... Iiyama ProLite XU2590HS-B1 25, Черный, DVI, HDMI, Full HD 25, Черный, DVI, HDMI, Full HD.. ... title='Аксессуар AOpen HDMI 19M to Micro HDMI 1.8m ACG588-1.8M' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . ...

Aims: We study the structure of the medium surrounding sites of high-mass star formation to determine the interrelation between the H ii regions and the environment from which they were formed. ... Methods: We present new Herschel/SPIRE 250 ЮМm, 350 ЮМm and 500 ЮМm data of LHA 120-N44 and LHA 120-N63 in the LMC. We construct average spectral energy distributions (SEDs) for annuli centered on the IR bright part of the star-formation sites. ... The source N44 does not show a systematic trend. ...

... RSDC . ... Press Releases (rus) || in Russian RSDC Quick Jump 9-year Galactic survey Catalog of sources 7-year Galactic Bulge Map Cleaning IBIS/ISGRI sky images IBIS/ISGRI Sensitivity vs. ... The INTEGRAL view of the Galaxy . ... May 2012: 9-year Galactic plane survey . ... They are ISGRI (higher plane detector of the IBIS telescope), JMX1 and JMX2 - two detectors of the JEM-X telescope. ... RSDC is actively participating in the all-sky survey carrying out with INTEGRAL observatory. ... 2016 IKI RAN...

... Figure 1 shows the line positions of Al and Mn for CCD4 with EPN CTI 0014.CCF and EPN CTI 0015.CCF. ... XMM­Newton CCF Release XMM­ CCF ­REL­203 Page: 3 Mn­K position FF old and new 200 400 600 800 1000 revolution 1160 1170 1180 1190 1200 energy in ADU old new nominal position slope old 0.000126819 slope_ new 0.000133674 res effect at rev 1000 ( old ) [%] 0.0107547 res effect at rev 1000 ( new ) [%] 0.0113360 Mn­K position EFF old and new 200 400 600 800 ...

... Observatory . ... Science . ... Science Users Information > Science Publications > Science Announcements > Revolution in Astronomy with ALMA -- The Third Year . ... Observing Facilities . ... ALMA . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... Held in central Tokyo, the aim of this workshop is to highlight the science results from ALMA obtained during the first three years of science...

... Glyn Moody charts this rapid transformation in his book Rebel Code: Linux and the Open Source Revolution and tells how chance and fortune combined with the Internet and the availability of cheap processing power to make the impossible pos-sible. ... Netscape taking its Communicator 5 browser open source made people sit up. ... Unix [and Linux] always had that from the start, so it made it perfect for the open source/free software methodology even though that hadn't been invented yet. ...

... The models provided are: . abs - absorption of x-rays by neutral gas with solar abundances. parameter 1 = . ... parameter 2 = . ... normalization - logarithmic value of the flux density at 1 keV in units of keV cm -2 s -1 keV -1 . ... normalization - logarithmic value of the normalization of the gaussian in units of keV cm -2 s -1 . ... absorption ( params )* model ( params ) . ... A single value for the normalization (i.e., fixed normalization) will force the program to use that value. ...

. Album : asv-album :: Travels to distant places and countries :: 1998/05 Boston (USA) :: 4 Harvard . Up . << Prev . Revolution books shop . Next >> . Album created by album a tool by David Madison on Tue Jun 23 14:46:44 2015 .

Marconi Applied Technologies IMAGING PROVISIONAL CCD65 576(H) X 288(V) PIXEL IMAGE AREA 525 or 625 LINE FORMAT (INTERLACED) INVERTED MODE OPERATION (MPP) 20 X 30 µm PIXELS NOVEL PREAMPLIFIER FOR EXTREMELY LOW NOISE AT HIGH PIXEL RATES 100% ACTIVE AREA The next revolution in imaging is here TM Marconi Applied Technologies IMAGING The CCD65 uses a completely ... Number of Output Amplifiers 1 The device has a 100% fill factor for maximum sensitivity. ...

... User Guide ] Task: uvfit Purpose: Fit point sources to a given vis file. ... Key: stokes Normal Stokes/polarisation parameter (e.g. i,q,u,v,ii etc). ... Key: object This gives the object type that uvfit fits for. ... Key: fix This gives a set a flag parameters, one parameter per source. Each parameter consists of a set of letters, which indicate which source parameters of a component are to be held fixed. These source parameters are fixed by the initial estimates given by the `spar' parameter. ...

