HUBBLE SPACE TELESCOPE DAILY REPORT #2498 PERIOD COVERED: 0000Z (UTC) 11/10/99 - 0000Z (UTC) 11/11/99 Daily Status Report as of 315/0000Z 1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED: 1.1 Completed Two Sets of STIS/CCD 8408 (STIS CCD Dark Monitor C8) The Space Telescope Imaging Spectrograph (CCD) was used to make a CCD bias calibration observation. This is to monitor the darks for the STIS CCD. ... The observations were completed as scheduled, and no problems were reported. ...

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• http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_02_10_00
• http://www.stsci.edu/ftp/observing/status_reports/hst_status_02_28_02
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_02_09_00

GALFA - H I Projects . The table below summarizes approved GALFA H I projects. Some project names link to project web sites. All scheduled project IDs link to the relevant proposal abstract in the telescope schedule database , which also lists scheduled observations for each project. If these exceed the requested observing time, a project is deemed completed ; otherwise, it is either in progress or not yet scheduled , depending on whether observations have begun. ... Goldston . ...

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• I-GALFA Coverage Complete
• Murray Lewis
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution

... Data Analysis SAS News What is SAS? How to use SAS SAS Workshops SAS Version Changes Download and Install SAS Science Simulator (SciSim) . ... Only two parameters of that task are of relevance here: the observation date and the analysis date . ... The observation date is available in sereval places, one of these is in the ODF constituent rrrr_oooooooooo_SCX00000SUM.ASC . ... This will generate a (Unix/Linux) shell script with which you can download via ftp all the CCF constituents in the CIF. ...

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• XMM-Newton Current Calibration File: Updates
• XMM-Newton Helpdesk
• XMM-Newton SAS Download Feedback

... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Phase 2 Submission . ... Service Mode Philosophy . ... OB Execution Overheads . ... Readme File . ... Checking OBs and README files in the ESO Database . ... These checks will also be automatically performed at the time of checking the Phase 2 material into the ESO Database, and non-compliant OBs or README files will be rejected. ... All Service Mode OBs and README files must be submitted to the ESO Database from P2PP....

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• ESO - Newsletter July 2014
• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
• FORS Sec Std and Abs Phot Project

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• Astronomy HyperText Book

... To schedule Mark III projects using non-VLBA control file stations or a Mark III correlator, it is best to use PC-SCHED, written by Alan Rogers and Dave Schultz at Haystack (unrelated to SCHED), or SKED, written by Nancy Vandenberg at Goddard Space Flight Center. ... It is recommended that most VLBA Mark III observers send their ``.drg files'' files to the AOC, where the staff will use SKEDCONV and SCHED, along with current setup files, to make the VLBA control files. ...

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• Archive of VLBI Observations Majordomo List
• Late Stages of Stellar Evolution
• VSOP Observing Schedule

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2011 . An automated method for mapping of vegetation cover over Russia using Earth observation data . ... The Space Research Institute of Russian Academy of Sciences . ... P.285-302. (in Russian) . ... P.103-116. (in Russian) . ... Main results of the experimental and theoretical research completed in 2010 . Main results of the experimental and theoretical research completed in 2009 ...

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• Main research and development work completed in 2009 and ready for
• Main results of the experimental and theoretical research completed in 2009
• Main research and development work completed in 2010 and ready for

... 4 "Magnetic stars" of the multilateral cooperation of the Academies of Sciences of Socialist countries on the problem "Physics and Evolution of stars", organized by the Astronomical Council and the SAO of the USSR AS , was held in the SAO, from October, 12 to October, 17 , 1987. ... The most important problems: origin and evolution of magnetic fields and chemical anomalies, interaction of magnetic fields and stellar matter are being analyzed. ... Investigation of CP stars with anomalous He lines; 2)...

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• Search for distant radio galaxies in SAO
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and
• On the problem of high spectral resolution observations of faint objects

... It provides long range planning information to the scheduling team; it provides bright object, timing, and orientation information to the observation planning team; and it provides graphical description of the observations and their constraints. ... The GUI graphically displays the constraints that are computed by Spike and stored in the description files and in the database. ... BOAS processes all bright objects that have entered the database since the last time BOAS was run. ...

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• The OPUS Pipeline: A Partially Object-Oriented Pipeline System
• Evolution of EUVE Guest Observer Data Reduction
• NICMOS Software: An Observation Case Study

Next: MASSES Up: EXTREME HELIUM STARS: PULSATION Previous: STELLAR PROPERTIES . ... Following main-sequence evolution, a red giant star in a close binary system may expand to fill its Roche lobe. ... Although Iben & Tutukov (1984) used this model to account for the EHes, the latter are not binaries (Jeffery et al. ... Final helium-shell flash in a post-AGB star. ... Accretion from the disk onto the surviving WD creates a star with a degenerate CO core and a helium envelope. ... Other models. ...

