J/ApJ/883/205 Ultracool SpeXtroscopic survey. I. M7-L5 sample (Bardalez+, 2019)

The ultracool SpeXtroscopic survey. I. Volume-limited spectroscopic sample and luminosity function of M7-L5 ultracool dwarfs. Bardalez Gagliuffi D.C., Burgasser A.J., Schmidt S.J., Theissen C., Gagne J., Gillon M., Sahlmann J., Faherty J.K., Gelino C., Cruz K.L., Skrzypek N., Looper D. <Astrophys. J., 883, 205-205 (2019)> =2019ApJ...883..205B 2019ApJ...883..205B (SIMBAD/NED BibCode)
ADC_Keywords: Stars, brown dwarf; Stars, M-type; Stars, L-type; Spectral types; Spectra, infrared; Photometry, infrared; Stars, distances; Radial velocities; Proper motions Keywords: astronomical databases: miscellaneous; binaries: close binaries: general; brown dwarfs; infrared: stars stars: fundamental parameters Abstract: We present a volume-limited, spectroscopically verified sample of M7-L5 ultracool dwarfs (UCDs) within 25pc. The sample contains 410 sources, of which 93% have trigonometric distance measurements (80% from Gaia DR2) and 81% have low-resolution (R∼120), near-infrared (NIR) spectroscopy. We also present an additional list of 60 sources that may be M7-L5 dwarfs within 25pc when distance or spectral-type uncertainties are taken into account. The spectra provide NIR spectral and gravity classifications, and we use these to identify young sources, red and blue J-KS color outliers, and spectral binaries. We measure very low gravity and intermediate-gravity fractions of 2.1-0.8+0.9 and 7.8-1.5+1.7, respectively; fractions of red and blue color outliers of 1.4-0.5+0.6 and 3.6-0.9+1.0, respectively; and a spectral binary fraction of 1.6-0.5+0.5. We present an updated luminosity function for M7-L5 dwarfs continuous across the hydrogen-burning limit that agrees with previous studies. We estimate our completeness to range between 69% and 80% when compared to an isotropic model. However, we find that the literature late-M sample is severely incomplete compared to L dwarfs, with completeness of 62-7+8 and 83-9+10, respectively. This incompleteness can be addressed with astrometric-based searches of UCDs with Gaia to identify objects previously missed by color- and magnitude-limited surveys. Description: In this paper, we present a new volume-limited sample of M7-L5 ultracool dwarfs within 25pc, accompanied by NIR spectra homogeneously acquired with the SpeX spectrograph on the NASA Infrared Telescope Facility (IRTF). Two hundred and forty 25pc sample members had SpeX spectra in the SpeX Prism Library (SPL; Burgasser 2014ASInC..11....7B 2014ASInC..11....7B) prior to 2015. We observed an additional 286 sources with SpeX (0.75-2.5um) between UT 2015-Feb-24 and 2018-Nov-22 as part of NASA IRTF programs 2015A074, 2015B087, 2016A079, 2016B114, 2017A102, 2018B120 (PI: Bardalez Gagliuffi), and 2016A038 (PI: Burgasser) over a total of 15 nights. The observations log is summarized in Table 7. See Section 3. