Catalogue of eclipsing variables (CEV) is the world's principal database of eclipsing binary systems with available classification. CEV contains identifications, classifications, photometry, periods, eclipses data, spectral types, references and notes for 7179 systems. Format of the current CEV . CEV main table (~1.0MB) . ... List of systems, erroneously classified as eclipsing binaries in GCVS (they are not included in the CEV main table) Download all files as a single archive (~0.6MB) . ...

. Sternberg Astronomical Institute, Moscow, Russia . GENERAL CATALOGUE OF VARIABLE STARS: References . File Summary: . GCVS References . NSV References . NSV Supplement References . The list of the abbreviations in the References .

... PmWiki . Summary: PmWiki group header. ... Page Variables | ... Defining page text variables . ... Page text variables are string variables created in the wiki text of a page, and can be automatically made available for inclusion in other pages. ... use a definition list - the normal pmwiki markup for a definition list will create a page text variable . ... This creates a new variable that can be accessed by {$:Name} (becomes: "{$:Name}") in the page. use a simple colon delimiter in normal text . ...

... Files . ... tcc.msg.formatObjFields Namespace Reference . ... Definition at line 36 of file formatObjFields.py . ... Definition at line 107 of file formatObjFields.py . ... Definition at line 115 of file formatObjFields.py . ... Definition at line 129 of file formatObjFields.py . ... Definition at line 122 of file formatObjFields.py . ... Definition at line 213 of file formatObjFields.py . ... Definition at line 139 of file formatObjFields.py . ... Definition at line 247 of file formatObjFields.py ....

OptInt PmWiki : Pm Wiki / Page specific variables . ... Page variables have the form {$ variable } , and can be used in page markup or in certain formatting strings in PmWiki. ... Prefixing the variable name with an asterisk (*) means the variable reflects the value related to the target page or main page. ... Namespaced} - spaced page name, as in "Page Variables" . ... Defines new Page Variable of name $CurrentSkin, which can be used in the page with {$CurrentSkin} (also for Conditional markup ). ...

THE 75th NAME-LIST OF VARIABLE STARS. ... The 75th Name-List consists of two tables. ... the literature, taken from positional catalogues, including USNO A1.0/A2.0 and GSC, or determined by the authors); the range of variability (sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol ( means that the star , in minimum light, becomes fainter, than the magnitude indicated); and the system of magnitudes used ( P are photographic ...

... See also MRC 1Jy sample I. and MRC 1Jy sample II. 20deg but excluding the R.A. range 14h03m--20h20m. Quasar classifications are based on high-resolution radio images, deep optical identifications, and follow-up spectroscopy of sources in the strip. The relatively low radio frequency of the finding survey and the complete optical identification of quasars to faint magnitudes ensure that the MQS is relatively free from orientation biases that affect most other samples of radio-loud quasars. ...

Peremennye Zvezdy ( Variable Stars ) 32 , No. ... We report on our photometric analysis of the poorly studied cataclysmic variable in Ophiuchus, 1RXS J174320.1-042953 (DDE 11). ... The long-term behavior of J1743-0429 shows that it is a probable magnetic cataclysmic variable (polar), with a large difference between its low and high states. The orbital period obtained from our observations is 0 0866, or 2 08, close to the lower boundary of the period gap of cataclysmic variables. ... Fig. ...

XMM-Newton Science Analysis System . ... Meta Index / Home Page . Environments . SAS_CLOBBER . Clobber | ... Environment Variable . SAS_COLUMN_WISE . ... SAS_FORMAT . ... Reference . ... clobber . ... XMM-Newton SOC/SSC -- 2003-01-10 ...

... Barbon, R.; Buondi, V.; Cappellaro, E.; Turatto, M.: 1999, Astron. Astrophys. Suppl. Ser. ... Barbon, R., Cappellaro, E., Ciatti, F., Turatto, M., Kowal, C.T.: 1984, Astron. ... Barbon, R., Cappellaro, E., Turatto, M.: 1989, Astron. ... 1986, Astrophys. and Space Sci. ... Cappellaro, E., et al.: 1997-2002, Asiago Supernova catalogue, electronic version. ... The STScI Digitized Sky Survey. http://archive.stsci.edu/cgi-bin/dss_form . ... 1993, Astron. ... SAI SN group | ...

... Using sl_array . Array information . ... Inline::SLang . Doug's Home Page . ... Since the support for arrays in S-Lang and Perl do not match, the conversion of array values between the two languages is not entirely seemless, as shown in the examples below. ... The third option is to use a Perl Array_Type object to store the data; the Array_Type class is part of Inline::SLang and is as inefficient as using an array reference but does retain knowledge about the array size and type. ...

