J/AJ/150/136        Speckle interferometry at USNO. XX.        (Hartkopf+, 2015)

Speckle interferometry at the U.S. Naval observatory. XX. Hartkopf W.I., Mason B.D. <Astron. J., 150, 136 (2015)> =2015AJ....150..136H 2015AJ....150..136H (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Interferometry Keywords: binaries: general - binaries: visual Abstract: Results are presented of 4222 intensified CCD observations of double stars, made with the 26 inch refractor of the U.S. Naval Observatory in 2013 and 2014. These observations are averaged into 2335 mean relative positions and range in separation from 0.53'' to 83.90'', with a median separation of 11.42''. This is the 20th in this series of papers and covers the period 2013 January 4 through 2014 December 18. Also presented are 13 pairs which are measured for the first time, 12 pairs which appear to be lost, linear elements for 17 pairs, and orbital elements for five additional pairs. Finally, we investigated apparent systematic residuals to earlier measures in this series, and modify scale factors for closer pairs observed between 1990 and the present. Description: This is the 20th in a series of papers from the U.S. Naval Observatory's speckle interferometry program, presenting results of observations obtained at the USNO 26inch telescope in Washington, DC. From 2013 January 4 through 2014 December 18, the 26inch telescope was used on 135 of 451 scheduled nights. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 64 13 New pairs table2.dat 84 2347 Relative astrometry of double stars table3.dat 122 5 New orbital elements table4.dat 141 17 New rectilinear elements refs.dat 215 64 References notes.dat 572 5 Notes -------------------------------------------------------------------------------- See also: B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2014) J/AJ/147/123 : Speckle interferometry at SOAR in 2012-2013 (Tokovinin+, 2014) J/AJ/142/56 : Speckle interferometry at the USNO station (Hartkopf+, 2011) J/AJ/138/813 : Speckle interferometry at Mount Wilson Obs. (Hartkopf+, 2009) J/AJ/135/1334 : Speckle interferometry at the USNO station (Hartkopf+, 2008) J/AJ/108/2299 : ICCD speckle observations of binary stars. XI. (Hartkopf+ 1994) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Hour of Right Ascension of primary (J2000) (1) 4- 5 I2 min RAm Minute of Right Ascension of primary (J2000) (1) 7- 11 F5.2 s RAs Second of Right Ascension of primary (J2000) (1) 13 A1 --- DE- Sign of the Declination of primary (J2000) (1) 14- 15 I2 deg DEd Degree of Declination of primary (J2000) (1) 17- 18 I2 arcmin DEm Arcminute of Declination of primary (J2000) (1) 20- 23 F4.1 arcsec DEs Arcsecond of Declination of primary (J2000) (1) 25- 34 A10 --- WDS WDS name (HHMMMm+DDMM; J2000) (2) 36- 42 A7 --- Disc Discoverer designation (3) 44- 48 A5 --- Comp Component 50- 54 F5.2 mag mag1 [10.4/12.9] Visual magnitude of the primary (1) 56- 60 F5.2 mag mag2 [10.8/14.1] Visual magnitude of the secondary (1) 62- 64 A3 --- n_Disc Circumstance of the discovery (1, 2, or 3) (4) -------------------------------------------------------------------------------- Note (1): Coordinate and magnitude information from CDS. Magnitude information is from one of the catalogs queried in the Aladin sky atlas, operated at CDS, Strasbourg, France. Note (2): Based on the epoch-2000 coordinates of the system primary. Note (3): WSI=Washington Stellar Interferometer. Note (4): The codes for the notes are defined as follows: 1 = Physicality status unknown, but closer than the published pair; 2 = Magnitudes are red, not visual; 3 = Measure originally assigned to WDS 23340+0334 = BAL2581 in Mason et al. 2002 (cat. J/AJ/124/2254), but does not match that pair closely enough. The measure has been reassigned to this new pair. