J/A+A/369/932       RI photometry of LMC carbon stars        (Kontizas+, 2001)

A Catalogue of carbon stars in the LMC. Kontizas E., Dapergolas A., Morgan D.H., Kontizas M. <Astron. Astrophys. 369, 932 (2001)> =2001A&A...369..932K 2001A&A...369..932K
ADC_Keywords: Magellanic Clouds ; Stars, carbon ; Photometry, VRI Keywords: galaxies: Magellanic Clouds - stars: carbon Abstract: A catalogue of 7760 carbon stars in the Large Magellenic Cloud is presented. The stars were identified during a systematic survey of objective-prism plates taken with the UK 1.2m Schmidt Telescope. The catalogue is compared with other lists of carbon stars and the distribution of the carbon stars is discussed. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 75 7760 Carbon star catalogue table5.dat 16 172 Stars with nearby resolved companions -------------------------------------------------------------------------------- See also: III/156 : Cool Galactic Carbon Stars, 2nd Edition (Stephenson 1989) B/2mass : The 2MASS database (IPAC/UMass, 2000) J/A+AS/122/463 : Carbon stars in Magellanic Clouds (Kunkel+ 1997) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- KDMK Identification Number (KDMK) 5 A1 --- f_KDMK [d] when the star has a nearby resolved companion (detailed in table5) 6- 7 I2 h RAh Right ascension (J2000) 9- 10 I2 min RAm Right ascension (J2000) 12- 16 F5.2 s RAs Right ascension (J2000) 19 A1 --- DE- Declination sign (J2000) 20- 21 I2 deg DEd Declination (J2000) 23- 24 I2 arcmin DEm Declination (J2000) 26- 29 F4.1 arcsec DEs Declination (J2000) 32- 36 F5.2 mag Rmag Kron-Cousins photoelectric R magnitude 39- 43 F5.2 mag R-I Kron-Cousins photoelectric R-I colour index 46- 47 A2 --- Meas Measurement field 50- 53 I4 --- CodeP Photometry code (1) 55 I1 --- CodeA ? Astrometry code (2) 57 I1 --- CodeS ? Spectrum code (3) 59- 60 A2 --- CodeG General code (4) 64 A1 --- CodeI [*] Identification code (5) 66- 75 A10 --- Name Cross-references (6) -------------------------------------------------------------------------------- Note (1): A 4-digit photometry code digit 1: image area with respect to the magnitude 0 appropriate 1 too large in R 2 too large in I 3 too large in R and I digit 2: images that are multiple 0 image unblended or deblended satisfactorily 1 image deblended but with possible error 2 image has a faint undeblended companion 3 image has an undeblended companion 4 image has an undeblended companion a little fainter 5 image has an undeblended companion of equal or brighter magnitude 9 no information available for this code digit 3: multiple images that are deblended in R but not in I 0 carbon star is fainter than the total in R by less than 0.1 mag 1 carbon star is fainter than the total in R by 0.1-0.3 mag 2 carbon star is fainter than the total in R by 0.3-0.5 mag 3 carbon star is fainter than the total in R by more than 0.5 mag 4 complex blend noted 5 possible deblending error noted digit 4: indicates the SuperCOSMOS deblending parameters 0 unblended or undeblended images in both R and I 1 deblended images in R 2 blended images in I 3 deblended images in both R and I Note (2): A 1-digit astrometry code 1 R and I coordinates differ by more than 1 arcsec 2 primary and secondary datasets for F56 differ by more than 1arcsec 3 measurements were made using the cursor (e.g. no R data available) 4 from the second F56 dataset 5 original approximate measurements 6 star is more than 6 deg from the plate centre Note (3): A 1-digit spectrum code 1 highly probably carbon 2 probably carbon 3 bands look weak Note (4): A 3-digit general code to indicate possible contamination by b a bright star g a galaxy t a satellite trail n nebulosity c cluster v the star is likely to be a variable (Note that the absence of `v' does not mean that the star is not a variable because there are insufficient images of each star to determine this over the typical periods for variable carbon stars.) Note (5): A 1-digit identification code which is * when there is a nearby star, resolved by SuperCOSMOS within 5 arcsec and no more than 1 mag fainter than the carbon star. Note (6): References are: BM**-** - Blanco V.M., McCarthy M.F., 1983AJ.....88.1442B 1983AJ.....88.1442B LMC-BM FF-NN in Simbad C****-**** - Kunkel W.E., Irwin M.J., Demers, S., 1997, Cat. J/A+AS/122/463, [KID97] CHHMM-DDMM in Simbad M92-**** - Morgan D.H., 1992MNRAS.258..639M 1992MNRAS.258..639M M92_N67 = LHA 120-N 67 M92_S63 = LHA 120-S 63 M92_LMC1 = LMC 1 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- KDMK Identification Number (KDMK) 6- 9 F4.1 mag Dmag R magnitude difference between the carbon star and its neighbouring (R(carbon)-R_(neighbour)) 11- 13 F3.1 arcsec Offset Extent of the separation between the two 15- 16 A2 --- Dir Direction of the companion from the carbon star -------------------------------------------------------------------------------- Acknowledgements: Anastasios Dapergolas
(End) Patricia Bauer [CDS] 17-May-2001
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