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J/A+A/464/909       JHK photometry near IRAS 06145+1455      (Brand+, 2007)

A star cluster at the edge of the Galaxy. Brand J., Wouterloot J.G.A. <Astron. Astrophys., 464, 909-920 (2007)> =2007A&A...464..909B
ADC_Keywords: Infrared sources ; Molecular clouds ; Photometry, infrared Keywords: stars: formation - stars: pre-main sequence - ISM: clouds - ISM: individual objects: WB 89-789 (IRAS 06145+1455) Abstract: Our goal in this paper is to study stars and molecular gas in the direction of IRAS 06145+1455 (WB89-789). The kinematic distance of the associated molecular cloud is 11.9kpc. With a galactocentric distance of ∼20.2kpc, this object is at the edge of the (molecular) disk of the Galaxy. We use near-IR (J, H, K), molecular line-, and dust continuum observations. Description: The data presented here were obtained on February 15, 1995, with the ESO 2.2-m telescope at La Silla (Chile). Images in J, H, and K-bands were taken with the IRAC-2 camera and objective C, which resulted in a scale of 0.49"/pixel. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 72 68 NIR photometry data
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 2 I2 --- [BW2007] Sequential number 4- 5 I2 h RAh Right ascension (J2000) 7- 8 I2 min RAm Right ascension (J2000) 10- 14 F5.2 s RAs Right ascension (J2000) 16 A1 --- DE- Declination sign (J2000) 17- 18 I2 deg DEd Declination (J2000) 20- 21 I2 arcmin DEm Declination (J2000) 23- 26 F4.1 arcsec DEs Declination (J2000) 28- 32 F5.2 mag Kmag K magnitude 34- 37 F4.2 mag e_Kmag rms uncertainty on Kmag 39- 43 F5.2 mag Hmag H magnitude 45- 48 F4.2 mag e_Hmag rms uncertainty on Hmag 50- 54 F5.2 mag Jmag J magnitude 56- 59 F4.2 mag e_Jmag rms uncertainty on Jmag 61- 65 F5.3 mag H-K H-K colour index 67- 72 F6.3 mag J-H J-H colour index
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 28-Sep-2007
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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