J/MNRAS/469/401     Known LT dwarfs in the Gaia DR1          (Smart+, 2017)

The Gaia ultracool dwarf sample. I. Known L and T dwarfs and the first Gaia data release. Smart R.L., Marocco F., Caballero J.A., Jones H.R.A., Barrado D., Beamin J.C., Pinfield D.J., Sarro L.M. <Mon. Not. R. Astron. Soc., 469, 401-415 (2017)> =2017MNRAS.469..401S 2017MNRAS.469..401S (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Stars, late-type ; Proper motions ; Photometry, infrared ; Stars, distances Keywords: binaries: visual - brown dwarfs - Hertzsprung-Russell and colour-magnitude diagrams - stars: late-type - solar neighbourhood Abstract: We identify and investigate known ultracool stars and brown dwarfs that are being observed or indirectly constrained by the Gaia mission. These objects will be the core of the Gaia ultracool dwarf sample composed of all dwarfs later than M7 that Gaia will provide direct or indirect information on. We match known L and T dwarfs to the Gaia first data release, the Two Micron All Sky Survey and the Wide-field Infrared Survey Explorer AllWISE survey and examine the Gaia and infrared colours, along with proper motions, to improve spectral typing, identify outliers and find mismatches. There are 321 L and T dwarfs observed directly in the Gaia first data release, of which 10 are later than L7. This represents 45 per cent of all the known LT dwarfs with estimated GaiaG magnitudes brighter than 20.3mag. We determine proper motions for the 321 objects from Gaia and the Two Micron All Sky Survey positions. Combining the Gaia and infrared magnitudes provides useful diagnostic diagrams for the determination of L and T dwarf physical parameters. We then search the Tycho-Gaia astrometric solution, Gaia first data release subset, to find any objects with common proper motions to known L and T dwarfs and a high probability of being related. We find 15 new candidate common proper motion systems. Description: table2.dat: an input catalogue of known L, T and Y dwarfs. This list began with the online census being kept by J. Gagne (https://jgagneastro.wordpress.com/list-of-ultracool-dwarfs) which included objects from the Dwarfarchives (https://www.dwarfarchives.edu), the work of Dupuy et al. (2012ApJS..201...19D 2012ApJS..201...19D), and the PhD thesis catalogue of Mace (2014yCat.5144....0M 2014yCat.5144....0M). To this compilation, we added the objects in Marocco (2015MNRAS.449.3651M 2015MNRAS.449.3651M) and Faherty (2016ApJS..225...10F 2016ApJS..225...10F). This list was used to search for know L/T dwarfs in the GAia DR1 and then also for common binary systems in the TGAS catalog. table4.dat: The catalogue of known LT dwarfs matched to Gaia DR1 entries. Proper motions were calculated from Gaia DR1 and 2MASS positions. table5.dat: The catalogue of candidate CPM systems with known LT dwarfs and the Gaia DR1 TGAS subsection. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 271 1886 The Gaia Ultracool Dwarf sample (GUCDS) input catalogue table3.dat 104 7 Input catalogue objects with mismatches in Gaia DR1 table4.dat 405 321 Parameters for the GUCDS-DR1 catalogue table5.dat 200 15 Parameters for the GUCDS-DR1 catalogue table6.dat 469 7 Probable late M dwarfs identified in the colour-colour and colour-spectral type diagrams -------------------------------------------------------------------------------- See also: I/337 : Gaia DR1 (Gaia, 2016) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- SName Short name used in text of paper 16- 45 A30 --- OName Longer name from discovery paper 47- 87 A41 --- DISCref Discovery paper reference BibCode (upto 2) 89-101 F13.8 deg RAdeg Right ascension (Equinox J2000) 103-115 F13.8 deg DEdeg Declination (Equinox J2000) 117-133 A17 --- SpType Spectral type 135-153 A19 --- r_SpType Spectral type reference BibCode (1) 155 I1 --- n_SpType [1/3] How Spectral type obtained (2) 157-165 F9.2 mas/yr pmRA ?