... Deductions from the net available orbits based on preallocated Cycle 13 orbits. ... Table 3: Summary of Remaining Current Cycle Visits as of 2004.061 Current Cycle Proposal Types Currently having plan windows Current Cycle (non-DD, non-ToO) without Plan Windows: Expected Current Cycle DD to be executed: Expected Current Cycle ToO to be executed: HOPR orbits for above orbit pool (2.5%): Subtotal: Orbits 1770 69 20 140 50 2049 Table 4: Weeks available within ...

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• http://www.stsci.edu/spst/lrpg/mission_planning/cycle_orbit_accounting/cycle13_S_orbit_accounting-final3.pdf
• http://www.stsci.edu/spst/lrpg/documentation/procedures/lrpg_orbit_accounting.html
• http://www.stsci.edu/spst/lrpg/documentation/procedures/cycle11_orbit_accounting.pdf

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Information & tools for observers . ... CSIRO ATNF Data Archives . ... What is a pulsar? ... Group . ... Parkes Pulsar Observing Wiki . ... In order to carry out observations using Parkes, the observer first requests observing time by submitting a proposal through the OPAL system ( http://opal.atnf.csiro.au ). ... Select 'Search', followed by 'Pulsar Search' to obtain the Parkes data. ...

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• VLBI Wiki | Main / Mark5eVLBI
• Required software
• Pulsar Group Main/Psrfits

... Proposal Type: General Category: Observation Category: Time Requested this semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time : Expected Data Storage: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 10 0 2 hour over 500 GB Towards a new model of interstellar turbulence using pulsar B0834 +06 Our previous speckle image towards the pulsar B0834 +06 revealed features in the sub-AU structure of the ...

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• http://www.naic.edu/vscience/schedule/2013Fall/KaspitagP2030.pdf
• http://www.naic.edu/vscience/schedule/2013Spring/StovalltagP2790.pdf
• http://www.naic.edu/vscience/schedule/2013Spring/ShepardtagR2795.pdf

... The space VLBI mission RadioAstron, led by the Astro Space Center (ASC) of Lebedev Physical Institute, . ... execution of a balanced scientific program for the Mission. The scientific program of the RadioAstron will consist of three major parts: the Early Science Program (ESP), . Key Science Program (KSP), and General Observing Time (GOT) projects. ... The KSP . ... a long-lasting scientific impact of the Mission. ... The RadioAstron Announcement of Opportunity - 1 and Final Notes ; . ...

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• Contingency Plans
• RadioAstron main page, english version
• RSOG Pre-Observation Products

... To date, a total of 1043 photometric observations have been collected with FIRPO. The statistics include 256, 279, 412 and 78 measurements in the main filters J1, H2, K3 and L4 respectively. ... A full listing of the measurements, ordered by date and with the filters and program name indicated, is available. Also available is a summary of the FIRPO runs, with details of the dates, telescopes and observers. ... The date are in the fmag.dat files. ... A message with more details has been posted. ...

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• FIRPO Runs
• IBIS: SolarNet Access
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Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

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• Design and Status of the NICMOS Cryocooler
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... Over the first 4 years, its X-ray telescopes eROSITA and ART-XC will survey the whole sky with a record sensitivity in the 0.5-10 keV energy band. ... The goal of the second international Spectrum-RG conference is to discuss the different scientific topics addressed by the mission, synergies with surveys at other wavelengths, and requirements to follow-up observations.Contributed talks and poster presentations are invited on the topics related to the SRG science goals. ... Active galactic nuclei . ...

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• Russian Turkish 1.5-m telescope
• Zeldovich-100 / International Conference / Moscow, Russia

... Bojan Nikolic web pages home . ... For some numerical experiments with CASA , I have recently been recompiling some parts of this package. ... That is before even touching the code! ... I used the SCons build system to build the CASACORE libraries. ... Apparently missing include for strlen: --- a/code/display/Display/Options.cc +++ b/code/display/Display/Options.cc @@ -30,6 +30,7 @@ #include <sys/stat.h> #include <iostream> #include <dirent.h> +#include <string.h> namespace casa { namespace viewer {...

