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J/AJ/136/1372       Very low-mass YSOs in NGC 1333           (Oasa+, 2008)

Luminosity and mass functions at the very low mass side in NGC 1333. Oasa Y., Tamura M., Sunada K., Sugitani K. <Astron. J., 136, 1372-1387 (2008)> =2008AJ....136.1372O
ADC_Keywords: Nebulae ; Photometry, infrared ; YSOs Keywords: infrared: stars - ISM: individual (NGC 1333) - stars: formation - stars: low-mass, brown dwarfs - stars: luminosity function, mass function - stars: pre-main sequence Abstract: We present the results of a deep near-infrared (NIR) imaging survey searching for very low mass young stellar objects (YSOs) in the embedded cluster associated with the Perseus molecular cloud. Our observations cover an area of ∼5'x5' in the NGC 1333-S region at J-, H-, and Ks-bands. The 10σ limiting magnitudes exceed 18mag in all three bands. Based on NIR color-color diagrams, embedded YSO candidates were identified using NIR excesses. Description: JHKs imaging observations of the star-forming core in NGC 1333 were conducted during the period from 1997 September 22-October 1 using the facility infrared array camera (OASIS) mounted on the 1.88m telescope of the Okayama Astronomical Observatory (OAO) in Japan. The region in common with the OASIS survey was imaged in the JHKs-bands with the Simultaneous-Color InfraRed Imager for Unbiased Survey (SIRIUS) on the 2.2m University of Hawaii telescope on Mauna Kea, Hawaii, on the night of 2000 August 15. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 76 76 NIR sources in the NGC 1333 region
See also: J/A+AS/106/165 : Near-IR imaging photometry of NGC 1333 (Aspin+ 1994) J/AJ/111/1964 : JHK photometry of NGC1333 (Lada+, 1996) J/AJ/127/1131 : NGC 1333 low-mass stars infrared photometry (Wilking+, 2004) J/ApJ/575/354 : Young stellar objects in the NGC 1333 (Getman+, 2002) J/ApJ/655/958 : 90-GHz observations in NGC 1333 (Walsh+, 2007) J/ApJ/674/336 : Spitzer observations of NGC 1333 (Gutermuth+, 2008) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Seq Sequential number, <[OTS2008] NN> in Simbad 4 I1 h RAh Right ascension (J2000) 6- 7 I2 min RAm Right ascension (J2000) 9- 13 F5.2 s RAs Right ascension (J2000) 15 A1 --- DE- Declination sign (J2000) 16- 17 I2 deg DEd Declination (J2000) 19- 20 I2 arcmin DEm Declination (J2000) 22- 26 F5.2 arcsec DEs Declination (J2000) 28- 32 F5.2 mag Jmag J magnitude 33 A1 --- n_Jmag [d] Source saturated in J (1) 35- 38 F4.2 mag e_Jmag ?=0.00 rms uncertainty on Jmag 40- 44 F5.2 mag Hmag H magnitude 45 A1 --- n_Hmag [d] Source saturated in H (1) 47- 50 F4.2 mag e_Hmag ?=0.00 rms uncertainty on Hmag 52- 56 F5.2 mag Kmag Ks magnitude 57 A1 --- n_Kmag [d] Source saturated in Ks (1) 59- 62 F4.2 mag e_Kmag ?=0.00 rms uncertainty on Kmag 64- 68 F5.2 mag J0mag ? Reddening-corrected J magnitude (2) 70 I1 --- Type [1/4] Numerical type (3) 71 A1 --- n_Type [d] Source saturated (1) 73- 75 I3 --- ASR ? ASR number (4) 76 A1 --- n_ASR [e] if sources not resolved in Aspin et al. 1994A&AS..106..165A
Note (1): 'd' indicates sources saturated in this survey. The values are substituted with Aspin et al., 1994A&AS..106..165A Note (2): For Class II objects, the J luminosity is corrected for the extinction and translated using the distance modulus. Note (3): Our source classification flag as follows: 1 = source classified as Class I object candidate 2 = source classified as Class II object candidate 3 = source classified as Class III object and field star candidate 4 = sources lying below the CTTS locus and to the right of reddening lines Note (4): Sources previously identified in the NIR survey by Aspin et al., 1994A&AS..106..165A
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 06-Apr-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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