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 106 472 Bona fide and 1σ samples of M7-L5 ultracool dwarfs in the 25pc volume table4.dat 210 470 Multi-wavelength photometry for bona fide and 1σ samples of M7-L5 ultracool dwarfs in the 25pc volume table5.dat 137 471 Bona fide and 1σ samples of M7-L5 ultracool dwarfs in the 25pc volume table6.dat 73 471 Trigonometric and spectrophotometric distances of bona fide and 1σ samples of M7-L5 ultracool dwarfs in the 25pc volume table7.dat 87 286 SpeX observing log table8.dat 175 69 Intermediate gravity and very low gravity sources in the M7-L5 25pc Sample table9.dat 64 23 Red and blue J-Ks color outliers table10.dat 92 57 Spectral binary candidates with M7-L7 primary components table11.dat 92 57 Ultracool binaries with M7-L5 primaries in the 25pc sample refs.dat 51 209 References -------------------------------------------------------------------------------- See also: B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020) III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997) I/284 : The USNO-B1.0 Catalog (Monet+ 2003) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) I/298 : LSPM-North Catalog (Lepine+ 2005) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012) I/322 : UCAC4 Catalogue (Zacharias+, 2012) V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018) J/ApJ/414/279 : Faintest stars (Tinney, 1993) J/ApJS/94/749 : RI photometry of cool dwarfs (Kirkpatrick+ 1994) J/A+A/338/1066 : Optical Spectra of DENIS Brown Dwarf Candidate (Tinney+ 1998) J/ApJ/540/1016 : K-band & NICMOS phot. of Trapezium Cluster (Luhman+, 2000) J/AJ/123/3356 : Palomar/MSU nearby star sp. survey. 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(Burgasser+, 2010) J/MNRAS/402/575 : Ultracool dwarfs in young moving groups (Clarke+, 2010) J/A+A/512/A37 : Velocities of 43 nearby L dwarfs (Seifahrt+, 2010) J/MNRAS/403/1949 : UBV(RcIc)JHK photometry of HIP nearby stars (Koen+, 2010) J/AJ/139/1808 : Colors and kinematics of SDSS L dwarfs (Schmidt+, 2010) J/ApJS/190/100 : NIR proper motion survey using 2MASS (Kirkpatrick+, 2010) J/MNRAS/407/2269 : Polarisation of a sample of late M dwarfs (Morin+, 2010) J/A+A/522/A112 : i'z' phot. of L5 and later dwarf candidates (Reyle+, 2010) J/ApJ/723/684 : NIRSPEC ultracool dwarf radial velocity survey (Blake+, 2010) J/AJ/141/97 : SDSS DR7 M dwarfs (West+, 2011) J/AJ/142/92 : New proper motion stars with pm≥0.18"/yr (Boyd+, 2011) J/AJ/142/138 : All-sky catalog of bright M dwarfs (Lepine+, 2011) J/ApJ/743/156 : NEOWISE obs. of NEOs: preliminary results (Mainzer+, 2011) J/ApJS/197/19 : First brown dwarfs discovered by WISE (Kirkpatrick+, 2011) J/ApJ/753/156 : T/Y brown dwarfs with WISE photometry (Kirkpatrick+, 2012) J/A+A/545/A85 : LHS1070 photometry and spectroscopy (Rajpurohit+, 2012) J/A+A/546/A69 : Orbits of visual binaries and dynamical masses (Malkov+, 2012) J/AJ/144/99 : Near-IR spectroscopy of 36 late M dwarfs (Deshpande+, 2012) J/MNRAS/427/3280 : Ultra-cool dwarfs at low Galactic latitudes (Folkes+, 2012) J/MNRAS/428/2824 : Rapid optical variability in ultracool dwarfs (Koen, 2013) J/ApJS/205/6 : T dwarf population revealed by WISE (Mace+, 2013) J/AJ/145/102 : Sp. of bright M dwarfs in the northern sky (Lepine+, 2013) J/MNRAS/430/1171 : Sub-stellar birth rate from UKIDSS (Day-Jones+, 2013) J/PASP/125/809 : New nearby M, L, and T dwarfs (Thompson+, 2013) J/A+A/556/A15 : Effective temperature scale of M dwarfs (Rajpurohit+, 2013) J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013) J/AJ/147/20 : Spectroscopy of 447 nearby M dwarfs (Newton+, 2014) J/AJ/147/34 : SpeX library of L-type dwarfs (Schneider+, 2014) J/ApJ/783/122 : AllWISE motion survey (Kirkpatrick+, 2014) J/ApJ/784/156 : Parallaxes for nearby