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS name (HHMMm+DDMM; J2000) 12- 19 A8 --- Disc Discover designation 21- 25 A5 --- Comp Component 29- 36 F8.3 yr Epoch [2007/2015]? Besselian year of observation 38- 42 F5.1 deg PA [0/360]? Mean position angle θ (1) 43 A1 --- u_PA [:] Uncertainty flag for PA 45- 49 F5.2 arcsec Sep [0.53/83.9]? Mean separation ρ 50 A1 --- u_Sep [:] Uncertainty flag for Sep 52- 53 I2 --- o_Sep [1/21]? Number of independent observations of system 55- 59 F5.1 deg (O-C)P [-12.2/65.1]? The (O-C) position angle residual (O-C)θ 61- 65 F5.2 arcsec (O-C)S [-3.1/1.9]? The (O-C) separation residual (O-C)ρ 67- 74 A8 --- Ref Published orbit or linear solution reference 76 A1 --- New [N] New pair (see Table1) 78- 80 A3 --- Note Comments about the observation (2) 82- 84 I3 yr Ny [53/121]? Length of time since the system were last measured (3) -------------------------------------------------------------------------------- Note (1): The position angle, measured from north through east, has not been corrected for precession, and is thus based on the equinox for the epoch of observation. Note (2): The codes for the notes are defined as follows: C = Confirming observation; G = First seen in the eyepiece of the Palomar 200in in Grf2012b (Section 4.49). The new measure is closer than that rough estimate, although the period is still probably well over 100y; I = The measure was assigned to this pair as it was the only likely double in the field, but the identification is uncertain; O = The older measure was significantly different from historical measure(s). The large change in position has been confirmed by other recent observations, either by us or in other publications; R = "Rapid-moving" pairs; defined as pairs having orbital periods under 100y; V = This is the vector addition of measures of other pairs in this multiple system. Note (3): Since priority is given to both unconfirmed systems and to systems not observed recently, the time since last observation can be surprisingly large. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS name (HHMMm+DDMM; J2000) 12- 19 A8 --- Disc Discover designation 21- 22 A2 --- Comp [AB] Component 24- 30 F7.3 yr Per [48.7/743.8] Period 32- 38 F7.3 yr e_Per [-0.09/114.2] Formal error in Per 40- 45 F6.4 arcsec a [0.7/1.9] The semimajor axis 47- 52 F6.4 arcsec e_a [0.003/0.18] Formal error in a 54- 59 F6.2 deg i [76.1/140.4] The inclination 61- 64 F4.2 deg e_i [0.2/6.2] Formal error in i 66- 71 F6.2 deg Omega [60.3/287] The longitude of the node Ω 73- 77 F5.2 deg e_Omega [0.17/13.2] Formal error in Omega 79- 86 F8.3 yr T0 [1897.2/1968.5] The epoch of the most recent periastron passage (T0 in Besselian years) 88- 93 F6.3 yr e_T0 [0.1/14.3] Formal error in T0 95-100 F6.4 --- e [0.2/0.91] The eccentricity 102-107 F6.4 --- e_e [0.003/0.05] Formal error in eccentricity 109-114 F6.2 deg omega [42.2/355.8] The longitude of periastron 116-120 F5.2 deg e_omega [0.6/18.5] Formal error in omega 122 I1 --- Gr [2/4] Grade for each orbit (2, 3, or 4) (1) -------------------------------------------------------------------------------- Note (1): See Hartkopf et al. (2001AJ....122.3472H 2001AJ....122.3472H) for the description of the orbit grading criteria (1=definitive to 5=indeterminate). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS name (HHMMm+DDMM; J2000) 12- 19 A8 --- Disc Discover designation 21- 22 A2 --- Comp Component 24- 33 F10.6 arcsec x0 Zero point in x (x0) (1) 35- 42 F8.6 arcsec e_x0 Error in x0 44- 52 F9.6 arcsec/yr ax Slope in x (ax) (1) 54- 61 F8.6 arcsec/yr e_ax Error in ax 63- 72 F10.6 arcsec y0 Zero point in y (y0) (1) 74- 81 F8.6 arcsec e_y0 Error in y0 83- 91 F9.6 arcsec/yr ay Slope in y (ay) (1) 93-100 F8.6 arcsec/yr e_ay Error in ay 102-109 F8.3 yr T0 [1699.4/2276.4] Time of closest apparent separation T0 (1) 111-115 F5.3 yr e_T0 [0.003/0.4] Error in T0 117-122 F6.3 arcsec Sep0 [1.8/45.2] Closest apparent separation ρ0 (1) 124-128 F5.3 arcsec e_Sep0 [0.03/3.4] Error in Sep0 130-135 F6.2 deg PA0 [36.4/329.7] Position angle θ0 (1) 137-141 F5.2 deg e_PA0 [0.45/31.25] Error in PA0 -------------------------------------------------------------------------------- Note (1): See Hartkopf & Mason (2011; http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/lin1) for a description of all terms. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Ref Reference identifier 10- 28 A19 --- BibCode Bibliographic code 30- 62 A33 --- Aut Author's name 64-215 A152 --- Com Comment -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS name (HHMMm+DDMM; J2000) 12-572 A561 --- Note Notes -------------------------------------------------------------------------------- History: From electronic version of the journal References: Douglass et al., Paper I 1997ApJS..111..289D 1997ApJS..111..289D Germain et al., Paper II 1999AJ....117.1905G 1999AJ....117.1905G, Cat. J/AJ/117/1905 Germain et al., Paper III 1999AJ....117.2511G 1999AJ....117.2511G, Cat. J/AJ/117/2511 Douglass et al., Paper IV 1999AJ....118.1395D 1999AJ....118.1395D, Cat. J/AJ/118/1395 Douglass et al., Paper V 2000AJ....119.3071D 2000AJ....119.3071D, Cat. J/AJ/119/3071 Mason et al., Paper VI 2000AJ....120.1120M 2000AJ....120.1120M, Cat. J/AJ/120/1120 Mason et al., Paper VII 2001AJ....122.1586M 2001AJ....122.1586M, Cat. J/AJ/122/1586 Mason et al., Paper VIII 2002AJ....124.2254M 2002AJ....124.2254M, Cat. J/AJ/124/2254 Mason et al., Paper IX 2004AJ....127..539M 2004AJ....127..539M, Cat. J/AJ/127/539 Mason et al., Paper X 2004AJ....128.3012M 2004AJ....128.3012M, Cat. J/AJ/128/3012 Mason et al., Paper XI 2006AJ....131.2687M 2006AJ....131.2687M, Cat. J/AJ/131/2687 Mason et al., Paper XII 2006AJ....132.2219M 2006AJ....132.2219M, Cat. J/AJ/132/2219 Mason et al., Paper XIII 2007AJ....134.1671M 2007AJ....134.1671M, Cat. J/AJ/134/1671 Mason et al., Paper XIV 2008AJ....136.2223M 2008AJ....136.2223M, Cat. J/AJ/136/2223 Mason et al., Paper XV 2010AJ....140..480M 2010AJ....140..480M, Cat. J/AJ/140/480 Mason et al., Paper XVI 2011AJ....141..157M 2011AJ....141..157M, Cat. J/AJ/141/157 Mason et al., Paper XVII 2011AJ....142...46M 2011AJ....142...46M, Cat. J/AJ/142/46 Mason et al., Paper XVIII 2012AJ....143..124M 2012AJ....143..124M, Cat. J/AJ/143/124 Mason et al., Paper XIX 2013AJ....146...56M 2013AJ....146...56M, Cat. J/AJ/146/56 Mason et al., Paper XXI 2017AJ....153...20M 2017AJ....153...20M, Cat. J/AJ/153/20 Mason et al., Paper XXII 2017AJ....154..183M 2017AJ....154..183M, Cat. J/AJ/154/183 Mason et al., Paper XXIII 2018AJ....156..240M 2018AJ....156..240M
(End) Prepared by [AAS]; Sylvain Guehenneux [CDS] 02-Feb-2016
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