Search catalogue
J/AJ/141/157 Speckle interferometry at USNO. XVI. (Mason+, 2011)
Speckle interferometry at the U.S. Naval Observatory. XVI. Mason B.D., Hartkopf W.I., Wycoff G.L. <Astron. J., 141, 157 (2011)> =2011AJ....141..157M
ADC_Keywords: Stars, double and multiple ; Interferometry Keywords: binaries: general - binaries: visual - techniques: interferometric Abstract: The results of 1031 speckle-interferometric observations of double stars, made with the 26 inch refractor of the U.S. Naval Observatory, are presented. Each speckle-interferometric observation of a system represents a combination of over two thousand short-exposure images. These observations are averaged into 457 mean relative positions and range in separation from 0.15" to 16.94", with a median separation of 3.03". The range in V-band magnitudes for the primary (secondary) of observed targets is 3.1-12.9 (3.2-13.3). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 58 320 Speckle-interferometric measurements of double stars table3.dat 111 144 Speckle-interferometric measurements and residuals to systems with orbits or linear elements
See also: J/AJ/117/1905 : Speckle interferometry at USNO. II (Germain+, 1999) J/AJ/117/2511 : Speckle interferometry at USNO. III (Germain+, 1999) J/AJ/118/1395 : Speckle interferometry at USNO. IV (Douglass+, 1999) J/AJ/119/3071 : Speckle interferometry at USNO. V (Douglass+, 2000) J/AJ/120/1120 : Speckle interferometry at USNO. VI (Mason+, 2000) J/AJ/122/1586 : Speckle interferometry at USNO. VII (Mason+, 2001) J/AJ/124/2254 : Speckle interferometry at USNO. VIII (Mason+, 2002) J/AJ/127/539 : Speckle interferometry at USNO. IX (Mason+, 2004) J/AJ/128/3012 : Speckle interferometry at USNO. X (Mason+, 2004) J/AJ/131/2687 : Speckle interferometry at USNO. XI (Mason+, 2006) J/AJ/132/2219 : Speckle interferometry at USNO. XII (Mason+, 2006) J/AJ/134/1671 : Speckle interferometry at USNO. XIII (Mason+, 2007) J/AJ/136/2223 : Speckle interferometry at USNO. XIV (Mason+, 2008) J/AJ/140/480 : Speckle interferometry at USNO. XV. (Mason+, 2010) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 10 A10 --- WDS WDS designation (HHMMm+DDMM, J2000) 12- 19 A8 --- Disc Discoverer designation 21- 24 A4 --- Comp Additional system components 27- 34 F8.3 yr Epoch Epoch of observation 36- 40 F5.1 deg PA Position angle θ 41 A1 --- u_PA [:] Uncertainty flag for PA 43- 47 F5.2 arcsec Sep Separation between components ρ 48 A1 --- u_Sep [:] Uncertainty flag for Sep 50 I1 --- N Number of observations contained in the mean 52- 54 I3 --- Nyr ? Number of years since last measure 56- 58 A3 --- Note [C1234] new or confirming observation (G1)
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 10 A10 --- WDS WDS Designation (HHMMs+DDMM, J2000) 12- 19 A8 --- Disc Discoverer designation 21- 24 A4 --- Comp Additional system components 26- 33 F8.3 yr Epoch Epoch of observation 35- 39 F5.1 deg PA Position angle θ 41- 44 F4.2 arcsec Sep Separation between components ρ 46 I1 --- N Number of observations contained in the mean 48- 52 F5.1 deg (O-C)PA The O-C position angle residual 54- 58 F5.2 arcsec (O-C)Sep The O-C separation residual 59 A1 --- L [L] O-C relative to linear mouvement (1) 60 A1 --- Note [C1234] new or confirming observation (G1) 62-111 A50 --- Ref Observation reference
Note (1): L = O-C relative to the most recent determination in the "Catalog of Rectilinear Elements" (Hartkopf et al., 2006, Hartkopf et al., 2006, http://ad.usno.navy.mil/wds/lin1.html)
Global notes: Note (G1): Notes as follows: C = confirming observation 1 = earlier 2006 data not published (Mason et al., 2007, Cat. J/AJ/134/1671) due to larger than expected positional change 2 = earlier 2004 data not published (Mason et al. 2006, Cat. J/AJ/131/2687) due to larger than expected positional change 3 = this pair was "rediscovered" and had its position corrected from arcminute to arcsecond in the WDS. 4 = earlier 2005 data not published (Mason et al., 2006, Cat. J/AJ/132/2219) due to larger than expected positional change
History: From electronic version of the journal References: Douglass et al., Paper I 1997ApJS..111..289D Germain et al., Paper II 1999AJ....117.1905G, Cat. J/AJ/117/1905 Germain et al., Paper III 1999AJ....117.2511G, Cat. J/AJ/117/2511 Douglass et al., Paper IV 1999AJ....118.1395D, Cat. J/AJ/118/1395 Douglass et al., Paper V 2000AJ....119.3071D, Cat. J/AJ/119/3071 Mason et al., Paper VI 2000AJ....120.1120M, Cat. J/AJ/120/1120 Mason et al., Paper VII 2001AJ....122.1586M, Cat. J/AJ/122/1586 Mason et al., Paper VIII 2002AJ....124.2254M, Cat. J/AJ/124/2254 Mason et al., Paper IX 2004AJ....127..539M, Cat. J/AJ/127/539 Mason et al., Paper X 2004AJ....128.3012M, Cat. J/AJ/128/3012 Mason et al., Paper XI 2006AJ....131.2687M, Cat. J/AJ/131/2687 Mason et al., Paper XII 2006AJ....132.2219M, Cat. J/AJ/132/2219 Mason et al., Paper XIII 2007AJ....134.1671M, Cat. J/AJ/134/1671 Mason et al., Paper XIV 2008AJ....136.2223M, Cat. J/AJ/136/2223 Mason et al., Paper XV 2010AJ....140..480M, Cat. J/AJ/140/480
(End) Patricia Vannier [CDS] 04-Aug-2012
| 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 |
© UDS/CNRS