mid-to-late M dwarfs (Dittmann+, 2014) J/ApJ/787/126 : WISE reduced proper motions and spectral types (Luhman+, 2014) J/ApJ/792/119 : Companions to nearby stars from Pan-STARRS 1 (Deacon+, 2014) J/MNRAS/443/2561 : CONCH-SHELL catalog of nearby M dwarfs (Gaidos+, 2014) J/ApJ/794/143 : New SpeX Observations of M7-L6 Dwarfs (Bardalez+, 2014) J/AJ/148/122 : YSOVAR: infrared photometry in Lynds 1688 (Gunther+, 2014) J/AcA/64/359 : Catalog of binary UV Ceti stars (Tamazian+, 2014) J/AJ/149/5 : Solar neighborhood. XXXV. Dist. to M dwarfs (Winters+, 2015) J/ApJ/800/85 : Teff, radii and luminosities of cool dwarfs (Newton+, 2015) J/A+A/577/A128 : CARMENES input cat. of M dwarfs. I (Alonso-Floriano+, 2015) J/AJ/149/158 : The BUD sample. I. L dwarf activity sample (Schmidt+, 2015) J/MNRAS/449/3651 : L and T dwarfs from UKIDSS LAS (Marocco+, 2015) J/AJ/150/57 : SLoWPoKES-II catalog (Dhital+, 2015) J/ApJ/810/158 : M,L,T dwarfs fundamental param. and SEDs (Filippazzo+, 2015) J/ApJS/220/16 : SpeX NIR survey of 886 nearby M dwarfs (Terrien+, 2015) J/ApJS/220/18 : BDKP IV. RVs of late-M & L dwarfs with MagE (Burgasser+, 2015) J/ApJ/812/3 : MEarth mid-to-late M dwarfs rot. & kinematics (West+, 2015) J/ApJ/814/118 : L/T transition dwarfs with PS1 & WISE. II. (Best+, 2015) J/ApJ/817/112 : NEOWISE/AllWISE high proper motion objects (Schneider+, 2016) J/ApJ/818/153 : MEarth photometry: nearby M-dwarf magnitudes (Dittmann+, 2016) J/ApJS/224/36 : The AllWISE motion survey (AllWISE2) (Kirkpatrick+, 2016) J/AJ/152/24 : Trig. parallaxes of 134 low-mass stars (Weinberger+, 2016) J/ApJS/225/10 : Kinematic analysis of M7-L8 dwarfs (Faherty+, 2016) J/ApJ/833/96 : Hawaii infrared parallax program. II. (Liu+, 2016) J/A+A/598/A92 : New ultracool subdwarfs (Lodieu+, 2017) J/AJ/153/92 : Late-Type Extension to MoVeRS (LaTE-MoVeRS) (Theissen+, 2017) J/MNRAS/466/2983 : Wide low very low-mass binary systems (Galvez-Ortiz+, 2017) J/MNRAS/469/401 : Known LT dwarfs in the Gaia DR1 (Smart+, 2017) J/AJ/154/112 : NIR sp. of new L and T dwarf candidates (Kellogg+, 2017) J/AJ/154/147 : Astrometry&phot. for late-type dwarfs&subdwarfs (Dahn+, 2017) J/AJ/154/151 : The solar neighborhood .XXXX. Young stars (Bartlett+, 2017) J/AJ/155/34 : Analysis of the NIR sp. of neighboring L dwarfs (Cruz+, 2018) J/ApJS/234/1 : Cat. of M, L, & T dwarfs from PS1 3π Survey (Best+, 2018) J/ApJ/856/23 : BANYAN. XI. The BANYAN Σ algorithm (Gagne+, 2018) J/ApJ/862/173 : Nearby low-mass stars proper motions (Theissen, 2018) J/A+A/619/L8 : Ultra-cool dwarfs candidates in Gaia DR2 (Reyle, 2018) J/ApJS/240/19 : Parallaxes of late-T and Y dwarfs (Kirkpatrick+, 2019) http://jgagneastro.wordpress.com/list-of-ultracool-dwarfs/ : List of UCDs http://www.browndwarfs.org/spexprism : SpeX Prism Spectral Libraries Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [1/2] Sample type (G1) 3- 29 A27 --- Name Star name 31- 51 A21 --- ID Identifier 53- 56 A4 --- SpT Adopted spectral type 58- 61 A4 --- n_SpT Note on how SpT was determined 63- 67 F5.2 mag Jmag [7.79/16.62]? The J band magnitude 69- 72 F4.2 mag e_Jmag [0.02/0.3]? Uncertainty in Jmag 74- 77 F4.2 mag J-Ks [0.5/2.6]? The (J-KS) color 79- 82 F4.2 mag e_J-Ks [0.03/0.31]? Uncertainty in J-Ks 84- 88 F5.2 pc Dist [3.58/35.71] Distance 90- 94 F5.2 pc e_Dist [0/28.01] Uncertainty in Dist 96-102 A7 --- n_Dist Note