Astronomical Data Center
ADC/CDS Standard Document for Catalog:
/catalogs/2/2106/
The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:
II/106 Search for Ultraviolet-Excess Objects (Noguchi+ 1980; Kondo+ 1984)
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A Search for Ultraviolet-Excess Objects
Noguchi T., Maehara H., Kondo M.
<Ann. Tokyo Astron. Obs., 2nd series, 18, 55 (1980)>
=1980AnTok..18...55N
Kondo M., Noguchi T., Maehara H.
<Ann. Tokyo Astron. Obs., 2nd series, 20, 130 (1984)>
=1984AnTok..20..130K
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ADC_Keywords: Photometry, ultraviolet
Description:
The catalog is a list of 1186 ultraviolet-excess objects found
during two surveys with the Kiso Schmidt telescope of the Tokyo
Astronomical Observatory. The UGR three-image method was used to
detect the objects cataloged, which range in blue magnitude from
about 10.0 to 18.5. The table contains equatorial positions to an
accuracy of about 0.5 seconds of arc (equinox and equator B1950.0,
epoch of observation), magnitudes (green of the "three-image [UGR]
method"), color indices (as estimated from the enhancement of the U
image relative to the G), object codes (white dwarf, QSO, diffuse
object, etc.), and alternate designations (in addition to a KUV
coordinate designation).
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
catalog.dat 80 1186 Catalog data
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Byte-by-byte Description of file: catalog.dat
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Bytes Format Units Label Explanations
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1- 5 I5 --- KUV_RA *KUV coordinate designation - RA
6- 10 I5 --- KUV_DE *KUV coordinate designation - DE
11 A1 --- Comp Component identification
13- 16 I4 --- KISO_a *KISO area number
18- 19 I2 --- KISO-n *Number within KISO area
23- 24 I2 h RAh Right Ascension (hours), equinox 1950
26- 27 I2 min RAm RA (minutes)
29- 33 F5.2 s RAs RA (seconds)
36 A1 --- DE- sign of declination zone, equinox 1950
37- 38 I2 deg DEd DEC (degrees)
40- 41 I2 arcmin DEm DEC (minutes)
43- 46 F4.1 arcsec DEs [0/60] DEC (seconds)
49- 53 F5.2 mag G *G magnitude
54 A1 --- u_G G uncertainty code
55- 58 F4.1 mag CI *Color index
59 A1 --- u_CI CI uncertainty code
61 A1 --- Ocode *Object code
63- 80 A18 --- Ref *Alternate designation
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Note on KUV_RA and KUV_DE:
KUV coordinate designation is composed of hours and minutes of right
ascension, sign, and degrees and minutes of arc of declination. Note that
this coordinate designation does not follow the standard IAU convention
because the coordinates are rounded and not truncated.
Note on KISO_a and KISO-n:
Another designation consisting of a Kiso area number (see Kiso Information
bulletin No. 1, 1979) and a serial number within the area.
Note on G:
The G (green) magnitude of the "three-image (UGR) method" used for
efficient detection of blue objects, e.g., by Haro & Herbig (1955), Iriarte
& Chavira (1957), Haro & Luyten *(1962), and others. See the source
reference for additional details. A colon (:) in byte 54 denotes an
uncertain value.
Note on CI:
Estimated as the enhancement in the U image relative to the G, calibrated
with known values of U-B color. A colon (:) in byte 59 denotes an uncertain
value.
Note on Ocode:
A letter object code to denote the following characteristics:
W spectroscopically confirmed white dwarf
Q quasar
D diffuse object with possible accompanying halo
V variable that is definitely brighter or fainter on print of the
Palomar Observatory Sky Survey than on the Kiso plate
Note on Ref:
An alternate object designation in a previous catalog, composed of a
reference number in bytes 63-64, followed by the designation in the cited
catalog.
Remarks and Modifications:
A magnetic tape containing the first and second Kiso Surveys in separate
files was received from Dr. M. Kondo on March 11, 1985. The following
modifications were made to produce the current catalog:
1. The two lists were moved to online storage and merged
2. Minus signs on negative declinations were moved to always occur in the
same byte. Zero declinations had lost their signs; these were added by
using the respective KUV designations. Plus signs were then added to all
positive declinations.
3. Uncertainty codes for G magnitude were moved to byte 54 so that they do
not occur within the magnitude field.
4. The combined list was sorted by increasing right ascension.
References:
Haro G., Herbig G.H. 1955, Bol. Obs. Tonantzintlay Tacubaya No. 14, 8
Haro G., Luyten W.J. 1962, Bol. Obs. Tonantzintlay Tacubaya No. 32, 37
Iriarte B., Chavira E. 1957, Bol. Obs. Tonantzintlay Tacubaya No. 16, 3
Kondo M., Noguchi T., Maehara H. 1984, Ann. Tokyo Astron. Obs.
2nd Ser., 20, 130
Noguchi T., Maehara H., Kondo M. 1980, Ann. Tokyo Astron. Obs.
2nd Ser., 18, 55
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(End) M.C. Larkin [SSDOO/ADC] C.-H. Joseph Lyu [Hughes STX/NASA] 25-May-1995
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