... Home All Namespaces All Classes Functions Coding Style Scripting Plugins File Structure . ... Manage textures loading. ... createTexture (const QString &filename, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams ()) . Load an image from a file and create a new texture from it. ... createTextureThread (const QString &url, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams (), const QString &fileExtension=QString(), bool lazyLoading=true) . ...

. Next: Widget routines Up: CHAMELEON Previous: dat_ Contents . Subsections . Widget routines . F ILE . A CCESS B ROWSE . A CCESS I NTERFEROMETRY . A CCESS P OINT D ATA . A CCESS W RITE . R EDUCE . R EDUCE P OINT D ATA P LOT . C ALIBRATE . C ATALOG . WAVE . Organization of data . Array configuration . Optical path lengths . Basic definitions and sign conventions . Command line procedures . Plotting . Adding plot variables . Adding plot classes . Christian Hummel 2015-04-28

... Welcome to the Boneyard. ... AA17666-11 sites several supernova mistakes from this period. 1998di (= KL Dra), IAUC 6982 discovered 1998/08/02 by Mike Schwartz . Found in MCG +10-27-12 NED01 at R.A. = 19h24m38s.19, Decl. ... Located 0".6 east and 3".8 north of the nucleus of MCG +10-27-12 NED01 ( Discovery image ( local mirror )) ( VSnet 98di web page ) . Mag 16.8, Type CV NOTE: This has now been confirmed to be not a supernova, but a cataclysmic variable (dwarf nova) of the CR Boo class. ...

... Figure c1.1 plots the spatial distribution and colour-magnitude diagrams for the 650 sources with J . ... We have cross-referenced the sample against the SIMBAD, using a search radius of 2.0 arcminutes centred on the 2MASS position. ... Figure c1.4: Stellar ultracool sources - optical/near-infrared distributions. 138 lie within 2-3 arcseconds of stars in one of either the Henry Draper, Bonner Durchmusterung, Cape Durchmusterung, Cape Photographic Durchmusterung, Guide Star Catalogue, or PPM...

... PUL VLBI Analysis Center . ... Pulkovo EOP and Reference Systems Analysis Center (PERSAC) is located at the Pulkovo Observatory . ... Processing of VLBI , GPS, and optical observations aimed at analysis of the Earth rotation, station displacement, and celestial reference system. ... Celestial Pole Offset (CPO) and Free Core Nutation (FCN) . Four daily updated CPO and FCN series (models) are provided. ... File fcn1.dat contains the ZM1 FCN model with variable amplitude and phase. ...

Next: Status of the BIMA Image Pipeline . ... We describe all the steps of the standard reduction including per pixel error propagation: Bias correction, treatment of bad pixels, flatfielding, and filtering of cosmic ray events. ... We build difference images via image convolution with a technique called OIS (optimal image subtraction, Alard & Lupton 1998), proceed with PSF-fitting, relative photometry on all pixels and finally apply an automatic detection of variable sources. ...

... The main periodicity in the Sun 's activity is the 11-year cycle called the solar cycle. ... During the cycle, changes occur in the Sun's internal magnetic field and in the surface disturbance level. ... At the beginning of a cycle the solar magnetic field resembles a dipole which axis is aligned with Sun's rotation axis. ... The sunspot number - and Sun's activity - is at maximum in the middle of a cycle, when the Sun's internal magnetic field is most chaotic. ... Space Physics Text Book of Oulu ...

1) Find the variable star and the comparison stars marked in the map. 2) Seeing the the variable star, try to imagine its location in the brightness interval between the reference stars. 3) Looking at the specially prepared scale, try to reproduce the location of variable in the brightness scale from memory. ... The grades of arbitrary scale are marked relative to brightness intervals between the reference stars. ...

... Available at http://www.hike.te.chiba-u.ac.jp/ikeda/CIE/publ/abst/15-2-86.html . ... Available at http://www.w3.org/TR/REC-CSS1-961217.html. ... HTML 4.0 Specification", D. Raggett, A. Le Hors, I. Jacobs, 8 July 1997. ... Available at ftp://ftp.internic.net/rfc/rfc1700.txt. ... Available at ftp://ds.internic.net/rfc/rfc1808.txt . ... Available at ftp://ds.internic.net/rfc/rfc2070.txt . ... Available at ftp://ds.internic.net/rfc/rfc2119.txt . ... Available at ftp://ds.internic.net/rfc/rfc2318.txt . ...