... Actually, the limits for cells surviving are not known yet. ... · Possibility of hardware operation at Europa surface environment · Duration of the experiment must fit to spacecraft life time ATR spectroscopy · Fits to all above-listed requirements · Does not request any complicated sample preparation · Detects directly proteins, DNA /RNA, carbohydrates, lipids and other metabolites · Does not destroy or damage cell , investigates object as is · Can detect ...

... В четверг, 14 апреля 2016 г., состоится семинар кафедры астрофизики. Повестка дня . ... Начало в 11 час.15 мин. Ауд. ... В четверг, 31 марта 2016 г., состоится семинар кафедры астрофизики . ... В четверг, 24 марта 2016 г. , состоится семинар кафедры. ... В четверг, 17 марта 2016 г. , состоится заседание кафедры. ... ОСП НИИ ПММ Национального исследовательского Томского государственного университета) . ... Copyright 2016 Астрономия в Санкт-Петербургском университете . ...

Educational program of the project is intended for training of specialists in different fields of space physics, astronomy and the Earth sciences. ... Special space-physics lab exercises are intended for the students of the senior courses of the Institutions, specialized in the field of space engineering and space physics. Its main task is to teach them some methods of satellites scientific and engineering data processing. ...

... The Astronomical Data Analysis Software and Systems (ADASS) conference is held each year at a different hosting astronomical institution. The conference provides a forum for scientists and programmers concerned with algorithms, software and software systems employed in the acquisition, reduction, analysis, and dissemination of astronomical data. ... The 26th annual ADASS conference will be held from October 16th to 20th, 2016 at the Stazione Marittima Conference Centre , Trieste, Italy. ...

... 20 th -23 rd April 2015 . ... In 2015 the 8th busy week takes place in Firenze, in Galileo GalileiтАЩs villa тАЬil GioielloтАЭ, located in the gorgeous hills in the southern side of the city. ... is pleased to host the 8th CALIFA Busy Week . in Firenze, at Galileo GalileiтАЩs Villa тАЬil GioielloтАЭ . After the second public data release on the 1st October 2014 ( DR2 , Garc†нa-Benito et al. 2014 ) and with more than 500 galaxies observed to-date, CALIFA has entered its maturity. ...

... We present data for the additional lines after processing and baseline fitting H91, H92 within this HII region. Integrated line profiles for H90 (top left), H91 (top right) and H92 (bottom left) are all 16MHz bands with a resolution of 512. ... The radio recombination lines of hydrogen H90, H91, H92, helium He91 and carbon C91 were detected from OrionA, and H90, H91, H92 from M17 and NGC3603 at 8GHz. ... The recombination lines from left to right are H90 and H91. ...

Storing and accessing the largest astronomical catalogues with the SAI CAS project S. Koposov1,2,3, O. Bartunov2, S. Karpov4 et al2. ... Why we want to build our own Catalogue Access Service The requirements for our CAS system The importance of the Database for the CAS (PostgreSQL & Q3C) The technical realization of CAS What has been already done Example of work TODO Storing and Accessing Astronomical Catalogues Existing projects CDS OpenSkyQuery CASjobs with SDSS They are all really great! ...

High-resolution near-infrared speckle interferometry and radiative transfer modeling of the OH/IR star OH 104.9+2.4 D. Riechers1 , T. Drieb e2 , Y. Y. Balega3 , K.-H. Hofmann2 , A. B. Men'shchikov4 , and G. Weigelt2 1 2 3 4 Max Planck Institute for Astronomy, Heidelberg Max Planck Institute for Radioastronomy, Bonn Special Astrophys. ... The reconstructed visibility reveals a spherically symmetric, circumstellar dust shell (CDS) surrounding the central star. ...

