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1. Journal "Peremennye Zvezdy"
Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Our BVR CCD photometric study of the globular cluster NGC 7006 permitted us to find two new suspected RR Lyrae variables. A cluster chart is presented with the position of known and suspected variables marked. ... According to the Catalogue of Variable Stars in Globular Clusters (Clement et al., 2001), it contains 76 variables, most of which are RR Lyrae variables, the RR1 to RR0 ratio being 8:55. ... for suspected and some of known variable stars. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1211025 -- 19.8 Кб -- 20.04.2006
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2. Radio patrol survey by Gregory and Taylor
... 371Gregory Taylor . ... We persent a catalog of 1274 discrete sources detected during a 5 yr, 6 cm, radio-patrol survey of the galactic plane for variavle sources. ... Seventy-five percent of the sources are weaker than 75 mJy, and as a consequence reliable sources and 27 possible variables were detected, of which 64 % exhibited shirt-term variability. ... A comparison with previous centimeter variability studies suggests the possible existence of two distinnct variability components. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/GT_patrol.html -- 7.9 Кб -- 18.03.2015
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3. Detection of Radio Transients and Variable Radio Sources Using the Archive Data
... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
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4. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Many of the fields are spatially . ... These include a pulsating white dwarf which appears to have a hot companion, a number of stars with A-type spectra that vary on a period in the range 20 35 min. Our primary goal is the discovery of new AM CVn systems: we find 66 sources which appear to show periodic modulation on a time-scales less than 40 min and a colour consistent with the known AM CVn systems. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2011/572.html -- 6.4 Кб -- 14.01.2011
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5. GENERAL CATALOGUE OF VARIABLE STARS
... We have compared visualized fields of GSC and USNO A1.0 catalog with unpublished photographic finding charts that were sent by L. Plaut to the compilers of the GCVS. ... 7-15 A9 --- GCVS GCVS or NSV name 17-25 F9.4 --- GSC GSC number 26 A1 --- NoteFlag *Nonstar (GSC) flag 28-29 I2 h RA2000GSC.h Hours RA (GSC), equinox 2000.0 31-32 I2 min RA2000GSC.m Minutes RA (GSC), equinox 2000.0 34-38 F5.2 s RA2000GSC.s Seconds RA (GSC), equinox 2000.0 40 A1 --- DE2000GSC.- ... Plaut, L., 1966, Bull. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/gcvs/gcvs/plaut/ -- 8.0 Кб -- 25.07.2002
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6. lsst.tcc: tcc.axis.ptCorrFromObs Namespace Reference
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... ptCorrFromObs . ... tcc.axis.ptCorrFromObs Namespace Reference . ... Compute pointing correction position from observed coordinates. ... position of target in observed coordinates (a coordConv.PVTCoord) . ... targPtCorrXY: position of target in pointing correction coordinates (a tcc.base.ArrayPVT2) (deg) i.e. a position in rotator coordinates where X is the direction of increasing azimuth . ... list tcc.axis.ptCorrFromObs.__all__ = ["ptCorrFromObs"] . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/html/namespacetcc_1_1axis_1_1pt_corr_from_obs.html -- 11.4 Кб -- 14.09.2015
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