Astronomical Data Center
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The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:
I/123 Lunar Occultations of IRAS Point Sources, 1986-1990 (Simon+ 1986)
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Lunar Occultations of IRAS Point Sources, 1986-1990
Simon M., Cassar L., Chen W.P.
<Astrophys. J. Suppl. Ser. 62, 673, (1986)>
=1986ApJS...62..673S
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ADC_Keywords: Infrared sources; Occultations
Description:
The Lunar Occultations of IRAS Point Sources lists objects in the IRAS
Point Source Catalog that were occulted by the Moon during 1986-1990.
Introduction:
The occultation predictions were based on the formulae for the lunar
ephemeris developed by Van Flandern and Pulkinnen (1979). The
topocentric predictions from this code are accurate to about +/-30s.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
data.dat 78 14148 Data
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Byte-by-byte Description of file: data.dat
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Bytes Format Units Label Explanations
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1- 10 A10 --- IRAS IRAS Point Source Cat. Object Name
12- 13 I2 a yr1 *Starting Year
15- 16 I2 a yr2 *Ending Year
19- 22 F4.3 Jy flux12 *? Mantissa for 12 um Flux Density
23- 26 I4 --- exp12 *? Exponent for 12 um Flux Density
28- 31 F4.3 Jy flux25 *? Mantissa for 25 um Flux Density
32- 35 I4 --- exp25 *? Exponent for 25 um Flux Density
37- 40 F4.3 Jy flux60 *? Mantissa for 60 um Flux Density
41- 44 I4 --- exp60 *? Exponent for 60 um Flux Density
46- 49 F4.3 Jy flux100 *? Mantissa for 100 um Flux Density
50- 53 I4 --- exp100 *? Exponent for 100 um Flux Density
55 A1 --- q_flux12 *[HMU] Quality of flux12
56 A1 --- q_flux25 *[HMU] Quality of flux25
57 A1 --- q_flux60 *[HMU] Quality of flux60
58 A1 --- q_flux100 *[HMU] Quality of flux100
60- 61 I2 --- cat *? Catalog Number
63- 75 A13 --- name *Object Name in Other Catalog
78 A1 --- rem *[*] Remark
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Note on yr*:
yr1 and yr2 are the starting and ending years of the interval during which
geometric events occur for the object. Some of the objects for which
the ending year indicated is 1990 may actually have events in
subsequent years because times later than 1990 were not considered in
the present work. For objects having two intervals during 1986-1990
in which geometric events occur, the second interval is indicated in
the line following the first entry.
Note on flux*:
flux fields list the mantissa of the 12, 25, 60 and 100 um flux densities,
in Janskys, as given in the IRAS Point Source Catalog.
Note on exp*:
exp fields list the exponent of the 12, 25, 60 and 100 um flux densities,
in Janskys, as given in the IRAS Point Source Catalog.
Note on q_flux*:
q_flux fields refer to the flux-quality flags at 12, 25, 60 and 100 um,
as indicated in the IRAS Point Source Catalog:
H = high-quality detection
M = medium-quality detection
U = upper bound
Note on cat:
For an object for which an identification with an object listed in some
other astronomical catalog is provided in the IRAS Point Source
Catalog, the catalog number, following the conventions of the IRAS
Point Source Catalog, is given.
Note on name:
For an object for which an identification with an object listed in some
other astronomical catalog is provided in the IRAS Point Source
Catalog, the first object name, following the conventions of the IRAS
Point Source Catalog, is given.
Note on rem:
An asterisk appears where there is more than one identification with an
object listed in another astronomical catalog. Only the first is
indicated in cat and name. The rest may be obtained from the original
catalog.
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Acknowledgement:
We thank Dr. Simon for forwarding this catalog to the ADC.
References:
Simon M., Cassar L., Chen W. P., 1986, Ap.J.Sup. 62, 673.
Van Flandern, T. C. and Pulkinnen, K. F., 1979, Ap.J.Sup. 41, 391.
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(End) Julie Anne Watko [SSDOO/ADC] 09-FEB-1996
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