... Searching for Far Out and Wandering Worlds . ... The Real Reality Show: Would aliens be anything like us? ... The SETI Institute is after alien signals. Assuming another world is beaming a 1-million-watt radio signal in our direction, how far away can that source be before the signal is lost in intergalactic noise? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...

Instrument Science Report WFC3 2008-11 WFC3 ETC Update Thomas M. Brown May 29, 2008 ABSTRACT The WFC3 ETCs have been updated to reflect our preliminary findings from the most recent campaign of thermal vacuum testing. ... We have changed the IR channel full well from 75,000 e-/pix to 70,000 e-/ pix; this is the point where the count rate of a bright source becomes nonlinear at the ~1% level. ... We have changed the UVIS channel full well from 75,000 e-/pix to 70,000 e-/pix. ...

... Briefly, the count rate at the detector from a source at a redshift z is . ... Another possible way that could lead to arising diverse peculiarities in the - distribution induced by the sources evolution is connected with a possible non-monotonic character of the star formation rate in galaxies. ... The most prominent feature of the obtained theoretical - is a notable sharp increase at low count rates due to evolutionary effects. ...

... Вия сунула мне рамку. ... Говорят, что не отлынивают от задач, связанных с охраной Земли. ... Кроме того, потеря возникшей на Земле цивилизации практически невосполнима, хотя подобные цивилизации имеются на других "землях". ... Первые простейшие микробы занесены на Землю 14 миллиардов лет назад, кольцевые ДНК - 10,4 миллиарда лет назад, тогда уже, параллельно, пошла развиваться наподобие вирусов, привнесенных извне, другая жизнь. ... Все ли растения и животные на Земле земного происхождения? ...

... Реклама: Фотобанк Mymicrostock http://www.mymicrostock.com/ . ... Войти на сайт: Имя: . ... Автор забыл указать имя ] . ... В интернете открылась самая полная база фото- и видеоматериалов, созданных при участии NASA. Проект был создан совместно NASA и некоммерческой цифровой библиотекой Internet Archive. В новую базу попали материалы из 21 главной коллекции NASA. ... 2008-12-15 17:33:00 NASA завершило миссию марсианского орбитального зонда . ... Имя: . ...

. Main . Turbina . Rs485 driver . Microcodes . Documentations . CVS . Feedback . ASM Kislovodsk . Name . Latest release date . Download link . MASS counters microcode . Sat, 19 Jun 2004 18:13:35 MSD . bicounter.tgz [13738] . MASS auxiliary module microcode . Sat, 19 Jun 2004 18:13:47 MSD . massdimm.tgz [11851] . MASS scanning mechanism . Sat, 19 Jun 2004 18:13:56 MSD . motor_eso.tgz [12629] . Copyright 2004-2012.

Next: Hierarchical Wiener filtering Up: Noise reduction from Previous: The convolution from . Let us consider a measured wavelet coefficient at the scale i . We assume that its value, at a given scale and a given position, results from a noisy process, with a Gaussian distribution with a mathematical expectation , and a standard deviation : . ... We get: . ... This is done from the study of the variation of the noise between two scales, with an hypothesis of a white gaussian noise; . ...

. XMM-Newton Science Analysis System . eregionanalyse (especget-1.27.7) [???] . Meta Index / Home Page / Description / Output The fraction of counts contained within the source region assuming a point source located at the centre of the region. The EXTENDED mode (King profile) PSF is used to calculate the fraction assuming a fixed photon energy of 1.5 keV. This is currently only implemented for circular source regions, other shapes will give the wrong factor. XMM-Newton SOC/SSC -- 2008-10-24

; CLEAR INTERRUPT FOR NETWORK COMUNICATION ; TITLE netcli.asm NAME netcli .286p .287 NETCLI_TEXT SEGMENT WORD PUBLIC 'CODE' NETCLI_TEXT ENDS _DATA SEGMENT WORD PUBLIC 'DATA' _DATA ENDS CONST SEGMENT WORD PUBLIC 'CONST' CONST ENDS _BSS SEGMENT WORD PUBLIC 'BSS' _BSS ENDS DGROUP GROUP CONST, _BSS, _DATA ASSUME CS:NETCLI_TEXT, DS: DGROUP, SS: DGROUP netcli_TEXT SEGMENT ASSUME CS:netcli_TEXT PUBLIC _netcli _netcli PROC FAR cli ; ; ret ; _netcli ENDP NETCLI_TEXT ENDS END

Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... Science Fiction . ... The New Horizons science team€а is inviting everyone worldwide to vote for the names that will be given to the most prominent features on Pluto and Charon, Pluto?s largest moon. The pre-listed names are€а an eclectic mix from mythology and the literature and history of exploration. You can even nominate names to be added to the list. ... Yuggoth (H. P. LovecraftтАЩs name for Pluto) . ... Name * . ...