=-99999 Proper motion in Rigth ascension 167-175 F9.2 mas/yr e_pmRA ?=-99999 Error in proper motion in RA 177-185 F9.2 mas/yr pmDE ?=-99999 Proper motion in declination 187-195 F9.2 mas/yr e_pmDE ?=-99999 Error in proper motion in Dec 197-215 A19 --- r_pm Proper motion reference BibCode (3) 217-226 F10.3 mag Jmag ?=-99999 J magnitude 228-237 F10.3 mag e_Jmag ?=-99999 Error in J magnitude 239 I1 --- Jtype [0/2] System of J magnitude (4) 241-259 A19 --- r_Jmag J magnitude reference 261-271 F11.4 --- Epoch ?=-99999 Epoch of position -------------------------------------------------------------------------------- Note (1): The SpT_ref is sometimes set to MAROCCOetal2017 for objects that have spectral types that are in a paper submitted but not yet published. Note (2): How Spectral type obtained code as follows: 1 = Spectral type from optical spectra 2 = Spectral type from Near Infrared spectra 3 = Spectral type from photometry Note (3): The r_pm is set to PMFROM2MASS--WISE when the input proper motion was found from the difference of the 2MASS and WISE survey positions. Note (4): System of J magnitude as follows: 1 = 2MASS system 2 = MKO system -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 26 A26 --- Name Name 28 I1 --- r_Name [1/6] Discovery references (1) 30- 48 I19 --- GaiaDR1 Gaia DR1 Source ID 50- 53 F4.1 mag DGmag Difference between Gaia DR1 G magnitude and estimated G magnitude, G-Gest 55-104 A50 --- Rem Remarks -------------------------------------------------------------------------------- Note (1): Discovery references as follows: 1 = Kirkpatrick et al. (2011, Cat. J/ApJS/197/19) 2 = Lodieu et al. (2007MNRAS.379.1423L 2007MNRAS.379.1423L) 3 = Lodieu et al. (2009A&A...505.1115L 2009A&A...505.1115L) 4 = Mace et al. (2013ApJ...777...36M 2013ApJ...777...36M) 5 = Folkes et al. (2012, Cat. J/MNRAS/427/3280) 6 = Thompson et al. (2013, Cat. J/PASP/125/809) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- SName Short name used in text of paper 17- 29 F13.9 deg RAdeg Right ascension (equinox J2000 epoch 2015) 34- 46 F13.9 deg DEdeg Declination (equinox J2000 epoch 2015) 48- 59 F12.5 mas/yr pmRA* Proper motion in RA from Gaia + 2MASS positions, pmRA*cosDE 61- 72 F12.5 mas/yr e_pmRA* Error in proper motion in RA, e_cosDE 74- 85 F12.5 mas/yr pmDE Proper motion in Dec from Gaia + 2MASS positions 87- 98 F12.5 mas/yr e_pmDE Error in proper motion in DE 100-111 F12.5 mag Gmag Gaia G band magnitude 113-124 F12.5 mag e_Gmag Error in Gaia G band magnitude (1) 126-130 I5 --- Nobs Number of Observations in Gaia DR1 134-152 I19 --- SourceID Gaia Source ID 154-158 F5.2 mag GmagGpred Gaia G magnitude minus predicted magnitude 160-161 I2 --- Nin3arcsec Number of matches within 3 arcseconds in Gaia DR1 163-164 I2 --- pmflag Flag to show pm differ (2) 166-191 A26 --- OName Longer name from discovery paper 193-211 A19 --- DISCref Reference bibCode for discovery (3) 213-222 A10 --- SpTypeO Spectral type in optical 224-242 A19 --- r_SpTypeO Reference BibCode for SpTypeO 244-253 A10 --- SpTypeN Spectral type in Near infrared 255-273 A19 --- r_SpTypeN Reference BibCode for SpTypeN (3) 275-284 F10.3 mag Jmag 2MASS J band magnitude 286-295 F10.3 mag e_Jmag 2MASS J band magnitude error 297-306 F10.3 mag Hmag 2MASS H band magnitude 308-317 F10.3 mag e_Hmag 2MASS H band magnitude error 319-328 F10.3 mag Kmag 2MASS K band magnitude 330-339 F10.3 mag e_Kmag 2MASS K band magnitude error 341-350 F10.3 mag W1mag ?