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II/15       Photometric Measurements in the UBVr 20 System (Magnenat 1973)

Catalogue of Photometric Measurements in the UBVr 20 System Magnenat P. <CDS Internal Report No. 6 (1973)>
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. See also: GCPD/69 : The General Catalogue of Photometric Data, maintained by Lausanne-Geneva File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file obs.dat 80 418 Observations of UBVr 20 colors mean.dat 80 366 Weighted means for stars in multiple lists refs.dat 80 41 References to individual lists codes.dat 80 169 *Definition of the coded numbering system
Notes on codes.dat: ampersands "&" in data files have been changed to "+"-------------------------------------------------------------------------------- Byte-by-byte Description of file: obs.dat mean.dat
Byte-by-byte Description of file: obs.dat mean.dat
Bytes Format Units Label Explanations
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_Nobs *Remark about Nobs (obs.dat only) 38- 40 I3 --- Nobs ? Number of measurements (obs.dat only) 43- 49 F7.3 mag Vmag ? V magnitude 76- 80 I5 --- ref ? Reference number (see refs.dat)
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_Nobs: / = N is unknown (1 is assumed) * = N is a minimum number blank = N is exact
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
2- 3 I2 --- ref ? Reference number 6- 80 A75 --- text Reference (multiline)
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. =1963ApJ...137.1057S Johnson H.L. and Harris D.L.III. =1954ApJ...120..196J Johnson H.L. and Morgan W.W. =1953ApJ...117..313J Mermilliod J.Cl., CDS RISP 5
(End) Julie Anne Watko [SSDOO/ADC] 30-MAY-1996
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

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