I/110       Occultation Double-Star Observations (Evans 1983)

Catalogue of Occultation Double-Star Observations Evans D.S. <IAU Colloquium No. 62, Current Techniques in Double and Multiple Star Research, Lowell Obs. Bull. 167, p. 73 (1983)> =1983LowOB...9...73E 1983LowOB...9...73E (Bull. 167, Volume 9)
ADC_Keywords: Stars, double and multiple ; Occultations Description: This catalog contains data on 224 double stars observed photoelectrically during lunar occultations. The author cites the advantages of this method of double star detection as increased resolution, accuracy of the vector separations of roughly one-half arcsecond or better, and the opportunity to make photometric determinations of the magnitude differences between components. The vector separation is the true separation projected along a line perpendicular to the actual lunar limb. The catalog is a compilation of twelve years of observations from the literature (through roughly 1980). It is divided into three files. The first file, data1.dat, contains information on stars brighter than visual magnitude 6.7. The second, data2.dat, lists SAO catalog stars fainter than magnitude 6.7. The third file, data3.dat, contains data on faint stars with no SAO number. For these stars, data on their magnitudes or spectral types may be absent. In many cases there are multiple records per star, reflecting separate observations. The records are arranged by SAO number or other identifier, and contain visual magnitudes, spectral type, observing run number, a subjective grade of the probability of being double, the vector separation with computed error, position angle, and the lunar limb slope and its error. It also includes the magnitude difference between the components in (somewhat arbitrarily assigned) blue and red band passes. In the case of a triple star, the run number is repeated and the data for the triple given with magnitude differences from the brightest star. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file data1.dat 100 178 m(v) ≤ 6.7 data2.dat 100 211 SAO m(v) > 6.7 data3.dat 100 14 Faint Non-SAO -------------------------------------------------------------------------------- Byte-by-byte Description of file: data1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-6 I6 --- SAO ?SAO Number 10-17 A8 --- NAME ?Other Name for Star 19-23 F5.2 mag MAG ?Magnitude 24-33 A10 --- Sp ?Spectral Type 35-42 A8 --- RUN *?Run Number of the Observation 44-45 I2 --- DAY ?Observation Date Day 46-47 I2 --- MONTH ?Observation Date Month 48-49 I2 --- YEAR ?Observation Date Year 51 I1 --- G *?Grade 52 A1 --- n_G *?Remark on G 54-60 F7.1 marcsec SEP ?Vector Separation 62-65 F4.1 marcsec e_SEP ?Computed Error of Vector Separation 66 A1 --- n_SEP ?Remark on SEP (see note on n_G) 68-70 I3 deg PA *?Position Angle 71 A1 --- n_PA ?Remark on PA (see note on n_G) 73-75 I3 --- SL ?Limb Slope 76 A1 --- n_SL ?Remark on SL (see note on n_G) 77-78 I2 --- e_SL ?Error of SL 80-83 F4.2 mag dB ?Blue Differential Magnitude 85-88 F4.2 mag e_dB ?Error of dB 89 A1 --- n_dB *?Remark on dB 90-94 F5.2 mag dR *?Red Differential Magnitude 96-99 F4.2 mag e_dR ?Error of dR 100 A1 --- n_dR ?Remark on dR (see note on n_dB) -------------------------------------------------------------------------------- Note on RUN: Sources McDonald Observations: M100-1871: Astron. J. 76, 1109, 1971: M1875-M1893, M2102-M22221, M2304-2711: Astron. J. 78, 482, 1973: M1902-M2020, M2250-2262: Astron. J. 80, 449, 1975: M2713-M3712: Astron. J. 80, 689, 1975: M3713-M4009: Astron. J. 81, 650, 1976: M4010-M4245, Astron. J. 82, 631, 1977 (but M4045, M4058, M4059, M4148, Astron. J. 82, 640, 1977): M36/7, M36/8, M4247-M4729: Astron. J. 83, 1100, 1978: M4730-M5222, Astron. J. 85, 478, 1980 (but M5100-M5112: Astron. J. 85, 490, 1980), and M5223-M5646, Astron. J., submitted. Geneva Observations: G12-G38: Astron. J. 80, 445, 1975. Tonantzintla Observations: T001-023: Astron. J. 79, 1299, 1974. Iowa Observations: EB002, EB021: Astron. J. 76, 1131, 1971: EB001-EB121, Astrophys. J. Supp. Ser. 28, 405, 1974: EB122-EB320, : Astrophys. J. Supp. Ser., 34, 493, 1977: EB321-562: Astrophys. J. Supp. Ser., 40, 475, 1979: EB585-592: Astrophys. J. Lett. 228, Llll, 1979. Hamburg Observations: All H numbers, Astron. Astrophys., 48, 245, 1976. Victoria Observations: Vl-V2: