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1. GOODS: The Great Observatories Origins Deep Survey
... GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer , Hubble , and Chandra , ESA's Herschel and XMM-Newton , and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. ... The space-based observations are complemented by ground-based imaging and spectroscopy, including extensive commitments of ESO and NOAO observing time. ... 2010-04-10: Deep VLA 1.4 GHz data for GOODS-North . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/goods/ -- 16.1 Кб -- 19.05.2010
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2. Parameter estimation
... In this context, (or, in the time domain, l ) are no longer independent variables. They are treated like any of the other parameters: i.e. are assumed to be random variables to be estimated from the observations by fitting a model. ... The MIDAS TSA package contains just one such model, namely Fourier series (SINEFIT/TSA) . ... In the time domain, the most important parameters to be estimated from the data are the correlation length of and time lag between the input signals. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node231.html -- 3.4 Кб -- 23.02.1996
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3. User Parameters - Data Location & Beam Selection CentralProcessor 0.11
... CentralProcessor 0.11 documentation . ... The following parameters determine where the measurement sets are that hold the data to be processed. The default behaviour is to read the MS from the given Scheduling Block (SB) directory. ... Location (on galaxy) of the scheduling blocks. This is used when specifying SB numbers - the default is the standard location for BETA operation. ... These parameters determine which beams in the data to process. ... User Parameters - Pipeline & job control . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/BETApipelines/DataLocationSelection.html -- 8.5 Кб -- 12.04.2016
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4. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The interface between the lower solar atmosphere where energy is generated by subsurface convection and the corona comprises the chromosphere, which is dominated by jet-like, dynamic structures, called mottles when found in quiet regions, fibrils when found in active regions and spicules when observed at the solar limb. ... In addition, how they affect the coronal heating and solar wind need to be further explored. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2012/609.html -- 7.0 Кб -- 17.07.2012
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5. Student Research at Manastash Ridge Observatory
Follow-up observations with the University of Washington 0.76 m telescope at Manastash Ridge Observatory (MRO) of the Sloan Digital Sky Survey (SDSS) cataclysmic variable (CV) SDSS J170053+400358 are presented. ... They estimate that the dimming amounted to about 0.028 mag (using two comparison stars that were each about 4 mag fainter than HD 209458). only UW affiliated authors have been listed, student researchers are marked with an ``*'' . ... XTE J1859+226" UW affiliated authors: *Kevin Krisciunas. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/users/morgan/MRO/home.page/Pubs.html -- 7.1 Кб -- 26.04.2006
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6. EPIC Related CAL Routines
Next: CAL_getHKwindows Up: Routines of the Calibration Previous: List of CCF Components Contents . ... CAL_getHKwindows . Procedure . ... Used CAL State Variables . List of CCF Components used . CAL_getAUXwindows . ... CAL_getBoresightMatrix . ... CAL_rawXY2mm . ... CAL_mm2rawXY . CAL_rawX2chipX . ... CAL_chipX2rawX . ... CAL_getBadPixelList & CAL_getBadPixelMap . ... CAL_mosCTIcorrection . ... CAL_getmosOffset . ... CAL_mosgainCorrect . ... CAL_getEventPatterns . ... CAL_getEbounds . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node44.html -- 17.9 Кб -- 20.09.2011
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7. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... Star Name: . GSC 02707-01173 . ... The new eclipsing variable star GSC 02707-01173 in the field of DM Cyg was discovered during cooperative observations of the latter variable star in the Astronomical Observatory of Odessa University and the Astronomical Observatory on Kolonica Saddle. ... The shape of the light curve indicates that the star is an EA eclipsing variable. ... Light Curve . Upper figure: The phased light curve of GSC 02707-01173 for 2008-2009. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1244693 -- 9.5 Кб -- 30.09.1971
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8. ETCs and Observations Simulation at the VLT
... Second, the observatory can control the configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. This paper presents the VLT object-oriented framework for the development of ETCs (Exposure Time Calculators) and data simulators. ... Instrument simulations are being developed for the purpose of predictive calibration, instrument configuration control, and evaluation of data analysis procedures. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P1-22/ -- 12.4 Кб -- 09.10.2000
