J/AJ/146/52 CCD measurements of multiple stars at NAOR and ASV (Pavlovic+, 2013)

CCD measurements of double and multiple stars at NAO Rozhen and ASV in 2011. Five linear solutions. Pavlovic R., Cvetkovic Z., Boeva S., Vince O., Stojanovic M. <Astron. J., 146, 52 (2013)> =2013AJ....146...52P 2013AJ....146...52P (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Photometry, CCD Keywords: binaries: visual - stars: individual (** STT 547AC, ** STT 547AD, ** STT 547AE, ** POP 217AP, ** MLB 259) - techniques: image processing Abstract: Using the 2m telescope of the Bulgarian National Astronomical Observatory at Rozhen, observations of 222 double or multiple stars were carried out during three nights in 2011. This is the sixth series of measurements of CCD frames of double and multiple stars obtained at Rozhen. Also in 2011, using the 0.6m telescope of the Serbian Astronomical Station on the mountain of Vidojevica, observations of 208 double or multiple stars were carried out during six nights. This is the first series of measurements of CCD frames of double and multiple stars obtained at this station. In this paper, we present the results for the position angle and angular separation for 337 pairs and residuals for 72 pairs with published orbital elements or linear solutions. These observations have angular separations in the range from 1.37'' to 172.81'', with a median angular separation of 7.66''. We also present the recalculated linear solutions for four pairs and one linear solution that has been calculated for the first time. Description: Using the 2m telescope of the Bulgarian National Astronomical Observatory at Rozhen (NAOR), observations of 222 double or multiple stars were carried out during three nights in 2011: one night on 2011 March 28/29 and two nights on 2011 October 27/28 and 28/29. This is the sixth series of measurements of CCD frames of double and multiple stars obtained at Rozhen. For each double or multiple star, 10 frames were obtained: 5 in the Johnson B filter and 5 in the Johnson V filter. From June to the end of 2011, we carried out CCD observations of 208 visual double or multiple stars at the new Astronomical Station on the mountain of Vidojevica (ASV). This station belongs to the Astronomical Observatory of Belgrade. It is located in southern Serbia near the town of Prokuplje. More details can be found at the observatory's Web site (http://belissima.aob.rs/). Observations were carried out during six nights: one night on June 18/19, August 19/20, and October 19/20, and three nights on November 2-5. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 68 409 CCD measurements of double and multiple stars table4.dat 82 129 CCD measurements of system with orbits or rectilinear solutions table7.dat 57 92 Measurements and residuals from old and new linear solutions for five pairs refs.dat 148 29 References -------------------------------------------------------------------------------- See also: B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2014) V/39 : 4th Catalog of Orbits of Visual Binaries (Worley+, 1983) J/AJ/142/73 : Multiple stars NAO Rozhen CCD measurements (Cvetkovic+, 2011) J/AJ/142/56 : Speckle interferometry at the USNO station (Hartkopf+, 2011) J/AJ/123/1023 : Binary star orbits (Seymour+, 2002) J/PAZh/27/456 : Astrometric study of ADS 48 (Kiyaeva+, 2001) http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/WDS : WDS catalog http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6 : 6th catalog of orbits of visual binary stars Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS designation (HHMMm+DDMM; J2000) 12- 18 A7 --- Disc Discoverer designation 20- 23 A4 --- m_Disc Designation for pair components 25- 33 F9.4 yr Epoch Epoch of the observation (Besselian year) 35- 40 F6.2 arcsec Sep Angular separation ρ (G1) 42- 47 F6.2 deg PA [0.11/360.88] Position angle θ (G1) 49- 52 F4.2 mag Dmag Magnitude difference (G2) 54- 68 A15 --- Camera Camera used in the observation (G3) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS designation (HHMMm+DDMM; J2000) 12- 18 A7 --- Disc Discoverer designation 19- 20 A2 --- m_Disc Designation for pair components 22- 30 F9.4 yr Epoch ? Epoch of the observation (Besselian year) 32- 37 F6.2 arcsec Sep ? Angular separation ρ (G1) 39- 44 F6.2 deg PA ? Position angle θ (G1) 46- 49 F4.2 mag Dmag ? Magnitude difference (G2) 51- 55 F5.2 arcsec (O-C)S Angular separation (O-C) value 57- 60 F4.1 deg (O-C)A Position angle (O-C) value 62- 66 A5 --- r_(O-C)A Reference to (O-C) residuals; in refs.dat file 68- 82 A15 --- Camera Camera used in the observation (G3) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Disc Discover designation of the pair of stars (1) 8- 9 A2 --- m_Disc Designation for pair components 11- 19 F9.4 yr Epoch [1911/2012] Epoch of the observation 20 A1 --- f_Epoch [*] Observation at NAOR (2) 22- 28 F7.3 arcsec Sep Angular separation (ρ) 30- 36 F7.3 deg PA Position angle (θ) 37- 41 F5.2 arcsec (O-C)1 ? Old angular separation (O-C) value 43- 46 F4.1 deg (O-C)2 ? Old position angle (O-C) value 48- 52 F5.2 arcsec (O-C)3 New angular separation (O-C) value 54- 57 F4.1 deg (O-C)4 New position angle (O-C) value -------------------------------------------------------------------------------- Note (1): STT 547AC, STT 547AD, STT 547AE, POP 217AP, or MLB 259. Note (2): Measurements obtained from observations with the 2m telescope at the Bulgarian National Astronomical Observatory (NAOR) at Rozhen from 2004 to 2010, and for which the separations were corrected after determining the telescope focal length more precisely. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Ref Reference identifier 7- 25 A19 --- BibCode Bibliographic code 27- 48 A22 --- Aut Author's name 50-148 A99 --- Com Comments -------------------------------------------------------------------------------- Global Notes: Note (G1): The separation and position angle are the average of data taken in both the B and V filters when we use the VersArray 1300B and Apogee Alta U42 CCD cameras. Note that the position angle has not been corrected for precession, and it is thus based on the equinox for the epoch of observation. Note (G2): Between components of pairs determined by using package IRAF. Note (G3): Apogee Alta, SBIG ST-10ME, VersArray 1300B. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Sylvain Guehenneux [CDS] 30-Jun-2014
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