J/A+AS/93/61    IR Stellar Population in Baade's window (Ruelas-Mayorga+ 1992)

Distribution and studies of the infrared stellar population in the galaxy. III. Baade's window photometry. Ruelas-Mayorga R.A., Teague P.F. <Astron. Astrophys. Suppl. Ser. 93, 61 (1992)> =1992A&AS...93...61R 1992A&AS...93...61R
ADC_Keywords: Photometry, infrared Keywords: Galaxy: bulge of - Galaxy: general - galaxy: stellar content of - infrared radiations - photometry Description: The 2.2um (K) scan (table1) was made on the Mt. Stromlo 1.9m telescope with the MSO IR-photometer, during several observation sessions in 1981, at sideral rate with a 12arcsec aperture; the rows of the scan were spaced by 6arcsec in declination, and were on the average 65arcmin long. Detailed JHK photometry of a sample of the brightest sources (table 2) was obtained during later observing sessions in 1981 and 1982. The photometric results are given in the AAO system (Jones & Hyland, 1980MNRAS.192..359J 1980MNRAS.192..359J) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 37 578 Sources found in the 2.2um scan of Baade's window table2 99 183 Photometric subsample of the Baade's window IR-scan table4 53 35 Photometry obtained in 1987 with 2.3m telescope of the sources in the galactic region (20, -5) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- BW Designation of the source 8- 9 I2 h RAh Right Ascension 1950 (hours) (1) 11- 12 I2 min RAm Right Ascension 1950 (minutes) 14- 17 F4.1 s RAs Right Ascension 1950 (seconds) 19 A1 --- DE- Declination 1950 (sign) 20- 21 I2 deg DEd Declination 1950 (degrees) (1) 23- 24 I2 arcmin DEm Declination 1950 (minutes) 26- 29 F4.1 arcsec DEs Declination 1950 (seconds) 32 A1 --- n_Kmag [S] S indicates that K is saturated 33- 37 F5.2 mag Kmag [8.7/11.1]? K magnitude (2.2um) -------------------------------------------------------------------------------- Note (1): The positions of the sources could be anywhere inside an aperture of 6" around the nominal position. All declinations end with .4 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Designation of the source 10 A1 --- Rem [ABCD] Remark (1) 12- 13 I2 h RAh Right Ascension 1950 (hours) 15- 16 I2 min RAm Right Ascension 1950 (minutes) 18- 21 F4.1 s RAs Right Ascension 1950 (seconds) 24 A1 --- DE- Declination 1950 (sign) 25- 26 I2 deg DEd Declination 1950 (degrees) 28- 29 I2 arcmin DEm Declination 1950 (minutes) 31- 32 I2 arcsec DEs Declination 1950 (seconds) 34- 38 F5.2 mag Jmag Filter J (1.2um) 40- 43 F4.2 mag e_Jmag Mean error on Jmag 47- 51 F5.2 mag Hmag Filter H (1.6um) 53- 56 F4.2 mag e_Hmag Mean error on Hmag 59- 63 F5.2 mag Kmag Filter K (2.2um) 65- 68 F4.2 mag e_Kmag Mean error on Kmag 71- 75 F5.2 mag J-H colour 77- 80 F4.2 mag e_J-H Mean error on J-H 83- 87 F5.2 mag H-K colour 89- 92 F4.2 mag e_H-K Mean error on H-K 95- 98 A4 --- Position Origin of the position -------------------------------------------------------------------------------- Note (1): Meaning of the remark flag: A = Faint star closer to a brighter source (misidentification) B = Several observations of the source. C = Faint source confused with a brighter one. D = These sources are out of the limits of our scan. -------------------------------------------------------------------------------- Table 3: Observed CCF (Cumulative K-Count Function) for BW -------------------------------------------------------- up to K-mag Nobs Ncorrected N1(per deg2) logN1 -------------------------------------------------------- 5.0 1 1 17.91 1.25 5.5 1 1 17.91 1.25 6.0 4 4 71.64 1.86 6.5 7 7 125.37 2.10 7.0 12 12 214.93 2.33 7.5 26 26 465.70 2 67 8.0 48 48 859.70 2.93 8.5 90 90 1611.94 3.21 9.0 129 129 2310.45 3.36 9.25A 192 151.68 2716.66 3.43 9.75A 287 226.73 4060.84 3.61 10.25A 403 318.37 5702.15 3.76 ----- --- ------ ------- ---- 11.0 21 21.42 19278 4.29 11.5 49 46.06 41454 4.62 12.0 80 63.20 56880 4.75 12.5 112 88.48 79632 4.90 13.0 157 124.03 111627 5.05 13.5 219 173.01 155709 5.19 -------------------------------------------------------- Byte-by-byte Description of file: table4 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Designation of the source 14- 18 F5.2 mag Jmag Filter J (1.2um) 21- 25 F5.2 mag Hmag Filter H (1.6um) 28- 32 F5.2 mag Kmag Filter K (2.2um) 35- 39 F5.2 mag J-H colour 42- 46 F5.2 mag H-K colour 49- 53 F5.2 mag J-K colour -------------------------------------------------------------------------------- History: Keypunched at CDS
(End) James Marcout, Francois Ochsenbein [CDS] 06-Apr-1994
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