... If you requested Exabyte or DAT tapes in your Phase II proposal, STScI will mail you one or more tapes containing your data within a few weeks of your HST observations. ... 1 Any FITS reader should be able to read these files; however, GEIS (Generic Edited Information Set) is the standard format for analyzing all HST data other than STIS and NICMOS data. ... To read FITS files from your tape and write them to your disk, you can use the strfits task in IRAF/STSDAS. ... Mount the tape. ... cl> stsdas ...

... This chapter describes the Plug-in API functions that allocate and free memory as needed by the plug-in. Because plug-ins share memory space with Communicator, they can take advantage of any customized memory-allocation scheme the browser has. ... NPN_MemAlloc allocates memory from Communicator's memory space. ... NPN_MemFlush requests Communicator to free up a specified amount of memory if not enough is currently available for the plug-in's requirements. ... Allocating and Freeing Memory . ...

. Next: Output Up: Calling Parameters Previous: Calling Parameters Contents . TYPE . type of bad pixels that is requested from CCF (see CCF BadPix , section 4.4.5 for a description of allowed values) - optional . rawX0/rawY0 . optional starting location of the readout window of the mode . rawXsize/rawYsize . optional size of the readout window of the mode . Michael Smith 2011-09-20

Modules | ... Apache HTTP Server Version 2.4 . ... Several changes in 2.0 and above affect the internal request processing mechanics. ... There were a number of different code paths in the Apache HTTP Server 1.3 to attempt to optimize subrequest or redirect behavior. ... The Request Processing Cycle . The Request Parsing Phase . ... If a module doesn't pass generated requests through this code, the author is cautioned that the module may be broken by future changes to request processing. ...

... SCHED STANDARD OBSERVING BANDS ---------------------------------------------- Center BAND Frequency(1) Bandwidth '90cm' 330.49 0.0 '50cm' 610.98 0.0 '21cm' 1465.49 128.0 '21cm' 1435.49 64.0 '21cm' 1416.49 0.0 '18cm' 1658.49 0.0 (2) '18cm' 1653.99 0.0 (3) '13cm' 2295.49 0.0 '6cm' 4990.49 0.0 '4cm' 8415.49 0.0 '2cm' 15285.49 0.0 '1cm' 22235.49 0.0 '24ghz' 23800.49 0.0 '7mm' 43135.49 0.0 'sx' 2295.49 and 8415.49 0.0 ---------------------------------------------- 1. ... Most 18 cm observing. ...

... Science . ... Science Users Information > Science Publications > Science Announcements > Call for Proposals for Period 97 . ... Observing Facilities . ... Observing with ESO Telescopes . ... The Call for Proposals for observations at ESO telescopes in Period 98 (1 October 2016 - 31 March 2017) has been released. ... Changes to the A & B scientific categories: The B9 category entitled "AGN host galaxies" has been renamed and moved to A9, at the request of the ESO Observing Programmes Committee (OPC)....

... 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. ...

Apache 1.1 and earlier let modules handle POST and PUT requests by themselves. The module would, on its own, determine whether the request had an entity, how many bytes it was, and then called a function ( read_client_block ) to get the data. ... This step also sends a 100 Continue response to HTTP/1.1 clients, so should not be called until the module is *definitely* ready to read content. (otherwise, the point of the 100 response is defeated). ... Finally, call ap_get_client_block in a loop. ...

... The Arecibo telescope upgrade is now nearing completion and we anticipate a resumption of tracking-mode observations for the carriage house, possibly as early as the second quarter of 1997. Therefore we are calling for the first round of observing proposals to use the 430- and 47-MHz carriage house instrumentation. ... 1) Obtain a cover sheet. This can be accomplished by either sending an empty e-mail to cover@naic.edu or by sending a request letter to the address given below. ...

... Up: Iraf Packages . ... IRAF Group, NOAO 1 , PO Box 26732, Tucson, AZ 85726 . This paper describes a new IRAF spectroscopy exposure time calculator. ... SPTIME takes an input source spectrum, either a reference blackbody, power law, or a user spectrum, a background ``sky'', observing parameters such as exposure time, central wavelength, seeing, airmass, and moon phase, instrument parameters such as aperture sizes and detector binning, a description of the spectrograph, and desired output. ...

Spacecraft ephemeris , or more generally, location of an observer, given as a function of time. ... The ephemeris data for spacecraft and target bodies are normally combined in a single file called the SPICE SPK file. ... Attitude data is contained in the SPICE CK file. ... Several miscellaneous kernel files - spacecraft clock (SPICE SCLK file) and leapseconds (SPICE LSK file) - are also part of SPICE; these are used in converting time tags between various time measurement systems. ...

. ОГЛАВЛЕНИЕ . Предисловие к четвертому изданию . Введение . § 1. Предмет и задачи астрономии . § 2. Подразделение астрономии . § 3. Возникновение и основные этапы развития астрономии . § 4. Практическое и идеологическое значение астрономии