... Путеводитель астронома по Inter Net. (9 лучших линков в интернете на каждую астрономическую тему) . ... Астрономические данные в Интернете. ... Официальные астрономические учреждения России. ... Лучшие астрономические персональные страницы - AstroTop. ... Приведу некоторые www-страницы астрономических учреждений России, которые могут послужить хорошей отправной точкой в поиске нужной Вам информации по астрономии. ... Недаром на данный ресурс есть ссылки со многих астрономических страниц России. ...

... Column (1): Source name from NED. ... Column (8): Log star formation rate, from SDSS. {\it Detected sources:} (1) (2) (3) (4) (5) (6) (7) IC0159 0.58±0.10 8.31 ± 0.07 8.25 ± 0.07 9.55 9.70 8.89 -0.06 UGC2004 5.98±0.65 9.32 ± 0.04 9.03 ± 0.04 9.83 9.61 9.15 0.36 NGC1234 0.24±0.06 7.92 ± 0.09 7.80 ± 0.09 9.67 9.58 8.98 -0.68 2MASJ0839+03 2.30±0.54 8.91 ± 0.09 8.69 ± 0.09 --- 9.94 9.08 0.58 2MASJ0846+02 2.75±0.47 8.98 ± 0.07 8.85 ± 0.07 --- 9.84 8.99 ...

... Read in a hires optical spectrum and mask out lines to be ignored ! ... a) just calculate a spectrum with fixed abundances ! ... c) Solve for all light elements abundances { 1 8.53 0.0 2 11.54 0.0 5 0.10 0.0 6 8.00 1.0 7 7.81 1.0 8 7.10 1.0 12 7.01 1.0 13 5.73 1.0 14 6.94 1.0 15 5.50 1.0 16 6.75 1.0 18 6.10 1.0 20 5.10 1.0 21 1.70 0.0 22 3.84 0.0 23 2.82 0.0 24 4.06 0.0 25 3.71 0.0 26 6.18 0.0 27 4.26 0.0 28 5.05 0.0 29 3.20 0.0 30 4.34 0.0 39 1.42 0.0 40 2.40 0.0 -1 0 0 } synth save end ...

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

Neutron Monitors ] [ Solar Neutrons ] [ Muon Telescopes ] [ Base Potchefstroom University ] [ Magnetometers ] [ GPS systems ] [ Ionosphere ] [ Related Data ] [ Space Weather ] . ... All Cosmic Ray Stations + InterPlanetary Data: WorldNet . Alma-AtaB (Mt.Tien Shan) DataBase of Kazakhstan Spectrograph Alma-AtaB (Mt.Tien Shan) new . ... Nagoya Muon Telescope and DATA or mail . ... Belgrade Muon Telescopes and DATA or ">mail . ... Real-Time database for Cosmic Ray Anisotropy (DB10) . ...

... In 1959 the Government Decree enacted OKB-1 to initiate work on the development of ballistic rockets using solid propellant RT-1 with a warhead flight range of 2 500 km, a launch mass of up to 35 t, and a combat charge mass of 500 kg. In parallel, the tasks were pursued to implement work on RT-2 assuming the development of a ballistic rocket with a warhead flight range from 10 000 to 12 000 km and a combat charge mass of up to 500 kg. ... Official WEB-site of S.P.Korolev RSC Energia . ...

... Find here a description of how to setup a new operational dfos installation. ... Therefore, we focus on the aspect of how to adapt the .dfosrc file and assume that anything else is then simply copied from the old ("reference") site to the new installation. ... dfos . ... click on 'download dfosExplorer' ; click on 'Save link target as' ; download dfosLog.tar into your $DFO_INSTALL_DIR; untar it (tar -xvf dfosExplorer.tar). click on 'description: dfosExplorer' and read the documentation . ...

... The first task assumes the searching for chemical composition and sizes of particles which give the wavelength dependence of the extinction efficiencies close to the observed dependence of . Figure 7: Wavelength dependence of the extinction efficiency factors for homogeneous spherical particles of different sizes consisting of astronomical silicate and amorphous carbon. The dashed segment shows the approximate wavelength dependence of the mean galactic extinction curve at optical wavelengths. ...

... Бережной А.А., Клумов Б.А., Фортов В.Е., Шевченко В.В. Письма в ЖЭТФ, Т. 63, N6, С. 387-391, 1996 . ... A. A. Berezhnoy1,2, N. Hasebe1, M. Kobayashi1, G. Michael3 and N. Yamashita1 1Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan 2Sternberg Astronomical Institute, Moscow, Russia 3German Aerospace Center, Institute for planetary research, Berlin, Germany . Brown University - Vernadsky Institute Microsymposium 40, 2004, Moscow, Russia . ...

... Geoffrey Bicknell . Following are my lecture notes more or less in the order that I give them, together with exercises and relevant papers and images. ... Lectures and tutorial Monday 09:30 Lecture - Duffield Lecture Theatre . Tuesday 11:00 Lecture - Duffield Lecture Theatre . Wednesday 09:30 Lecture - Duffield Lecture Theatre . ... Lecture notes: . Overview of High Energy Astrophysics . ... Questions 1-4; due 27 Feb . Questions 5-8; due 6 March . ... Figure 1 for above paper . ...