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Detailed Description of J/A+AS/90/327
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J/A+AS/90/327 1612MHz OH survey of IRAS point sources (te Lintel Hekkert+ 1991)
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1612 MHz OH survey of IRAS point sources
I. Observations made at Dwingeloo, Effelsberg and Parkes
te Lintel Hekkert P., Caswell J.L., Habing H.J., Haynes R.F., Norris R.P.
<Astron. Astrophys. Suppl. Ser. 90, 327 (1991)>
=1991A&AS...90..327T
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ADC_Keywords: Stars, masers ; Masers ; Radio lines
Keywords: OH maser --- OH/IR stars
Description: 2703 sources have been observed at the 1612MHz transition
of OH, and 783 OH/IR stars were detected; 597 of these detections are
new discoveries. The IRAS sources were detected on the basis of their
IRAS fluxes at 12, 25 and 60um. The survey is 70% complete for IRAS
sources in the Southern hemisphere (Dec<-10°) with F(12um)>3Jy,
with IR colors log(F25/F12)>-0.2 and log(F60/F12)<0.6
Note that the file catalog.dat contains all observed sources,
with a flag indicating the detection or non-detection; the
detected sources only are listed in the printed version of Table2,
while sources without detectable 1612MHz emission are listed in
Table3 (on microfiche)
File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file
catalog.dat 106 2703 Observations results (tables 2 and 3)
See also:
II/125 : The IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
Byte-by-byte Description of file: catalog.dat
Bytes Format Units Label Explanations
2- 12 A11 --- IRAS IRAS name
15- 26 A12 --- OH-Name OH name
28 I1 --- Dflag [1,3] Detection flag (1)
30 I1 --- Peaks Number of peaks in spectrum
33- 39 F7.3 deg GLON Galactic longitude
42- 48 F7.3 deg GLAT Galactic latitude
50- 55 F6.1 km/s VL ?=0.0 Lower velocity (blue shifted pike) (2)
57- 62 F6.1 km/s VH ?=0.0 Higher velocity (red shifted pike) (2)
65- 70 F6.2 Jy SL ?=0.00 1612MHz Flux density at VL (2)
73- 78 F6.2 Jy SH ?=0.00 1612MHz Flux density at VH (2)
81- 88 E8.2 Jy F25 ? 25-micron IRAS flux
90- 94 F5.2 --- R21 ? log(F(25)/F(12)) ratio of IRAS fluxes
96-100 F5.2 --- R32 ? log(F(60)/F(25)) ratio of IRAS fluxes
102-103 I2 --- VAR Variability probability from IRAS
105-106 I2 --- LRS Number of IRAS Low Resolution Spectra
Note (1): The detection flag is
1 = non-detection
2 = likely detection
3 = standard profile
Note (2): for single-peak detections, the values are in VL and SL,
(VH and SH are set to 0)
History:
* December 1992: the electronic version of the table was e-mailed to
CDS by Hekkert te Lintel.
* April 1998: Non-measured sources without OH-Name were removed.
The documentation (this ReadMe file) was revised and completed.
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(End) Francois Ochsenbein [CDS] 18-Dec-1992, 15-Apr-1998
| 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 |