Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...

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• COROT-7b: Exoplanet with a sky made of stone | Astronotes
• Kepler-10c: the First Mega-Earth | Astronotes
• Pseudoscientific ideas so bad that they're not even wrong | Astronotes

CFITSIO Interface Library CFITSIO is a library of ANSI C routines for reading and writing FITS format data files. ... The CFITSIO library is built on Unix systems by typing: > ./configure [--prefix=/target/installation/path] > make (or 'make shared') > make install (this step is optional) at the operating system prompt. The configure command customizes the Makefile for the particular system, then the `make' command compiles the source files and builds the library. ...

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... Bad Astronomy . ... Bitesize Astronomy . ... even the brightest star won't last forever.' ... The pressure and heat are so enormous inside the star's core that hydrogen is fused into helium. ... A star like the Sun has enough hydrogen to keep its fusion fires going for billions of years, but a star like Rigel, a massive star in Orion, burns its hydrogen so fast it may run out in just a few million years. ... The problem is, at this point something bad happens: silicon fuses to iron. ...

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• Phil Plait's Bad Astronomy: Phil's Los Angeles Adventure

... 1 - 5 m HgCdTe Detector Material . Hybridization of 2048 x 2048 Arrays . ... Options for Extension to Visible Wavelengths . ... MBE HgCdTe Capability at Rockwell Science Center . ... Over the last two decades, dramatic improvements in the performance of 1 - 5 m infrared detector materials combined with the leap from single detectors to million pixel arrays have led to a billion-fold improvement in our ability to observe astronomical sources at these wavelengths. ...

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... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... On-Line Proposal Applications and Links (OPAL) . ... Parkes | ... Astronomical tools & software . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Photometry Theory . ... Colour Indices provides details and values for colour indices for different spectral and luminosity classes of stars...

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• first_mm_light
• TWENTY-FIVE YEARS OF AUSTRALIAN IR
• Yiannis Web Page

... Imaging spectrometer for atmosphere and ionosphere spectral investigation consist the static Michelson interferometer and CCD camera. The prototype of the onboard CCD camera for the spectrometer used the Toshiba 2048 pixels CCD linear array (TCD 1201D) with FPGA-based controller. The controller is building on ACTEL A1020A field programmable gates array with maximum data rate 40 MHz and can be used with linear and area array CCD. ... Toshiba CCD Linear Image Sensor Data Book, 1997. ...

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HARP is the Heterodyne Array Receiver Programme for the James Clerk Maxwell Telescope. The programme is beginning with HARP-B, . ... February 2006 . ... The HARP-B project is a collaboration between Cavendish Astrophysics (MRAO) at the University of Cambridge, UK, The Joint Astronomy Centre at Hilo in Hawaii (operators of the JCMT), The UK Astronomy Technology Centre at the Royal Observatory Edinburgh, The Herzberg Institute of Astrophysics of the National Research Council Canada . ...

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• Finder Documentation

... NVIDIA, the NVIDIA logo, NVIDIA nForce, GeForce, NVIDIA Quadro, Vanta, TNT2, TNT, RIVA, RIVA TNT, Quincunx Antialiasing, and TwinView are registered trademarks or trademarks of NVIDIA Corporation in the United States and/or other countries. Linux is a registered trademark of Linus Torvalds. ... OpenGL is a registered trademark of Silicon Graphics Inc. ... Installing the NVIDIA Driver . ... Configuring X for the NVIDIA Driver . Using nvidia-xconfig to configure the X server . ...

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• vertex drive system

... Date : the picture was taken on December 14th 1998 . Location : Courroux / Ju (Switzerland) . Equipement : telescope Celestron Ultima 8 operating at F/D=6.3 camera CCD ST7 operating at high resolution autoguided mode . Exposures : 6 exposures of 10 minutes each . Pictures treatment : logarithmic . Software : Prism98 version 3.0 for acquisition and treatment of the pictures . ... 2822 Courroux . ... David Bishop Last modified: Wed Dec 16 13:55:05 EST 1998 ...

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Celestron Discussion Forum . ... Celestron SP - C6 - onesolar - July 17, 2010 - 03:01 UTC . ... Celestron Secondary Mirror Housing - lannding - April 19, 2009 - 21:20 UTC . Celestron CGE 1100 XLT secondary mirror housing repair - lannding - April 19, 2009 - 21:17 UTC . Celestron gear problem - megrez1 - October 9, 2008 - 18:56 UTC . ... No Help at Celestron - robertandbob - March 30, 2008 - 00:17 UTC . ... celestron c8 question - tdogc8 - April 5, 2005 - 03:15 UTC . ... www.astronomy.net . ...

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Supernovae are simply stars which explode. ... To understand supernovae, we need to understand stars. ... In this stage our Sun will swell up hundreds of times its current size, swallowing the Earth, and glowing hundreds of times brighter than it is now. ... Stars more than 10 times the mass of our sun have much more exciting lives. ... A Type II supernova to be precise. ... Since 1995 two teams have been discovering these objects: Our team, the High-Z SN Search, and the Supernova Cosmology Project. ...

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... ARC 3.5m | TripleSpec . ... Fowler sampling, read noise, and minimum integration time . ... The integration time for the slit viewer is adjustable, but 30 seconds represents a maximum practical integration for positioning the source and for guiding. Longer integration times are possible, but the delay between exposures makes guiding and/or positioning the source on the slit tedious. ... Decide on your guider integration time and acquire a frame to serve as the background image with "Expose". ...

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... C Cette focale fournit en effet un grossissement intermИdiaire sur bon nombre de tИlescopes d'amateur (lire encadrИ "Comment bien choisir son oculaire", p. 82). ... 78 Ciel & Espace FиVRIER 2011 Rubrique rИalisИe par Jean-Luc Dauvergne champ au banc d'essai Photos : J.-L. Dauvergne Le principe de ce comparatif Les oculaires sont des objets optiques complexes, constituИs de nombreuses lentilles. ... Son champ est trХs large avec des images aussi nettes dans les coins que sur un Nagler. ...

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Разработка, исследование и изготовление мощных полупроводниковых лазеров, излучающих в диапазоне длин волн 800 - 1800 нм. ... 30-летний опыт работы по разработке и изготовлению полупроводниковых лазеров . ... Диапазон длин волн - 800 - 1800 нм . ... Ознакомление с физическими и технологическими принципами работы мощных импульсных полупроводниковых лазеров с интегрированным тиристорным переключателем . ... Мощные импульсные полупроводниковые лазеры - физические основы и практическое применение . ...

195. Eyepiece Field of View Table