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1. Imaging Performance of HST Compared to Future Ground-Based Adaptive Optics
... Simulations of a distant cluster of galaxies at z 2 are presented for the HST cameras COSTAR-corrected FOC, WFPC II, the Advanced Camera, and for an adaptive optics system that may equip a future 8-meter class telescope. ... Keywords: cluster of galaxies, simulations . ... Simulation of a Distant Cluster of Normal Galaxies . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/cauleta.dir/cauleta.html -- 3.0 Кб -- 15.04.1994
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2. See Spike Run... Run, Spike, Run
... It provides long range planning information to the scheduling team; it provides bright object, timing, and orientation information to the observation planning team; and it provides graphical description of the observations and their constraints. ... The GUI graphically displays the constraints that are computed by Spike and stored in the description files and in the database. ... BOAS processes all bright objects that have entered the database since the last time BOAS was run. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass00/P2-20/ -- 9.5 Кб -- 29.05.2001
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3. compare dlpf shapes
Jeff mock supplied 6 different types of filters to use with the high resolution mode of the mock spectrometer. ... Plots were made of the time domain voltage response as well as the frequency domain power response. A decimation of 10 was used for the filter decimation. this gave a filter length of 80 coeff. The plots compare the filter shapes for these filter types (.ps) ( .pdf ) . ... Each color is a different filter type . middle: spectral density reponse for each filter . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/hardware/pdev/pdevgain/lpdfTypesCompare.html -- 3.2 Кб -- 03.10.2013
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4. Image: Nijo castle, Shogun palace. The main building. Comparing to temples and
. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 20/08 Nijo castle (ancient shogun palace). Assembly opening. Maiko . Up . Nijo castle, Shogun palace. The main building. Comparing to temples and shrines, royal architecture looks modest. Next >> . Photo album generated by album generator from Marginal Hacks by David Madison on Tue Jun 23 14:46:11 2015 .
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/album/trips/1997.08.Japan/20.Nijo/tn/b34l.jpg.index.html -- 6.2 Кб -- 23.06.2015
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5. Generation from Ground Calibration Data
. Next: Generation from In-Orbit Data Up: EPN_ADUCONV Previous: Description Contents . Ground calibration data obtained from extensive measurements of X-ray emission lines and synchrotron lines (mainly flat fields). The gains of the individual readout nodes are derived by comparing the positions of the CTE corrected calibration lines (in ADU) with their energies. Michael Smith 2011-09-20
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node675.html -- 3.4 Кб -- 20.09.2011
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6. Bright prospects: Comparing the H Survey with large-scale radio continuum
... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Australia Telescope 20GHz Survey . ... Bright prospects: Comparing the H Survey with large-scale radio continuum emission . ... Prospects for comparisons between the AAO/UKST H \ survey and large-scale radio continuum emission are considered, with particular reference to the recently completed Parkes 2.4-GHz survey of the southern Galactic Plane. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/duncan/paper/index.html -- 52.4 Кб -- 08.04.2016
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7. Astronomy HyperText Book: Interstellar Medium
Photon Scattering: Basic Principle of Photon Scattering . Audio Narration is available . No Scattering: Photon Source and Detector . ... For optical photons, scattering goes as wavelength to the -4 power. In the case of blue photons compared to red photons, this means that blue photons are about 10 times more likely to get scattered than red photons. ... Watch the blue photons scatter away from the detector . ... Interstellar dust make stars appear redder than they really are . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/ism.html -- 4.2 Кб -- 23.01.1998
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8. ESO - Thesis Topic: Next generation Fornax Cluster surveys
... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Next generation Fornax Cluster surveys . ... Data Handling and Products . ... Science Data Products Forum . ... An international team, with Dr. Hilker as Co-PI, has started to gather wide-field optical and infrared imaging data as well as spectroscopic data on the whole extent of the Fornax cluster, mainly based on observations with ESO telescopes (VLT, VST, VISTA). ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/activities/thesis-topics/abstr-hilker04.html -- 27.3 Кб -- 10.04.2016
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9. PINTofALE EXAMPLE : Simulation for Chandra ACIS-I
... This thread uses PINTofALE to generate a simulated Chandra spectrum. ... define a DEM . ... pset marx .par ExposureTime=50000 OutputDir='sim_ marx ' \ ; GratingType='NONE' DetectorType=' ACIS-I ' SourceFlux=-1 \ ; SpectrumType='FILE' SpectrumFile='spec_ marx .dat' \ ; SourceType='POINT' DitherModel='INTERNAL' ; marx TSTART=2006.46 ; marx2fits sim_ marx / spec_ marx .evt ; dmextract infile= spec_ marx .evt[EVENTS][(x,y)=circle(4018,4141,10)] ; [bin pi=1:1024:1] outfile= spec_ ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PINTofALE/doc/EXAMPLE_Chandra.html -- 11.5 Кб -- 01.10.2012
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10. Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA
... ALMA . ... OOF software . ... Software . ... We present a framework for modelling atmospheric phase errors and their correction by both the fast-switching and water vapour radiometeric techniques. Notable features are simulating three dimensional turbulent volumes instead of flat phase screens, considering three representative configurations of ALMA and parametrisation in terms of phase fluctuations on a 300m baseline, allowing referencing to the site-testing interferometer data. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/alma/memo-turb.html -- 13.7 Кб -- 25.11.2009
