... Science . ... Science Users Information > Science Publications > Science Announcements . 10 Apr 2016 jump to navigation jump to content . ... ALMA . ... Observing with ESO Telescopes . ... Public Surveys . ... ESO-MIDAS . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... ESO Data Access Policy . ... Science Announcements . ... Published: 26 May 2014 . ... A brief description of the ALMA calibrator survey was recently published . ... Published: 23 Apr 2014 . ...

Еще в разделе: (Показать все результаты (>42009) - www.eso.org/ )

• ESO - Newsletter May 2014
• Different X-ray Spectra

... Archives . ... If you do not mind the time predictor, it is hard to believe that this is a light curve, time dependent data. ... It?s hard to say this data set is designed for time series analysis apart from the complication in statistical inference due to measurement errors. How to design the statistical study with measurement errors, huge gaps in time, and unequal time intervals is complex and unexplored. ... The following is R output without measurement errors. ... Chandra Blog . ...

Еще в разделе: (Показать все результаты (>3742) - hea-www.harvard.edu/ )

• The AstroStat Slog 2009 July
• The AstroStat Slog light curve
• The AstroStat Slog VO

. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .

Еще в разделе: (Показать все результаты (>177) - comet.sai.msu.ru/ )

... This calibration approach is recommended when dealing with high frequency data from the old ATCA correlator, especially at 3mm wavelengths. ... The approach described here exploits the dual frequency bands that were available with the old correlator. ... Rather the current approach assumes that you have a single Miriad dataset containing bandpass calibrator, phase calibrator, flux density calibrator and program source. ... MFCAL . ... Input multi-source, dual-band dataset. select=source(1921-293) . ...

Еще в разделе: (Показать все результаты (>13223) - www.atnf.csiro.au/ )

• VLBI Wiki | Main / LBALogs
• Southern Cross Astrophysics Conference Series
• Preprocessing for Selavy CentralProcessor 0.11 documentation

Next: Order Merging Up: Instrument Response Correction Previous: Using a Standard . ... It consists of a correction for the blaze function by using a suitable model of the blaze effect introduced by the echelle grating. ... This method uses the overlapping region of adjacent orders to estimate, in a few iterations, the parameter k of the blaze function which is, as before, assumed to be a sinc square. ... The method minimises the difference of the corrected orders in each of the overlapping intervals. ...

Еще в разделе: (Показать все результаты (>2007) - www.sao.ru/ )

• Echelle Spectra
• mod_version - Apache HTTP Server
• Multi-Processing Modules (MPMs) - Apache HTTP Server

... If some entries are missing, which might turn out later, add them in a way that the library remains downward compatible. (13aug97) XAW3D 3D widget library 1.3 . ... ASCII Art library 1.2 (by Hung-Chi Chu , aa.dll for XFree86, aa.dll.noX for non-X environments) . ... MPEG library 1.2.1 (by Hung-Chi Chu , DLL only ) . PNG library 1.0.2 (by Hung-Chi Chu , requires zlib , DLL only ) . TIFF library 3.4beta037 (by Hung-Chi Chu , requires zlib and jpeg , DLL only ) . ... Xpm 3.4k (by Hung-Chi Chu ) . ...

Еще в разделе: (Показать все результаты (>2056) - crydee.sai.msu.ru/ )

• Introduction
• Specifications

Peremennye Zvezdy", . ... GSC 4232-02515, NSVS 3147658, NSVS 3174760 . ... 14.2-14.9 (R, NSVS); . ... During observations of a secondary eclipse of GSC 04232-02830 (Goranskij et al., 2005) on August 8, 2007, we identified GSC 4232-02515 as a W UMa eclipsing binary. ... VAST software was used for aperture photometry. ... This method produces a light curve with an arbitrary zero point. ... Light Curve . Light curve of GSC 4232-02515 in NSVS magnitude scale. ... gsc423202515_kadar_nsvs.dat . ...

Еще в разделе: (Показать все результаты (>39495) - www.astronet.ru/ )

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

Еще в разделе: (Показать все результаты (>210) - ocl.sai.msu.ru/ )

... Since GCVS IV, there was no new GCVS edition. ... Main reasons for the automatic-survey new variables remaining outside the GCVS for a long time:  different level of detail of the classification systems, no perfect software for automatic classification available;  individual approach to each star that was always used in the GCVS cannot be applied any longer, but the experience of automatically- updated catalogs evidences for the number of errors ...

Еще в разделе: (Показать все результаты (>84) - sai.msu.ru/ )

... Since GCVS IV, there was no new GCVS edition. ... Main reasons for the automatic-survey new variables remaining outside the GCVS for a long time: •   different level of detail of the classification systems, no perfect software for automatic classification available; •   individual approach to each star that was always used in the GCVS cannot be applied any longer, but the experience of automatically- updated catalogs evidences for the number of errors ...

