... Star formation . ... The puzzling core of the Phoenix cluster: deep X-ray observations . ... SPT-CLJ2344-4243 shows a strong cool core with a potential mass deposition rate of ~3000 Msun/yr derived from the X-ray luminosity. ... The spectral analysis of the deep XMM-Newton observation of the Phoenix cluster found an average mass-deposition rate between 210 and 620 Msun/yr for the gas in the temperature range 0.15-3.0 keV (subject to calibration uncertainties). ...

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• FIRPO Runs
• Arcetri Guaranteed Time
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Lessons learned from the Thirty Meter Telescope site testing Tony Travouillon Sebastian Els, Angel Otarola, Reed Riddle, Matthias Schoeck, Warren Skidmore TMT.XXX.PRE.05.0XX.DRF01 1 Introduction TMT and its Site testing. Important choice before going on site. ... Considerations during analysis of the data. TMT.XXX.PRE.05.0XX.DRF01 2 Some Background about the TMT Site Testing TMT is a 30m, segmented, RitcheyChretien telescope design. ... ASCA Cloud Cover Analysis So how do we do it in practice? ...

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• Methods and instruments to measure/monitor major site properties

Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

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• High Energy Astrophysics Department at IKI RAN

The LCDM paradigm: successes and challenges on scales of galaxies Anatoly Klypin (NMSU) LCDM · · · · DM profiles, concentrations, .. Clustering of galaxies: P(k) and correlation functions Satellites: abundance, number-density profiles Galaxies and Dark Matter: abundances Dwarfs. ... Springel et al 2008. ... Klypin et al 2010. ... Observations - LCDM: just enough Magellanic Clouds Observations LCDM Vmax > 50 km/s Busha et al 2010 Dark matter profiles: standard LCDM Aquarius simulation. ...

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• Radio sources identfification
• Search for distant radio galaxies in SAO
• GRB follow-up team

... arXiv.org . astro-ph . ... We fit the near-infrared to radio spectral energy distributions of 30 luminous and ultra-luminous infrared galaxies with pure starburst models or models that include both starburst and AGN components to determine important physical parameters for this population of objects. In particular we constrain the optical depth towards the luminosity source, the star formation rate, the star formation efficiency and the AGN fraction. ...

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Observation and modelling of main sequence star chromospheres. ... We compare our calculations to recent high res­ olution observations for selected stars in a narrow spectral range ((R­I) џ =0.875\Sigma0.05); we show that Hff line profiles behave as expected, with a tight correlation be­ tween the line width and equivalent width. ... We show that the hydrogen series dominate the radiative cooling in the spectral lines (form 40% to 90%) for Hff emission line stars. ...

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• http://star.arm.ac.uk/~ambn/abstract293.html
• Armagh Observatory
• Abstract

... Our scientific interest is an accuracy of asteroid CCD observations obtained by amateurs and professional astronomers all over in the World. ... These data help us to analyse an accuracy of real CCD positions in the MPC Database. ... Do you test your observations of the small Solar System bodies permanently before sending them to the International Minor Planets' Center? ... Do you know a real accuracy of your positional CCD-observations in comparison with the other observatories' one ? ...

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... An estimate the rotation period of cometary nuclei is important for understanding and describing the physical processes of the cometary activity. Unfortunately, the measurements of the rotation periods of the comet nucleus depend on the model assumptions and it is one of the main reasons for the scatter of the estimates given in various articles for a given comet. ... Right: the image of the comet 29P/Schwassmann-Wachmann 1 obtained at the 6-m telescope. ...

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• RCJ0311+0507
• Multiple System iUMA
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Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...

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• The Stellar Population in the NICMOS Parallel Fields
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... Moscow, August 25-30, 2007 . ... Main topics: . Idempotent and tropical mathematics including: . Idempotent analysis, . ... Tropical and idempotent convex geometry, . Mathematics of idempotent semirings, . ... Quantization, dequantization, and related topics of mathematical physics . Official languages of the workshop: English and Russian. ... To participate please fill in the following registration form and return it to our contact addresses by the deadline May 15, 2007. ...

