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J/MNRAS/404/1475    JHK photometry of Leo I AGB and red giants   (Held+, 2010)

A near-infrared study of AGB and red giant stars in the Leo I dSph galaxy. Held E.V., Gullieuszik M., Rizzi L., Girardi L., Marigo P., Saviane I. <Mon. Not. R. Astron. Soc., 404, 1475-1489 (2010)> =2010MNRAS.404.1475H
ADC_Keywords: Galaxies, nearby ; Stars, giant ; Photometry, infrared Keywords: stars: AGB and post-AGB - stars: carbon - galaxies: individual: Leo I - Local Group - galaxies: stellar content Abstract: A near-infrared imaging study of the evolved stellar populations in the dwarf spheroidal galaxy Leo I is presented. Based on JHK observations obtained with the WFCAM wide-field array at the United Kingdom Infrared Telescope, we build a near-infrared photometric catalogue of red giant branch (RGB) and asymptotic giant branch (AGB) stars in Leo I over a 13.5arcmin2 area. The V-K colours of RGB stars, obtained by combining the new data with existing optical observations, allow us to derive a distribution of global metallicity [M/H] with average [M/H]=-1.51 (uncorrected) or [M/H]=-1.24±.05(int)±0.15(syst) after correction for the mean age of Leo I stars. Description: Observations of Leo I were carried out on 2005 April 19-20 using the NIR Wide Field Camera (WFCAM) at the UKIRT at Mauna Kea, Hawaii. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 48 7471 The NIR catalogue of Leo I stars over WFCAM array No. 2 table4.dat 75 39 Candidate O-rich AGB stars in Leo I, as selected from the NIR two-colour diagram (Fig. 6, region 1) table5.dat 75 37 *Candidate C-rich AGB stars in Leo I
Note on table5.dat: All stars were selected from the NIR two-colour diagram (Fig. 6, region 4), with the exception of stars 7125 and 11242 which are spectroscopically identified C stars fainter than the TRGB
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 6 I6 --- [HGR2010] Sequential number 8- 9 I2 h RAh Right ascension (J2000) 11- 12 I2 min RAm Right ascension (J2000) 14- 18 F5.2 s RAs [0/60] Right ascension (J2000) 20 A1 --- DE- Declination sign (J2000) 21- 22 I2 deg DEd Declination (J2000) 24- 25 I2 arcmin DEm Declination (J2000) 27- 30 F4.1 arcsec DEs [0/60] Declination (J2000) 32- 36 F5.2 mag Jmag 2MASS J magnitude (1) 38- 42 F5.2 mag Hmag 2MASS H magnitude (1) 44- 48 F5.2 mag Ksmag 2MASS Ks magnitude (1)
Note (1): Our raw photometric catalogue was transformed to the 2MASS photometric system by applying the colour terms between WFCAM and 2MASS systems derived for the UKIRT Infrared Deep Sky Survey (UKIDSS; Dye et al. 2006MNRAS.372.1227D), and zero-points directly computed from the median of the J H K magnitude differences between 2MASS and our WFCAM photometry in the colour range 0.0<J-K<1. 0, for stars in common with the 2MASS/PSC.
Byte-by-byte Description of file: table[45].dat
Bytes Format Units Label Explanations
1- 6 I6 --- [HGR2010] Sequential number 8- 9 I2 h RAh Right ascension (J2000) 11- 12 I2 min RAm Right ascension (J2000) 14- 18 F5.2 s RAs [0/60] Right ascension (J2000) 20 A1 --- DE- Declination sign (J2000) 21- 22 I2 deg DEd Declination (J2000) 24- 25 I2 arcmin DEm Declination (J2000) 27- 30 F4.1 arcsec DEs [0/60] Declination (J2000) 32- 36 F5.2 mag Bmag ?=- Johnson B magnitude 38- 42 F5.2 mag Vmag ?=- Johnson V magnitude 44- 48 F5.2 mag Jmag 2MASS J magnitude 50- 54 F5.2 mag Hmag 2MASS H magnitude 56- 60 F5.2 mag Ksmag 2MASS Ks magnitude 62- 75 A14 --- Note Cross-identifications (only in table5) (1)
Note (1): Cross-identifications with the surveys of Azzopardi et al. (1986A&A...161..232A, ALW, <ALW Leo I NN> in Simbad), Demers & Battinelli (2002AJ....123..238D, DB, <[DB2002] Leo I CNN> in Simbad) and Menzies et al. (2002MNRAS.335..923M, M02, <[MFT2002] A> in Simbad) are given. Probable variable stars in M02 are labelled 'v'.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 01-Dec-2010
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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