DISCLAIMER: The larger the aperture, the more light a telescope will gather and the fainter the object you can see. Here is a range of magnitudes you might expect to see. Given excellent sky conditions and good optics, a well trained eye can sometimes add up to 0.8 magnitude to these values. Limiting Magnitude depends on much more than the instruments aperture. ... One formula is for aperture in inches the other is for aperture in millimeters. ... Aperture (inches) . ... 15.2 . ...

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The Keep-Alive extension to HTTP, as defined by the HTTP/1.1 draft, allows persistent connections. ... Apache 1.1 comes with Keep-Alive support on by default, however there are some directives you can use to modify Apache's behavior: . Note : Apache 1.2 uses a different syntax for the KeepAlive directive. ... Default: KeepAlive 5 . Context: server config . ... This directive enables Keep-Alive support. ... In order for Keep-Alive support to be used, first the browser must support it. ...

... During all period of our investigations Dr. N.Sumzina from the Institute of Applied Astronomy of RAS had prepared the Numbered Minor Planet positions from MPC Database for our processing with kind permission of the Director of Minor Planet Center Prof. Braian Marsden. ... Our extensive processing of the MPC data allows us to conclude that CCD observations of the Numbered and Unnumbered Minor Planets have the errors, sometimes very crude. ...

... Space flight . ... Zero Gravity . ... The airplane volume (3,4m У 3,2m У 14.1 Л), as well as the payload of experimental equipment, allocated in the laboratory compartment, advantageously single out our airplane from the similar ones in the world. The results of tests and experiments are registered by the standard on-board aircraft systems and additional test- and measuring equipment of the customer. ... Length of the airplane . ... Flight duration . ... Auxiliary Radio Communication Equipment: . ...

Nova 1998 2 in M31 this image of the second Nova in M31 in 1998, was made from 38 exposures of 45 seconds integration time. It was made at September 21, 22h 20m UT. Telescope was a CG11 at f/6.3, no filters were used. The long list of processing steps caused the artefacts at the overexposed center of the galaxy and in many of the brighter stars. During the exposures thin clouds covered the sky but the CCD cuts through them, allowing me to obtain this result. ...

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. Yu.A.Shokin . Accurate positions of variable stars in the western part of the Large Magellanic Cloud bar . (published in IBVS and SAI Proceedings ) . B.S.Vozdvijenski, N.P.Gorbatko, V.A.Yeliseev, G.V.Romanova . The results of the observations of the selected minor planets in Sternberg State Astronomical institute . (published in SAI Proceedings ) .

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