J/AJ/121/3160       JHK photometry near the Trapezium region  (Carpenter+, 2001)

Near-infrared photometric variability of stars toward the Orion A molecular cloud. Carpenter J.M., Hillenbrand L.A., Skrutskie M.F. <Astron. J. 121, 3160 (2001)> =2001AJ....121.3160C 2001AJ....121.3160C
ADC_Keywords: Stars, variable ; Stars, pre-main sequence ; Photometry, infrared Keywords: infrared radiation - stars: individual (YY Orionis, BM Orionis) - stars: pre-main-sequence - stars: variables: general Abstract: We present an analysis of J, H, and Ks time-series photometry obtained with the southern 2MASS telescope over a 0.84°x6° region centered near the Trapezium region of the Orion Nebula cluster. These data are used to establish the near-infrared variability properties of premain-sequence stars in Orion on timescales of ∼1-36days, ∼2 months, and ∼2 years. A total of 1235 near-infrared variable stars are identified, ∼93% of which are likely associated with the Orion A molecular cloud. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 87 1235 Near-Infrared Variable Stars table7.dat 42 233 Periodic Stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- [CHS2001] Star identification number 7- 15 F9.6 deg RAdeg Right ascension in decimal degrees (J2000) 17- 25 F9.6 deg DEdeg Declination in decimal degrees (J2000) 27- 32 F6.3 mag Jmag ? The average J magnitude 34- 39 F6.3 mag Hmag The average H magnitude 41- 46 F6.3 mag Kmag The average Ks magnitude 48- 52 F5.3 mag e_Jmag ? Observed rms in Jmag 54- 58 F5.3 mag e_Hmag ? Observed rms in Hmag 60- 64 F5.3 mag e_Kmag ? Observed rms in Kmag 66- 67 I2 --- o_Jmag Number of high-quality Jmag photometric measurements used to assess the variability 69- 70 I2 --- o_Hmag Number of high-quality Hmag photometric measurements used to assess the variability 72- 73 I2 --- o_Kmag Number of high-quality Kmag photometric measurements used to assess the variability 75- 79 F5.2 --- Index Stetson variability index 81 I1 --- Flag1 [0/1] Variable on 16 nights common to entire area (1) 82 I1 --- Flag2 [0/1] Variable in March-April 2000 data (1) 83 I1 --- Flag3 [0/1] Long-term variability in 2000 February and/or 1998 March (1) 84 I1 --- Flag4 [0/1] Periodic variable (1) 85 I1 --- Flag5 [0/1] Eclipsing candidate (1) 86 I1 --- Flag6 [0/1] Selected as variable from subjective inspection of light curve (1) -------------------------------------------------------------------------------- Note (1): 1 = star exhibits this type of variability; 0 = star does not exhibits this type of variability. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- [CHS2001] Star identification number 7- 11 F5.2 d PerJ ? The J band period 13- 17 F5.2 d PerH The H band period 19- 23 F5.2 d PerK The Ks band period 25 A1 --- l_FAPJ Limit flag on FAPJ 26- 29 F4.2 --- FAPJ ? The J band false-alarm probability (FAP) that the power spectrum peak could have resulted from random noise 31 A1 --- l_FAPH Limit flag on FAPH 32- 35 F4.2 --- FAPH The H band false-alarm probability (FAP) that the power spectrum peak could have resulted from random noise 37 A1 --- l_FAPK Limit flag on FAPK 38- 41 F4.2 --- FAPK The Ks band false-alarm probability (FAP) that the power spectrum peak could have resulted from random noise -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 27-Sep-2001
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