on how Dist was determined 104-106 I3 --- Ref [2/118] Reference code (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [2/3] Sample type (G1) 3- 29 A27 --- Name Star name 31 A1 --- f_Name [abcd] Flag on Name (1) 33- 36 A4 --- SpT Adopted spectral type 38- 41 A4 --- n_SpT Note on how SpT was determined 43- 47 F5.2 mag rmag [14.6/24.9]? SDSS r band magnitude 49- 52 F4.2 mag e_rmag [0/0.9]? Uncertainty in SDSS rmag 54- 58 F5.2 mag imag [13.2/21.11]? SDSS i band magnitude 60- 63 F4.2 mag e_imag [0/0.09]? Uncertainty in SDSS imag 65- 69 F5.2 mag zmag [11.7/18.62]? SDSS z band magnitude 71- 74 F4.2 mag e_zmag [0/0.04]? Uncertainty in SDSS zmag 76- 80 F5.2 mag 2Jmag [7.79/16.62]? 2MASS J band magnitude 82- 85 F4.2 mag e_2Jmag [0.02/0.3]? Uncertainty in 2MASS Jmag 87- 91 F5.2 mag 2Hmag [7.24/15.32]? 2MASS H band magnitude 93- 96 F4.2 mag e_2Hmag [0.02/0.21]? Uncertainty in 2MASS Hmag 98-102 F5.2 mag 2Ksmag [6.89/14.41] 2MASS Ks band magnitude 104-107 F4.2 mag e_2Ksmag [0.01/0.16]? Uncertainty in 2MASS Ksmag 109-113 F5.2 mag MJmag [8.34/16.53]? MKO J band magnitude 115-118 F4.2 mag e_MJmag [0.01/0.22]? Uncertainty in MKO Jmag 120-124 F5.2 mag MHmag [7.9/15.4]? MKO H band magnitude 126-129 F4.2 mag e_MHmag [0.01/0.15]? Uncertainty in MKO Hmag 131-135 F5.2 mag MKmag [7.5/14.4]? MKO K band magnitude 137-140 F4.2 mag e_MKmag [0.01/0.14]? Uncertainty in MKO Kmag 142-146 F5.2 mag UJmag [11/15.72]? UKIDSS J band magnitude 148-151 F4.2 mag e_UJmag [0/0.01]? Uncertainty in UKIDSS UJmag 153-157 F5.2 mag UHmag [10.5/19.23]? UKIDSS H band magnitude 159-162 F4.2 mag e_UHmag [0/0.21]? Uncertainty in UKIDSS UHmag 164-168 F5.2 mag UKmag [10/18.15]? UKIDSS K band magnitude 170-173 F4.2 mag e_UKmag [0/0.16]? Uncertainty in UKIDSS UKmag 175-179 F5.2 mag W1mag [6.64/13.77]? WISE W1 band magnitude 181-184 F4.2 mag e_W1mag [0.02/0.13]? Uncertainty in WISE W1mag 186-190 F5.2 mag W2mag [6.3/13.61]? WISE W2 band magnitude 192-195 F4.2 mag e_W2mag [0.02/0.05]? Uncertainty in WISE W2mag 197-201 F5.2 mag W3mag [6.29/13]? WISE W3 band magnitude 203-206 F4.2 mag e_W3mag [0.02/0.5]? Uncertainty in WISE W3mag 208-210 I3 --- Ref [2/118] Reference code (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Flag as follows: a = Individual component flux photometry for LP 881-64BC is reported in Rajpurohit+ (2012, J/A+A/545/A85). We converted these fluxes to JHK_S magnitudes using Vega as a reference star. b = LHS 1901AB does not have reported resolved photometry. We used the relative JHK' magnitudes from Montagnier+ (2006A&A...460L..19M 2006A&A...460L..19M) to compute the individual magnitudes. For the MKO K' band we used the measurement from 08 Jan 2004 that has the largest angular separations to minimize the effect of blending. c = Individual component JHK' absolute magnitudes from Konopacky+ (2010ApJ...711.1087K 2010ApJ...711.1087K) were converted to apparent magnitudes using Vega as a reference star. d = Magnitudes are for combined system. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [1/2] Sample type (G1) 3- 29 A27 --- Name Source name 31- 34 A4 --- SpT Adopted spectral type 36- 39 A4 --- n_SpT Note on how SpT was determined 41- 50 A10 --- SpT-o Literature optical spectral type 52- 66 A15 --- SpT-ir Literature NIR spectral type 68- 82 A15 --- SpT-s SIMBAD spectral type 84- 89 A6 --- SpT-sdss SDSS spectral type 91- 95 A5 --- SpT-B07 Burgasser+ 2007ApJ...659..655B 2007ApJ...659..655B spectral type (1) 97- 99 F3.1 --- e_SpT-B07 [0.3/1.2]? Uncertainty in SpT-B07 101-104 A4 --- SpT-A07 Allers+ 2007ApJ...657..511A 2007ApJ...657..511A spectral type (1) 106-108 F3.1 --- e_SpT-A07 [0.3/1]? Uncertainty in SpT-A07 110-114 A5 --- SpT-R01 Reid+ 2001AJ....121.1710R 2001AJ....121.1710R spectral type (1) 116-118 F3.1 --- e_SpT-R01 [0.8/1.4]? Uncertainty in SpT-R01 120-123 A4 --- SpT-Std Standard spectral type 125-137 A13 --- Ref Reference codes for spectral type classification: optical, NIR, SIMBAD, Standard (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Classification by indices. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [1/2] Sample type (G1) 3- 29 A27 --- Name Source name 31- 34 A4 --- SpT Adopted spectral type 36- 39 A4 --- n_SpT Note on how SpT was determined 41- 46 F6.2 mas plx [25.8/280]? Parallax 48- 52 F5.2 mas e_plx [0.06/40]? Uncertainty in Plx 54- 58 F5.2 pc DTrig [3.58/35.71]? Trigonometric distance 60- 64 F5.2 pc e_DTrig [0/16]? Uncertainty in DTrig 66- 67 I2 pc DSpec [3/37]? NIR spectrophotometric distance 69 I1 pc e_DSpec [0/4]? Uncertainty in DSpec 71- 73 I3 --- Ref [1/198]? Reference code for plx (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [1/2] Sample type (1) 3- 24 A22 --- ID Identifier 26 A1 --- f_ID [ab] Flag on ID (2) 28- 33 F6.3 mag Jmag [7.3/17.3]? 2MASS J band magnitude 35- 40 F6.3 mag Ksmag [6.5/15.8]? 2MASS Ks band magnitude 42- 47 A6 arcsec Slit Slit size ("0.5x15" or "0.8x15") 49- 52 I4 s Texp [29/4894] Total exposure time 54- 58 F5.3 --- Air [1/3.1] Airmass 60- 69 A10 "Y/M/D" Date Observation date 71- 77 F7.2 --- S/N [25/1561] Median signal-to-noise 79- 87 A9 --- Std Identifier of A0 standard used -------------------------------------------------------------------------------- Note (1): Sample type as follows: 1 = within 25 pc; 2 = outside 25 pc. Note (2): Flag as follows: a = Magnitudes are for combined system. b = Background source. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Set [1/4] Sample type (1) 3- 29 A27 --- Name Source name 31 A1 --- f_Name [bedc] Flag on Name (2) 33- 41 A9 --- SpT-o Optical literature spectral type 43- 57 A15 --- SpT-ir NIR literature spectral type 59- 62 A4 --- SpT-f SpeX field spectral type 64- 76 A13 --- SpT-l SpeX low gravity spectral type 78- 86 F9.3 mas/yr pmRA [-2291/3430]? Proper motion along RA 88- 93 F6.3 mas/yr e_pmRA [0.15/21]? Uncertainty in pmRA 95-102 F8.2 mas/yr pmDE [-3807/1471]? Proper motion along DE 104-108 F5.2 mas/yr e_pmDE [0.1/21]? Uncertainty in pmDE 110-116 F7.2 km/s RVel [-177/74]? Radial velocity 118-123 F6.2 km/s e_RVel [0.05/198]? Uncertainty in RVel 125-129 F5.2 pc Dist [3.8/28.6]? Trigonometric distance 131-134 F4.2 pc e_Dist [0/6.7]? Uncertainty in Dist 136-154 A19 --- YMGProb BANYAN Σ young moving group membership probability (3) 156-175 A20 --- Ref Reference codes: proper motion, RV, Distance, Low gravity classification (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Sample type as follows: 1 = Very Low Gravity Source; 2 = Intermediate Gravity Source; 3 = Peculiar and/or Low Metallicity Source; 4 = Rejected Low Gravity Candidates from Visual Inspection. Note (2): Flag as follows: b = Red J-K_S color outlier. c = Blue J-K_S color outlier. d = Member of extended 1σ sample. e = Teegarden's star. Note (3): We used BANYAN Σ (Gagne+ 2018, J/ApJ/856/23) on our low-gravity candidates to assess possible membership in 27 young moving groups using new kinematic data from Gaia DR2. See Section 4.3. