. Diameter of circular antenna . 576 m . Number of antenna elements . 895 . Size of an element . 11.4 x 2 m . Geometrical area . 15000 m 2 . Effective area of full circle . 3500 m 2 . Wavelength range . 1 - 50 cm . Frequency range . 610 - 30000 MHz . Maximum angular resolution . 2 arcsec . Accuracy of coordinate determination . 1-10 arcsec . Flux density limit . 0.500 mJy . Absolute brightness temperature limit . 0.050 mK . Tracking time (South sector + Flat mirror) . 1-3 h . [RATAN-600 Homepage]

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• Radio telescope short description

In the PROJECT we are using the following peculiar . features of RATAN-600 . ... Brightness temperature sensitivity being equal to the antenna temperature sensitivity .. ... Receiver system .. ... Using aperture averaging effect. dual- beam and dual (multi-) frequency filtration, we demonstrated full filtration of the atmosphere noise down to the receiver noise at all scales of acoustics peaks ( Fig.1 , Fig 2 ). ... We select this frequency as the central one in our project. ... Antenna surface . ...

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• harak_e
• RATAN-600 antenna

Instrument Science Report ACS 00-01 PREDICTED SENSITIVITY AND DISPERSION OF THE PRISMS AND GRISM R. C. Bohlin, G. Hartig, and F. R. Boffi 2000 May ABSTRACT The three prisms and the grism in ACS are characterized in terms of the dispersion relations and sensitivity, so that a user can predict count rates and S/N of sources with known flux. ... The wavelength coverage in first order is from 5500 to 11,000е. Outside this Copyright© 1999 The Association of Universities for Research in Astronomy, Inc. ...

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• COS Data Handbook
• Imaging Bright Object Protection Limit
• Absorption line spectra of the UV bright z=2.4 QSO HE 1122-1649

Linear Array Spectrometric Detectors RY-512 · RY-1024 · PDA-512 · PDA-1024 · High performance single diode array Quantum Efficiency, % 100 90 PDA detectors for spectroscopic systems · Full 25 mm coverage on 1024 element array Large well capacity Low cost 80 70 60 50 40 30 20 10 0 200 300 400 500 600 700 800 900 1000 1100 · · Wavelength, nm Linear Arrays Reticon diode array models RL-512SAQ or RL-1024SAQ with 512 and 1024 ...

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• Maximum limits
• WSRT deep surveys
• Optical spectroscopy

RTT150 . ... One of the image, obtained in the May, 2003, with Andor DW436 CCD. Cluster 1541+6626, filter R, exposure 15 minutes, the resolution is 1", limiting star magnitude is 23m, the field of view is 8' x 8'. At the left: image of cluster 0720+7132 (z=0.268) obtained in the beginning of November, 2002 with RTT-150 and AP-47P CCD. 25 minutes exposure in R. The resolution is 0.7" (angular size of the image element - 0.23"), limiting stellar magnitude is 23.5-24. ...

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• Spectrum-Roentgen-Gamma - The astrophysical Project at IKI RAN

... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...

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• MASTER GLOBAL ROBOTIC TELESCOPES NET

The aim of this section of the course is to familiarise you with celestial Coordinates. ... I found some good notes explaining the celestial coordinate system on the web: . ... 1st Dec: 04hr, 00min In addition to the equatorial coordinates described in the notes above, astronomers also use (at least) two other coordinate systes: galactic coordinates and ecliptic coordinates. ... Ecliptic coordinates use the ecliptic (the Earth's path around the sun) as the equator, and are used for solar system work. ...

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The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...

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• AO on AR 8970
• CHIANTI atomic database

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. ...

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• Thermodynamics
• Astronomy HyperText Book: Fusion Sequences in Stars
• QSO Absorption Lines and Other Cosmological Probes

... At the Limit of Diffraction . ... Credit Copyright: Yuri Beletsky ( Las Campanas Observatory , Carnegie Institution ) Explanation: Did you ever want to just look through the eyepiece of a large telescope in space ? If you could, you would see a sharp view that was diffraction limited . ... Still, in this working earth-based snapshot a new active adaptive optics system (MagAO) is being used to cancel out the atmospheric blurring in a visual observation of famous double star system Alpha Centauri . ...

