... epevents performs a pattern analysis to identify and characterize split events: the charge distribution in split events is analysed and the detected patterns are described by four parameters: . ... NULL value is set for trailing events which are excluded from the pattern analysis and MIPs. ... for doubles: neighbouring pixel (i.e. pixel with smaller PHA than the main pixel) to the right (1), bottom (2), left (3), top (4) with respect to the local maximum in the pattern . ...

Еще в разделе: (Показать все результаты (>31419) - xmm.vilspa.esa.es/ )

Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence in the detection. ...

Еще в разделе: (Показать все результаты (>2548) - www.sao.ru/ )

• IRAS IDS
• Noise distributions
• A 20 cm VLA survey of Abell clusters of galaxies

... Classes . ... casa . casa::DiscreteUniform . ... DiscreteUniform ( RNG *gen, Int low=-1, Int high=1) . ... low () const . ... range ( Int low, Int high) . ... These function allow you to manipulate the parameters (low & high) described above through the base class. virtual Vector < Double > . ... The DiscreteUniform class implements a quantized uniform random variable over the closed interval ranging from [low..high] . ... Int casa::DiscreteUniform::high . ... Int casa::DiscreteUniform::low . ...

Еще в разделе: (Показать все результаты (>18426) - www.atnf.csiro.au/ )

• casacore: casa::Uniform Class Reference
• Research - All-sky map of high-velocity clouds
• The Peculiar Spiral Galaxy NGC 1808

... People . Posts tagged ?citation? ... Astronomy is ruled by Gaussian distribution with a Poisson distribution duchy. ... Among these distributions, Pareto deserves a high rank. ... ArXiv] Pareto Distribution? Tags: asteroid , citation , IMF , nebula , Pareto distribution , survival function , truncated . ... 4 Comments . ... The full article is found from [arXiv/astro-ph:0712.1037] . ... ArXiv] The Importance of Being First: Position Dependent Citation Rates on arXiv:astro-ph? ... Entries RSS . ...

Еще в разделе: (Показать все результаты (>4273) - hea-www.harvard.edu/ )

• The AstroStat Slog Power
• The AstroStat Slog RMF
• The AstroStat Slog gamma

Next: Optical Jets in Up: QSOsGalaxies, and Previous: Quasar Spectral Features . ... High luminosity and high redshift combine in quasars to give conditions that allow studies of the intergalactic medium, as well as the emission mechanism in quasars. ... We present results of the modeling of the spectrum of the high redshift ( z =2.72), high luminosity ( 10 ergs s ) quasar, HS1700+6416 (Reimers et al. 1989), observed with HST FOS (Reimers et al. 1992) and GHRS (Reimers 1995). ... 1995). ...

Еще в разделе: (Показать все результаты (>20208) - www.stsci.edu/ )

• Method
• ACS Data Handbook
• Power Spectral Analysis

Еще в разделе: (Показать все результаты (>4) - aberrator.astronomy.net/ )

... Accurate identification of physical binary star systems has become of increasing interest in recent years. ... Identification of physical binary star systems, with an estimated reliability of such identifications based on the theory of probability, is also important for current and future efforts to find binary star systems that are candidates for observations with the aim of determining their orbits and component masses. ... probability of the proximity of proper motions and ; . ...

Еще в разделе: (Показать все результаты (>1996) - www.adass.org/ )

• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Integrating the HST Guide Star Catalog into the NASA/IPAC Extragalactic
• The IUE Archive at Villafranca

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

Еще в разделе: (Показать все результаты (>492) - zebu.uoregon.edu/ )

• U of O High Energy Physics Seminars

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

Еще в разделе: (Показать все результаты (>315) - www.gao.spb.ru/ )

• Pulkovo NEO Page: Ephemeris Support

... The distribution of redshifts among the DXRBS FSRQs identified so far (Figure 3) is quite similar to that of the 1 Jy and S4 samples. ... A more thorough comparison will have to await completion of our survey and the convolution of the redshift distribution with the WGACAT sky coverage. As has already been mentioned by Hook et al. (1996), selecting flat-spectrum sources is an efficient way of finding high-redshift, radio-loud quasars. ...

