... Kicks ass -I love it sooooooooooooooooo -Michael Krause nosun2.zip: second of this series: the space ship at the end of nosun (oh, so that's what it was) nosun3.zip: wad of the day at Macdoom -I'm sorry but this level is just to cool. superb - Elf66 >dk.zip: dk.wad, a high quality fortress level< !This last zip was postponed. ... THE BEST WADS: Darkcvnt.wad. By keith phipps Cabal*.wad By Sverre Kvernmo MEANT TO BE PLAYED SEPERATELY FROM NOSUN 1-4!! ... Check out his "Blakgate.wad" It kicks ass. ...

WCSLIB љ 5.15 . ... WCSLIB 5.15 and PGSBOX 5.15 . Example code, testing and verification . ... twcs tests closure of wcss2p() and wcsp2s() for a number of selected projections. twcsmix verifies wcsmix() on the grid of celestial longitude and latitude for a number of selected projections. ... Closure has been verified at all test points for SUN workstations. ... Although tests for closure help to verify the internal consistency of the routines they do not verify them in an absolute sense. ...

... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...

... The routine processing of STIS data in the calibration ``pipeline" requires an interrelated set of software tasks and databases developed and maintained by many groups at STScI. We present the systems-level design of this calibration pipeline from the perspective of the STIS instrument group at STScI. We describe the multiple interfaces to the pipeline processes that the STIS group works across in an effort to provide for the routine calibration of STIS data. ... For example, the STIS group: . ...

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

... It can perform any or all of the following variability tests on the light curve to determine whether the source is variable, however if insufficient good bins remain, no variability tests are carried out. a Kolmogorov-Smirnov test carried out either on: the cumulative probability functions of the observed count distribution and the observed background distribution; or the cumulative probability function of the observed net count distribution and the cumulative time distribution. ...

... the results for the runs whose output rms was close to the optimum value (.ps) ( .pdf ) . ... See radar datataking with pdev for a description of how the datataking works. 4 bit data was taken with different input rms voltages, decimations, and shifts. ... For those runs with 4bit rms close to optimum, the results were displayed as well had plots of the average bandpass. 31 different runs were made. for each run, the rms from the scope was recorded . ... Top: input rms voltage measured at scope . ...

The XPA source code directory contains two test programs, stest.c , and ctest.c that can serve as examples for writing XPA servers and clients, respectively. ... The stest program can be executed with no arguments to start an XPA server that contains the access points: xpa, xpa1, c_xpa (containing sub-commands cmd1 and cmd2), and i_xpa. ... xpaset xpa # send to xpa cat xpa.c | xpaset "xpa*" # send to xpa and xpa1 xpaget xpa # receive from xpa xpaget xpa* # receive from xpa and xpa1 etc. ...

... Keywords: globular clusters,M3,photometry,HST . ... Perform the most accurate test of the ``stellar clock'' used in dating globular clusters. ... These data will provide the first complete sample of post-main sequence stars over the entire area of the cluster, and will allow the most stringent tests of stellar evolution and dynamics models. ... M3 contains the largest population of Blue Straggler Stars (BSS) detected in a globular cluster so far ( ). ...

Next: TESTB/CCD Up: CCD Test Commands Previous: Purpose . The quality control can be done by six test commands in the MIDAS CCD context. The commands are called TESTX/CCD where X can be: B for the bias, D for dark, F for flat, T for transfer, S for shutter, and C for charge transfer efficiency. All output ( i.e. ASCII and MIDAS tables, postscript files of graphics and display output) will be put in the users working directory. ... TESTB/CCD . ... Tue Mar 28 16:52:29 MET DST 1995 ...

... A bright flare-up of emission (>1000 Jy) was found in OH-maser source during tests of 18cm receiver in observations with Kalyazin 64-m radio telescope (August 2004). ... Appendix (The list of used acronyms) ASC Cold Plate DC Astro Space Center of Lebedev Physical Instutute cooled LNAs and antenna feed hermetic device container (part of payload ); it contains Formatter, Rb oscillators, synthesizer, control unit and is placed under dish DM Device Module = DC + H-maser EGSE ...