J/AJ/128/1684         NGC 2264: VRIHα photometry             (Sung+, 2004)

The initial mass function and young brown dwarf candidates in NGC 2264. I. The initial mass function around S Monocerotis. Sung H., Bessell M.S., Chun M.-Y. <Astron. J., 128, 1684-1693 (2004)> =2004AJ....128.1684S 2004AJ....128.1684S
ADC_Keywords: Clusters, open ; Stars, pre-main sequence ; Photometry, VRI ; X-ray sources ; Photometry, CCD Keywords: open clusters and associations: individual (NGC 2264) - stars: low-mass, brown dwarfs - stars: luminosity function, mass function Abstract: The young open cluster NGC 2264 was observed on 2002 January 67 with the CFH12K mosaic CCD on the 3.6m Canada-France-Hawaii Telescope to investigate the shape of the initial mass function (IMF). In order to select the pre-main-sequence (PMS) members more completely, Chandra X-Ray Observatory archival data were retrieved and used for the identification of X-ray-emitting weak-line T Tauri stars. In addition, the (R-I, V-I) diagram was used to exclude background late-type giants, and a statistical approach was applied to estimate the number of contaminating foreground main-sequence stars. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 128 3037 Photometric data table3.dat 94 19 X-Ray sources detected from pwdetect -------------------------------------------------------------------------------- See also: J/AJ/127/2659 : CHANDRA observations of NGC 2264 (Ramirez+, 2004) J/A+A/345/521 : BVRI photometry of NGC 2264 (Flaccomio+, 1999) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- [SBC2004b] Source identification number 6 I1 h RAh Hour of right ascension (J2000) 8- 9 I2 min RAm Minute of right ascension (J2000) 11- 15 F5.2 s RAs Second of right ascension (J2000) 16 A1 --- DE- Sign of the Declination (J2000) 17- 18 I2 deg DEd Degree of declination (J2000) 20- 21 I2 arcmin DEm Arcminute of declination (J2000) 23- 26 F4.1 arcsec DEs Arcsecond of declination (J2000) 28- 33 F6.3 mag Imag The I-band magnitude 35- 36 I2 mmag e_Imag ? The error in Imag in millimagnitudes 38 A1 --- f_Imag [*] Indicates error greater than 0.1mag 40- 45 F6.3 mag R-I ? The (R-I) colour index 47- 48 I2 mmag e_R-I ? The error in R-I in millimagnitudes 50 A1 --- f_R-I [*] Indicates error greater than 0.1mag 52- 57 F6.3 mag V-I ? The (V-I) colour index 59- 60 I2 mmag e_V-I ? The error in V-I in millimagnitudes 62 A1 --- f_V-I [*] Indicates error greater than 0.1mag 65- 70 F6.3 mag R-Ha ? The (R-Hα) colour index 72- 73 I2 mmag e_R-Ha ? The error in R-Ha in millimagnitudes 75 A1 --- f_R-Ha [*] Indicates error greater than 0.1mag 77 I1 --- o_Imag ? Number of observations in Imag 79 I1 --- o_R-I ? Number of observations in R-I 81 I1 --- o_V-I ? Number of observations in V-I 83 I1 --- o_R-Ha ? Number of observations in R-Ha 85 A1 --- Memb Membership code (1) 87- 89 A3 --- Data Data source (2) 91-127 A37 --- Notes Additional notes (3) -------------------------------------------------------------------------------- Note (1): The membership code is defined as follows: X = Strong X-ray source; x = Weak X-ray source; H = Strong Hα emission star; h = Hα emission candidate; + = Hα emission star with X-ray emission; - = Hα emission candidate with X-ray emission; Q = Early-type star. Note (2): The data source is defined as follows: C = New photometric data obtained at CFHT; S = Data from Sung et al. (1997AJ....114.2644S 1997AJ....114.2644S). Note (3): Additional notes give other identification, with the following abbreviations: SBL = Sung et al. 1997AJ....114.2644S 1997AJ....114.2644S, Cl* NGC 2264 SBL NNNN in Simbad; S = ID used in Tables 4 and 5 of Sung et al. 1997AJ....114.2644S 1997AJ....114.2644S, Cl* NGC 2264 SBL NNNN in Simbad; FX = Flaccomio et al. 2000, Cat. J/A+A/355/651, [FMS2000] XNNN in Simbad; LH = Herbig 1954ApJ...119..483H 1954ApJ...119..483H, Em* LkHA NN in Simbad; O = Ogura 1984PASJ...36..139O 1984PASJ...36..139O, KHA NNN in Simbad. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- PID pwdetect source sequential number 6 I1 h RAh Hour of right ascension (J2000.0) 8- 9 I2 min RAm Minute of right ascension (J2000.0) 11- 15 F5.2 s RAs Second of right ascension (J2000.0) 17 A1 --- DE- Sign of the Declination (J2000) 18 I1 deg DEd Degree of declination (J2000.0) 20- 21 I2 arcmin DEm Arcminute of declination (J2000.0) 23- 26 F4.1 arcsec DEs Arcsecond of declination (J2000.0) 29- 32 F4.2 --- Sig Significance 35- 38 I4 --- [SBC2004b] ? CFHT number 41- 44 I4 --- SBL ? SBL number (Sung et al. 1997AJ....114.2644S 1997AJ....114.2644S, Cl* NGC 2264 SBL NNNN in Simbad) 47- 94 A48 --- Rem Remark -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 19-Apr-2005
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