... MOUSER Over View . The design of a new generation fast spectrograph MOUSER (Multi Object Universal Spectrograph for Extragalactic Research) to be installed at the 6 m telescope is proposed. ... photometric observations in broad and narrow spectral bands with a 6'x6' field of view and an image scale of 0".30/pixel; . ... The spectrograph is to be installed on the field rotator of the 6 m telescope prime focus without a standard field corrector. ... Back to Laboratory Home Page . ...

... user-defined data file formats . ... better integration with a user's analysis routines To add such functionality to SAOimage, we developed the XPA Messaging System that allows X programs to define points of public access through which data and commands can be exchanged with external programs. ... We have utilized XPA to develop "SAOimage: The Next Generation" (SAOtng), an extensible image display service that can cooperate with other processes and programs. ... SAOtng help pages . ...

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Next generation Fornax Cluster surveys . ... Data Handling and Products . ... Science Data Products Forum . ... An international team, with Dr. Hilker as Co-PI, has started to gather wide-field optical and infrared imaging data as well as spectroscopic data on the whole extent of the Fornax cluster, mainly based on observations with ESO telescopes (VLT, VST, VISTA). ...

... For SIMS (Secondary Ion Mass Spectrometry) analysis, a solid surface is bombarded by primary ions of some keV energy. ... The subsequent mass analysis of the emitted ions provides detailed information on the elemental and molecular composition of the surface. ... Extremely short ion pulses with a duration below . ... By rastering a fine-focussed ion beam over the surface, like an electron beam in an electron microprobe, mass resolved secondary ion images (chemical maps) can be obtained...

... Proposed location of the new generation Russian VLBI network radio telescopes Kaliningrad St. Petersburg Zelenchukskaya (Zc) Badary (Bd) Ussurijsk Working frequency bands for the new generation Russian VLBI network S X Ka 2.2 2.6 7.0 9.5 27 33 F, GHz Data acquisition parameters 4 frequency bands : 512 MHz bandwidth x 2 polarisations or 1024 MHz bandwidth x 1 polarisation 2-bit sampling ...

... The planet in orbit around 51 Peg has, according to theoretical models, moved into its current position from farther away and its atmosphere may therefore be strongly evaporating. The molecules released by the upper parts of the atmosphere must be rapidly ionized and could form an envelope around the planet. If the planet passes in front of the star, this envelope is in favorable geometric conditions (the inclination angle of the orbit is close to 90?) which allow it to occult the star. ...

Go to the previous , next section. ... Define the plot device you want to use with the device command. ... Declare the data file with the data command, see section How should I get data into SM? , or you could see section 'Data' in The SM Manual . ... If you want to plot points, you should first define the point style with the ptype command. ptype allows you to define the point as a type of polygon, with any number of sides, and 4 basic forms (see section 'Ptype' in The SM Manual ). ...

Photon Scattering: Basic Principle of Photon Scattering . Audio Narration is available . No Scattering: Photon Source and Detector . ... For optical photons, scattering goes as wavelength to the -4 power. In the case of blue photons compared to red photons, this means that blue photons are about 10 times more likely to get scattered than red photons. ... Watch the blue photons scatter away from the detector . ... Interstellar dust make stars appear redder than they really are . ...

Next: PSF1DRB Up: PIXTOPIXSENS Previous: Generation from Ground Calibration Contents . Ideally the in-orbit PixToPixSens file will be generated from internal calibration measurements using the fullframe high resolution engineering mode. However due to their large data volume the fullframe high resolution data won't be available frequently enough to base the in-flight generation of the PixToPixSens file on the high resolution data. ... i.e. the average counts per pixel per CCD-frame . ...

... title='Алкотестер Inspector AT100' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . Цвет: белый . Коллекция: Осень-зима 2015/2016 . ... Размер FR: 59 . ... Лонгслив Z Generation. ... Сезон: Осень-зима 2015/2016. ... Модель полностью изготовлена из EVA (вспененного полимера), надежного и легкого материала. ... Коллекция: Весна-лето 2016 . ... Материал подошвы: искусственный материал . ... Размеры: длина 37 см высота 25 см ширина 16 см Цвет: коричневый . ...

