... The SMS program is a critical endeavor to investigate whether the predictions of standard cold dark matter cosmology are consistent with the observed matter distribution in the Milky Way halo. It is the deepest, most extended search for optically elusive dwarf satellite galaxies and tidal streams to date, covering the entire Southern hemisphere. ... However only a few dwarf satellites have been found around the Milky Way to date - 22 dwarfs compared to 500-10,000 predicted by theory (Klypin et al. ...

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• COALA - Computational Astrophysics Laboratory

... Authors: R.I. Hynes, E.L. Robinson . ... Authors: S.P. Ellingsen et al. arxiv:1201.5424 Практически все кеплеровские кандидаты в многопланетные системы действительно имеют планеты (Almost All of Kepler's Multiple Planet Candidates are Planets) . Authors: Jack J. Lissauer et al. arxiv:1201.4413 Природа GRB 051103 по данным LIGO (Implications For The Origin Of GRB 051103 From LIGO Observations) . Authors: The LIGO Scientific Collaboration . ... arxiv:1201.2189 Свойства холодных KOI: III. ...

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Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Amplitude Distribution
• Initial binary parameters
• Test of the Initial Mass-Ratio Distribution

The spectrophotometrical complex of the 6-m telescope in Nasmyth-1 focus . ... A new sample of 360 blue compact galaxies with a strong star formation was build on the base of the Second Byurakan Survey. ... More that 20 galaxies with the extremely low-abundances of heavy elements in the range of 1/30-1/10 of the Sun's one, were found. ... During the 15-years observation term near 500 spectra of the unique source SS~433, from which the relativistic jets were found for the first time, were obtained. ...

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• THE 4.85 GHZ NORTHERN SKY CATALOG
• SEARCH for the YOUNGEST GALAXIES
• Corrections to the probability distribution

My main field of interest is modelling dust extinction and emission in the disk of spiral galaxies. Radiative transfer simulations are compared to optical, FIR and sub-mm observations to assess the dust mass, distribution relative to star and optical/emission properties. ... I'm also interested in the formation, evolution and survival of dust grains in high-redshift objects, and in comparing the extinction / emission properties of dust with observations of distant sources. ...

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• Arcetri Solar Physics Group - Corona and Solar Wind
• The CHIANTI atomic database
• LASG - Distribution specific information

... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . Dept. for Space Plasma Physics . Dept. for Physics of Minor Celestial Bodies . Dept. for Physics of Planetary Systems . Dept. for Solar Physics . ... 2016,MNRAS, 2016MNRAS.tmp.. ... WASP- 22, WASP-41, WASP- 42 and WASP- 55. ... in the visible range - land 10th Keck (USA), 2 x 8.4-m LBT (USA), 8.0-m Gemini (USA), 6.5-m MMT (USA), 4th KPNO (USA), 3.5-m APO (USA), 8.2-m VLT (ESO), 3.5-m NTT (Chile); . ...

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• Dept. for Physics of Stars&Galaxies

Radiative Bhabhas in the IFR Nick Blount David Strom Babar Collaboration Meeting December 7, 2004 Table of Contents 3. ... Predicted Bhabha rate 5. ... Back of the envelope calculation of neutron hits in the IFR 7. ...

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• http://zebu.uoregon.edu/~uochep/talks/talks04/ts.pdf
• The Galaxy Gallery Page VII: Infrared Imaging
• Evidence for Dark Matter

We present a database of UV-to-FIR data of 83 nearby starburst galaxies. ... The NIR data are from new observations obtained at the NASA/IRTF and the Mount Laguna Observatory, combined with the published results from observations at the Kitt Peak National Observatory. ... In conjunction with IRAS and ISO FIR flux densities, all these data form a set of observed spectral energy distributions (SEDs) of the nuclear regions of nearby starburst galaxies. ...

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• The Spectral Energy Distribution and Mass-Loss Rate of the A-Type Supergiant
• HERschel Observations of Edge-on Spirals (HEROES). I. Far-infrared morphology
• SODRM Statistical Summary 2012

Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...

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... Archives . ... ArXiv] SVM and galaxy morphological classification, Sept. 10, 2007 . ... On the Metallicity-Color Relations and Bimodal Color Distributions in Extragalactic Globular Cluster Systems by M. Cantiello and J. P. Blakeslee . Many observations on globular cluster systems (GCS) show bimodal distributions in color and metallicity space. ... Based on their simulation study, (V-H) and (V-K) are confirmed to be good colors for revealing unbiased bimodal metallicity distributions in GCS. ...

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• Spectral Energy Distribution: Microquasar LS 5039
• Why Spectral Energy Distributions?
• Comments on: chi-square distribution [Eqn] By: Alex By: vlk By: aneta By: aneta

The IAA RAS . ... View details . ... Observatories 'Svetloe' and 'Zelenchukskaya' participate in frequent VLBI-observation sessions organized by the International VLBI Service for Geodesy and Astrometry . ... As part of collaboration with the U. S. Naval observatory in the areas of EOP determination and analysis the USNO uses IAA RAS daily EOP data obtained from SLR and VLBI. ... The IAA RAS and the Centre National d'Etudes Spatiales carry out joint DORIS observations on the Badary observatory. ...

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• Keywords_262
• Laboratory of minor bodies of Solar system
• Keywords_88

. Next: Related Programs Up: INSTALLING, AND RUNNING SCHED Previous: Running SCHED on a Contents . Once SCHED has been used to make schedules for an observation, those files need to be sent to the stations, usually by way of a distribution center at NRAO or in Europe. When time for a project is allocated, instructions for how to accomplish this will be provided. Craig Walker 2014-04-14