... 607L..33Bird+ J/ApJ/607/L33 First IBIS Catalog: 20-100keV (Bird+, 2004) ================================================================================ The first IBIS/ISGRI Soft Gamma-Ray Galactic Plane Survey Catalog. ... The outstanding IBIS capability to locate soft {gamma}-ray emitters has allowed us to identify most of the detected sources with already known Galactic X-ray binary systems, while 28 of the objects are of unknown nature. ... Count-rate in 40-100keV band 57- 60 F4.2 ct/s e_F40-100...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Quasi-stationary electron distributions for the different values of the particle escape time. ... The electron-cyclotron maser instability is widespread in the Universe, producing, e.g., radio emission of the magnetized planets and cool substellar objects. ... The model used takes into account the radiation escape from the source region and the particle flow through this region. ...

... 03.32 AM - the first impulse is performed using the Progress M1-5 eight thrusters to construct the pre-descent orbit. ... maximal distance from earth surface - 219 km . minimal distance from earth surface - 188 km . ... 05.00.24 AM - the second impulse is performed using the Progress M1-5 eight thrusters to construct the pre- descent orbit. ... 08.08 AM - the final third breaking impulse is performed using a combination of the Progress M1-5 main engine and eight thrusters to deorbit Mir OC. ...

Asteroseismology - the study of stellar oscillations - is a powerful tool to probe the structure and evolution of stars. In addition to the large number of newly discovered exoplanets, space-based telescopes such as Kepler have revolutionized asteroseismology by detecting oscillations in thousands of stars from the main sequence to the red-giant branch. In this talk I will highlight recent asteroseismic discoveries by Kepler, focusing in particular on exoplanet host stars. ...

... RC0133+0459 . ... RC0154+0459 . ... Radio source parameters . R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( B1950) Freq. Comp. ... Parameters of optical candidates for identification . ... B1950) Magn. ... Crosses mark radio source components ps . Last updated 19 Dec 2000 ...

First results of X/S and X/Ka-band catalog combinations with full covariance information Andreas Iddink , Christopher Jacobs, Thomas Artz, Axel Nothnagel 22.09.2014 First results of S/X and X/Ka-band catalog combinations with full covariance information Andreas Iddink ­ 22.09.2014 Motivation Features of the ICRF2 ICRF2 (Defining- Sources ) 3414 ... Step: Import of the X/Ka catalog with full covariance information (Data provided by Christopher Jacobs et al. ...

Hide Zen home . ... sncat2sntab.pl - convert old catalog to table sn . ... CREATE TABLE cats ( id integer PRIMARY KEY, name text ); -- a list of properties of galaxy CREATE TABLE properties ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy _property ( gid integer REFERENCES galaxy (id), pid integer REFERENCES properties(id), value float, UNIQUE( gid ,pid) ); CREATE t=# select * from galaxy; id | ...

I n 1705 Edmond Halley predicted, using Newton's newly formulated laws of motion, that the comet seen in 1531, 1607, and 1682 would return in 1758 (which was, alas, after his death). ... T he average period of Halley's orbit is 76 years but you cannot calculate the dates of its reappearances by simply subtracting multiples of 76 years from 1986. ... T he nucleus of Comet Halley is approximately 16x8x8 kilometers. ... The Return of Halley's Comet from the ASP . ... Comets .. Halley .. ...

Plans are under way to create a new way of performing non-interactive observations which will be called auto-observing . ... Non-interactive observing with CIMA has for a long time been available with the use of CIMA command files. Contrary to normal command file observing which requires a command file with a set of commands to be executed sequentially, auto-observing will use a list of sources and a list of instructions on how to observe each of the sources. ...

... Moon Story . ... There is a lesson in the poem, however: We on Earth always see the same side of the Moon because the Moon rotates exactly once and revolves exactly once in a month. ... see activity . ... children learn that the Moon is a sphere, and we always see the same side . ... why do we only see one side of the Moon? ... children learn that the Moon is always facing us because of its monthly cycle of rotation and revolution, and that the Sun affects how much of the Moon we see each night . ...