Access to Astronomical Catalogues

← Click to display the menu
J/ApJS/155/401 Magellanic clouds globular clusters ISOCAM obs. (Tanabe+, 2004)

ISOCAM observations of globular clusters in the Magellanic clouds: the data. Tanabe T., Kucinskas A., Nakada Y., Onaka T., Sauvage M. <Astrophys. J. Suppl. Ser., 155, 401-419 (2004)> =2004ApJS..155..401T
ADC_Keywords: Magellanic Clouds ; Clusters, globular ; Infrared sources Keywords: galaxies: star clusters - infrared: stars - Magellanic Clouds - stars: AGB and post-AGB - stars: evolution Abstract: Seventeen globular clusters in the Large and Small Magellanic Clouds were observed in the mid-infrared wavelength region with the ISOCAM instrument on board the Infrared Space Observatory (ISO). Observations were made using the broadband filters LW1, LW2, and LW10, corresponding to the effective wavelengths of 4.5, 6.7, and 12µm, respectively. We present the photometry of point sources in each cluster, as well as their precise positions and finding charts. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 75 17 Magellanic Cloud clusters observed with ISOCAM and aperture corrections applied with the PSF photometry table5.dat 151 272 ISOCAM photometry of individual point sources in the Magellanic Cloud clusters notes.dat 80 34 Notes
See also: II/181 : IR sources in Magellanic Clouds (Schwering+ 1990) J/MNRAS/272/391 : Globular clusters in the Magellanic Clouds (Ferraro+, 1995) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Cluster Cluster name 10- 11 I2 h RAh Right Ascension (J2000), from Simbad 13- 14 I2 min RAm Right Ascension (J2000), from Simbad 16- 19 F4.1 s RAs Right Ascension (J2000), from Simbad 21 A1 --- DE- Declination sign (J2000), from Simbad 22- 23 I2 deg DEd Declination (J2000), from Simbad 25- 26 I2 arcmin DEm Declination (J2000), from Simbad 28- 29 I2 arcsec DEs Declination (J2000), from Simbad 31- 40 A10 --- Date Observation date 42- 49 I8 --- TDT TDT number (1) 52- 59 A8 --- SWB SWB type (2) 62- 65 F4.2 --- LW1 Aperture correction/mag in LW1 (3) 67- 70 F4.2 --- LW2 Aperture correction/mag in LW2 (3) 72- 75 F4.2 --- LW10 Aperture correction/mag in LW10 (3)
Note (1): The observation of one cluster consists of 3 AOTs, i.e., 3 TDTs. This number is the first one corresponding to the observation with LW1 filter Note (2): SWB type from Searle et al. (1980ApJ...239..803S), young (SWB IIII), intermediate-age (SWB IV-VI) and old (SWB VII) clusters Note (3): -2.5log(PSFflux/aperture flux)
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Cluster Cluster name (1) 10 A1 --- n_Cluster [aijr] Note on Cluster, see notes.dat file 12- 13 I2 --- Seq The I-band image number in the cluster (1) 15 A1 --- n_Seq [b-u] Note on Seq, see notes.dat file 17- 18 I2 h RAh Hour of Right Ascension (J2000) 20- 21 I2 min RAm Minute of Right Ascension (J2000) 23- 26 F4.1 s RAs Second of Right Ascension (J2000) 28 A1 --- DE- Sign of the Declination (J2000) 29- 30 I2 deg DEd Degree of Declination (J2000) 32- 33 I2 arcmin DEm Arcminute of Declination (J2000) 35- 36 I2 arcsec DEs Arcsecond of Declination (J2000) 38- 42 F5.2 mJy FLW1 ? The ISOCAM LW1 (4.5um) flux density 44- 48 F5.2 mJy e_FLW1 ? The 1σ error in FLW1 50- 54 F5.2 mJy FLW2 ? The ISOCAM LW2 (6.7um) flux density 56- 59 F4.2 mJy e_FLW2 ? The 1σ error in FLW2 61- 66 F6.2 mJy FLW10 ? The ISOCAM LW10 (12um) flux density 68- 71 F4.2 mJy e_FLW10 ? The 1σ error in FLW10 73-150 A78 --- ID Literature identifications
Note (1): Objects are identified as [TKN2004] Kron 3 NN and [TKN2004] NGC NNNN NN in Simbad.
Byte-by-byte Description of file: notes.dat
Bytes Format Units Label Explanations
1 A1 --- Note Code of the note 3- 79 A77 --- Text Text of the note
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 30-Jun-2005
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

catalogue service

© UDS/CNRS

Contact