... Cosmological Applications of the Cornell HI Archive . ... We find marginal evidence to suggest that the HIMF has a shallower slope in higher density regions than lower density regions. We have also combined the HI archive with a separate compilation of optical photometry and spectroscopy to generate a catalog of Tully-Fisher distances and peculiar velocities, the SFI++. Using this catalog, we have examined the peculiar velocity field in and around the Pisces-Perseus Supercluster (PPS). ...

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

... 08.04.2016 12 апреля состоится гала-концерт Студенческой весны СГАУ . ... 08.04.2016 Аспирант Самарского университета Артем Богатырев принял участие в торжественной конференции . ... Информация Новости В Самарской области завершился трек Aerospace акселератора GenerationS . ... Оператором трека стал Региональный центр инноваций (СГАУ). 11 проектов, отобранные из 330 заявок в результате многоступенчатой экспертизы, продемонстрировали итоги своей трехмесячной работы в акселераторе. ... О GenerationS ....

Next: Time Series Analysis Up: No Title Previous: Command Syntax Summary . This manual is intended as a guide to the use of the digital stellar photometry reduction program DAOPHOT II: The Next Generation. ... In DAOPHOT II: The Next Generation all of the major algorithms and actual FORTRAN coding are done by Stetson, with the exception of those Figaro, IRAF, or MIDAS routines which are used for the image input and output. Stetson is solely responsible for bugs and algorithm-related problems. ...

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . Available Languages: en | ... httxt2dbm is used to generate dbm files from text input, for use in RewriteMap with the dbm map type. ... f DBM_TYPE . ... Available types are: GDBM for GDBM files, SDBM for SDBM files, DB for berkeley DB files, NDBM for NDBM files, default for the default DBM type. -i SOURCE_TXT . ... Name of the output dbm files. httxt2dbm -i rewritemap.txt -o rewritemap.dbm . ...

... 2008 August 29 . Generations of Stars in W5 . ... JPL-Caltech , NASA . Explanation: Giant star forming region W5 is over 200 light-years across and about 6,500 light-years away in the constellation Cassiopeia . ... New evidence indicates that successive generations of stars formed in the W5 region in an expanding pattern of triggered star formation . The older, earlier generations of stars seem to cluster near the middle of the enormous cavities, with younger stars seen near the rims. ...

... Generations of Stars in W5 . ... JPL-Caltech , NASA Explanation: Giant star forming region W5 is over 200 light-years across and about 6,500 light-years away in the constellation Cassiopeia . ... New evidence indicates that successive generations of stars formed in the W5 region in an expanding pattern of triggered star formation . ... NASA Official: Jay Norris. ... Publications with keywords: star formation - infrared . Publications with words: star formation - infrared . ... Central IC 1805 . ...

... We are developing the following problems: a) combine optical and microwave technic to the indication of non-linear surface waves and wave breaking field; b) modelling of microwave propagation in a multiphase air-water interface; c) obtain quantitative dependencies of microwave radiation on geometry and statistics of wave breaking field in ocean surface; d) monitoring of ocean surface states using optical amd microwave airspace data sets. ... Important issue is spray and underwater bubbles. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... This will include: efficient polarized and unpolarized spectrum synthesis; critical compilations of atomic data; determination of fundamental physical parameters; quantitative spectroscopy for abundance determination; magnetic field detection and modelling. ... Evelyne Alecian (Royal Military College of Canada) . ... Abundance analysis in magnetic and non magnetic stars (part I) . ... COFFEE BREAK . ... Herbig Ae/Be stars ....

MFS . Data archive MFS . ... Data archive HSFA . ... Catalogue of solar flares . Atlas MFS . Data archive MFS [FTS, AVI] . Data MFS-2009 . Data MFS-2010 . Data MFS-2011 . Data MFS-2012 . Flares archiv with asymmetry absorption . ... Catalogue of prominence 2011 . Catalogue of prominence 2012 . ... Data MFS-2013 . Data MFS-2014 . Data MFS-2015 . ...