... Incorrect Resolution Element Used by COS ETC for new G130M Modes . ... HST Overview . ... The resolving power of the two new COS/FUV G130M modes (cenwave=1055 and cenwave=1096) decreases with increasing wavelength, from R ~ 3000 at 950 ? ... Since the ETC uses a 6-pixel resolution element that is 5 and 19 times smaller, respectively, it will overestimate the time required to achieve a certain S/N per 30-pixel or 115-pixel resolution element, while underestimating the S/N obtained for a given time. ...

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• Introduction to NICMOS
• What is the meaning of the 2x2 resolution element in the ACS ETC for an
• FUV-MAMA Repeller Off as an Available Mode for High Resolution Spectroscopy

... Extreme sensitivity photon counting systems . ... Resolution to 3080 x 2304 pixels x 16 on photon counting systems . ... These can be coupled to a suitable scintillator to match customers' requirements, and to provide imaging covering the electromagnetic spectrum from UV to high energy gamma rays and particles. ... Photek image intensifiers and photon counting tubes are used in CERN and are chosen for the ACE explorer satellite system for reading out arrays of scintillating plastic fibre. ...

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• Direct electron imaging-performance
• Electron bombarded sensors-intro
• Product Folder: TC213, 1024- X 512-PIXEL CCD IMAGE SENSOR

... For SIMS (Secondary Ion Mass Spectrometry) analysis, a solid surface is bombarded by primary ions of some keV energy. ... The subsequent mass analysis of the emitted ions provides detailed information on the elemental and molecular composition of the surface. ... Extremely short ion pulses with a duration below . ... By rastering a fine-focussed ion beam over the surface, like an electron beam in an electron microprobe, mass resolved secondary ion images (chemical maps) can be obtained...

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• Crystalline scintillators for physics, medicine, safety, engineering

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

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• ENERGETIC PARTICLE EXPERIMENT DOK-2
• Energetic Particles

... Next: Unsupervised Catalog Classification Up: Object Detection and Previous: Classification of Objects . ... Multi-resolution allows for image analysis in terms of different scales. ... This approach is used for the detection (and subsequent analysis) of globular cluster systems around elliptical galaxies, and for image characterization and object trawling in large image databases. ... The applicability of this approach to object detection in large image collections has been investigated. ...

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• An Integrated Procedure for Tree N-body Simulations: FLY and AstroMD
• Calibration and Performance Control for the VLT Instrumentation
• PICsIM - the INTEGRAL/IBIS/PICsIT Observation Simulation Tool for Prototype

... GgiRealize realize created elements. ... GgiPlotField create a PGPLOT-compatible plot area. ... Updates: Jan 14, 1998: JPT, Document created. Feb 24, 1998: JPT, GgiWidget and GgiContext added. Feb 26, 1998: JPT, Plot field added. Mar 4, 1998: JPT, GgiPlotXor added. ... Mar 31, 1998: JPT, Shell element added. ... May 13, 1998: JPT, Form element added. ... Sep 11, 1998: JPT, Improved plot driver, added GgiHandleEvents. ... Jan 10, 2001: JPT, Check for pseudocolor visual; added GgiSetDisplay. ...

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• Number input
• USER-INTERFACE general subroutines
• How the rendering is done

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...

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• Elements of Nearby Spiral M33
• XWare > APOD

Multi-element X-ray detection module . ... Detection and spectrometry of hard X-ray radiation with the possibility of assembling of large area position-sensitive detectors. ... The design of module enables tight mounting for composing of detection plane the required size. ... Detector size љљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљ 4.0 4.0 2.5 mm . ... Energy range љљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљљ 10?150 keV . ... 6.0 (150) keV . ... X-ray detection modules . ...

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• About modification of the INTERBALL orbital elements
• DOK-2 Results Page
• The INTERBALL Auroral PROBE orbital elements collections

... The collecting area is increased by nesting concentric mirror pairs, all having the same focal length. ... Figure shows the largest optical element being ground at HDOS. ... X-ray testing demonstrated that the CXO mirrors are indeed the largest high-resolution X-ray optics ever made; the nominal effective area (based on the ground calibrations) is shown as a function of energy in the left panel of Figure , along with those of their Einstein and ROSAT predecessors. ...

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• AXAF-Chandra

Next: Detection Efficiency Up: CCD Scientific Performance Previous: CCD Scientific Performance . The X-ray energy required to liberate a charge pair in a semiconductor is approximately an order of magnitude lower than in gas detectors, hence the potential spectroscopic advantage of CCD detectors. ... For a number of years, good scientific CCDs attained noise performance of electrons rms, but this limited the energy resolution for X-ray energies 3keV. ...