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Out "red" or "blue" outlier 6- 28 A23 --- Name Source name 30 A1 --- f_Name Flag on Name (1) 32- 35 A4 --- SpT Adopted spectral type 37- 40 A4 --- n_SpT Note on SpT 42- 45 F4.2 mag J-Ks [0.5/2.52] J-Ks color index 47- 50 F4.2 mag e_J-Ks [0.03/0.3] J-Ks uncertainty 52- 56 F5.2 mag E(J-Ks) [-0.72/0.9] J-Ks excess 58- 60 I3 --- Disc Discovery reference (see refs.dat file) 62- 64 I3 --- Ref ? Young moving group reference (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Flag as follows: b = Here 2MASS J0355+1133 and 2MASS J1741-4642 are members of the AB Doradus young moving group, while G196-3B is a young, unassociated source. c = Also classified as INT-G, indicating low metallicity rather than low gravity. d = Member of extended 25pc +1σ sample. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Set "Within 25pc", "Outside 25pc" or "Rejected candidates" 14- 37 A24 --- Name Name of the source 39- 42 A4 --- SpT-c Combined spectral type 44- 47 A4 --- SpT-P Primary spectral type (1) 49- 51 F3.1 --- e_SpT-P [0/1] SpT-P uncertainty 53- 56 A4 --- SpT-S Secondary spectral type (1) 58- 61 A4 --- e_SpT-S SpT-S uncertainty 63- 66 F4.2 --- DelJ [0.8/5.1] 2MASS J-band difference, ΔJ 68- 71 F4.2 --- e_DelJ [0.1/0.9] DelJ uncertainty 73 A1 --- l_Conf Limit flag on Conf 75- 77 I3 % Conf [32/100] Confidence 79- 80 I2 --- SpInd [4/12] Spectral index (2) 82- 88 A7 --- Ref-P Candidate reference(s) (see refs.dat file) 90- 92 I3 --- Ref-S [63/205]? Confirmed reference (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Primary and secondary spectral types are a weighted average of the best binary template fits, inversely proportional to their ranked χ2. Note (2): Strong candidates have been selected by eight or more index-index plots up to 12, weak candidates by four to eight. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Set Sample (1) 7- 31 A25 --- Name Main name of the source 33 A1 --- f_Name a: Member of extended 25pc +1σ sample 35- 53 A19 --- SpT-c Combined spectral type 55- 59 A5 --- SpT-P Ultracool dwarf primary spectral type 61- 70 A10 --- SpT-S Ultracool dwarf secondary spectral type 72- 76 F5.2 pc Dist [4/33.33] Adopted distance 78- 81 F4.2 pc e_Dist [0/9.11] Dist uncertainty 83- 88 A6 pc Dist2 Second value of distance for 2MASS J15200224-4422419AB 90- 92 I3 --- Ref [10/213] Binary reference -------------------------------------------------------------------------------- Note (1): Sample as follows: ultra = ultracool binaries mult = higher-order multiples containing ultracool dwarf binaries comp = ultracool companions to main-sequence primaries -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref [1/226] Reference code 5- 23 A19 --- BibCode Bibcode of the reference 25- 51 A27 --- Comm Comment -------------------------------------------------------------------------------- Global notes: Note (G1): Sample type as follows: 1 = Bona fide sample; 2 = 1σ sample. 3 = 25 pc sample; -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 10-Mar-2021
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