... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

This page is devoted to information on Supernova 1999eb in NGC 664 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main supernova page. Information on the original web pages for many of these images can be found on the Supernova links web page. ... Normally, I wait until I get about 6 or so images before starting a web page for a specific SN, with 3 images and a spectrum the first day, I decided to get started while I had time. ...

... In this case you have to write in your answer (in English or Russian): «impossible situation ­ ». ... The name of the moon in the solution and in the drawings should be written (or duplicated) in English. ... The answers "which moon" and "in what case" (configurations at the moment of Jupiter disappearance) have to be given in the form of drawings, and calculations should be the base for the answers. The names of the moons in the solution and in the drawings should be written in English. ...

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

Space VLBI Mission RadioAstron Announcement of Opportunity -- 1 for the period July 2013 ­ 30 June 2014 Key Science Program ( KSP ) Final Notes Proposals Due: 8 February 2013, 23:59 UT 1 RadioAstron KSP meeting follow-up Based on the fruitful discussions, questions and suggestions from the RadioAstron Key Science program meeting in Bonn (December 3-4, 2012), we would like to emphasize the following specific aspects for the preparation of the AO-1 ...

... Aims: Today, large ground-based instruments, like VISIR on the VLT, providing diffraction-limited (about 0.3 arcsec) images in the mid-infrared where strong PAH features appear enable us to see the flaring structure of the disks around Herbig Ae stars. Although great progress has been made in modelling the disk with radiative transfer models able to reproduce the spectral energy distribution (SED) of Herbig Ae stars, the constraints brought by images have not been yet fully exploited. ...

... We address a question if globular clusters (GC) in a protogalaxy could for some time evolve chemically as isolated systems, enriching themselves with heavy elements produced in first supernova events that follow initial star formation. We determine both the critical mass of a protoglobular cluster that is needed to retain the ejecta of the very first supernova, and the critical energy (i.e., number of supernovae) that is needed to expel the residual gas from a cluster of a given mass. ...

Stellarium 0.12.3 . ... CodingљStyle . ... FileљStructure . Coding Style Conventions in Stellarium . ... File Names . ... C/C++ Code . ... Source code should use the ASCII character set. ... The only exception is names of slots that use Qt's automatic connections to controls in .ui files. ... You can use the astyle program to format your code according to these conventions. ... There are different ways to comment C++ code with Doxygen, in Stellarium use the following for headers files: //! ...

Обзоры hep-ex: тематический рубрикатор . ... hep-ex/0306011 . Рождение векторных мезонов и инклюзивного канала K s K s на HERA . ... Authors: M. Barbi (McGill University), for the H1 Collaboration, ZEUS Collaboration . Comment: 6 pages, 6 figures, to appear in the proceedings of the International Conference on the Structure and Interactions of the Photon, Frascati (Italy), 7-11 April 2003 . ... Comments: 9 pages 5 figures submitted to PRL . ... Comments: 13 pages, 1 table and 4 figures . ...

I. Installation . ... AMPLE package distributive (created with program InstallShield for Microsoft Visual C++) has been downloaded on FTP server of IAA RAS as archive Ample.zip. ... Note: If the window "file download" appears, select Open... switch button, then press OK button. ... The shortcut for AMPLE will be linked with this folder, and auxiliary files will be created here during AMPLE work. ... When running AMPLE all auxiliary and new configuration files are created in the WORK folder. ...

The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

. О лаборатории . Welcome to WordPress. This is your first post. Edit or delete it, then start blogging! . This entry was posted on Saturday, June 12th, 2010 at 12:17 am and is filed under Uncategorized . You can follow any responses to this entry through the RSS 2.0 feed. You can leave a response , or trackback from your own site. Click here to cancel reply. You must be logged in to post a comment. Лаборатория лазерной интерферометрии is proudly powered by WordPress . Entries (RSS) and Comments (RSS) .

... Тhis new concept touches our simple lives, yet for those intrigued by the natural sciences, especially experts deeply engaged in the 'eternal' questions of general geology and astronomy, it is all the more fascinating. The problems to be faced by any theory for the formation of the Solar System . Any theory has to account for certain rather tricky facts about the Solar System. These are in addition to the obvious facts that the Sun is at the centre with the planets in orbit around it. ...

... MASTER Net is 56 square degrees per 1 exposition . ... 06 Dec 2015: GRB 151205B: MASTER-NET early optical observations GCN18665 . ... 18 Nov 2015: GRB 151118A: MASTER-NET optical observations GCN18613 . ... 12 Nov 2015: GRB 151112A: MASTER-NET optical limit GCN18591 . ... 07 Nov 2015: GRB 151107A: MASTER-NET optical observations GCN18565 . ... 31 Oct 2015: Five OTs detected by Global Robotic MASTER Net ATel8232 . ... 02 Oct 2015: GRB 151001B: MASTER-NET early optical observations GCN18380 . ...

. Comment on J0405+3803 . Our image contains a feature of 25 mJy at 14 mas E-NE from the brightest component. It is not visible in the Caltech-Jodrell (CJ) survey image at 5 GHz (Xu et al. 1995) obtained about 6 years earlier. The 1.6 GHz CJ image (Polatidis et al. 1995) does show an extended feature close to the position in question, but somewhat displaced toward west. VLBApls home page . Last modified: 16 Oct 2000

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...

The light beams of the Moon’s craters. The centres of the Moon’s beams are the crater Copernic, Kepler, Aristarch. But the most powerful light system has Tikho the crater. ... What substance forms the rays of the Moon craters? ... In 1960 two soviet scientists Kirill Petrovich Stanukovich and Vitally Aleksandrovich Broshtein supposed the following explanation of these beams. The meteorite shock at the Moon’s surface is accomplished by the burst: the kinetic energy is used for gushing out. ...

. Home . Structure of Data . Description . Catalog . Publications . VO . ЮБ 2000 . 11:14:20.2 . ЮД 2000 . -57:33:04 . l . 290.172 . b . 2.895 . diameter . 14.0' . (m - M) 0 . 11.4 0.05 . distance . 1900 50 pc . E(B - V) . 0.08 0.01 . log(t) . 9.65 0.05 . (J, J-H) isochrone VOTable . 2MASS data VOTable . Developed by the Team . Send us your questions or feedback

... A Proposal for an International Atlas of Lunar Exploration Philip J. Stooke Department of Geography University of Western Ontario London, Ontario, Canada N6A 5C2 Introduction. ... I propose the creation of an International Atlas of Lunar Exploration to tell this story in cartographic form. ... Many new products would be based primarily on spacecraft images rather than drawn maps, which will also reduce costs and help illustrate the primary data products of the principal lunar missions. ...

... Phil Creed's Astronomy Bowl! ... Hidden Hollow's Astronomy Bowl is a fast-paced question-and-answer game designed to both enlighten and challenge stargazers. ... Astronomy Bowl follows the traditional format of alternating toss-up and bonus questions, with a few tweaks. ... The host will read a toss-up question. ... Once a toss-up is correctly answered, that team is given a bonus question. ... If only 14 toss-ups are answered correctly, that means 20 toss-ups and 14 bonus questions will be read. ...