SAI VO . ... SAI CAS . ... Access . ... We present the results of the development of Sternberg Astronomical Institute Catalog Access Services (SAI CAS) project - the first and the only project in Russia, which provides online access to the major astronomical catalogues and different services on top of them. ... SAI CAS is an open-source implementation of the general Catalogue access service (influenced by SDSS CAS CASjobs project), based on original algorithms and open-source software. ... SAI MSU | ...

... Although each chapter has its own set of links, this page offers the complete collection, with additional sites for those interested in general astronomy, amateur astronomy, professional astronomical institutions, and astronomy news. General Astronomy Links . Sky Telescope 's vast collection of astronomy sites . ... Space Telescope Science Institute . ... A page dedicated to sundial links across the Web . ... A page dedicated to sundial links . ... Overview of the moon . About the moon . ...

Estimations of dome seeng by results of optics quality tests with Shack-Hartman wavefront sensor. ... Measurements on AZT-22 Telescope diameter: 1000 mm F/7.7 Effective subaperture: 37.5 mm Exposure time: 100 ms Time between exposures: 5 s Individual image with tilts in X direction AZT-22 tower The spatial spectrum evolution (top) and wind direction in measurements processes . AZT-22. ... ZTSH dome Zeiss-1000 dome The spatial spectrum evolution (up) end wind direction through time. ...

Peremennye Zvezdy", . ... Star Name: . 2MASS 20031968+6504085 . ... The variability of 2MASS 20031968+6504085 was discovered using a series of 58 unfiltered CCD images obtained with the MASTER-Amur robotic telescope (D = 400 mm, F = 1000 mm, Apogee Alta U16m CCD camera; Lipunov et al. 2010) between January 26 and March 27, 2011. After the standard calibration (dark subtraction, flat fielding) the images were processed with the VaST variability search software (Sokolovsky Lebedev 2005). ...

Microsymposium 40, abstract 56, 2004 (A4 format) AUTOMATIC COMPILING OF HYPSOMETRIC MAP OF A PART OF THE 1 VENUSIAN SURFACE. ... The main principles applied in compiling the map such as the scale of the heights, types of prints and using of pictures of surface shall be apply in the compiling of the Hypsometric Map of Hemispheres of Venus in future. We consider that contours are the necessary features for hypsometric maps because allow to make measurement more accurate. ... Moscow., ...

... We apply an additional restrictions on the model which follow from recent helioseismic results: 1) calibration of the surface helium abundance and the specific entropy in the convection zone (Vorontsov et al. ... AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... A most promising problem is to investigate the interaction of two VHF powerful radiowave beams in the ionosphere, whose difference frequency is equal to the plasma frequency in some ionospheric area (that is, the difference frequency is taken in the range 1-8 MHz). ... Two-frequency interaction effects are based on radiowave non-linear mixing, which is rather complicated when describing and modelling the experiment. ...

. Currently . student of the 5th course of Moscow Institute of Physics and Technology . Field of research interest . Network software developing, Image processing. Position . Laboratory assistant of Space Research Institute . Department Number . 902 (Space Monitoring Information Support) . Postal Address . Space Research Institute . Russian Academy of Sciences . Profsoyuznaya St. 84/32 . Moscow, RUSSIA . Postal Code . 117810 . Telephone Number . +7(095) 333-53-13 . E-mail . ugine@d902.iki.rssi.ru .

. The Cassini image reveals dark regions relatively free of high clouds where methane is strongly absorbed, and bright zones where high, thick clouds shield the methane below. Markedly different cloud attributes appear in different latitude bands. The image also shows a high-altitude atmospheric disturbance just south of the equator that has persisted since the 1990s. NASA / JPL / Space Science Institute

RadioAstronomy department of SAI was found in 1953 by prof I.S. Shklovsky. The basic direction of our works is development of new methods and devices for astronomical observations in different spectral regions, making observations and its interpretations. Department includes: laboratory RATAN-600, Infrared Group and several another scientific workgroups, that leads any big different projects. ... Go back to RadioAstronomy Dept ] . Andrew A. Martis . martis @ sai.msu.ru . ...