J/ApJS/274/40     The BDKP. VI. Radial & rot. vel. from APOGEE     (Hsu+, 2024)

The Brown Dwarf Kinematics Project (BDKP). VI. Ultracool dwarf radial and rotational velocities from SDSS/APOGEE high-resolution spectroscopy. Hsu C.-C., Burgasser A.J., Theissen C.A., Birky J.L., Aganze C., Gerasimov R., Schmidt S.J., Blake C.H., Covey K.R., Moreno-Hilario E., Gelino C.R., Serna J., Brownstein J.R., Cunha K. <Astrophys. J. Suppl. Ser., 274, 40 (2024)> =2024ApJS..274...40H 2024ApJS..274...40H
ADC_Keywords: Spectra, infrared; Optical; Radial velocities; Stars, brown dwarf; Rotational velocities; Space velocities; Effective temperatures; Spectral types; Proper motions Keywords: Brown dwarfs ; Low mass stars ; Radial velocity ; Stellar rotation ; High resolution spectroscopy ; Stellar kinematics Abstract: We present precise measurements of radial (RV) and projected rotational (vsini) velocities of a sample of 258 M6 to L2 dwarfs with multiepoch, high-resolution (λ/Δλ=22500), near-infrared (1.514-1.696µm) spectroscopic observations reported in the Apache Point Observatory Galactic Evolution Experiment Data Release 17. The spectra were modeled using a Markov Chain Monte Carlo forward-modeling method, which achieved median precisions of σRV=0.4km/s and σvsini=1.1km/s. One-half of our sample (138 sources) are previously known members of nearby young clusters and moving groups, and we identified three new kinematic members of the Argus or Carina Near moving groups, 2MASS J05402570+2448090, 2MASSJ14093200+4138080, and 2MASS J21272531+5553150. Excluding these sources, we find that the majority of our sample have kinematics consistent with the Galactic thin disk, and 11 sources are associated with the intermediate thin/thick disk. The field sample has a velocity dispersion of 38.2±0.3km/s, equivalent to an age of 3.30±0.19Gyr based on empirical age-velocity dispersion relations, and a median vsini of 17km/s. For 172 sources with multiepoch observations, we identified 37 as having significant RV variations, and determined preliminary orbit parameters for 26 sources with four or more epochs, nine of which are short-period binary candidates. For 40 sources with photometric variability periods from the literature less than 5 days and vsini>20km/s, we find a decline in projected radii (Rsini) with age congruent with evolutionary models. Finally, we also present multiepoch RV and vsini measurements for additional 444 candidate ultracool dwarfs. Description: Our ultracool dwarf (UCD) sample was curated from APOGEE DR17 (Abdurro'uf+ 2022, III/286) of SDSS-IV based on observations obtained with the 2.5m Sloan Foundation Telescope at the Apache Point Observatory and the 2.5m du Pont Telescope at the Las Campanas Observatory. Our "gold" sample was based on sources with classifications of M6 and later as reported in SIMBAD, the Late-Type Extension to MoVeRS (Theissen+ 2016, J/AJ/151/41 & 2017, J/AJ/153/92), Reyle (2018, J/A+A/619/L8), Best+ (2021, J/AJ/161/42), or reported in this work. We use the most recent spectroscopic classification as our adopted value. See Section 2.1. The majority of sources in our full sample lack published spectroscopic classifications. To bolster this sample, we obtained additional low-resolution optical spectra with the Kast Double Spectrograph on the Shane 3m Telescope at the Lick Observatory over multiple nights between 2018 January 21 and 2022 March 11. We used the 600/7500 grating and 2" slit to obtain 6000-9000Å spectra at an average resolution of R∼1800. See Section 2.2. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 144 258 APOGEE DR17 gold sample table4.dat 184 979 Spectral model fit parameters for gold sample table5.dat 105 258 Radial velocity and vsini measurements with ASPCAP and literature comparison table6.dat 110 258 Radial velocities and heliocentric space motions table7.dat 103 258 Galactic orbital parameters tablea1.dat 125 468 APOGEE DR17 full sample tablea2.dat 184 1543 Spectral model fit parameters for full sample tablea3.dat 52 444 Summary of RV and vsini measurements of APOGEE DR17 full sample refs.dat 71 121 References -------------------------------------------------------------------------------- See also: III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997) II/179 : Southern Spectrophotometric Standards. 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(Wilson+, 2018) J/A+A/623/A127 : Homogeneous sample of 34000 M7-M9.5 dwarfs (Ahmed+, 2019) J/A+A/626/A11 : Corona Australis ALMA and X-Shooter data (Cazzoletti+, 2019) J/MNRAS/485/2167 : M-type stars in LAMOST DR5 unclassified spectra (Guo+, 2019) J/AJ/157/231 : MLSDSS-GaiaDR2 sample of M and L dwarfs (Kiman+, 2019) J/AJ/157/196 : Close companions around young stars (Kounkel+, 2019) J/ApJS/243/28 : M-type star magnetic activities (Lu+, 2019) J/ApJ/878/21 : Vertical motions of APOGEEGaia red clump stars (Ting+, 2019) J/ApJS/244/8 : M-type stars in LAMOST DR5 (Zhong+, 2019) J/ApJ/892/31 : Metallicities of M dwarfs in APOGEE DR14 (Birky+, 2020) J/A+A/633/A99 : Gaia DR2 open clusters in the MW. II (Cantat-Gaudin+, 2020) J/A+A/640/A1 : Portrait Galactic disc (Cantat-Gaudin+, 2020) J/AJ/159/199 : OCCAM. IV. Open cluster abund. using APOGEE (Donor+, 2020) J/MNRAS/493/4533 : NIR spectroscopic study of young M dwarfs (Khata+, 2020) J/MNRAS/498/5972 : Variables & dippers in young associations (Nardiello, 2020) J/ApJ/903/55 : APOGEE parameters through 83 open clusters (Poovelil+, 2020) J/AJ/160/38 : Spitzer variability in 79 brown dwarfs (Vos+, 2020) J/AJ/161/42 : Volume-limited sample of cool dwarfs. I. L0-T8 (Best+, 2021) J/A+A/649/A6 : Gaia Catalog of Nearby Stars (Gaia collaboration, 2021) J/ApJS/257/45 : BDKP. V. Radial & rot. veloc. of M, L, T dwarfs (Hsu+, 2021) J/ApJ/916/77 : K2 rot. periods for SDSS & Gaia M dwarfs (Popinchalk+, 2021) J/A+A/649/A147 : Spectroscopic parameters for 313 M dwarfs (Sarmento+, 2021) J/A+A/645/A100 : SPECULOOS. Ultracool dwarf transit survey (Sebastian+, 2021) J/A+A/647/A19 : 3D Kinematics and age of OCs (Tarricq+, 2021) J/AJ/161/63 : M dwarfs with 0.1≲M☉≲0.3 within 15pc (Winters+, 2021) J/ApJS/258/16 : TESS Eclipsing Binary stars. I. Sectors 1-26 (Prsa+, 2022) J/MNRAS/528/5703 : 23 low mass stars photometry (Swayne+, 2024) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) 25- 34 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 36- 45 F10.6 deg DEdeg Declination in decimal degrees (J2000) 47- 65 I19 --- Gaia ? Gaia eDR3 identifier 67- 74 A8 --- SpType Spectral type 76- 81 A6 --- r_SpType Reference code(s) for SpType (see refs.dat file) 83- 84 I2 --- NObs [1/20] Number of observations 86- 91 F6.3 mag Hmag [7.6/14.7] 2MASS H band apparent magnitude 93- 97 F5.3 mag e_Hmag [0.01/0.1] Uncertainty in Hmag 99-106 F8.2 mas/yr pmRA [-1114/647] Gaia eDR3 Proper motion along RA 108-112 F5.2 mas/yr e_pmRA [0.02/44] Uncertainty in pmRA 114-120 F7.2 mas/yr pmDE [-835/598] Gaia eDR3 Proper motion along DE 122-126 F5.2 mas/yr e_pmDE [0.02/40] Uncertainty in pmDE 128-129 I2 --- pmRef [15/99] Reference code for proper motions (see refs.dat file) 131-136 F6.2 mas plx [2.4/280] Gaia eDR3 parallax 138-141 F4.2 mas e_plx [0.02/7] Uncertainty in plx 143-144 I2 --- r_plx [33/99] Reference code for plx (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) 25- 29 I5 --- Plate [5217/12810] Plate number 31- 34 I4 --- Loc [2048/7240] Location identifier 36- 38 I3 --- Fiber [1/300] Fiber identifier 40- 50 F11.3 d JD Julian Date of the observation 52- 57 F6.2 km/s Bary [-31/31] Barycentric correction 59- 61 I3 --- S/N [8/275] Signal-to-Noise 63- 67 F5.1 km/s RVel [-76.4/71] Radial velocity (2)(3)(1) 69- 72 F4.1 km/s E_RVel [0.2/13] Upper uncertainty in RVel 74- 76 F3.1 km/s e_RVel [0.2/6] Lower uncertainty in RVel 78- 82 F5.1 km/s RVavg [-76.4/70]? Weighted average over all epoch's radial velocity (1)(2)(3) 84- 86 F3.1 km/s E_RVavg [0.3/2]? Upper uncertainty in RVavg 88- 90 F3.1 km/s e_RVavg [0.3/2]? Lower uncertainty in RVavg 92- 95 F4.1 km/s vsini [0.4/100] Projected rotation velocity (1)(2) 97- 99 F3.1 km/s E_vsini [1/5.2] Upper uncertainty in vsini 101-103 F3.1 km/s e_vsini [1/7] Lower uncertainty in vsini 105 A1 --- l_vsiniAvg Limit flag on vsiniAvg 106-110 F5.1 km/s vsiniAvg [10/100]? Weighted average over all epoch's projected rotation velocity (1)(2)(4) 112-114 F3.1 km/s E_vsiniAvg [0.6/4.1]? Upper uncertainty in vsiniAvg 116-118 F3.1 km/s e_vsiniAvg [1/7]? Lower uncertainty in vsiniAvg 120-125 F6.1 K Teff [2283/3574] Effective temperature (1)(5) 127-130 F4.1 K E_Teff [0.1/89] Upper uncertainty in Teff 132-135 F4.1 K e_Teff [0.2/96] Lower uncertainty in Teff 137-142 F6.1 K TeffAvg [2380/3574]? Weighted average over all epoch's effective temperature (1)(5) 144-147 F4.1 K E_TeffAvg [0.1/60]? Upper uncertainty in TeffAvg 149-152 F4.1 K e_TeffAvg [0.1/86]? Lower uncertainty in TeffAvg 154-157 F4.2 [cm/s2] logg [3.5/5.5] Log surface gravity (1)(5) 159-162 F4.2 [cm/s2] E_logg [0/0.4] Upper uncertainty in logg 164-167 F4.2 [cm/s2] e_logg [0/0.4] Lower uncertainty in logg 169-172 F4.2 [cm/s2] loggAvg [3.5/5.5]? Weighted average over all epoch's log surface gravity (1)(5) 174-177 F4.2 [cm/s2] E_loggAvg [0/0.2]? Upper uncertainty in loggAvg 179-182 F4.2 [cm/s2] e_loggAvg [0/0.3]? Lower uncertainty in loggAvg 184 A1 --- Models Models used (6) -------------------------------------------------------------------------------- Note (1): Measurements from individual spectra over individual or multiple epochs are combined using inverse uncertainty weighting (weight=1/(σ2upper2lower)); upper and lower uncertainties are also combined using inverse uncertainty-squared weighting. In cases where individual spectra have S/N<10, spectral data are combined first, then modeled. Note (2): Systematic uncertainties of 0.19km/s and 0.95km/s are added to RVel and vsin(i) measurements, respectively. See Sections 4.1 and 4.2 for details. Note (3): We did not apply the effective temperature dependent correction to RV from Kounkel+ 2019, J/AJ/157/196 for 2MASS J04201611+2821325, 2MASS J04262939+2624137, 2MASS J04294568+2630468, 2MASS J04330945+2246487, and 2MASS J04363893+2258119. See Section 4.1 for details. Note (4): Averaged vsin(i)<10km/s is below our vsin(i) detection limit; see Section 4.2 for details. Note (5): Readers should not take our Teff and log g measurements as accurate. We report these values only for the reproducibility of our work. See Section 4.4 for details. Note (6): Model as follows: S = Sonora 2018 (Marley+ 2018, doi:10.5281/zenodo.2628068, 