J/A+AS/100/473       IRAS pointed observations data           (Assendorp+, 1993)

IRAS pointed observations data processing ASSENDORP R., WESSELIUS P.R. <Astron. Astrophys. Suppl. Ser. 100, 473 (1993)> =1993A&AS..100..473A 1993A&AS..100..473A (SIMBAD/NED Reference)
ADC_Keywords: Infrared sources Keywords: methods: data analysis - techniques: image processing - infrared: general Abstract: We have developed a system to process raw IRAS Pointed Observation (PO) data, using software developed at the Laboratory for Space Research, Groningen, The Netherlands. Several PO's can be coadded into one image. As an example we processed 99 PO's in the Chamaeleon I molecular cloud in to one image for every IRAS band. The list of extracted point sources contains some 300 new IRAS sources, down to a flux level of 21mJy at 12um. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table6 91 132 Associated Source List (ASL) table7 49 297 New Source List (NSL) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (1950) 4- 5 I2 min RAm Right ascension (1950) 7- 8 I2 s RAs Right ascension (1950) 11 A1 --- DE- Declination sign 12- 13 I2 deg DEd Declination (1950) 15- 18 F4.1 arcmin DEm Declination (1950) 20- 24 F5.1 mJy F12 []? Flux at 12um 25 A1 --- n_F12 [*] When '*' the flux value is in Jy 27- 31 F5.1 --- SN12 []? Signal to noise ratio (2) 33- 35 A3 --- Cat12 Catalogue in which the flux is listed (1) 36- 41 F6.1 mJy F25 []? Flux at 25um 42 A1 --- n_F25 [*] When '*' the flux value is in Jy 44- 49 F6.1 --- SN25 []? Signal to noise ratio (2) 50 A1 --- n_SN25 [*] When '*' only the first quality index in the table is reported 51- 53 A3 --- Cat25 Catalogue in which the flux is listed (1) 55- 59 F5.1 mJy F60 []? Flux at 60um 60 A1 --- n_F60 [*] When '*' the flux value is in Jy 62- 67 F6.1 --- SN60 []? Signal to noise ratio (2) 68 A1 --- n_SN60 [*] When '*' only the first quality index in the table is reported 69- 71 A3 --- Cat60 Catalogue in which the flux is listed (1) 74- 78 F5.1 mJy F100 []? Flux at 100um 79 A1 --- n_F100 [*] When '*' the flux value is in Jy 83 I1 --- SN100 []? Signal to noise ratio (2) 84 A1 --- n_SN100 [*] When '*' only the first quality index in the table is reported 90- 91 A2 --- Cat100 Catalogue in which the flux is listed (1) -------------------------------------------------------------------------------- Note (1): P= PO (Pointed Observation) map (Young E.T. et al. 1985, A users's guide to IRAS pointed observation products) F= FSS (Faint Source Survey) (Moshir M. et al. 1989 Explanatory supplement to the IRAS FSS, IPAC preprint 0044) I= IPSC (IRAS Point Source Catalog) (Joint IRAS Science Working Group, 1988, Infrared Astronomical Satellite, Catalogs and Atlasses, Explanatory Supplement, eds Beichman C.A. et al.) Note (2): Signal to noise if the source is found in the PO map, otherwise it is the flux quality from the catalogue(s) mentioned in the corresponding column 'C' -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (1950) 4- 5 I2 min RAm Right ascension (1950) 7- 8 I2 s RAs Right ascension (1950) 11 A1 --- DE- Declination sign 12- 13 I2 deg DEd Declination (1950) 15- 18 F4.1 arcmin DEm Declination (1950) 21- 23 I3 mJy F12 []? Flux at 12um 25- 28 F4.1 --- SN12 []? Signal to noise ratio 31- 33 I3 mJy F25 []? Flux at 25um 36- 39 F4.1 --- SN25 []? Signal to noise ratio 42- 44 I3 mJy F60 []? Flux at 60um 46- 49 F4.1 --- SN60 []? Signal to noise ratio -------------------------------------------------------------------------------- Historical Notes: Keypunched at CDS
(End) James Marcout, Simona Mei [CDS] 12-Apr-1995
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