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J/ApJS/196/4     New young star candidates in Taurus-Auriga     (Rebull+, 2011)

New young star candidates in the Taurus-Auriga region as selected from the Wide-field Infrared Survey Explorer. Rebull L.M., Koenig X.P., Padgett D.L., Terebey S., McGehee P.M., Hillenbrand L.A., Knapp G.R., Leisawitz D., Liu W., Noriega-Crespo A., Ressler M.E., Stapelfeldt K.R., Fajardo-Acosta S., Mainzer A. <Astrophys. J. Suppl. Ser., 196, 4 (2011)> =2011ApJS..196....4R
ADC_Keywords: Photometry, infrared ; YSOs ; Surveys ; Stars, pre-main sequence ; Molecular clouds Keywords: circumstellar matter - infrared: stars - stars: formation - stars: pre-main sequence Abstract: The Taurus Molecular Cloud subtends a large solid angle on the sky, in excess of 250deg2. The search for legitimate Taurus members to date has been limited by sky coverage as well as the challenge of distinguishing members from field interlopers. The Wide-field Infrared Survey Explorer has recently observed the entire sky, and we take advantage of the opportunity to search for young stellar object (YSO) candidate Taurus members from a ∼260deg2 region designed to encompass previously identified Taurus members. We use near- and mid-infrared colors to select objects with apparent infrared excesses and incorporate other catalogs of ancillary data to present a list of rediscovered Taurus YSOs with infrared excesses (taken to be due to circumstellar disks), a list of rejected YSO candidates (largely galaxies), and a list of 94 surviving candidate new YSO-like Taurus members. There is likely to be contamination lingering in this candidate list, and follow-up spectra are warranted. Description: In the context of Rebull et al. (2010ApJS..186..259R), we assembled a substantial multi-wavelength database, spanning Sloan u through Spitzer/MIPS 160um (with some X-rays) for point sources throughout the Taurus region. We use that catalog as the core for our analysis here, updating it with confirmed Taurus members from, e.g., Kenyon et al. (2008hsf1.book..405K) and Luhman et al. (2010ApJS..186..111L) outside of our original Spitzer map. We have also searched SIMBAD (and literature references therein) for known galaxies and other contaminants in this vicinity. Our Taurus Spitzer Survey spanned ∼44deg2 (figure 1). WISE data acquisition and reduction are discussed in Wright et al. (2010AJ....140.1868W), Jarrett et al. (2011, ApJ, submitted), and in the Explanatory Supplement to the WISE Preliminary Data Release Products. There are four WISE bands, with central wavelengths at 3.4, 4.6, 12, and 22um, and a spatial resolution of 6" (12" at 22um). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 168 196 Multiband measurements of WISE-identified YSOs with previous indications of youth in the literature towards the Taurus region table2.dat 168 724 Multiband measurements of WISE-identified rejected YSO candidates in Taurus region table3.dat 168 94 Multiband measurements of WISE-identified new YSO candidates in Taurus region
See also: II/307 : WISE Preliminary Data Release (Cutri+ 2011) J/A+A/519/A83 : T Tau stars toward the Taurus-Auriga region (Takita+ 2010) J/ApJ/703/1964 : Spectra of three nearby star-forming regions (Furlan+, 2009) J/ApJS/176/457 : Taurus dark cloud background star catalog (Shenoy+, 2008) J/PASJ/60/209 : Faint companions around YSOs in TMC (Itoh+, 2008) J/AJ/132/2665 : QUEST2 BRI photometry of Taurus-Auriga PMS (Slesnick+, 2006) J/ApJ/647/1180 : Infrared photometry of Taurus SFR (Luhman+, 2006) J/ApJ/581/1194 : Taurus-Auriga PMS stars ages and Teff (Palla+, 2002) J/A+AS/145/187 : uvby-β photometry of WTTS (Chavarria-K+, 2000) J/A+AS/132/173 : New weak-line T Tauri stars in Taurus-Auriga (Li+ 1998) J/A+AS/124/449 : Young stars south of Taurus-Auriga (Magazzu+ 1997) J/A+A/312/439 : New T Tauri stars in Taurus-Auriga (Wichmann+, 1996) J/ApJS/101/117 : UBVRIJHKLMNQ photometry in Taurus-Auriga (Kenyon+ 1995) http://irsa.ipac.caltech.edu/Missions/wise.html : WISE Infrared Science page Byte-by-byte Description of file: table[123].dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq Sequential number within the table 5- 23 A19 --- WISE Catalog identification (JHHMMSS.ss+DDMMSS.s) 25- 49 A25 --- Name Source name (1) 51- 55 F5.2 mag W1mag WISE 3.4 micron band magnitude 57- 60 F4.2 mag e_W1mag Uncertainty in W1mag 62- 66 F5.2 mag W2mag WISE 4.6 micron band magnitude 68- 71 F4.2 mag e_W2mag Uncertainty in W2mag 73- 77 F5.2 mag W3mag WISE 12 micron band magnitude 79- 82 F4.2 mag e_W3mag Uncertainty in W3mag 84- 88 F5.2 mag W4mag WISE 22 micron band magnitude 90- 93 F4.2 mag e_W4mag Uncertainty in W4mag 95 A1 --- St [b] status (2) 97-168 A72 --- Notes Additional source notes
Note (1): Note added by CDS: In table 2 (Rejected YSO), the Name "TYC1823-680-1" (04 11 22.762 +26 52 43.35, J2000) is very doubtfully linked to WISE J041121.83+293320.5. Note (2): b = Object identified in Rebull et al. (2010ApJS..186..259R) as a candidate Taurus member, but discussed there as needing additional data to confirm/refute it as a Taurus member.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 14-Nov-2011
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

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