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9. Restrictions on the Scenario Parameters
... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node41.html -- 6.6 Кб -- 26.02.1997
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10. A computer controlled low light photometer for nightglow observations
A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/~lapchuk/Photometer.htm -- 15.9 Кб -- 21.02.2000
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11. Multiwavelength Study of Mira Ceti-Type Variable Stars
... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/~gmr/miras.html -- 13.9 Кб -- 25.11.2015
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12. OptInt PmWiki : PmWiki / Debug Variables
OptInt PmWiki : Pm Wiki / Debug Variables . Basic Variables | Variables | ... EnableDiag . The following actions are available only if you set $EnableDiag = 1; in your configuration file. They can be used for debugging and should not be set in a production environment. ?action= ruleset . ... If you have a wiki that composes a HTML page from multiple pages, such as a normal layout with a sidebar, you'll get separate timings for each subpage and for the total page.) ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/PmWiki/DebugVariables?action=print -- 13.5 Кб -- 01.03.2014
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13. http://www.naic.edu/~astro/School/Talks/large_pdf/handson_ao2_2.pdf
... The Search of a pulsar Once the dedispersed time series is obtained, a Fourier transformation is performed. ... 2 Binary parameters The orbit of a pulsar , as well as any object, in a binary system is determined in its geometrical characteristics, space displacement and syncronised in time by the following parameters : Semimajor axis Eccentricity Longitude of periastron Binary period Time of ascending node a e PB T0 True spin period and observed spin period The ...
[ Текст ]  Ссылки http://www.naic.edu/~astro/School/Talks/large_pdf/handson_ao2_2.pdf -- 120.0 Кб -- 17.07.2005
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14. Pulkovo Observatory
. 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.
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/ -- 4.5 Кб -- 06.04.2009
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15. SAO RAS 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 ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/ -- 11.4 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/ -- 11.4 Кб -- 09.04.2016
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16. Science Innovations
. Сайт временно не работает.
[ Сохраненная копия ]  Ссылки http://www.sai.crimea.ua/ -- 1.9 Кб -- 17.05.2015
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17. http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf
High-resolution near-infrared speckle interferometry and radiative transfer modeling of the OH/IR star OH 104.9+2.4 D. Riechers1 , T. Drieb e2 , Y. Y. Balega3 , K.-H. Hofmann2 , A. B. Men'shchikov4 , and G. Weigelt2 1 2 3 4 Max Planck Institute for Astronomy, Heidelberg Max Planck Institute for Radioastronomy, Bonn Special Astrophys. ... The reconstructed visibility reveals a spherically symmetric, circumstellar dust shell (CDS) surrounding the central star. ...
[ Текст ]  Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf -- 428.8 Кб -- 05.05.2009
[ Текст ]  Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf -- 428.8 Кб -- 24.02.2010
[ Текст ]  Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf -- 428.8 Кб -- 24.02.2010
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18. RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, tabl
... Characteristic parameters of subsystems RR Lyrae field stars and globular clusters . ... RR Lyrae . ... 0.05 . ... lim R max , kpc . ... Z o , kpc . ... grad R [Fe/H], kpc -1 . ...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/paper7/p7tab1.htm -- 9.9 Кб -- 02.02.2007
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19. Program parameters
Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/Radio/red/searchdup/node2.html -- 8.0 Кб -- 30.06.2000
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20. http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf
... A star was observed at different zenith distances during one night at the Engelgardt's Astronomical Observatory in the program of atmospheric extinction study at blue. ... The determination of the star's brightness was performed with the method of photon counting. ... Variable star. ... The brightness of the variable star was measured occasionally during the other nights, and moments of maximal values of brightness (15.59m) were received on nights 2­5, the 2nd table. ... JD 2452805. ...
[ Текст ]  Ссылки http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf -- 173.2 Кб -- 03.12.2015
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