J/AJ/150/151  DSSI observations of binaries. VI. Measures in 2014 (Horch+, 2015)
Observations of binary stars with the Differential Speckle Survey Instrument.
VI. Measures during 2014 at the Discovery Channel Telescope.
    Horch E.P., Van Belle G.T., Davidson J.W.JR, Ciastko L.A., Everett M.E.,
    Bjorkman K.S.
   <Astron. J., 150, 151 (2015)>
   =2015AJ....150..151H 2015AJ....150..151H    (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Photometry
Keywords: astrometry - binaries: visual - techniques: interferometric -
          techniques: photometric
Abstract:
    We present the results of 938 speckle measures of double stars and
    suspected double stars drawn mainly from the Hipparcos Catalog, as
    well as 208 observations where no companion was noted. One hundred
    fourteen pairs have been resolved for the first time. The data were
    obtained during four observing runs in 2014 using the Differential
    Speckle Survey Instrument at Lowell Observatory's Discovery Channel
    Telescope. The measurement precision obtained when comparing to
    ephemeris positions of binaries with very well-known orbits is
    generally less than 2mas in separation and 0.5° in position angle.
    Differential photometry is found to have internal precision of
    approximately 0.1mag and to be in very good agreement with Hipparcos
    measures in cases where the comparison is most relevant. We also
    estimate the detection limit in the cases where no companion was
    found. Visual orbital elements are derived for six systems.
Description:
    We have started a new program of speckle observations of double stars
    at Lowell Observatory's Discovery Channel Telescope (DCT), a 4.3-m
    telescope.
    The Differential Speckle Survey Instrument (DSSI) was on the telescope
    on four occasions during 2014: two nights in March, two in June, eight
    nights from September 30 to October 7, and four more in November for a
    total of 16 nights, of which approximately five were used for binary
    star observations reported here. In Table3, we present our measures of
    double stars.
    There are a number of binaries observed that have orbits of relatively
    high quality in the Sixth Catalog of Visual Orbits of Binary Stars
    (Hartkopf et al., 2001AJ....122.3472H 2001AJ....122.3472H) that were not used in the
    determination of the scale. We may use these to further judge the
    intrinsic accuracy and precision of the measures in Table3. A listing
    of these objects is given in Table4, together with the orbit
    information.
    We also estimate the detection limit at 0.2'' in the cases where no
    companion was found (see Table5).
File Summary:
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 FileName   Lrecl   Records   Explanations
--------------------------------------------------------------------------------
ReadMe         80         .   This file
table3.dat     83       944   Discovery Channel Telescope (DCT) double star
                              speckle measures
table4.dat    128        36   Ephemeris positions and residuals used in the
                              astrometric accuracy study
table5.dat    166       104   High-quality nondetections and 5σ detection
                              limits
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See also:
       B/wds  : The Washington Visual Double Star Catalog (Mason+ 2001-2014)
       I/239  : The Hipparcos and Tycho Catalogues (ESA 1997)
 J/AJ/143/10  : WIYN speckle observations of binaries. VII. (Horch+, 2012)
 J/AJ/141/45  : Speckel observations of HIP stars (Horch+, 2011)
 J/AJ/139/205 : 2007-2008 WIYN speckle observations of binaries (Horch+, 2010)
 J/AJ/136/312 : 2001-2006 WIYN binary stars speckle observations (Horch+, 2008)
Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes Format Units  Label   Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---    WDS     Washington Double Star catalog designation
                                (HHMMm+DDMM, J2000)
  12- 22  A11   ---    OName   Other identifier (HR, ADS, HD, or DM)
  24- 36  A13   ---    Disc    Discoverer designation and component(s)
  38- 43  I6    ---    HIP     [96/118054]? Hipparcos number
  45- 53  F9.4  yr     Date    [2014.2/2014.9] Besselian date of observation
  55- 59  F5.1  deg    PA      [0.8/359.8]? Position angle (θ) (1)
  61- 66  F6.4  arcsec Sep     [0.009/1.2]? Separation of pair (ρ)
  68- 71  F4.2  mag    Dmag    [0/5.39]? Magnitude difference of pair in filter
                                used
  73- 75  I3    nm     lambda  [692/880] Center wavelength of filter used
                                λ
  77- 78  I2    nm     FWHM    [40/50] Full-Width at Half-Maximum of filter used
                                (Δλ)
  80- 83  A4    ---  f_FWHM    Flag for quadrant problem, or other remark (2)
--------------------------------------------------------------------------------
Note (1): Of the secondary star relative to the primary, with North through
     East defining the positive sense.