Еще в разделе: (Показать все результаты (>8123) - www.sai.msu.su/ )

• Sternberg Astronomical Institute
• Frozen Text Tutorial
• APOD: 2007 June 2 - 3D Full Moon

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

Еще в разделе: (Показать все результаты (>361) - lnfm1.sai.msu.ru/ )

... Data . ... In general, Dolphin finds good agreement with the Whitmore, Heyer, and Casertano results, and the longer baseline and more extensive data set used by Dolphin result in less scatter in the residuals. ... In these case the Dolphin corrections are larger than the Whitmore et al. corrections. ... Figure 1 shows the ratio of counts from a 14 second exposure of Omega Cen in August, 2000 to the counts in a 100 second exposure, vs. the Y position on the chip (WF2 in this case with gain=15). ...

Еще в разделе: (Показать все результаты (>13282) - www.stsci.edu/ )

• New Approach: Space Variant Hyperparameter
• FUV-MAMA Repeller Off as an Available Mode for High Resolution Spectroscopy
• COS Target Acquisition Strategies

... Of the 4 buttons in the bottom part of the configuration screen, three deals with power level adjustments: the 'Power control' button brings up the power control window where You can adjust the power levels of the different parts of the IF/LO system, the 'Power levels' button brings up the power level monitoring window (which also can be run outside CIMA as the 'powerwin' program), and the 'Adjust Mock power' button which adjusts the power levels on the Mock spectrometer (but nowhere else). ...

Еще в разделе: (Показать все результаты (>3058) - www.naic.edu/ )

• The CIMA Homepage
• Backends Available with CIMA
• The CIMA Observing Modes

... We used many different approaches and the resulting success grad was mixed. ... We use either mean processing time per input sample in ns, or the resulting sampling speed , in unit of 106 samples/s. # buffe r s 256 512 1024 1536 2048 # buffe r s 256 512 1024 1536 2048 # buffe r s 256 512 1024 # buffe r s 256 512 1024 ATI GPU F F T t i me ( 0.47 0.48 0.48 0.48 0.48 ATI GPU Read speed (GB/s) FFT time ( 2.69 0.58 3.52 0.58 3.96 0.58 4.24 0.58 4.42 ...

Еще в разделе: (Показать все результаты (>9294) - www.arcetri.astro.it/ )

• mod_version - Apache HTTP Server
• Multi-Processing Modules (MPMs) - Apache HTTP Server
• Apache IP-based Virtual Host Support - Apache HTTP Server

... International Astronomy Olympiad 2002 . ... The 7th International Astronomy Olympiad will be held on October 22-29, 2002 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) in North Caucasus. ... Authorized National Representative Astronomy Organizations (ANRAO) of the participating countries are authorized to form the teams of the Olympiad member-states. ... VII IAO . ... Information about the International Astronomy Olympiad 2003 will be known in the late 2002. ...

Еще в разделе: (Показать все результаты (>1046) - www.issp.ac.ru/ )

• III International Astronomy Olympiad, Problems to solve
• VI International Astronomy Olympiad: information available before
• VIII International Astronomy Olympiad: information available before

... Status of the numerical solutions and validation 2. ... Coupling of "solid" Earth components, e.g. core ­ mantle (Dehant et al.) ... Consistent relativistic formulation of Earth rotation (Gerlach, Klioner, Soffel) Status of the numerical solutions - 2 · The results from numerical solutions suffer from ­ Simplified solid Earth models ­ Incomplete Earth system models or neglecting of certain parts or neglecting of certain coupling mechanisms ­ Methodological limitations of computations...

Еще в разделе: (Показать все результаты (>288) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/personal/malkin/publ/zm10c.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm11d.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12n.pdf

. Where observers see Rosetta depends on their location. At 21:51 UT, 19 minutes before closest approach, viewers in London, Paris, Berlin, and Rome will see Rosetta in different parts of the constellation Taurus. More detailed finder charts are available here. Astronomy: Roen Kelly

Еще в разделе: (Показать все результаты (>5782) - www.astronomy.com/ )

• New high-resolution atlas of asteroid Vesta is available to the public |
• Does the time it takes different methods to create all the elements coincide
• Why do some stars appear to flash a variety of different colors when you look

. Previous slide . Back to first slide . View graphic version .

Еще в разделе: (Показать все результаты (>11142) - xmm.vilspa.esa.es/ )

• Errors
• Generation from In-Orbit Data

... There are a lot of computer codes simulating this scattering and freely available in the Internet (see e.g. links on our JPDOC page ). ... The code and input file are available in the directory . ... A slightly modified code of Barber Hill with a C-shell and input files is available in the directory . ... The code, input and test output files are available in the directory . ... See also readme file. file. ... The code, input file and their description (a TeX file) are available in the directory . ...

Еще в разделе: (Показать все результаты (>282) - www.astro.spbu.ru/ )

• Database of Optical Constants -- Level: welcome
• Database of Optical Properties -- Level: database
• Database of Optical Properties -- Level: subsubsubpage

This section of AMPLE enables one to make ephemeris calculations in various coordinate systems (spherical, rectangular) connected with different main planes (equator, ecliptic, horizon) and having origin in different points: geocenter, any point on the Earth surface, the Sun, any major planet, any minor planet. The choice of some minor planet as a center gives possibility to find approaches of the minor planet with any set of major planets and minor planets. ... equinox . 1950 2000 true . ...

Еще в разделе: (Показать все результаты (>536) - www.ipa.nw.ru/ )

• IAA GPS Analysis Center
• Keywords_279