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J/other/SAAOC/15.30              DDO photometry of E-region stars (Cousins 1993)

DDO photometry of E-region stars and equatorial standards (Paper I). Cousins A.W.J. <South Afr. Astron. Obs. Circ. 15, 30 (1993)> =1993SAAOC..15...30C (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, DDO Abstract: This paper describes the observations and gives the results of a series of observations of bright E-region stars (Cousins A.W.J. and Stoy R.H., 1962RGOB...49....3C) for use as zero point stars for DDO photometry in the southern hemisphere. The list comprises 45 stars, all brighter than V=6.0, and gives the colours in the instrumental system with internal s.e. ±0.001mag and m48 with s.e. ±0.002mag. The observed m48 is indistinguishable from McClure's system and has the same zero point (±0.002mag). The individual E-region zero points have been established with s.e. ±0.001 relative to the instrumental system, but the colour equations (and zero point corrections) to transform the instrumental colours to McClure's system have still to be finalised. For a description of the DDO photometric system, see e.g. GCPD/12 File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 87 20 Observed and computed zero point differences table2 101 9 Zero point errors table3 43 45 DDO photometry of E region stars (Colours in the instrumental system) table1a 65 30 Transmissions of DDO filters used at Cape Town table2b 13 40 B-V and m48-V colours
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
1 A1 --- Group [ab] Group 2- 6 A5 --- E E-regions (1) 8- 11 F4.1 mmag Obs35 Observed zero point differences in C(35-38) 13- 16 F4.1 mmag Cor35 ? Corrected zero point differences in C(35-38) 18- 21 F4.1 mmag Comp35 ? Computed zero point differences in C(35-38) 23- 27 F5.1 mmag Obs38 Observed zero point differences in C(38-41) 29- 33 F5.1 mmag Cor38 ? Corrected zero point differences in C(38-41) 35- 39 F5.1 mmag Comp38 ? Computed zero point differences in C(38-41) 42- 45 F4.1 mmag Obs41 Observed zero point differences in C(41-42) 47- 50 F4.1 mmag Cor41 ? Corrected zero point differences in C(41-42) 52- 55 F4.1 mmag Comp41 ? Computed zero point differences in C(41-42) 58- 61 F4.1 mmag Obs42 Observed zero point differences in C(42-45) 63- 66 F4.1 mmag Cor42 ? Corrected zero point differences in C(42-45) 68- 71 F4.1 mmag Comp42 ? Computed zero point differences in C(42-45) 74- 77 F4.1 mmag Obs45 Observed zero point differences in C(45-48) 79- 82 F4.1 mmag Cor45 ? Corrected zero point differences in C(45-48) 84- 87 F4.1 mmag Comp45 ? Computed zero point differences in C(45-48)
Note (1): For each group, the region labelled Total indicates the total observed zero point differences in each colours
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
1 I1 --- E E-region number 3- 6 F4.1 mmag zpe135 Zero point error for adjacent regions in C(35-38) 8- 11 F4.1 mmag zpe235 Zero point error for alternate regions in C(35-38) 13- 16 F4.1 mmag zpeM35 Means zero point error in C(35-38) 18- 21 F4.1 mmag zpeR35 Revised means zero point error in C(35-38) 23- 26 F4.1 mmag zpe138 Zero point error for adjacent regions in C(38-41) 28- 31 F4.1 mmag zpe238 Zero point error for alternate regions in C(38-41) 33- 36 F4.1 mmag zpeM38 Means zero point error in C(38-41) 38- 41 F4.1 mmag zpeR38 Revised means zero point error in C(38-41) 43- 46 F4.1 mmag zpe141 Zero point error for adjacent regions in C(41-42) 48- 51 F4.1 mmag zpe241 Zero point error