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J/A+A/409/147       J magnitude of IC 348 brown dwarfs       (Preibisch+, 2003)

Constraints on the IMF and the brown dwarf population of the young cluster IC 348. Preibisch T., Stanke T., Zinnecker H. <Astron. Astrophys. 409, 147 (2003)> =2003A&A...409..147P
ADC_Keywords: Clusters, open ; Stars, pre-main sequence ; Photometry Keywords: stars: pre-main sequence - stars: low-mass, brown dwarfs - stars: luminosity function, mass function - open clusters and associations: general Abstract: We use a deep near-infrared census of the young stellar cluster IC 348 to construct and analyze its luminosity function. Our mosaic image of IC 348 covers the full extent of the cluster with a completeness limit of J∼19.5 and is therefore sensitive for 2Myr old cluster members with masses as low as M≥0.005M or the mean extinction of the known cluster members (AV∼3.5mag). Description: The observations discussed in this paper were obtained during the night of 2nd Dec. 2001 using the Omega Prime wide-field near-infrared camera on the Calar Alto 3.5m telescope in service observing mode. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 21 1899 J-band magnitudes of the sources detected in our IC 348 image.
See also: J/AJ/122/866 : X-ray sources in IC 348 from Chandra (Preibisch+, 2001) J/ApJ/541/977 : Low-mass IMF in IC 348 (Najita+, 2000) J/A+AS/137/305 : IC 348 proper motion catalogue (Scholz+, 1999) J/ApJ/525/466 : Young low-mass stars & brown dwarfs in IC 348 (Luhman+, 1999) J/ApJ/497/736 : The young cluster IC 348. (Herbig, 1998) J/A+A/324/549 : Deep UVBRI photometry in IC 348 (Trullols+ 1997) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 15 A15 --- [PSZ2003] IC348-J Name (HHMMSS.s+DDMMSS) (1) 17- 21 F5.2 mag Jmag J magnitude
Note (1): The source names contain the J2000 coordinates. [PSZ2003] JHHMMSS.s+DDMMSS in Simbad
History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 06-Nov-2003
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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