... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

. Remote Access to Northern Hemisphere Telescopes . Roll Roof telescopes . Shared Skies image archive . Restricted Access . Observatory site camera . Live night sky camera . CDK20N video server . CDK20N telescope power control . Observing Conditions . Observatory weather . Observatory sky background . Regional weather . Clear Sky Clock for Moore Observatory . Coordinated Universal Time . Local time . Last update: June 21, 2012 . kielkopf at louisville edu .

Control the truss lamps: calibration lamps mounted on the secondary cage. Press a button to immediately toggle the state of the associated lamp. The control background color will change to pink (or the "Bad Background" preference) until the lamp has changed state. ... So if you want to use TUI to monitor or control the truss lamps, make sure that all users control the lamps via TUI! ... If the lamp controls say "Rebooting" then you should wait until the tlamps controller finishes rebooting. ...

Pulkovo NEO Page . ... Instrumentation and Observations . ... This Windows application serves for determination of spherical coordinates and magnitudes of the objects. ... The objects coordinates are referred to the system of chosen star catalog. ... 2. choice of reference stars with mouse, . 3. measurement of rectangular frame coordinates of objects and reference stars taking account of predefined background parameters, . 4. calculation of the spherical coordinates of objects. ...

. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:

C C C C C C lass lass lass lass lass lass 1 2 3 4 5 6 Introduction, Background Solar System Stars Galaxies Cosmology Special Topics Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light T lescopes e 1. ... Kirchoff's Laws trum Emission Line Spectrum 2. A low-density, hot gas emits light whose spectrum consists of a series of bright emission lines. ... Absorption Spectrum 3. ...

... Report on Cosmic Call 1999 . ... Cosmic Call Sessions . ... This Report outlines methodology, hard- and software, which were developed to transmit first public Interstellar messages from Evpatoria Deep Space Center (EDSC), and describes four Cosmic Call Sessions, which were fulfilled in EDSC on May 24 and June 30 - July 1, 1999. ... Each Cosmic Call consists of two parts. ... Dutil Message, . ... The software for gathering all messages and creating the Cosmic Call stream, was written on C language. ...

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arxiv:1307.8241 Кривая вращенияи распределение массы в центре Галактики --- от черной дыры до самых до окраин (Rotation Curve and Mass Distribution in the Galactic Center --- From Black Hole to Entire Galaxy) . Authors: Yoshiaki Sofue . ... Authors: D. Thornton et al. arxiv:1307.2944 Архив экзопланет NASA: Данные и инструменты для экзопланетных исследований (The NASA Exoplanet Archive: Data and Tools for Exoplanet Research) . ... обзор arxiv:1307.0041 Галактическая археология. ...

... The 99 files presented here contain 21 cm HI emission contours around 98 Super Nova Remnants (SNR) in the - V coordinates. ... SNR's were selected mainly from the List of Green (2001) [4] and from some other papers with angular diameters more than 10' and morphological type in continuum emission - S (shell). Four files each contain two objects (these objects have near declinations). ... b) emission of structureless medium, . ... Astrophys. ... Gosachinskij I.V., Bull. ... Gosachinskij I.V., Astr. ...

The Equatorial Inertial (GEI) coordinate system: . The X GEI axis is directed to the point of the spring equinox, . The Z GEI axis is coincide with the Earth's rotation axis, . The Y GEI supplements the right three. The Geographic (GEO) coordinate system: . ... The Solar Magnetic (SM) coordinate system: . ... About space physics coordinate transformation see Russel [1971] and Hapgood [1992] . ... M.A. Hapgood , Space physics coordinate transformations: A user guide // Planet Space Sci. ...

The new view on the population of Galactic open clusters A.E.Piskunov1, N.V.Kharchenko2, S.RЖser3, E.Schilbach3, R.-D.Scholz4 1 2 3 4 Institute of Astronomy, Moscow, Russia Main Astronomical ... Observatory, Kiev, Ukraine Astronomisches Rechen-Institut, Heidelberg, Germany Astrophysikalisches Institut Potsdam, Germany What are open clusters and what do they teach us Groups of Population I ... Cluster complexes: OCC-1 = Gould's Belt cluster complex? ...

JSC History . ... NASA History . ... Search . ... Most of these publications were published by the Government Printing Office as Special Publications in the 4000 - history series. For a listing of all NASA history publications available go to the NASA History Office publications page ( http://history.nasa.gov/publications.html ) . ... Researchers are encouraged to utilize these databases to expedite their research requests and narrow their focus for available materials. ... History Search Index . ...