Most of these images were obtained by Mike Bessell, Michelle Buxton, Hwankyung Sung, Ralph Sutherland and Bob Watson at SSO using a 2Kx2K Site CCD behind a Nikon or Hasselblad lens or directly on the 1m telescope. A few images are from the Hubble Space Telescope. Some of the M42 images were obtained with the KPNO 1m and ESO NTT telescope. One image is a mosaic of IRAS images. ... Details of the CCD imaging program at MSSSO. ... antenna.jpg (53KB) . ... ngc6744.jpg (59KB) . ...

. Main Page . Space flight . Crew training . Airshow . Zero Gravity . Hydrospace . Centrifuge . Simulators . Survival . Piloting . Baikonur . Order . Space camp . Space Hotel . "Odyssey" . "Parus" . "Tros" . "Zerkalo" . Photos . On-line Data . We in press . Services / Baikonur: General description Technical description Shedule of launches Photo gallery Price . Info: Industry news On-line Data Company ATLAS news Events We in press Contact . Copyright 2000-2016 ATLAS Aerospace . Old version of site .

... 2010 . ... The following images are mosaics obtained on 03 August 2010 at the National Solar Observatory/Dunn Solar Telescope with the Interferometric Bidimensional Spectrometer (IBIS). ... The final images are approximately 238 x 242 arcseconds, or 4 x 4 arcminutes, with a pixel scale of 0.0976 arcseconds per pixel. ... The images show a broad range of typical chromospheric structures, including sunspots, superpenumbra, plage, filaments, and quiet internetwork. ...

... Астронет | Картинка дня | ... планета Астронет | ... Астрономическая картинка дня . ... Около равноденствия магнитное поле Земли ориентировано так, что создаются благоприятные условия для взаимодействия с солнечным ветром, которое и вызывает прекрасное северное сияние. ... Полярные сияния и магнитосфера Юпитера . ... Слегка сжатое магнитное поле словно через воронку несет заряженные частицы к полюсам Юпитера, опуская их прямо в его атмосферу. ... Туманность Пузырь крупным планом . ...

... The Great Nebula in Carina . ... Eta Carinae , the most energetic star in the nebula, was one of the brightest stars in the sky in the 1830s, but then faded dramatically. Eta Carinae is the brightest star near the image center, just left of the Keyhole Nebula . While Eta Carinae itself maybe on the verge of a supernova explosion, X-ray images indicate that much of the Great Carina Nebula has been a veritable supernova factory . Tomorrow's picture: open space . ...

. Next: FSRQs Up: THE DEEP X-RAY RADIO Previous: Redshift Distribution . DXRBS' unique combination of a dual X-ray/radio survey method and high sensitivity has opened up important, large new regions of parameter space for both blazar sub-classes, within which a large fraction of our sample (nearly 50%) lie. This section is devoted to discussing these discoveries and their impact upon our understanding of the blazar class. љ . FSRQs . BL Lacs . Paolo Padovani . 1/5/1998

... The table is used/accessed by: . CAL_getHKwindows() : Table with HK parameter validity data; data outside the given validity intervals may indicate degraded science quality and ought to be screened in the pipeline reduction by means of GTI filtering . ... 5-character short ID of parameter as found in the ODF HK data (e.g. F1123) . ... validity interval of the parameter in the form of a valid selectlib expression; '@' characters may be used instead of the parameter name; e.g. @ in [-91.0:-89.0] . ...

... Abstract Given a sample time string, create a time format picture suitable for use by the routine timout_c . ... Detailed_Input sample is a representative time string to use as a model to format time strings. lenout is the allowed length for the output picture. ... This routine allows CSPICE users to supply a sample time string from which a corresponding time format picture can be created, freeing users from the task of mastering the intricacies of the routine timout_c . ... Link to routine source ....

9th of May 2015 . GASS III, Parkes Galactic All Sky Survey, new data release . by Peter Kalberla Urmas Haud . A new version of the Parkes Galactic All Sky Survey (GASS) is available at arXiv:1505.01011 (Kalberla Haud 2015). ... The channel map, displayed above, shows as an example a clean picture of the large scale Galactic HI emission at a velocity of 4 km/s. Brightness temperatures T B . ... today * ATNF | Parkes | ...

... 19-Jan-2013 12:53 . ... 2.8K . ... 11K . ... 10K . ... 15K . Apache/2.2.15 (CentOS) Server at rp.iszf.irk.ru Port 80 ...

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

... 07-Dec-2015 13:17 . ... 14-Jan-2011 11:40 . ... 06-Apr-2016 08:30 . 111K . ... 106K . ...

Next: File Formats Required Up: OPTOPUS Commands and Previous: Optopus commands . Below follows a description of all parameters that can be set by the SET/OPTOPUS command, the commands which use these parameters and the default values. ... If an OPTOPUS command the default value is not used the command will, in addition to actual OPTOPUS operation, also overwrite the setting of this parameter and hence will change the default value. ... set the equinox . ... Table: Command parameters . ...

The MOD and IOPT parameters value depend of the external magnetic field model (MOD), used during magnetic mapping and IOPT version (IOPT = Kp + 1), see the table: . MOD . External model . IOPT range . ... N.A.Tsyganenko, Planet. Space Sci., ... N.A. Tsyganenko, A magnetospheric magnetic fields model with a warped Tail current sheet: Planet. Space SCI., ...

. Progress of the RadioAstron Project in Pictures . Basic Information . Spacecraft Design . Orbit . Space Radio Telescope . Multi-Frequency Synthesis in K-band . Data and Phase Links . Ground Support of the RadioAstron . Observations . Data Processing . Status of the Mission . Progress of the RadioAstron Project in Pictures . back to top .

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

... Bad Astronomy . Misconceptions . ... I have a fun video on how to stand an egg on end on my blog at Discover Magazine . ... At the end of the show, one of the characters looks up the words "egg" and "equinox" on the web... and says it sent him to "thingsthatarewrong.com". ... Bad Astronomy : Only on the day of the Vernal (spring) Equinox, can you stand a raw egg on its end. Good astronomy : If you can stand a raw egg on end, it has nothing to do with the Equinox. ... 2008 Phil Plait. ...

. Next: Participants Up: Front Cover Previous: Preface . љ . Figure 1: Conference Participants . љ . Figure 2: Some of the participants enjoying the relaxed Mediterranean atmosphere . Norbert Pirzkal . 1998-07-09

... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...