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• OptInt PmWiki : Main / Home Page
• The Status of Hungarian Space VLBI Assistance Software
• OptInt PmWiki : PmWiki / Wiki Group

Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 05 - 11.11.2012, Forecast on 12 - 19.11.2012, Carrington Rotations 2130 (04,86.11.2012) SUNSPOT-FORMING ACTIVITY OF THE SUN WAS REMAINED ON THE AVERAGE LEVEL. ... NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVERAGE. ... FLARE ACTIVITY WAS AT THE AVERAGE LEVEL ON NOVEMBER 8 AND 11, LOW - 5 AND 9 AND ON VERY LOW IN OTHER DAYS. ... THE GREATER THAN 2 MeV ELECTRON FLUX AT GEOSTATIONARY ORBIT VERY HIGH LEVEL WAS NOT OBSERVED. ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20121210.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20121022.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20121015.en.txt

... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...

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• GROUP/ROMAFOT
• General Information
• Quasars

.

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CAL/OPS meetings M. Kirsch ESA/ESOC with input from the XMM FCT XMM-Newton | ESA/ESOC | HSO-OAX | ... Page 8 special events Collision avoidance in place (November 2011 ­ March 2012) Reaction wheel cage instability: · · XMM_SC-72, 2011-08-16, Reaction Wheel 1 unexpected increase in torque and current during stable pointing Switch of reaction wheel configuration from 1-2-3 to 2-3-4 in December 2011 4WD project · Wheel4 tested up to 3750 rpm in July MCS migration Fuel migration XMM-Newton | ...

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• http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0014-1-0.ps.gz
• XMM-Newton SAS: Watchout Page
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The two main numerical libraries in Fortran 90 are . NAG Numerical Libraries for Fortran 90 Users . IMSL Fortran 90 MP Library Both of these offer both a modified version of the Fortran 77 library, recompiled for Fortran 90, and a completely new library, using all the new facilities of Fortran 90. ... On the Sun using Sun OS 4.2.1 we also got completely wrong results when using library functions in single precision, since the C system on Sun converted all function calls into double precision. ...

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• XFree86/OS2 Available Ported Software - Libraries
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... At 22:42:27 UT 26/07/09, the Burst Alert Telescope (BAT) on board of the SWIFT multi-wavelength space observatory triggered and located GRB 090726 gamma-ray burst event. ... About half an hour after the BAT trigger, the first images were obtained with the SAO RAS Zeiss-1000 telescope in four BVRI filters (see Fig.1). ... The spectrum of the optical transient was obtained with the SAO RAS 6-m BTA telescope 1.54 hours after the burst, using the SCORPIO instrument in the spectroscopic mode (Fig.2). ...

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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and
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Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...

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• Exoplanet HD 209458b: A planet that thinks it?s a comet | Astronotes
• Vesta: Asteroid seen by Dawn spacecraft | Astronotes
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... Science Users Information > Science Activities > Call for Public Surveys with the Arizona Radio Observatory . ... Call for Public Surveys with the Arizona Radio Observatory . ... As part of the Agreement for transferring ownership the AEM ALMA prototype antenna to the University of Arizona to install it on Kitt Peak as a telescope of the Arizona Radio Observatory (ARO), ESO will distribute to its user community a total of 3600h of observing time on the ARO telescopes over the next five years. ...

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• ESO - Newsletter May 2014
• ESO - mboss98
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... Space flight . Crew training . ... Space camp . ... acquiring practical habits and skills of performing all the flight operations envisaged for a flight participant; . maintaining and honing professionally required qualities and skills for a successful activity in conditions of effect of adverse factors of a space flight, as well . ... preparing for the activity outside the spacecraft; . ... preparing for professional activity in conditions of effect of the space flight factors; . ...

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... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

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