=-99999 ALLWISE W1 Band magnitude 352-361 F10.3 mag e_W1mag ?=-99999 ALLWISE W1 Band magnitude error 363-372 F10.3 mag W2mag ?=-99999 ALLWISE W2 Band magnitude 374-383 F10.3 mag e_W2mag ?=-99999 ALLWISE W2 Band magnitude error 385-394 F10.3 mag W3mag ?=-99999 ALLWISE W3 Band magnitude 396-405 F10.3 mag e_W3mag ?=-99999 ALLWISE W3 Band magnitude error -------------------------------------------------------------------------------- Note (1): The Gaia DR1 does not provide a direct G magnitude error rather a error on the flux, e_, we convert this to an estimate of the magnitude error using the relation eGmag=1.0857*photgmeanfluxerror/photgmeanflux. Note (2): Flag to show pm differ as follows: 0 = Difference of input and calculated proper motion is less than 20% 1 = Difference of input and calculated proper motion is more than 20% Note (3): In one case the bibcode that is provided is "MAROCCOetal2017" for an object that has parameters that are in a paper submitted but not yet published. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- HIP/TYC HIPPARCOS or TYCHO2 name of primary 17- 35 I19 --- SourceID Gaia SourceID primary 37- 48 F12.8 deg RAdeg Right ascension (equinox J2000 epoch 2015) 50- 61 F12.8 deg DEdeg Declination (equinox J2000 epoch 2015) 63- 70 F8.1 mas/yr pmRA* Primary RA Proper motion from DR1, pmRA*cosDE 72- 75 F4.1 mas/yr e_pmRA* Error in proper motion in RA, e_pmRA*cosDE 77- 84 F8.1 mas/yr pmDE Primary Dec Proper motion from DR1 86- 89 F4.1 mas/yr e_pmDE Error in proper motion in Dec 91- 94 I4 mas plx Primary DR1 parallax rounded value 96- 97 I2 mas e_plx Error in parallax rounded value 99-110 A12 --- SName Name of UCD in input catalog 112-119 F8.1 mas/yr pmRA*B UCD RA Proper motion from input catalog, pmRA*cosDE 121-124 F4.1 mas/yr e_pmRA*B Error in UCD proper motion in RA, e_pmRA*cosDE 126-133 F8.1 mas/yr pmDEB UCD Dec Proper motion from input catalog 135-138 F4.1 mas/yr e_pmDEB Error in UCD proper motion in Dec 140-143 I4 mas spDist UCD Spectroscopic parallax rounded 145-146 I2 mas e_spDist Error in parallax rounded value 148-154 E7.1 --- Prob chance probability of not being a companion 156-164 A9 --- SpTypeO Optical UCD Spectra type from input catalog 166-174 A9 --- SpTypeN NIR UCD Spectra type from input catalog 176-187 F12.8 deg RABdeg UCD Right ascension (equinox J2000 epoch 2015) 189-200 F12.8 deg DEBdeg UCD Declination (equinox J2000 epoch 2015) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 22 A22 --- Name Long name 25- 27 A3 --- SpTypeO Optical spectral type 29- 31 A3 --- r_SpTypeO Reference for SpTypeO (1) 33- 42 A10 --- SName Short name 45- 46 A2 --- SpTypeN NIR spectral type 48- 50 A3 --- r_SpTypeN Reference for SpTypeN (1) 52 I1 --- NPlot Plot label 54- 58 F5.2 mag DGmag Difference between Gaia DR1 G magnitude and estimated G magnitude, G-Gest 60-469 A410 --- Rem Remarks -------------------------------------------------------------------------------- Note (1): Spectral type references as follows: (1) = Reid et al. (2008AJ....136.1290R 2008AJ....136.1290R, Cat. J/AJ/136/1290) (2) = Lodieu et al. (2005A&A....436..853L, Cat. J/A+A/436/853) (3) = Schmidt et al. (2010AJ....139.1808S 2010AJ....139.1808S, Cat. J/AJ/129/1808) (4) = Bardalez Gagliuffi et al. (2014ApJ...794..143B 2014ApJ...794..143B) (5) = West et al. (2008AJ....135..785W 2008AJ....135..785W, Cat. (J/AJ/135/785) -------------------------------------------------------------------------------- Acknowledgements: Richard Laurence Smart, smart(at)oato.inaf.it
(End) Richard Laurence Smart [OATo-INAF], Patricia Vannier [CDS] 18-Mar-2020
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