Title : SERENITY II aka ETERNITY (v1.1) A full replacement for the second episode of Doom (which means there are 8 levels - sorry, no bonus level in this one, but you won't miss it.. ... Description : This set of 8 levels has been made with the word quality in mind. ... New Music : Yes (Doom 1.2 and earlier only 8-( (Doom 1.666 crashes on level 3 when you play it WITH the new music.. ... Level 8 Description : "Serenity Forever" This level is a farewell to Eternity, but also a hello to Serenity. ...

... Archives . ... When it comes to survey, the first thing comes in my mind is the census packet although I only saw it once (an easy way to disguise my age but this is true) but the questionaire layouts are so carefully and extensively done so as to give me a strong impression. Such survey is designed prior to collecting data so that after collection, data can be analyzed according to statistical methodology suitable to the design of the survey. ... Chandra Blog . ... SAMSI AstroStat Prog. ...

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. ...

The INS Master Schedule is used to track the "project-level" work being done by people in the INS Division. ... The current schedule shows each task as a light blue bar with progress indicated by a black bar partially overlaying the task bar. ... In this version, the current schedule is denoted by light blue bars for each task, work progress by the dark blue bar overlaying the current schedule bar, and the baseline schedule is indicated by a gray bar immediately below the current schedule bar. ...

... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...

... Clearing the library. Note the different flooтАж . Sidebar Left . Sidebar Top . ... Title: Clearing the library. Note the different floor levels. There were at least 4 different levels of underfloor in the library. Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ...

... Since the invention of the telescope over 400 years ago, they have been built in many shapes and sizes, and for many different uses. Not many people know this, but the first telescopes were created by the Dutch around 1600 and were used to spot far-off enemy ships. Back then, telescopes were called БЂњlooking glassesБЂќ. ... With his telescope, Galileo became the first person to see many amazing features of our Solar System, including craters on the Moon and Jupiter's four largest moons. ...

Fasti is an innovative design for infrared detector control. ... to use largely accepted standards as boundaries, as a PCI bus, a parallel interface or a serial, and to use few of them . ... The building blocks of Fasti are: . ... the serial bus for controlling housekeeping devices (temperature and pressure sensors or motor controllers) and programming data acquisition . ... Though not so fast, and lacking some forms of data integrity check, this bus is so widely used to be nearly unavoidable. ...

... As I mentioned at the recent Groningen international SKA meeting, there is a need for a large-area multi-beaming demonstrator for at least two reasons. ... The LOFAR instrument, to operate in the frequency range 10-250 MHz, will contribute vital information to the design and operation of a new class of multi-beaming telescope. ... The different operating frequency range also means that LOFAR cannot illustrate the scientific potential of area re-use (multi-beaming) in the cm-wave band. ...

... Welcome to the ADLab home page! Advanced Design Laboratory of the Special Astrophysical Observatory is concerned with research on low light level imaging and development of scientific digital imaging systems. About ADLab . ... Current project "A New Generation Multipurpose CCD Controller" . Project Contents . ... Publications on the Project . ... Other Web Sites of Interest . Created: 24 March 1998 . ... people have visited our web site. ... Copyright 1998 Advanced Design Laboratory. ...

... Meta Index / Home Page This program is designed to allow a user to recompute the photometry of one or more sources in an OM product source-list file, in one of several different ways, using specified parameters. ... This can significantly increase the accuracy of the photometry in the case of sources with one or more close neighbours. ... For the case of FAST mode data, omlcbuild uses the PSF to compute the photometry and obtains the background from pixels surrounding the source from. ...

... It includes level converters and a optional radio modem designed to decode the radio timecode signals transmitted by the Canadian time and frequency station CHU. A complete set of schematics, PCB artwork, drill templates is in the pub/ntp/gadget.tar.Z file on ftp.udel.edu. ... One of these converts a TTL positive edge into a fixed- width pulse at EIA levels and is for use with a timecode receiver or oscillator including a TTL PPS output. ... See the schematic diagram gadget.s01 for reference. ...

Nalini Chandra & John Percy, University of Toronto . ... Some works to refer to when using multicultural astronomy in your classroom: . ... Nalini Chandra is a doctoral candidate at the University of Toronto in the Department of Curriculum Teaching and Learning at OISE/UT. ... OISE-University of Toronto . ... John Percy, Professor of Astronomy at the University of Toronto, is a Past President of the ASP, and is active in astronomy education at all levels. ... ASP Multicultural Astronomy Resources . ...

. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .

Astronomical Data Analysis Software and Systems XIII ASP Conference Series, Vol. ... Skysoft is a YAASD (Yet Another Astronomical Software Directory), but with a different overall approach. To be useful, Skysoft needs to be a long­lived pro ject, setting little pressure for maintenance, imposing a very low nuisance level to the developers community, and requiring a lowmaintenance cost. ... This site is designed so that software developers acquire more visibility because of astronomical context. ...

Computers become more and more popular nowadays. That means that the amount of people who are able to work with computer programmes and play computer games has increased. In many cases computer games are the only thing that a person is accustomed to. ... As a result of this epidemic "homo playing" may put on the isoreality helmet which makes a person, crazy about games, forget about food, slumber and all other components of real life: "homo playing" becomes isolated from community. ...

Catalogue of designations . HyperLeda home | Documentation | Search by name | ... Search the designations of an object . This catalogue (table a101 in the database) presents the compilation of the designations of objects. ... A given object may have several names. ... The colon behing a galaxy designation means that this name is given to 2 (or more) objects. ... The pair keeps the name given in the catalogue and the 2 objects members of the pair have the same name + the colon. code . ...

... See spectral jumps at 2^n channels Intro for a description of pshift,pfb, term s . ... pshift . ... 0x1ff5 . ... 0x1555 . ... noise pshift . ... noise pshift, first butterfly no shift . ... 0x1555 shift every other butterfly (this should work for noise) . ... the black trace has pshift=0x1ff5 (the current standard). the red trace uses 0x1555. shift every other butterfly (with a shift on the first butterfly) . ... When a pshift of 0x1555 is used (shift every other butterfly) no jumps are seen . ...

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

... Oleg V. Verkhodanov . ... The last few years have changed our view on the evolution of galaxies: the most distant galaxies (i.e. systems having stellar population) have been found at redshift z=6.68 (Chen H.-W., Lanzetta, K. M., Pascarelle, S. 1999, Nature, 398 , 586) and radio galaxy at z=5.19 (van Breugel W., De Breuck C., Stanford S. A., Stern D., Rottgering H., Miley G. 1999. astro-ph/9904272 ). ... Redshifts and age of stellar systems of distant radio galaxies from multicolour photometry data. ...