2021ApJ...920...85M 2021ApJ...920...85M) B = BT-Settl (Baraffe+ 2015A&A...577A..42B 2015A&A...577A..42B) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) 25- 30 F6.2 km/s RVavg [-76.1/67] Weighted average over all epochs radial velocity (1)(2) 32- 35 F4.2 km/s E_RVavg [0.19/2] Upper uncertainty in RVavg 37- 40 F4.2 km/s e_RVavg [0.2/1.7] Lower uncertainty in RVavg 42- 48 F7.2 km/s RVASP [-891.4/1047]? Radial velocity from DR17 ASPCAP pipeline 50- 56 F7.2 km/s e_RVASP [0.1/1087]? Uncertainty in RVASP 58- 63 F6.2 km/s RVLit [-76.5/54]? Literature radial velocity 65- 69 F5.2 km/s e_RVLit [0.01/30]? Uncertainty in RVLit 71- 73 I3 --- r_RVLit [101/120]? Reference code for RVLit (see refs.dat file) 75 A1 --- l_vsiniAvg Limit flag on vsiniAvg 76- 80 F5.2 km/s vsiniAvg [10/93] Weighted average over all epochs projected rotation velocity (1) 82- 85 F4.2 km/s E_vsiniAvg [0.9/4]? Upper uncertainty in vsiniAvg 87- 90 F4.2 km/s e_vsiniAvg [0.9/2]? Lower uncertainty in vsiniAvg 92- 96 F5.2 km/s vsiniLit [7/63]? Literature projected rotation velocity 98-101 F4.2 km/s e_vsiniLit [0.17/8]? Uncertainty in vsiniLit 103-105 I3 --- r_vsiniLit [104/118]? Reference code for vsiniLit (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Measurements from individual spectra over individual or multiple epochs are combined using inverse uncertainty weighting (weight=1/(σ2upper2lower)); upper and lower uncertainties are also combined using inverse uncertainty-squared weighting. In cases where individual spectra have S/N<10, spectral data are combined first, then modeled. Note (2): We did not apply the effective temperature dependent correction to RV from Kounkel+ 2019, J/AJ/157/196 for 2MASS J04201611+2821325, 2MASS J04262939+2624137, 2MASS J04294568+2630468, 2MASS J04330945+2246487, and 2MASS J04363893+2258119. See Section 4.1 for details. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) 25- 27 A3 --- f_2MASS Flag on ID (1) 29- 32 A4 --- SpT Spectral type 34- 39 F6.2 km/s RVel [-76.1/67] Adpoted radial velocity 41- 44 F4.2 km/s E_RVel [0.19/2] Upper uncertainty in RVel 46- 49 F4.2 km/s e_RVel [0.2/1.7] Lower uncertainty in RVel 51- 55 F5.1 km/s U [-74.6/83.3] Heliocentric U space motion 57- 60 F4.1 km/s e_U [0/44.4] Uncertainty in U 62- 66 F5.1 km/s V [-85/33.3] Heliocentric V space motion 68- 71 F4.1 km/s e_V [0/72.5] Uncertainty in V 73- 77 F5.1 km/s W [-33/51] Heliocentric W space motion 79- 82 F4.1 km/s e_W [0/80] Uncertainty in W 84- 87 F4.2 --- P[TD]/P[D] [0.01/4.4] Galactic population probability ratio of thick disk to thin disk (2) 89- 92 A4 --- Pop Galactic population type (2) 94- 98 A5 % Prob BANYAN Σ membership probability 100- 110 A11 --- Mem BANYAN Σ membership (3) -------------------------------------------------------------------------------- Note (1): Flag as follows: b = Known or candidate binary. d = Reported in the literature or a new member of young moving groups. e = Reported as a member of NGC 1333 in Cantat-Gaudin+ 2018, J/A+A/618/A93; Yao+ 2018, J/ApJ/869/72; Cantat-Gaudin & Anders 2020, J/A+A/633/A99; Cantat-Gaudin+ 2020, J/A+A/640/A1, but we did not identify because NGC 1333 is not included in BANYAN Σ. f = Reported as a member of the Castor Moving Group in Zuckerman+ 2013ApJ...778....5Z 2013ApJ...778....5Z, but we did not identify it because the Castor Moving Group is not included in BANYAN Σ. Note (2): Galactic thin disk (D), thick disk (TD), intermediate populations (D/TD) are assigned according to probability ratios P(TD)/P(D)<0.1, P(TD)/P(D)>10, and 0.1<P(TD)/P(D)<10, respectively, following Bensby+ 2003, J/A+A/410/527 Note (3): BANYAN Σ young moving group name abbreviation follows those defined in Gagne+ 2018, J/ApJ/856/23: AB Doradus (ABDMG), Argus (ARG), Carina- Near (CARN), Coma Berenices (CBER), Corona Australis (CRA), Hyades (HYA), Taurus (TAU), Upper Centaurus-Lupus (UCL), Upper Corona Australis (UCRA), and Upper Scorpius (USCO). