IRAS Explanatory Supplement
X. The Formats of the IRAS Catalogs and Atlases
B. Point Sources
B.4 Meaning of the Source Association Fields
Catalog Field and Meaning*
1 GCVS Type Blank
Field1 = Code gives meaning for Fields 2-3
if Field1 = 1 Field2 and Field3 are B mag [decimag] at max,min
= 2 Field2 and Field3 are V mag [decimag] at max,min
= 3 Field2 and Field3 are photographic mag [decimag] at max,min
= 4 Field2 and Field3 are estimated V mag [decimag] at max,min
= 5 Field2 is 999 and Field3 is 0
2 Dearborn Obs. Type Blank
Field1 Code for Field2 (1,2)
Field2 if Field1 is 1, Field2 is red magnitude
[decimag]* if field1 is 2, field2 is 999
Field3 0
3 Revised AFGL Type Blank
Field1 Magnitude at 4.2 µm [decimag]
Field2 Magnitude at 12 µm [decimag]
Field3 Magnitude at 25 µm [decimag]
4 2-µm Sky Survey Type Blank
Field1 K magnitude [decimag]
Field2 I magnitude [decimag]
Field3 0
5 Globules (Wesselius) Type Blank
Field1 999
Field2 Minimum diameter [arcsec]
Field3 Maximum diameter [arcsec]
6 RC2 Type Blank
Field1 Harvard V magnitude [decimag]
Field2 BT [decimag]
Field3 Do [arcsec]
7 Stars with em. lines Type Blank
Field1 V magnitude [decimag]
Field2 999
Field3 0
8 Equatorial IR Cat. Type Blank
Field1 Flux density [10-16 W
cm-2 µm-1]
at 2.7 µm
Field2 999
Field3 0
9 UGC Type Blank
Field1 Zwicky magnitude [decimag]
Field2 Minimum diameter [arcsec] in B
Field3 Maximum diameter [arcsec] in B
10 MCG Type Blank
Field1 999
Field2 Minimum diameter [arcsec] in B
Field3 Maximum diameter [arcsec] in B
11 Strasbourg Planetary Nebulae Type Blank
Field1 V magnitude of Nebula [decimag]
Field2 B magnitude of Center Star [decimag]
Field3 Minimum diameter of Nebula [arcsec]
12 Zwicky Type Blank
Field1 Zwicky magnitude [decimag]
Field2 999
Field3 0
13 SAO Type Spectral Type
Field1 V magnitude [decimag]
Field2 p g magnitude [decimag]
Field3 0
14 ESO/UPPSALA Type First 3 characters of object type
Field1 B magnitude [decimag]
Field2 Maximum diameter [arcsec]
Field3 Minimum diameter [arcsec]
15 Bright Stars Type Spectral Type
Field1 V magnitude [decimag]
Field2 B-V [centimag]
Field3 U-B [centimag]
16 Suspected Var. Type Spectral Information
Field1 V magnitude at maximum [decimag]
Field2 999
Field3 0
17 Carbon Stars Type Spectral Type (May be truncated)
Field1 p g magnitude [decimag]
Field2 V magnitude [decimag]
Field3 I magnitude [decimag]
18 Gliese Type Spectral Type (May be truncated)
Field1 V magnitude [decimag]
Field2 B-V magnitude [millimag]
Field3 U-B magnitude [millimag]
19 S Stars Type Blank
Field1 p g magnitude [millimag]
Field2 V magnitude [decimag]
Field3 I magnitude [decimag]
20 Parkes HII Survey Type Blank
Field1 999
Field2 Minimum diameter [arcsec]
Field3 Maximum diameter [arcsec]
21 Bonn HII Survey Type Blank
Field1 Flux density at 4.875 GHz (Jy)
Field2 Diameter [arcsec]
Field3 0
22 Blitz Type Blank
Field1 Diameter [arcsec]
Field2 Vco [Km/s]
Field3 Peak TA [K]
23 OSU Type Blank
Field1 999
Field2 999
Field3 Diameter [arcsec]
24 IRC Type C if 2.2 µm sources are possibly confused, w/good pos. blank otherwise
Field1 Right ascension difference (IRC-IRAS) [deciseconds of time]
Field2 Declination difference (IRC-IRAS) [seconds of time]
Field3 0
25 DDO Type Blank
Field1 999
Field 2 999
Field3 0
26 Arp Type Blank
Field1 999
Field2 999
Field 0
27 Markarian Type Blank
Field1 999
Field2 999
Field3 0
28 Strong 5 GHz Type Object type (GAL or QSO)
Field1 V magnitude [decimag]
Field2 5 GHz flux density [deciJy]
Field3 0
29 Veron-Veron Type Object classification
Field1 V magnitude [decimag]
Field2 Redshift × 1000
Field3 0
30 Zwicky 8 Lists Type Blank
Field1 999
Field2 999
Field3 0
31 VV Type Blank
Field1 Special flag, (see below) 999 otherwise
Field2 999
Field3 0
* In the printed version FIELD1 is listed if present except for
catalogs 2 and 19, where FIELD2 is given.
Field1 Explanation
10 VV10 has the same coordinates as VV 29 in the VV Atlas. The UGC was used to confirm that the coordinate is correct for VV 29 and erroneous for VV 10. The UGC position for VV 10 = UGC 10814 was adopted.
11 The VV position is substantially different (>400") from positions for the object in other catalogs. The VV position has been assumed to be in error because two or more other catalogs agree on a different position. The UGC position has been adopted.
12 Same as for 11, but the OSU position has been adopted.
13 The position in the VV Atlas, and the position listed for the VV objest in the OSU are in disagreement. The true position has been established to be close to that of the OSU by the use of overlay transparencies
on the POSS, The OSU position has been adopted.
14 Same as for 13, but the OSU position is not very good either, so a new position has been measured (accurate to about 1').
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