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• Journal "Peremennye Zvezdy"
• Astronet > Sky Map, professional edition
• Supernova Remnant: Cooking Elements In The LMC

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• Towards a General Definition for Spectroscopic Resolution
• ADASS 2002 Conference Proceedings
• ADASS 2003 Conference Proceedings

... The SUB and SUP elements are used for subscripts and superscripts respectively, and are preferably rendered in reduced font. ... Some times you will want to place superscripts to the left of a term. ... For instance: X<sub align=right>a</sub> <sup align=left>b</sup>Y X<sub align=right>a</sub>Y<sup align=left>b</sup> b both render to X Y a while X<sub align=right>a</sub><sup align=left>b</sup>Y b renders to X Y a . ... The ID, LANG and CLASS attributes for SUB and SUP are not used within MATH...

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• Comet Center of SAI
• Fill-Out Forms
• The Body Element and Related Elements

... Keywords-- superconducting integrated terahertz receivers, oscillators and spectrometers. nanostructures, G. de Lange2, V.L. Vaks3, J. Yuan4, H.B. Wang 2 4 4 SRON Netherlands ... Physics of Microstructure RAS, Nizhny Novgorod, Russia; National Institute for Materials Science, Tsukuba, Japan I. I NTRODUCTION A Superconducting Integrated Receiver ( SIR ) [1] comprises on one chip a low-noise SIS mixer with quasioptical antenna, an Flux-Flow Oscillator ( ...

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• http://www.cplire.ru/html/lab234/pubs/2012_08.pdf
• http://www.cplire.ru/html/lab234/pubs/2011_08a.pdf
• Lab234 - Design, fabrication and experimental studies of a novel device: Cold

Next: Limiting Energy Channels Input Up: *fit* - Fit Data Previous: Raymond Model . The model is a two-temperature Raymond thermal spectrum, low temperature range is 0.55 to 0.65 keV, high temperature range is 1 to 2 keV, element abundance table is cosmic, abundance of heavy elements (atomic number >2 ) is 50% of the value in the table. Note that 0.7 = log(5.0), specifies that the second component normalization will be 5 times the normalization of the first component. ...

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• The AstroStat Slog Confidence Limits
• The AstroStat Slog upper limit
• The AstroStat Slog Upper Limits

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• Celestial Mechanics
• Eclipse elements for Computer Ephemeris for 2015 (DE200/LE200).
• Eclipse elements for Computer Ephemeris for 2014 (DE200/LE200).

I read with interest the letter from Stephen White in the June 2001 edition of the ATNF Newsletter, pointing out that the current 3-mm upgrade of the ATCA, while providing powerful new facilities, will not provide the first 3-mm interferometer in the Southern Hemisphere. ... The interferometer and eclipse results, taken together, indicated that the solar brightness distribution at a wavelength of 3-mm was constant over the disc except for a narrow bright ring at the solar limb. ...

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• casacore: casa::SpectralList Class Reference
• Sensitivity Limits
• Australia Telescope Compact Array Home Page

There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...

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• Keywords_79
• ENGAMPLE
• AY2011 (preface)

... These are just the bare bones--just three basic ideas and rules for handling relations ("equations") involving unknown quantities whose values you are trying to find. In most calculations you try to find a number . ... To get a solution, one must replace the given equation (or equations) with others, containing the same information but cleaner in appearance. ... If you have an equation and modify both its sides in exactly the same way, what you get is also a valid equation. ...

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• The INTERBALL Auroral PROBE orbital elements collections
• About modification of the INTERBALL orbital elements
• The INTERBALL Tail PROBE orbital elements

... It may be added, subtracted, divided or multiplied in any way appropriate for ordinary numbers. A mathematical relationship involving known numbers (like 25 or 40) and unknown ones (like x ) is known as an equation . ... To get a solution, one must replace the given equation (or equations) with others, containing the same information but cleaner in appearance. ... If you have an equation and modify both its sides in exactly the same way , what you get is also a valid equation. ...

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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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• astro-ph