Note (2): Flag defined as follows:
    a = Quadrant ambiguous;
    b = Quadrant inconsistent with previous measures in the 4th Interferometric
        Catalog of Hartkopf et al. (2001AJ....122.3480H 2001AJ....122.3480H);
    c = Third component noted, but above 1.2arcsec;
    d = This object was used in the determination of the pixel scale and
        detector orientation, so only the magnitude difference measure is
        reported here.
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Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
   Bytes Format Units    Label     Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---      WDS       Washington Double Star catalog designation
                                    (HHMMm+DDMM, J2000)
  12- 23  A12   ---      Disc      Discoverer designation and component(s)
  25- 30  I6    ---      HIP       [981/117761] Hipparcos number
  32- 40  F9.4  yr       Date      [2014.2/2014.8] Besselian date of observation
  42- 46  F5.1  deg      PA        [0.3/341.8] Position Angle (θ)
  48- 52  F5.2  deg    e_PA        [0.02/15.1] Error in PA
  54- 59  F6.4  arcsec   Sep       [0.012/1.12] Separation (ρ)
  61- 66  F6.4  arcsec e_Sep       [0.0001/0.05] Error in Sep
  68- 73  A6    deg      (O-C)t    The position angle residual (Δθ)
  75- 81  A7    arcsec   (O-C)r    The separation residual (Δρ)
  83-126  A44   ---      Ref       Orbit reference
     128  A1    ---    f_Ref       [a] Flag on Ref (a=separation not used) (1)
--------------------------------------------------------------------------------
Note (1): Although the separation uncertainty meets the criteria discussed in
     the text, this object will probably need an orbit refinement after passing
     through periastron, as discussed in Horch et al. (2015AJ....149..151H 2015AJ....149..151H), so
     we have not used the separations here. This does not affect the position
     angles, as it is an edge-on system.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label  Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---     WDS    Washington Double Star catalog designation
                                (HHMMm+DDMM, J2000)
  12- 17  I6    ---     HIP    [7141/110672]? Hipparcos number
  19- 27  F9.4  yr      Date   [2014.2/2014.9] Besselian date of observation
  29- 32  F4.2  mag     Dl692  [2.79/4.71] The 5σ detection limit at 0.2''
                                in the 692nm filter (1)
  34- 37  F4.2  mag     Dl880  [2.48/4.48] The 5σ detection limit at 0.2''
                                in the 880nm filter (1)
  39-166  A128  ---     Note   Notes (2)
--------------------------------------------------------------------------------
Note (1): The 0.2'' value is just above the "knee" in the curve, which gives a
     good reference point for the rest of the curve.
Note (2): If previous observations are mentioned, these are drawn from the 4th
     Interferometric Catalog of Binary Stars (Hartkopf et al.,
     2001AJ....122.3480H 2001AJ....122.3480H).
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History:
    From electronic version of the journal
References:
    Horch et al.,     Paper I         2009AJ....137.5057H 2009AJ....137.5057H
    Horch et al.,     Paper II        2011AJ....141...45H 2011AJ....141...45H, Cat. J/AJ/141/45
    Horch et al.,     Paper III       2011AJ....141..180H 2011AJ....141..180H
    Horch et al.,     Paper IV        2012AJ....144..165H 2012AJ....144..165H
    Horch et al.,     Paper V         2015AJ....149..151H 2015AJ....149..151H
    Horch et al.,     Paper VII       2017AJ....153..212H 2017AJ....153..212H, Cat. J/AJ/153/212
    Horch et al.,     Paper VIII      2019AJ....157...56H 2019AJ....157...56H
(End)                 Prepared by [AAS]; Sylvain Guehenneux [CDS]    18-Apr-2016