for alternate regions in C(41-42) 53- 56 F4.1 mmag zpeM41 Means zero point error in C(41-42) 58- 61 F4.1 mmag zpeR41 Revised means zero point error in C(41-42) 63- 66 F4.1 mmag zpe142 Zero point error for adjacent regions in C(42-45) 68- 71 F4.1 mmag zpe242 Zero point error for alternate regions in C(42-45) 73- 76 F4.1 mmag zpeM42 Means zero point error in C(42-45) 78- 81 F4.1 mmag zpeR42 Revised means zero point error in C(42-45) 83- 86 F4.1 mmag zpe145 Zero point error for adjacent regions in C(45-48) 88- 91 F4.1 mmag zpe245 Zero point error for alternate regions in C(45-48) 93- 96 F4.1 mmag zpeM45 Means zero point error in C(45-48) 98-101 F4.1 mmag zpeR45 Revised means zero point error in C(45-48)
Byte-by-byte Description of file: table3
Bytes Format Units Label Explanations
1- 4 A4 --- Star E-region star name 6- 10 F5.3 mag C(45-48) C(45-48) colour 12- 17 F6.3 mag C(42-45) C(42045) colour 19- 23 F5.3 mag C(41-42) C(41-42) colour 25- 30 F6.3 mag C(38-41) C(38-41) colour 32- 36 F5.3 mag C(35-38) C(35-38) colour 38- 42 F5.3 mag m48 ? m48 magnitude 43 A1 --- n_m48 [Vm] Note for variable stars (1)
Note (1): Six stars are variable in light. A 'm' indicates mean magnitudes for two stars with small ranges. E542 is an EA type star and the maximum magnitude is given. A 'V' indicates other variables.
Byte-by-byte Description of file: table1a
Bytes Format Units Label Explanations
1- 5 F5.1 nm W35 ? Wavelength in 35 filter 7- 10 F4.1 % T35 ? Transmition in 35 filter 12- 16 F5.1 nm W38 Wavelength in 38 filter 18- 21 F4.1 % T38 Transmition in 38 filter 23- 27 F5.1 nm W41 ? Wavelength in 41 filter 29- 32 F4.1 % T41 ? Transmition in 41 filter 34- 38 F5.1 nm W42 ? Wavelength in 42 filter 40- 43 F4.1 % T42 ? Transmition in 42 filter 45- 49 F5.1 nm W45 ? Wavelength in 45 filter 51- 54 F4.1 % T45 ? Transmition in 45 filter 56- 60 F5.1 nm W48 ? Wavelength in 48 filter 62- 65 F4.1 % T48 ? Transmition in 48 filter
Byte-by-byte Description of file: table2b
Bytes Format Units Label Explanations
1- 5 F5.2 mag B-V B-V colour index 7- 12 F6.3 mag m48-V m_48-V colour index -------------------------------------------------------------------------------- Table 1b. Effective Wavelengths, Widths and Second Moments of DDO Filters ------------------------------------------------------------------------- Cousins ------------------------------------------------------------------------- lambdam (nm) 353.1 381.6 416.4 425.8 452.1 488.0 FWHM (nm) 28.0 28.7 7.6 7.9 6.8 18.3 mu2 (nm) 9.75 10.52 2.80 2.70 2.23 6.16 ------------------------------------------------------------------------- McClure's "Yale" filters ------------------------------------------------------------------------- lambdam (nm) 347.4 382.3 416.4 425.6 452.1 488.3 FWHM (nm) 37.2 33.0 8.0 7.1 7.3 18.6 mu2 (nm) 12.35 11.40 2.58 2.31 2.36 6.28 ------------------------------------------------------------------------- John Caldwell has computed a polynomial transformation to derive m-V from (B-V-0.800), and finds that the following coefficients give a good fit. (Zero order is the constant term). ------------------ Order Coefficient ------------------ 0 0.2960158 1 0.3250211 2 0.1475044 3 - 0.0216403 4 - 0.0875551 5 0.3587868 6 0.0220998 7 -0.2140784 ------------------ Table2b may be useful when a few stars are involved.
History: Prepared via OCR at CDS.
(End) James Marcout, Patricia Bauer [CDS] 28-Jan-1997
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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