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• Errors
• Generation from In-Orbit Data

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) MASSIVE PHOTOMETRY OF LOW-ALTITUDE ARTIFICIAL SATELLITES ON MINI-MEGATORTORA S. Karpov, 1, 3 E. Katkova,2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Davydov5 E. Ivanov,2 A. Perkov,2 V. Sasyuk3 RESUMEN Favor de prop orcionar un resumen en espanol. ... The nine-channel Mini-MegaTORTORA (MMT-9) optical widefield monitoring system with high temporal resolution system is in operation since June 2014. ...

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October 14, 2002 (Monday) David Jackson, Rutherford Appleton Lab, UK . ... Fall 2000 . ... The resolution obtained is compared with the starting point, based on an optical survey, and is shown to achieve the design performance. 4:00 pm, 472 Willamette Hall . return to top . ... Amplitude analysis of the D + , D s + decays to KK p and D 0 decay to K s KK are presented using the data collected by Fermilab High Energy Photoproduction Experiment E831(FOCUS). 2:30 pm, 472 Willamette Hall . ...

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• Astronomy HyperText Book: Fusion Sequences in Stars
• Flywheels and Energy Storage

As in the last years, the Ephemerides of Minor Planets for 2015 are prepared by the IAA RAS only in the electronic form. ... Orbital elements of all numbered planets have been determined in IAA all over again on the ground of available observations in the catalog of the Minor Planet Center. ... More detailed information on orbital elements used in the present volume of EMP and their accuracy is given in section "Information on new orbital elements". ... a) information on new orbital elements; . ...

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• AY2011 (preface)
• AY2008 (preface)
• AY2014 (preface)

... The three optical trains for the cameras, and the pupil reimaging system, are mounted on a wheel, accurately driven by an external motor. ... The low-resolution spectroscopic mode uses the wide field camera and a suitable set of grisms and order sorting filters that are inserted in the parallel beam after the pupil. ... One of the five grisms can operate at four different orders, depending on the filter selected on the first filter wheel that acts as order sorter. ...

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• Observing capabilities
• mod_xml2enc - Apache HTTP Server
• Descrizione tecnica NICS

ION AND ELECTRON ENERGY DETECTOR PAN-2 . ... The energy and angular distributions of charged particles can bring further information on the nature and spatial scales of magnetospheres processes. ... It permits the fast measurements of energy and angular parameters of charged particles in the range 40eV-40keV. ... The sensor unit is an electron electrostatic, axially symmetrical, toroidal analyzer. ... The energy range for both types of charged particles must stepped according to the logarithmic scale. ...

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• Laboratory static Fourier-spectrometer
• Introduction to Astronomy
• Optical static Fourier spectrometer

Microsymposium 40, abstract 28, 2004 (A4 format) HIGH PURITY GE GAMMA-RAY SPECTROMETER ON JAPANESE LUNAR POLAR ORBITER SELENE. ... GRS consists of three parts; gamma-ray detector (GRD), compressor driver unit (CDU) and gammaray and particle electronics (GPE). ... It is retained at ~80K, by means of a mechanical cryostat. ... The asymmetric shape makes it efficient to veto gamma-rays from the SELENE vehicle and leakage photons from the Ge detector, as well as to avoid charged particles. ...

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• http://selena.sai.msu.ru/Ber/Publications/ms40/88_Yamashita%20et_al.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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• APOD: 2001 September 27 - Elements of Nearby Spiral M33
• APOD: Galileo Views Ganymede
• APOD: 2002 July 25 - NGC 1569: Heavy Elements from a Small Galaxy

... Category. ... Continue reading ?[ ... Tags: book , Brieman , cigar , Clinton , data mining , Friedman , Hastie , KDD , light curve , machine learning , SCMA , shaking hands , SN , statistical learning , Supernova , Tibshirani . ... mini-Workshop on Computational Astro-statistics: Challenges and Methods for Massive Astronomical Data . ... In two years of this slog?s life, there?s no posting by a statistician, except one about BEHR . ... 1 ] Continue reading ?data analysis system and its documentation...

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• The AstroStat Slog data mining
• Astro Jargon
• The AstroStat Slog particle physics

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

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FLAMES is the multi-object, intermediate and high resolution spectrograph of the VLT. Mounted at UT2, FLAMES can access targets over a field of view 25 arcmin in diameter. ... GIRAFFE allows the observation of up to 130 targets at a time or to do integral field spectroscopy, with intermediate resolution (either R ~ 25000 or R ~ 10000). ... Questions related to service mode observations and proposal preparation should be addressed to the User Support Department. ... Instrument Operation Team . ...

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• ESO - Science Announcements
• CRIRES - VLT High-Resolution IR Echelle Spectrometer
• ESO - Thesis Topic: Constraining Stellar Interiors and Mixing via Depletion