J/A+A/474/35     JKs photometry of C stars in IC10 and WLM   (Battinelli+, 2007)

The assessment of the near infrared identification of carbon stars. I. The Local Group galaxies WLM, IC 10 and NGC 6822. Battinelli P., Demers S., Mannucci F. <Astron. Astrophys., 474, 35-41 (2007)> =2007A&A...474...35B 2007A&A...474...35B (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, nearby ; Stars, carbon ; Photometry, infrared Keywords: galaxies: individual: IC 10 - galaxies: individual: WLM - galaxies: individual: NGC 6822 - stars: carbon - stars: AGB and post-AGB - galaxies: dwarf Abstract: The selection of AGB C and M stars from NIR colours has been done in recent years using adjustable criteria that are in needs of standardization if one wants to compare, in a coherent manner, properties of various populations. We intend to assess the NIR colour technique to identify C and M stars. We compare the NIR colours of several C stars previously identified from spectroscopy or narrow band techniques in WLM, IC 10 and NGC 6822. We demonstrate that very few M stars have (J-K)0>1.4 but a non negligible number of C stars are bluer than this limit. Thus, counts of M and C stars based on such limit do not produce pure samples. C/M ratios determined from NIR colours must be regarded as underestimates mainly because the M numbers include many warm C stars and also K stars if no blue limit is considered. Description: The J,H,Kp observations were secured with NICS (Near Infrared Camera Spectrometer) installed at the Nasmyth focus of the TNG (Telescopio Nazionale Galileo) on the island of La Palma. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 59 62 Known C stars in the WLM NICS field table3.dat 59 52 Known C stars in the IC 10 NICS field -------------------------------------------------------------------------------- See also: J/A+A/416/111 : C stars in Wolf-Lundmark-Melotte galaxy (Battinelli+, 2004) J/A+A/424/125 : Carbon stars in IC10 (Demers+, 2004) J/A+A/466/501 : JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007) J/A+A/493/1075 : JKs photometry of IC1613 & NGC3109 C stars (Battinelli+ 2009) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [BD2004a] Sequential number from Battinelli & Demers, 2004, Cat. J/A+A/416/111 5- 10 F6.3 mag Imag I magnitude 12- 16 F5.3 mag R-I R-I colour index 18- 22 F5.3 mag CN-TiO CN-TiO index 24- 29 F6.3 mag Ksmag Ks magnitude 31- 35 F5.3 mag e_Ksmag rms uncertainty on Ksmag 37- 41 F5.3 mag J-Ks J-Ks colour index 43- 47 F5.3 mag e_J-Ks rms uncertainty on J-Ks 49- 53 F5.3 mag H-Ks H-Ks colour index 55- 59 F5.3 mag e_H-Ks rms uncertainty on H-Ks -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [DBL2004] Sequential number from Demers et al., 2004, Cat. J/A+A/424/125 5- 10 F6.3 mag I0mag Dereddened I magnitude 12- 16 F5.3 mag (R-I)0 Dereddened R-I colour index 18- 22 F5.3 mag CN-TiO CN-TiO index 24- 29 F6.3 mag Ksmag Ks magnitude 31- 35 F5.3 mag e_Ksmag rms uncertainty on Ksmag 37- 41 F5.3 mag J-Ks J-Ks colour index 43- 47 F5.3 mag e_J-Ks rms uncertainty on J-Ks 49- 53 F5.3 mag H-Ks H-Ks colour index 55- 59 F5.3 mag e_H-Ks rms uncertainty on H-Ks -------------------------------------------------------------------------------- History: From electronic version of the journal References: Battinelli & Demers, Paper II 2009A&A...493.1075B 2009A&A...493.1075B, Cat. J/A+A/493/1075
(End) Patricia Vannier [CDS] 05-Feb-2018
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