Еще в разделе: (Показать все результаты (>24314) - www.eso.org/ )

• Sample Identification
• Sample Properties
• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)

... High spectral, spatial and temporal resolution UV observations of the quiet Sun transition region show a highly structured and dynamical environment where transient supersonic flows are commonly observed. ... Estimates of the kinetic and enthalpy fluxes associated with these events show that explosive events are not important so far as solar coronal heating is concerned. ... In some cases, non-Gaussian line profiles are associated with supersonic flows in small magnetic loops. ...

Еще в разделе: (Показать все результаты (>3289) - star.arm.ac.uk/ )

• An Overview of the Coupled Earth-Sun System PPARC Introductory Solar System
• STFC Introductory Solar System Plasmas Summer School
• Terry Mosely's Bulletins

... gradients dependencies on solar wind parameters and IMF; . ... fate of thermal plasma at the dayside magnetopause. velocity-dispersed injections of the thermal and superthermal ions from LLBL at cusp and cleft (lowest energy VDIS-2 events); . ... outer cusp processes, role of outer cusp indentation, plasma entry (laminar reconnection, turbulent diffusion, others), role of turbulent boundary layer; . how is the magnetosheath plasma heated near magnetopause and cusp? . ... cusp/cleft wave emissions. ...

Еще в разделе: (Показать все результаты (>1663) - www.cosmos.ru/ )

• The TAIL 1996/1997 campaign
• The plot of the magnetic conjugation's time distribution
• OFO IKI / KKVO

... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...

Еще в разделе: (Показать все результаты (>3400) - www.sai.msu.su/ )

• Further Information and Bibliography
• Oleg Bartunov's Home Page

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

Еще в разделе: (Показать все результаты (>260) - mavr.sao.ru/ )

• Galaxy sector, archive 2014
• Hardware sector, archive 2006

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. ...

Еще в разделе: (Показать все результаты (>558) - xray.sai.msu.ru/ )

• Binary Pulsar Diversity and High Neutron Star Birth Velocity
• Why must a radiopulsar coupled with an optical star have high eccentricity?
• Test of the Initial Mass-Ratio Distribution

Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...

Еще в разделе: (Показать все результаты (>591) - www.mao.kiev.ua/ )

• MAO NASU :: Topic: "International Journal of Geosciences" - High Visibility and
• MAO NASU :: Topic: list of studentships/ positions (1/1)

The weight and positions for the objects on the rotary floor were obtained from ecastro on nov03 and used to plot the weight distribution on the rotary floor. ... The figure shows the weight distribution by turret position. ... Fig 1 top: Each object on the floor is plotted with its weight vs its turret position. Fig 1 middle: The weight is averaged by turret position quadrant to show the imbalance in weight distribution. ... The turret position is that of the receiver or read off of the drawing. ...

Еще в разделе: (Показать все результаты (>5415) - www.naic.edu/ )

• pointing
• Slide 25
• a2488 dps the 800Mhz rcvr.

... Identification and Analysis of Binary Star Systems using Probability Theory E. Grocheva and A. Kiselev Photographic Astrometry Department, Pulkovo Observatory, S.Petersburg, 196140, Russia, Email: gl@spb.iomail.lek.ru Abstract. Accurate identification of physical binary star systems has become of increasing interest in recent years. ... We chose 76 double stars from Pulkovo's observation program and calculated the probabilities of a random distribution for these pairs. ...

Еще в разделе: (Показать все результаты (>277) - www.stecf.org/ )

• http://www.stecf.org/conferences/adass/adassVII/reprints/barylakm.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/alexova.ps.gz
• NICMOS Data Calibration and Analysis

FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...

Еще в разделе: (Показать все результаты (>117) - selena.sai.msu.ru/ )

• http://selena.sai.msu.ru/Symposium/ant.doc
• http://selena.sai.msu.ru/Symposium/ant.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf

... Routines for accessing I/O ports are in /usr/include/asm/io.h (or linux/include/asm-i386/io.h in the kernel source distribution). ... Before you access any ports, you must give your program permission to do so. This is done by calling the ioperm() function (declared in unistd.h , and defined in the kernel) somewhere near the start of your program (before any I/O port accesses). ... For example, ioperm(0x300, 5, 1) would give access to ports 0x300 through 0x304 (a total of 5 ports). ...

Еще в разделе: (Показать все результаты (>1100) - jet.sao.ru/ )

• Spectral energy distribution
• Determination of atmospheric parameters and calculation of chemical composition
• Linux I/O port programming mini-HOWTO: High-resolution timing