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) (1) 25- 30 F6.4 kpc Rmin [3.8/8.5] Minimum distance from galactic center 32- 37 F6.4 kpc e_Rmin [0.0002/2] Uncertainty in Rmin 39- 46 F8.5 kpc Rmax [8/15] Maximum distance from galactic center 48- 55 F8.5 kpc e_Rmax [0.0001/17] Uncertainty in Rmax 57- 63 F7.5 kpc Zmax [0.005/1] Maximum height above the galactic plane 65- 71 F7.5 kpc e_Zmax [3e-05/3] Uncertainty in Zmax 73- 79 F7.5 --- e [0.006/0.4] Eccentricity 81- 87 F7.5 --- e_e [9e-05/0.3] Uncertainty in e 89- 95 F7.5 deg i [0.038/5.4] Inclination 97-103 F7.5 deg e_i [0.0001/7] Uncertainty in i -------------------------------------------------------------------------------- Note (1): The large uncertainties of Galactic orbital parameters of 2MASS J05350162-0521489 are due to its large proper motion uncertainty (µRAcos(DE)=0±44mas/yr and µDE=0±40mas/yr; Cutri+ 2014, II/328). -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) 25- 34 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 36- 45 F10.6 deg DEdeg Declination in decimal degrees (J2000) 47- 65 I19 --- Gaia Gaia eDR3 identifier 67- 70 A4 --- SpT Spectral type 72- 73 I2 --- NObs [1/32] Number of observations 75- 80 F6.3 mag Hmag [9/14.7] 2MASS H band apparent magnitude 82- 86 F5.3 mag e_Hmag [0.015/0.1] Uncertainty in Hmag 88- 95 F8.2 mas/yr pmRA [-1483/931] Gaia eDR3 Proper motion along RA 97-100 F4.2 mas/yr e_pmRA [0.02/0.8] Uncertainty in pmRA 102-108 F7.2 mas/yr pmDE [-712/807] Gaia eDR3 Proper motion along DE 110-113 F4.2 mas/yr e_pmDE [0.02/0.8] Uncertainty in pmDE 115-120 F6.2 mas plx [2.5/117] Gaia eDR3 parallax 122-125 F4.2 mas e_plx [0.02/0.8] Uncertainty in plx -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [2MASS] 7- 23 A17 --- 2MASS APOGEE identifier (JHHMMSSss+DDMMSSs) 25- 29 F5.1 km/s RVel [-76.4/70] Weighted average over all epoch's radial velocity 31- 33 F3.1 km/s E_RVel [0.3/2] Upper uncertainty in RVel 35- 37 F3.1 km/s e_RVel [0.3/2] Lower uncertainty in RVel 39 A1 --- l_vsini Limit sign on vsini 40- 44 F5.1 km/s vsini [10/100] Weighted average over all epoch's projected rotation velocity 46- 48 F3.1 km/s E_vsini [0.6/4.1]? Upper uncertainty in vsini 50- 52 F3.1 km/s e_vsini [1/6.6]? Lower uncertainty in vsini -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference code 5- 29 A25 --- Auth First author's name(s) 31- 49 A19 --- BibCode Bibcode of the reference 51- 71 A21 --- Cat Reference of the catalog in VizieR -------------------------------------------------------------------------------- History: From electronic version of the journal References: Faherty et al. Paper I. 2009AJ....137....1F 2009AJ....137....1F Cat. J/AJ/137/1 Faherty et al. Paper II. 2010AJ....139..176F 2010AJ....139..176F Faherty et al. Paper III. 2012ApJ...752...56F 2012ApJ...752...56F Cat. J/ApJ/752/56 Burgasser et al. Paper IV. 2015ApJS..220...18B 2015ApJS..220...18B Cat. J/ApJS/220/18 Hsu et al. Paper V. 2021ApJS..257...45H 2021ApJS..257...45H Cat. J/ApJS/257/45
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 11-Mar-2025
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