J/AJ/155/235  Speckle interferometry at SOAR in 2016 and 2017 (Tokovinin+, 2018)

Speckle interferometry at SOAR in 2016 and 2017. Tokovinin A., Mason B.D., Hartkopf W.I., Mendez R.A., Horch E.P. <Astron. J., 155, 235 (2018)> =2018AJ....155..235T 2018AJ....155..235T (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Interferometry ; Photometry, VRI ; Spectral types ; Parallaxes, trigonometric Keywords: binaries: visual Abstract: The results of speckle interferometric observations at the 4.1 m Southern Astrophysical Research Telescope in 2016 and 2017 are given, totaling 2483 measurements of 1570 resolved pairs and 609 non-resolutions. We describe briefly recent changes in the instrument and observing method and quantify the accuracy of the pixel scale and position angle calibration. Comments are given on 44 pairs resolved here for the first time. The orbital motion of the newly resolved subsystem BU 83 Aa,Ab roughly agrees with its 36-year astrometric orbit proposed by J. Dommanget. Most Tycho binaries examined here turned out to be spurious. Description: The observations reported here were obtained with the high-resolution camera (HRCam) - a fast imager designed to work at the 4.1 m SOAR telescope (Tokovinin & Cantarutti 2008PASP..120..170T 2008PASP..120..170T; Tokovinin 2018PASP..130c5002T 2018PASP..130c5002T). For practical reasons, the camera was mounted on the SOAR Adaptive Module (SAM, Tokovinin et al. 2016PASP..128l5003T 2016PASP..128l5003T). However, the laser guide star of SAM was not used (except in 2016 January) because it was not needed and, moreover, reduced the productivity by adding an overhead. The deformable mirror of SAM was passively flattened and the images are seeing-limited. The SAM module contains the atmospheric dispersion corrector (ADC) and helps to calibrate the pixel scale and orientation of HRCam (see SOAR14). The transmission curves of HRCam filters are given in the instrument manual. We used mostly the Stromgren y filter (543/22 nm) and the near-infrared I filter (788/132 nm). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 102 2483 Measurements of double stars at SOAR table4.dat 69 612 Unresolved stars table5.dat 81 44 Newly resolved pairs refs.dat 83 163 List of references -------------------------------------------------------------------------------- See also: B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2014) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/337 : Gaia DR1 (Gaia Collaboration, 2016) J/AJ/139/743 : Speckle interferometry in 2008-09 (Tokovinin+, 2010) J/AJ/143/42 : Speckle interferometry with SOAR in 2010 & 2011 (Hartkopf+, 2012) J/AJ/144/56 : Speckle interferometry at SOAR in 2012 (Tokovinin+, 2012) J/AJ/147/123 : Speckle interferometry with SOAR in 2012-2013 (Tokovinin+, 2014) J/AJ/150/50 : Speckle interferometry at SOAR in 2014 (Tokovinin+, 2015) J/AJ/151/153 : Speckle interferometry at SOAR in 2015 (Tokovinin+, 2016) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS idenfitication (HHMMm+DDMM, J2000) 12- 19 A8 --- Disc Discoverer designation 21- 25 A5 --- Comp Components designation 27- 36 A10 --- OName Other name 38- 46 F9.4 yr Epoch [2009.6693/2017.83] Epoch of observation (expressed as a fractional Julian year) 48 A1 --- Filt [VRIy] Filter used 50 I1 --- Nobs [1/7] Number of observation(s) used 52- 56 F5.1 deg PA [0/359.9] Position angle θ 58- 61 F4.1 mas err [0/27.9] Internal error in tangential direction (pσθ) 63- 68 F6.4 arcsec Sep [0.0176/4.1081] Separation ρ 70- 73 F4.1 mas e_Sep [0/27.8] The 1σ uncertainty in Sep 75- 78 F4.1 mag Dmag [0/7.6] Magnitude difference of pair Δm 80 A1 --- f_Dmag [*:q] Flag on Dmag (G1) 82- 86 F5.1 deg (O-C)PA [-92.4/260.4]? The (O-C) in PA 88- 93 F6.3 arcsec (O-C)Sep [-0.544/0.304]? The (O-C) in Sep 95-102 A8 --- Ref Reference code (see refs.dat file) (1) -------------------------------------------------------------------------------- Note (1): Reference codes for this Table are also available at http://ad.usno.navy.mil/wds/orb6/wdsref.txt. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS idenfitication (HHMMm+DDMM, J2000) 12- 21 A10 --- Disc Discoverer designation 23- 27 A5 --- Comp Components designation 29- 38 A10 --- OName Other name 40- 48 F9.4 yr Epoch [2016.0481/2017.83] Epoch of observation (expressed as a fractional Julian year) 50 A1 --- Filt [RIyH] Filter used 52 I1 --- Nobs [1/4] Number of observation(s) used 54- 58 F5.3 arcsec Sepmin [0.028/0.214] Mininimum resolvable separation ρmin 60- 63 F4.2 mag Dm0.15 [0/5.51] The 5σ magnitude difference at 0.15" Δm(0.15") 65- 68 F4.2 mag Dm1 [0/7.15] The 5σ magnitude difference at 1" Δm(1") 69 A1 --- f_Dmag [:] Flag for noisy data -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS idenfitication (HHMMm+DDMM, J2000) 12- 19 A8 --- Disc Discoverer designation 21- 25 A5 --- Comp Components designation 27- 37 A11 --- OName Other name 39- 45 F7.4 yr Epoch [16.133/17.8248] Epoch of observation (expressed as a fractional Julian year, -2000) 47 A1 --- Filt [Iy] Filter used 49- 54 F6.2 deg PA [27.3/350.6] Position angle θ 56- 61 F6.4 arcsec Sep [0.0294/2.618] Separation ρ 63- 65 F3.1 mag Dmag [0.1/6.1] Magnitude difference of pair Δm 66 A1 --- f_Dmag [*:q] Flag on Dmag (G1) 68- 75 A8 --- SpType Spectral type (as given in SIMBAD) 77- 80 F4.1 mas Plx [1.2/44.5]? The Hipparcos parallax (van Leeuwen 2007, Cat. I/311) 81 A1 --- f_Plx [*] Denotes a Gaia parallax (Gaia Collaboration et al. 2016, Cat. I/337) -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Ref Reference code 10- 41 A32 --- Aut Author's name(s) 43- 61 A19 --- Bibcode Bibcode of the reference 63- 83 A21 --- Com Comment on the reference -------------------------------------------------------------------------------- Global notes: Note (G1): Flag as follows: * = Δm and the true quadrant are determined from the resolved long-exposure image; : = Data are noisy and Δm is likely over-estimated (see Tokovinin et al. 2010, J/AJ/139/743 for details); q = True quadrant is established from the shift-and-add (SAA) image (Section 2.4). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Tiphaine Pouvreau [CDS] 14-Dec-2018
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