of observation; JD-2440000 22- 27 A6 --- Filt Filter used 29 A1 --- f_Filt [a] Flag on Filt (1) 31- 38 F8.3 s delt [0.5/2490]? Integration time, Δt 40- 43 I4 --- Array [128/1024]? Collecting array used with Keck/NIRC2 45 A1 --- Comp "c"=confirmed companion; otherwise candidate companions -------------------------------------------------------------------------------- Note (1): Flag as follows: a = Companion not resolved in filter, bad data, too small of a collecting area, or coronagraph used and occulted companion. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table[89].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Target name (1) 10- 11 A2 --- m_Name Component identifier 13- 19 A7 --- Filt Filter used 21- 24 F4.2 mag Delmag [0.4/6.1]? Magnitude difference in Filt (2) 26- 30 F5.3 mag e_Delmag [0/0.7]? Uncertainty in Deltamag (2) 32- 36 F5.2 mag CompMAG [1.3/10.8]? Companion absolute magnitude in Filt (2) 38- 41 F4.2 mag e_CompMAG [0.02/10]? Uncertainty in Mcomp (2) 43 A1 --- f_CompMAG [d] Flag on CompMAG (3) 45- 51 F7.2 mas Sep [75.9/4778] Angular separation 53- 57 F5.2 mas e_Sep [0.1/18] Uncertainty in Sep 59- 64 F6.2 deg PA [5/356] Position angle (4) 66- 69 F4.2 deg e_PA [0.01/4] Uncertainty in PA 71- 76 F6.2 AU ProjSep [6.7/393] Projected separation 78- 81 F4.2 AU e_ProjSep [0.01/2] Uncertainty in ProjSep 83- 89 F7.2 m/s/yr vdot [-366/643]? Instantaneous acceleration (2) 91- 95 F5.2 m/s/yr e_vdot [0.07/16.1]? Uncertainty in vdot (2) 97-101 F5.2 Msun MRVmin [0.02/80]? Minimum mass (2)(5) 103-106 F4.2 Msun e_MRVmin [0.01/5]? Uncertainty in MRVmin (2) 108-111 F4.2 Msun MPhot [0.08/1.4]? Photometric mass (2) 113-116 F4.2 Msun e_MPhot [0.01/0.4]? Uncertainty in MPhot (2) -------------------------------------------------------------------------------- Note (1): In Table 9, "HD156828 AC" was very likely a misprint for "HD156826 AC"; corrected at CDS. Note (2): A blank entry indicates that the observation set-up (see Table 7) did not allow for analysis of this value due to any of the following: Companion not resolved in filter, bad data, too small of collecting area, or coronograph used and occulted companion. Note (3): Flag as follows: d = Low quality results from 2MASS Survey (very poor photometry; see II/246) Note (4): Measured as East of North. In the event the images were taken in vertical angle mode, de-rotation of the images was performed to place each frame back into position angle mode. Note (5): SPOCS catalog used to obtain stellar mass measurement of the primary star and infer the dynamical minimum mass of the companion. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Crepp et al. Paper I. 2012ApJ...761...39C 2012ApJ...761...39C Crepp et al. Paper II. 2013ApJ...771...46C 2013ApJ...771...46C Crepp et al. Paper III. 2013ApJ...774....1C 2013ApJ...774....1C Montet et al. Paper IV. 2014ApJ...781...28M 2014ApJ...781...28M Crepp et al. Paper V. 2014ApJ...781...29C 2014ApJ...781...29C Crepp et al. Paper VI. 2016ApJ...831..136C 2016ApJ...831..136C Crepp et al. Paper VII. 2018ApJ...864...42C 2018ApJ...864...42C Gonzalez et al. Paper VIII. 2020ApJ...893...27G 2020ApJ...893...27G This catalog
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 04-Oct-2021
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