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11. ISOGAL YSO Candidates (Abstract)
... The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by IRAS because of lower sensitivity or confusion problems. ... The main indications of the previous analysis are confirmed, but the criteria for selecting YSO candidates had to be revised to select only bright objects, in order to limit the contamination of the sample by Post-MS stars. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/igysocand/abstract.html -- 3.0 Кб -- 11.09.2007
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12. Space Research Institute (IKI) Seminar
... Future seminars . ... Asymptotic dynamo-wave models of solar magnetic activity " . ... In the framework of mean-field hydromagnetic dynamo theory we constructed an asymptotic model of traveling dynamo waves for the limiting case of strong generation (large magnetic Reynolds numbers). The 1D and 2D asymptotic WKB-solutions describe magnetic field generation in solar and stellar convective envelopes. ... inhomogeneity of turbulence) revealed from observable magnetic fields in solar active regions. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/galeev/abs_eng/e040121.htm -- 4.6 Кб -- 14.01.2004
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/galeev/abs_eng/e040121.htm -- 4.6 Кб -- 14.01.2004
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13. :: Generated By JQueryForm.Com
First Name . Last Name . ... A contributed talk . A poster . ... Tentative title of your oral contribution/poster . Required if ask for a Poster or Talk . ... Required if you are member of a collaboration . Short abstract of your oral contribution/poster . Required if you ask for a Poster or Talk . Options . ... Please select additional options . ... Please check the required fields. Powered by jqueryform.com . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/multispin16/form.html -- 12.0 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/multispin16/form.html -- 12.0 Кб -- 09.04.2016
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14. LPCBC: Abstract 2_35
... Electronic Raman scattering in Tl 2 Ba 2 CuO 6+ d : Symmetry of the order parameter, oxygen doping effects, and normal-state scattering. Abstract: . Single crystals of the optimally doped, moderately and strongly overdoped high-temperature superconductor Tl 2 Ba 2 CuO 6+ d (Tl-2201) with T c = 80, 56, and 30 K, respectively, have been investigated by polarized Raman scattering. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lpcbc/ABST/2_35.html -- 3.7 Кб -- 24.12.1999
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15. On the problem of high spectral resolution observations of faint objects
... December 21, 1997 . ... Advantages are briefly discussed of gaining in spectral resolution, which is accompanied by losses in signal level, as compared with the attempts to improve the accuracy of measurement of line parameters by means of rising the S/N ratio alone with increasing the exposure time. To partially solve the problem of observations of faint objects at the BTA a new design echelle spectrometer is proposed. high resolution spectroscopy . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/PFES/pan2.html -- 4.1 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/PFES/pan2.html -- 4.1 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/PFES/pan2.html -- 4.1 Кб -- 01.10.2012
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16. SNe related preprints
A comparative study of type I and type II supernovae . ... Sternberg State Astronomical Institute, Moscow, U.S.S.R. (Received 26 November, 1985) . ... No significant difference between SNe I and SNe II has been found in their radial distribution and frequency of outbursts in spiral galaxies. ... The radial distribution of type Ia SNe in spiral galaxies is only slightly steeper than the one for SNe II, while SNe Ib/c are more concentrated towards the central regions. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/sn/preprints/ -- 3.7 Кб -- 22.12.2007
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17. ADS Abstract Service Results
Find Similar Abstracts . ... The turbulent dynamo in astrophysics . ... Astrophysics . ... ASTROPHYSICS, DYNAMO THEORY, GALACTIC STRUCTURE, INTERSTELLAR MAGNETIC FIELDS, TURBULENCE EFFECTS, COSMIC PLASMA, COSMOLOGY, MAGNETIC FIELD CONFIGURATIONS, PLASMA TURBULENCE, SOLAR MAGNETIC FIELD, VORTICES . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/html/Z/biblio/80.6.html -- 5.8 Кб -- 29.05.1996
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18. A CS and NH3 Survey
... 205Anglada+ 0) and NH3(1,1) observations towards 172 different star forming regions (99 observed in both molecules) associated with H2O maser emission. We make a comparative study between the physical parameters obtained from the CS and NH3 spectra, and their relationship with the H2O maser emission. ... We find that both the CS and the NH3 lines are significantly wider in regions with H2O masers than in other regions. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/H2O_masers.html -- 2.8 Кб -- 18.03.2015
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19. Conference "Zeta Functions"
Organisers: Michel Balazard (CNRS, Laboratoire Poncelet) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics) . ... General Information . ... By comparing several restrictions of Siegel-Eisenstein series of degree 3, B.Heim recently found a remarkable (and somewhat mysterious) formula relating central values of triple L-functions to other critical values. ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/lifr/zykin/eng/zeta/talks/bocherer.html -- 4.1 Кб -- 30.06.2010
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20. Comparing files under SCCS control
. You can compare any two versions of a file that is under the control of SCCS with the sccsdiff command: /usr/sccs/sccsdiff -r version -r version s. filename . Using this command produces a line by line difference between the two versions of the file. Results are shown in the same format as that produced by the diff command. Examples .
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/utilities1/sccs_compare.html -- 2.2 Кб -- 17.01.1997
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