J/ApJS/201/19       Hawaii Infrared Parallax Program. I.     (Dupuy+, 2012)

The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition. Dupuy T.J., Liu M.C. <Astrophys. J. Suppl. Ser. 201, 19 (2012)> =2012ApJS..201...19D 2012ApJS..201...19D
ADC_Keywords: Stars, double and multiple; Stars, late-type ; Positional data; Infrared sources; Parallaxes, trigonometric; Photometry, infrared; Proper motions; Spectral types Keywords: astrometry - brown dwarfs - infrared:stars - parallaxes - proper motions - stars: low-mass Description: Astrometry and photometry for 318 ultracool dwarfs in 265 systems that have measured trigonometric parallaxes. To be included in this tabulation, an object must have a spectral type ≥M6 or a K-band absolute magnitude >8.5mag. Parallaxes, proper motions, and coordinates at a specified epoch are given for all objects. Photometric measurements in MKO, 2MASS, Spitzer, and WISE systems are given when available. Various other flags that provide additional information about the object or photometry are included. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file plx-phot.dat 538 318 All astrometry, photometry, and flags refs.dat 48 220 References -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/311 : WISE All-Sky Data Release (Cutri+ 2012) Byte-by-byte Description of file: plx-phot.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 29 A29 --- Name Name of object (SIMBAD compatible if possible) 32- 38 A7 --- SpTopt ? Spectral type from optical data (1) 41- 47 A7 --- SpTnir ? Spectral type from near-IR data (1) 50- 58 A9 --- r_SpT ? Spectral type references in refs.dat file 61- 73 A13 --- Notes ? Flag providing notes on the object (2) 76- 84 F9.5 deg RAdeg Right ascension at J2000 and epoch Epoch 87- 95 F9.5 deg DEdeg Declination at J2000 and epoch Epoch 98-107 F10.2 d Epoch Epoch of RA, DE position (JD) 110-115 F6.2 mas plx Parallax 118-123 F6.2 mas e_plx Parallax error 126-132 F7.2 mas/yr pm Proper motion amplitude (total proper motion) 135-140 F6.2 mas/yr e_pm ? Proper motion amplitude error 143-149 F7.3 deg pmPA Proper motion position angle 152-157 F6.3 deg e_pmPA ? Proper motion PA error 160-162 A3 --- r_plx Parallax and pm references in refs.dat file 165-170 F6.3 mag Ymag ? MKO Y-band magnitude 173-177 F5.3 mag e_Ymag ? MKO Y-band magnitude error 180 I1 --- f_Ymag MKO Y-band magnitude flag (3) 183-188 F6.3 mag Jmag ? MKO J-band magnitude 191-195 F5.3 mag e_Jmag ? MKO J-band magnitude error 198 I1 --- f_Jmag MKO J-band magnitude flag (3) 201-206 F6.3 mag Hmag ? MKO H-band magnitude 209-213 F5.3 mag e_Hmag ? MKO H-band magnitude error 216 I1 --- f_Hmag MKO H-band magnitude flag (3) 219-224 F6.3 mag Kmag ? MKO K-band magnitude 227-231 F5.3 mag e_Kmag ? MKO K-band magnitude error 234 I1 --- f_Kmag MKO K-band magnitude flag (3) 237-242 F6.3 mag L'mag ? MKO L'-band magnitude 245-249 F5.3 mag e_L'mag ? MKO L'-band magnitude error 252 I1 --- f_L'mag MKO L'-band magnitude flag (3) 255-260 F6.3 mag J2mag ? 2MASS J-band magnitude 263-267 F5.3 mag e_J2mag ? 2MASS J-band magnitude error 270 I1 --- f_J2mag 2MASS J-band magnitude flag (3) 273-278 F6.3 mag H2mag ? 2MASS H-band magnitude 281-285 F5.3 mag e_H2mag ? 2MASS H-band magnitude error 288 I1 --- f_H2mag 2MASS H-band magnitude flag (3) 291-296 F6.3 mag K2mag ? 2MASS Ks-band magnitude 299-303 F5.3 mag e_K2mag ? 