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• The Chemical Evolution of FGSge
• Staff Movements
• Solar System Research

SUMMARY OF THE RESEARCH PROPOSAL by Maxim Vsemirnov Research topic: Hurwitz and (2,3)-generated matrix groups and related problems. ... The reason to study these groups arises from the fact that the class of (2, 3)-generated groups together with three cyclic groups {1}, C2 and C3 is exactly the class of quotients of the classical modular group PSL2 (Z). ... The answer is known for sporadic groups, some exceptional groups of Lie type and for the most series of classical matrix groups of large rank. ...

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• Conference "Random Processes, Conformal Field Theory and Integrable Systems"

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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• Group for study of galaxies and cosmology, history

... Just to learn how to generate a system call, I created a simple system call that basically sets and resets the value of a global parameter "PREFETCH". SYSTEM CALL code ********************************** int PREFETCH = 0; /* this is a global variable */ . ... To execute the sys_prefetch system call, I wrote a prefetch.c file with the following code. ************************code to call sys_prefetch***************** #include <linux/unistd.h> _syscall2 (int, prefetch, int, mode, int, nr_hints) . ...

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• SCHED_FIFO scheduling
• Realtime Problem
• Slide 9

... Bojan Nikolic web pages (r. 329) . ... Note however that the radiospec is built in the ?build? sub-directory of the directory you installed it to and is not installed ? ... Build radiospec wget http://www.mrao.cam.ac.uk/~bn204/soft/radiospec-1.0.tar.gz tar --strip-components = 1 -xzvf radiospec-1.0.tar.gz PATH = $INSTALLDIR/bin:$PATH scons PKG_CONFIG_PATH = $INSTALLDIR/lib/pkgconfig/ . ... You will at least also need the numpy package for Python . ... Download & building of the radiospec package . ...

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• Galaxy Evolution Bojan Nikolic web pages (r. 329)
• Astrophysics Group Opening of Battcock Centre for Experimental Astrophysics
• Galaxy Evolution: EVN Deadline

Sergey B. Popov Research experience My research interests and activity are centered around two fields of astrophysics: star formation and evolution and physics of compact objects. My research work on the population synthesis of binary stars was done in the Department of Relativistic astrophysics under supervision of Prof. Lipunov. ... In the future I would like to work on the evolution of isolated and binary neutron stars, accreting isolated neutron stars and young neutron stars in SNRs. ...

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• The Evolutionary Status of Radiopulsars in Massive Binary Systems
• Cosmic Rays and Evolution of Binary Systems
• Evolution of the Double Neutron Star Merging Rate andthe Cosmological Origin of

Chiaki Kobayashi, Ralph Sutherland How galaxies did form and evolution? - to answer this unsolved problem, we are simulating the formation and evolutionary history of galaxies in the Universe, including star formation, supernovae feedback, and chemical enrichment. Comparing the spacial distribution of elements within galaxies with observations, we will examine fundamental physical processes that drive galaxy formation. ... COALA : Universe Galaxy AGN Star Planet ...

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• Benefits of the Exercise
• The Common Room roof is completed
• Completed dome

A problem, that can arise when moving from Fortran 77 to Fortran 90, is dependent on a usual deviation from the standard, and has to do especially with user programs. ... With many Fortran 77 implementations we wrote PROGRAM TEST REAL X WRITE(*,10) 10 FORMAT('Give X = ',$) READ(*,*) X WRITE(*,*) X END In Fortran 90 we use "non-advancing I/O" instead. ... In some old Fortran dialects the statement TYPE was used to write on a typewriter terminal and PRINT was used to write on the line printer. ...

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• Use of program libraries

... at the ISSP RAS. ... MSU student Kostretsova N.B. successfully defended her thesis entitled "Investigation of Thermal and Chemial Expansivity of Ceria-Based Solid Solutions". ... V.A. Kolotygin successfully defended his PhD thesis "Perovskite-Like Oxide and Composite Anode Materials for Solid Oxide Fuel Cells: Functional Properties and Electrochemical Behavior in Contact with Gallate- and Silicate-Based Solid Electrolytes" and was awarded PhD degree in the area of Materials Science and Engineering ....

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... Previous: Ground Tracking Station (GTS) Products . ... GRT Log File . ... GRT Gain Curves . ... What: Co-observing GRTs will each generate a log file identical to those for ground-based VLBI experiments. ... Where: Files are placed by GRTs on their regional server ( Regional Servers for GRT logs etc ) in the sub-directory named for the month and year (e.g. may97 ) below the sub-directory named gps . ... Where: Files are placed by GRTs on their regional server ( Regional Servers for GRT logs etc ). ...

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• GOCG Pre-Observation Products
• RSOG Pre-Observation Products
• Correlator Products

... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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• Solar Physics
• Celestial Mechanics