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• Introduction to probability and Statistics (Spring 2010)
• Special Year in Multiscale Mathematical Modeling in Biology and Medicine
• Mathematical statistics: an introduction (Fall 2011)

. My astronomical research interests center on galaxy structure and evolution. Current topics include: . Polar-ring and interacting galaxies (see also new catalogue ) . Galaxy warps: statistics, properties and origin . Spiral galaxies at z~1: radial and vertical structure of stellar disks, statistics of interactions . Surface photometry and kinematics, dynamical modeling . Observational cosmology . Joomla Counter since Sep 1997

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• Introduction
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Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• The Radiopulsar PSRB1259-63 - a Probe in the Stellar Wind Plasma
• The ``Reflection'' Effect
• Concluding Remarks and Future Prospects

... In electron-positron colliders, effect of the lattice modification by opposing bunch focusing on the equilibrium radiation emittance is important at high values of the space charge parameter, so one should correctly evaluate this dynamic radiation emittance of the weak beam, which may differ a lot from the nominal emittance, already in the linear beam-beam force model. ... The linearized beam-beam force is equivalent to focusing insertion in linear lattice of the collider. ...

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... VLBA+Italy survey (to contact the schedulers) (closed) E.Fomalont and J.Romney: To provide some review of problems happened with fringe search in VSOP project. (closed) M.Popov : To compose a tentative time -table of possible observations , and inform the observatories on the specific time slots that might be requested for fringe search program in October-November. (continued) C. Gwinn: to try to compile FAKERAT software on modern platforms. (closed) GBT and ...

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• Description of the RadioAstron project, english version
• DPC Post-Observations Products
• MEMORANDUM

... ursa in Unknown (configure /etc/snmp/snmpd.local.conf) . ... Max Speed: . ... at which time 'ursa' had been up for 233 days, 1:27:12 . Max . Average . Current . ... 90.0 kB/s (0.4%) . ... 152.0 kB/s (0.6%) . ... 144.0 kB/s (0.6%) . ... Incoming Traffic in Bytes per Second . ... Outgoing Traffic in Bytes per Second . ...

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Next: Analysis of a Up: No Title Previous: One example . We will start with a simple wavelet: the `Mexican hat', shown on Fig. ... Figure 2: The Mexican hat wavelet . It is important to note that, for this to be a wavelet, the positive and negative areas `under' the curve must cancel out. This is known as the admissibility condition. Analytically, the Mexican hat wavelet is represented by . ... Selection of the wavelet shape is one of the important decisions on the user's part. ...

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• No Title
• List of books on Statistics and thermodynamics
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. Statistics of sunspot activity . The sunspot indices . My observations . NGDC's observations . The solar regions . Links . About authors . Russian pages . Last updated 6.04.2016 .

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• The Sunspot Observer - Average annual indices of solar activity NGDC -
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Probably a Planet for Beta Pic . ... Explanation: A mere 50 light-years away, young star Beta Pictoris became one of the most important stars in the sky in the early 1980s. Satellite and ground-based telescopic observations revealed the presence of a surrounding outer, dusty, debris disk and an inner clear zone about the size of our solar system -- strong evidence for the formation of planets . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ...

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• Probably a Planet for Beta Pic
• Journal "Peremennye Zvezdy" > PZ Authors and Statistics of Publications
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... Latest Supernovae . ... Sorted by Name For the years covered, 7501 supernovae and 114 extragalactic novae were reported. 376 of these supernovae were named by CBAT, 1714 were given possible supernova designations, and 5411 were not reported to CBAT. 219 supernovae were found in NGC/IC galaxies, 874 were found in named galaxies 341 objects were discovered by amateurs 4 were brighter than 13th Magnitude 208 were brighter than 16th Magnitude 1079 were brighter than 18th Magnitude 1349 ...

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• Bright Supernova pages - Statistics for 2001

Summary by Month . Generated 04-Feb-2011 23:59 MSK . ... Month . ... Monthly Totals . Hits . Files . ... Feb 2011 . ... Jan 2011 . ... Dec 2010 . ... Nov 2010 . ... Oct 2010 . ... Sep 2010 . ... Aug 2010 . ... Jul 2010 . ... Jun 2010 . ... May 2010 . ... Apr 2010 . ... Mar 2010 . ... Generated by Webalizer Version 2.21 ...

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• Six-Centimeter Radar Observations of 4179 Toutatis
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