Publ. Dom. Astrophys. Obs. 14, 271, 1974: Vl-V32, J. Roy. Astron. Soc. Canada, 72, 305, 1978. Illinois Observations:-I7701-I7865: Astron. J. 85, 1053, 1980. Flagstaff Observations: F, Astron. J. 84, 872, 1979 and private communications. Peterson et al.: P: Astron. J. 86, 280, 1981. Special Stars: Beta Scorpii: Astron. J. 82, 414, 1977. Astron. J. 82, 495, 1977, Astron. J. 83, 438, 1978: Astron. J. 84, 257, 1979. Sigma Scorpii: Publ. Astron. Soc. Pac. 86, 116, 1974. Beta Capricorni: Astrophys. J. 228, 497, 1979. Note on G: 0 No Duplicity 1 Possible Duplicity 2 Probable Duplicity 3 Certain Duplicity Grades are based on statements by observers. Note on n_G: Asterisks (*) denote places where corrections have been applied to published figures, whether errors of star numbers or run numbers in original records or notes. Most commonly corrections have been made as far as can be deduced from the original sources, to bring the column of position angle values to those appropriate to position angles from the brighter to the fainter component. Most changes have been made by 180 degrees. Note on PA: Position Angle on the lunar limb as modified by the slope deduced in favorable cases from the spacing of the diffraction bands on the occultation trace. Note on n_dB: An asterisk indicates that the magnitude difference between components had to be computed from values expressed in different style in the original papers. Note on dR: A negative sign indicates that the "secondary" is fainter in the blue channel and brighter in the red. -------------------------------------------------------------------------------- Byte-by-byte Description of file: data2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-6 I6 --- SAO ?SAO Number 7-8 A2 --- SAOsuf SAO Suffix 10-17 A8 --- NAME Other Name for Star 19-23 F5.2 mag MAG ?Magnitude 24-33 A10 --- Sp Spectral Type 35-42 A8 --- RUN *Run Number of the Observation 44-45 I2 --- DAY ?Observation Date Day 46-47 I2 --- MONTH ?Observation Date Month 48-49 I2 --- YEAR ?Observation Date Year 51 I1 --- G *?Grade 52 A1 --- n_G *Remark on G 54-60 F7.1 marcsec SEP ?Vector Separation 62-65 F4.1 marcsec e_SEP ?Computed Error of Vector Separation 66 A1 --- n_SEP Remark on SEP (see note on n_G) 68-70 I3 deg PA *?Position Angle 71 A1 --- n_PA Remark on PA (see note on n_G) 73-75 I3 --- SL ?Limb Slope 76 A1 --- n_SL Remark on SL (see note on n_G) 77-78 I2 --- e_SL ?Error of SL 80-83 F4.2 mag dB ?Blue Differential Magnitude 85-88 F4.2 mag e_dB ?Error of dB 89 A1 --- n_dB *Remark on dB 90-94 F5.2 mag dR *?Red Differential Magnitude 96-99 F4.2 mag e_dR ?Error of dR 100 A1 --- n_dR Remark on dR (see note on n_dB) -------------------------------------------------------------------------------- Note on RUN: Note on G: Note on n_G: Note on PA: Note on n_dB: Note on dR: For all notes, see notes for data1.dat -------------------------------------------------------------------------------- Byte-by-byte Description of file: data3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-8 F8.4 --- DM ?DM Number 10-17 A8 --- NAME Other Name for Star 19-23 F5.2 mag MAG ?Magnitude 24-33 A10 --- Sp Spectral Type 35-42 A8 --- RUN *Run Number of the Observation 44-45 I2 --- DAY ?Observation Date Day 46-47 I2 --- MONTH ?Observation Date Month 48-49 I2 --- YEAR ?Observation Date Year 51 I1 --- G *?Grade 52 A1 --- n_G *Remark on G 54-60 F7.1 marcsec SEP ?Vector Separation 62-65 F4.1 marcsec e_SEP ?Computed Error of Vector Separation 66 A1 --- n_SEP Remark on SEP (see note on n_G) 68-70 I3 deg PA *?Position Angle 71 A1 --- n_PA Remark on PA (see note on n_G) 73-75 I3 --- SL ?Limb Slope 76 A1 --- n_SL Remark on SL (see note on n_G) 77-78 I2 --- e_SL ?Error of SL 80-83 F4.2 mag dB ?Blue Differential Magnitude 85-88 F4.2 mag e_dB ?Error of dB 89 A1 --- n_dB *Remark on dB 90-94 F5.2 mag dR *?Red Differential Magnitude 96-99 F4.2 mag e_dR ?Error of dR 100 A1 --- n_dR Remark on dR (see note on n_dB) -------------------------------------------------------------------------------- Note on RUN: Note on G: Note on n_G: Note on PA: Note on n_dB: Note on dR: For all notes, see notes for data1.dat --------------------------------------------------------------------------------
(End) Julie Anne Watko [SSDOO/ADC] 03-Nov-1995
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