2MASS Ks-band magnitude error 306 I1 --- f_K2mag 2MASS Ks-band magnitude flag (3) 309-328 A20 --- r_NIR ? MKO and 2MASS references in refs.dat file 331-336 F6.3 mag [3.6] ? IRAC channel 1 magnitude 339-343 F5.3 mag e_[3.6] ? IRAC channel 1 magnitude error 346-351 F6.3 mag [4.5] ? IRAC channel 2 magnitude 354-358 F5.3 mag e_[4.5] ? IRAC channel 2 magnitude error 361-366 F6.3 mag [5.8] ? IRAC channel 3 magnitude 369-373 F5.3 mag e_[5.8] ? IRAC channel 3 magnitude error 376-381 F6.3 mag [8.0] ? IRAC channel 4 magnitude 384-388 F5.3 mag e_[8.0] ? IRAC channel 4 magnitude error 391-396 F6.3 mag W1mag ? WISE band 1 magnitude 399-403 F5.3 mag e_W1mag ? WISE band 1 magnitude error (4) 406-411 F6.3 mag W2mag ? WISE band 2 magnitude 414-418 F5.3 mag e_W2mag ? WISE band 2 magnitude error (4) 421-426 F6.3 mag W3mag ? WISE band 3 magnitude 429-433 F5.3 mag e_W3mag ? WISE band 3 magnitude error (4) 436-441 F6.3 mag W4mag ? WISE band 4 magnitude 444-448 F5.3 mag e_W4mag ? WISE band 4 magnitude error (4) 451 I1 --- nbflg ? WISE number of blends flag 454 I1 --- naflg ? WISE active deblend flag 457-460 A4 --- ccflg ? WISE artifacts flag 463 I1 --- extflg ? WISE extended source flag 466-469 A4 --- varflg ? WISE variability flag 472-475 A4 --- qflg ? WISE photometric quality in each band 478-484 A7 --- r_MIR ? IRAC and WISE references in refs.dat file 487-489 I3 --- Sys Unique system ID to track multiple systems 492 I1 --- M [1/2] Multiplicity flag, 2=known multiple (5) 495-502 F8.3 arcsec sep ? Separation of wide companion, when applicable 505-510 A6 --- HRes ? High-resolution imaging flag (6) 513-538 A26 --- r_HRes ? High-res imaging references in refs.dat file -------------------------------------------------------------------------------- Note (1): Uncertainties in spectral types are 0.5 subtypes unless otherwise noted by an appended ":" (±1.0 types), ":." (±1.5 types), "::" (±2.0 types), or "::." (±2.5 types). An appended "p" denotes that the object is spectrally peculiar. Subdwarf classifications are denoted by the prefixes d/sd, sd, esd. Note (2): Object flag meanings are as follows: lowg = low surface gravity features noted in the literature lowZ? = suspected low metallicity object, either from known companion or unusual spectral features over-L = overluminous for its spectral type, possible binary pl = planetary mass object subd = spectroscopically confirmed subdwarf v-red = unusually red object, possibly young or dusty young = known young object, either from an age-dated companion that is ∼300 Myr or younger, or from membership in a young moving group TWA = member of this young moving group bPic = member of this young moving group ABDor = member of this young moving group Tuc-Hor = member of this young moving group triple = known to be a tight triple system Note (3): Magnitude flag meanings are as follows: 0 = real photometry 1 = converted between 2MASS/MKO using object's spectrum 2 = synthesized from spectral decomposition constrained by another band's flux ratio (binaries only) 3 = all synthesized (binaries only) 9 = no measurement Note (4): Null WISE magnitude errors indicate that the magnitude value given is the 2-σ upper limit provided in the WISE All-Sky Catalog Note (5): Multiplicity flag meanings are as follows: 1 = object has no direct evidence for being a tight multiple system 2 = known to be a tight multiple system Note (6): High-resolution imaging flags contain one character for each instrument that has observed an object. The meanings of these characters are as follows: A = HST/ACS C = CFHT AO G = Gemini AO K = Keck AO L = Lick AO N = HST/NICMOS P = Palomar AO S = Subaru AO s = speckle imaging T = HST/STIS V = VLT AO W = HST/WFPC2 Y = Lucky imaging -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference number 6- 14 A9 --- Name Abbreviated author and year NNNN (AuthNNNN) 17- 35 A19 --- BibCode ADS bibliographic code 38- 48 A11 --- Com Comments -------------------------------------------------------------------------------- Acknowledgements: Trent J. Dupuy, tdupuy(at)cfa.harvard.edu
(End) Patricia Vannier [CDS] 22-Jun-2012
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