Astronomical Data Center
ADC/CDS Standard Document for Catalog:
/catalogs/2/2015/
The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:
II/15 Photometric Measurements in the UBVr 20 System (Magnenat 1973)
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Catalogue of Photometric Measurements in the UBVr 20 System
Magnenat P.
<CDS Internal Report No. 6 (1973)>
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ADC_Keywords: Photometry, UBVr20; Colors
Description:
In the UBVr photometric system defined by Sandage and Smith (1963), (U-B)20,
(B-V)20, and (V-r)20 color indices are given for stars from ten reference
lists, along with a LID coded number, V magnitude, number of observations and
reference. A list of weighted means is included for stars appearing on
more than one list. The reference list and an explanation of the coded
numbering system are included in separate files.
Introduction:
The UBVr system is defined by Sandage and Smith (1963). The then recent
availability of photomultipliers with S20 cathodes sensitive to the
wavelength range 3000 to 8000 A suggested that the customary tricolor
photometric system could be extended to include a red point close to 6700 A.
The V-r color index can be employed as a good indicator of effective
temperature, thanks to its relatively small blanketing effect, compared to
B-V.
Sandage and Smith also tried to obtain the U, B and V colors as closely as
possible to those of Johnson and Morgan's system. In 1960, 64 standard
stars of the UBV system (Johnson and Morgan 1953; Johnson and Harris 1954)
were measured. Comparison of colors obtained in the natural photometric
system ubvr 20 with colors from Johnson, Morgan and Harris give:
B-V = 1.100(b-v)20 + 1.023
+/-0.004 +-/0.003
U-B = 1.015(u-b)20 - 1.575
+/-0.003 +/-0.006 (Sandage and Smith 1963)
These equations show that the UBVr 20 system is close to the UBV system
without being identical.
Means were calculated for stars appearing in multiple references according
to the customary manner at CDS, based on the number of measures and the
weight of each list. All ten lists were given weight 4.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
obs.dat 80 418 Observations of UBVr 20 colors
wtdmns.dat 80 366 Weighted means for stars in multiple lists
refs.dat 80 42 References to individual lists
codes.dat 80 169 Definition of the coded numbering system
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Byte-by-byte Description of file: obs.dat, wtdmns.dat
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Bytes Format Units Label Explanations
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1- 11 F11.8 --- LID *Coded number (see codes.dat)
12 A1 --- rem *Remark
13- 18 F6.3 mag U-B20 *? (U-B)20 index
21- 26 F6.3 mag B-V20 *? (B-V)20 index
29- 34 F6.3 mag V-r20 (V-r)20 index
37 A1 --- n_N *Remark about N (obs.dat only)
38- 40 I3 --- N ? Number of measurements (obs.dat only)
43- 49 F7.3 mag V ? V magnitude
76- 80 I5 --- ref ? Reference number (see refs.dat)
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Note on LID:
Defined in J.Cl. Mermilliod, CDS RISP 5 (see codes.dat)
Note on rem:
D = a multiple system
1 or 2 = only one component of a binary was measured
Note on U-B20:
Note on B-V20:
If either field is empty, that signifies that the star was not measured on
the filters in question.
Note on n_N:
/ = N is unknown (1 is assumed)
* = N is a minimum number
blank = N is exact
Byte-by-byte Description of file: refs.dat
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Bytes Format Units Label Explanations
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2- 3 I2 --- ref ? Reference number
6- 80 A75 --- text Reference (multiline)
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Byte-by-byte Description of file: codes.dat
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Bytes Format Units Label Explanations
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1- 80 A80 --- text *Definition of the coded numbering system
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Note on text:
ampersands "&" in data files have been changed to "+"
Acknowledgement:
The text of the introduction is taken from P. Magnenat [CDS], translated
from French to English by J.A. Watko [SSDOO/ADC].
References:
Sandage A. and Smith L. 1963, Astrophys. J., 137, 1057.
Johnson H.L. and Harris D.L.III. 1954, Astrophys. J., 120, 196.
Johnson H.L. and Morgan W.W. 1953, Astrophys. J., 117, 313.
Mermilliod J.Cl., CDS RISP 5
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(End) Julie Anne Watko [SSDOO/ADC] 30-MAY-1996
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