... GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer , Hubble , and Chandra , ESA's Herschel and XMM-Newton , and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. ... The space-based observations are complemented by ground-based imaging and spectroscopy, including extensive commitments of ESO and NOAO observing time. ... 2010-04-10: Deep VLA 1.4 GHz data for GOODS-North . ...

... The evolution of magnetic fields in OB-type stars from the study of open clusters of different ages . ... Wade G. A. The MiMeS Project: Magnetism in Massive Stars . ... Polosukhina N., Shavrina T., Drake N., Kudryavtsev D. Smirnova M. New results of the spectral observations of CPstars in the Li I 6708? spectral region with BTA telescope of SAO RAS . ... Magnetic Stars-2010 . ... List of participants . List of reports . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

Общая Астрономическая Конференция . ... Правила форума . ... Сообщения за день . ... Добро пожаловать на Общая Астрономическая Конференция. ... Форумы общей направленности . Любые вопросы от новичков (просматривают: 17) . ... Общий форум любителей астрономии (просматривают: 7) . ... Новости магазина Starshop.ru . ... Менее астрономические товары (просматривают: 1) . ... Форум исключительно для сообщений об испытаниях астрономической техники. ... Общая Астрономическая Конференция статистика . ...

Next: Using Image Memories Up: Image Displays Previous: True Colour or . With the term XWindow display we refer to a bitmapped screen supporting the XWindow environment. ... For example, display screens of different sizes may be created and different number of image channels may be connected to any one display. ... You may create several image displays at the same time on your bitmapped screen even though only one display can be the current active display at any time. ... Using Image Memories . ...

... You are referred to Section 17.3 for extensive discussion of the many common keywords in the cg suite of software. cgspec allows you to display an image, and then overlay small plots of spectra at different locations on the image. ... In addition, you can bin the spectra up over some spatial region centred on the given locations. cgspec uses the value spectrum for the keyword type to indicate that spectra are to be extracted from that image listed in the keyword in . ... Unset for no spatial binning...

Next: Visualizing Data Cubes on the Grid . ... 314 Astronomical Data Analysis Software and Systems XIII, eds. F. Ochsenbein, M. Allen, & D. Egret (San Francisco: ASP), 505 . ... Until recently, a typical FITS file was composed of a single image less than 100Mb in size. ... And along with this explosion of new data file representations comes demands for more flexibility in visualization, support for external and remote analysis, and seamless Web integration. ...

Our group includes both theoreticians and observers working on problems related to many different aspects of star formation. You can learn more about us by following the links provided here below. We will try to keep these pages updated as frequently as possible, however do not hesitate to contact us directly if you encounter problems while browsing or do not find the specific information that you are looking for. Click on the following for more information . Our Group . ...

... 2013 April 13 . Sun with Solar Flare . Image Credit: NASA Solar Dynamics Observatory . Explanation: This week the Sun gave up its strongest solar flare so far in 2013, accompanied by a coronal mass ejection (CME) headed toward planet Earth. ... The flash, a moderate, M6.5 class flare erupting from active region AR 11719, is near the center of the solar disk. ... Loops and arcs of glowing plasma trace the active regions' magnetic field lines . ... About APOD | ...

... We have developed a suite of analysis tools and an on-line database for both the primary ChaMPlane X-ray data (source catalogs) as well as the optical counterpart data. ... The ChaMPlane VO provides access to our deep Mosaic optical (V,R,I,Halpha) images, catalogs of their optical photometry, Chandra images with exposure-map correction, X-ray source data and details of X-ray sources with identified optical counterparts. ... Chandra sources are displayed (right) in a smoothed Chandra X-ray . ...

... Astrophysics Group . ... Pulsars . ... Stars ? ... The array was designed to detect compact radio sources such as these by virtue of the fact that they would scintillate (twinkle) when observed from the Earth through the interplanetary medium ? ... One of Antony Hewish?s research students, Jocelyn Bell, was set the task of operating the telescope and inspecting the daily charts for the kind deflections in the trace which occurred when a scintillating source passed over the array. ...

... SAI CAS . ... Catalog Access Services . ... This site is about the Virtual Observatory project at the Sternberg Astronomical Institute, Moscow University ( SAI MSU ). We provide a public access to the growing set of astronomical services developed by the SAI RVO development team in accordance with the Virtual Observatory standards. ... We provide access (programmatic and interactive) to the all major and biggest astronomical catalogs (about 4 billions objects total) as well as other web-services. ...

. The XMM-Newton website has moved to the following location: . http://www.cosmos.esa.int/web/xmm-newton

In the current version .. ... Apogee Alta . Many SBIG cameras and filter wheels . ... FITS file format with exposure, camera, telescope, object and filter header information . Interactive image display and analysis with latest SAOimage ds9 . Interactive data processing in real time with AstroImageJ . ... XmCCD creates FITS image files with comprehensive header information and displays the images using ds9. ... Latest version 5.1 for Apogee and SBIG cameras updated June 17, 2015 . ...