... Current projects MNRF1997 - 3/12mm systems Construction of the new Mopra MMIC-based 3/12mm receiver is proceeding, with installation scheduled in September. ... Good performance up to 115GHz is expected. The fabrication of a set of spare components for the ATCA and Mopra 3/12mm receivers will be completed by July. ... MNRF2001 - ATCA Broadband Upgrade (CABB) A design for the LO/conversion system in the antenna has been chosen and work towards the construction of a prototype is proceeding. ...

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• http://www.atnf.csiro.au/management/atuc/2004dec/docs/5.1_ATUC_TechDev_Report.doc
• http://www.atnf.csiro.au/management/atuc/2005dec/docs/5.0_ATUC_TechDev_Report_dec05.doc
• http://www.atnf.csiro.au/management/atuc/2007may/docs/3_TechDev.pdf

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Antenna system . ... The Irkutsk incoherent scatter radar is one of the world's nine active radars which give the opportunity to investigate ionosphere by the incoherent scatter method. ... Antenna gain coefficient . ... Antenna . ... Two antennas . ... To get an idea what station "Dnepr" antenna system looks like, let us consider some of the radar views which are given by the photographs General view and Side view . ...

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• East Siberian Center for the Earth's Ionosphere Research. Modernization...

... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• ESO - Science Announcements
• ESO - Swedish Heterodyne Facility Instrument Science Verification
• ESO - Reflex

Status of the RadioAstron project development . The engineering model of the Space Radio Telescope (SRT) was assembled in Lavochkin Association (LA) in the configuration consisting of 10-m parabolic radio astronomical antenna made of carbon-fiber, F ocal and Device cabins of the scientific payload and on-board and ground complex of high data rate up-down radio link (VIRK). ... Then,radio astronomical tests were conducted using real radio sources. ... Space Radio Telescope . ... Data Processing . ...

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• RadioAstron Announcement of Opportunity - 1, english version
• ОТЧЕТ

... A growing collection of images showing progress with the Telescopes and Telescope Domes restoration project is available on the Armagh Observatory web-site (see star.arm.ac.uk/history/Domes/ ). The project has been progressed satisfactorily and close to its original budget. ... The outer copper skin of the dome has been replaced with new pre-patinated copper sheeting. ... The Sinden Optical Company has made considerable progress with the restoration of the 1835 Grubb 15-inch reflector. ...

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• The Linux Documentation Project
• Buildings, Telescopes and Telescope Domes Project
• C.J. Butler, Research Astronomer

STScI . ... Phase I Proposing . ... Astronomer's Proposal Tool . ... STScI solicits proposals for HST Observing, Archival Theoretical Research. ... HST Cycle 24 Phase II Proposal Deadline . The Call for Proposals (CP) invites the astronomical community to propose for observing time on HST in a given cycle (nominally one year in duration). It summarizes the policies and procedures for proposing in that cycle of HST observing, including requests for funding research on archival HST data. ...

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• FUV-MAMA Repeller Off as an Available Mode for High Resolution Spectroscopy
• A.3 Getting IRAF and STSDAS
• cgvc 121

In the PROJECT we are using the following peculiar . features of RATAN-600 . ... Brightness temperature sensitivity being equal to the antenna temperature sensitivity .. ... Receiver system .. ... Using aperture averaging effect. dual- beam and dual (multi-) frequency filtration, we demonstrated full filtration of the atmosphere noise down to the receiver noise at all scales of acoustics peaks ( Fig.1 , Fig 2 ). ... We select this frequency as the central one in our project. ... Antenna surface . ...

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• Grants

... Astrophysics Group . Graduate Research Opportunities 2016 . Available research projects/areas . ... Astrophysics Admissions Form . ... This includes active participation in the development of new instruments as well as the use of ground and space observatories. ... Further details are available at the following web site: http://www.mrao.cam.ac.uk/research/extragalactic-group-2/ . ... Our research group has a wide range of expertise in the development of receivers for radio astronomy. ...

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• Astrophysics Group Admissions Procedures
• Astrophysics Group FIRST
• Astrophysics Group PhD Thesis Projects

... Richard F. Gordon, Jr. ... NASA Astronaut (former) . ... ORGANIZATIONS: Fellow, American Astronautical Society; Associate Fellow, Society of Experimental Test Pilots; and Navy League. ... Gordon, R. F., FJ-4B FUEL CONSUMPTION AND PERFORMANCE REPORT, Flight Test, NAS Patuxent River, Maryland, 1958. ... In 1957, he attended the Navy's Test Pilot School at Patuxent River, Maryland, and served as a flight test pilot until 1960. ... He served as backup pilot for the Gemini 8 flight. ...

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• JSC Oral History Project
• Astronaut Bio: H. Stefanyshyn-Piper (2/2009)
• as11-40-5875

... The properties of the currently available receivers are given in Table 3 . The columns of the table give the receiver name, frequency range, the typical System Temperature (T ), Gain, System Equivalent Flux Density (SEFD) and Half Power Beamwidth (HPBW) for zenith angles below 15 (as measured by Arecibo staff.) ... Full details of the ALFA observing system, its performance, how to join an ALFA Consortium, and the latest ALFA news is to be found via, http://www.naic.edu/alfa/ . ...

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• Arecibo Observatory 430-MHz Gregorian Receiver
• system Performance
• GALFA - H I Projects

... We used many different approaches and the resulting success grad was mixed. ... We use either mean processing time per input sample in ns, or the resulting sampling speed , in unit of 106 samples/s. # buffe r s 256 512 1024 1536 2048 # buffe r s 256 512 1024 1536 2048 # buffe r s 256 512 1024 # buffe r s 256 512 1024 ATI GPU F F T t i me ( 0.47 0.48 0.48 0.48 0.48 ATI GPU Read speed (GB/s) FFT time ( 2.69 0.58 3.52 0.58 3.96 0.58 4.24 0.58 4.42 ...

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• Using Apache With RPM Based Systems (Redhat / CentOS / Fedora) - Apache HTTP
• Radioastronomy laboratory
• Observing capabilities

... Space Research Institute . Main . ... Main research and development work completed in 2012 and ready for implementation . ... Main research and development work completed in 2011 and ready for implementation . Main research and development work completed in 2010 and ready for implementation . Main research and development work completed in 2009 and ready for implementation . Main research and development work completed in 2008 and ready for implementation ...

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• Onboard data collecting system (STS)
• Main research and development work completed in 2009 and ready for
• Instrumentation for Fundamental and Applied Space Projects

The XV_VTDF is a viewer for TDF format files (extension to TIFF 6.0 format for storage of high-resolution satellite data). More information about TDF format and relevant topics, as well as satellite data in this format you may receive from Space Monitoring Information Support lab (Space Research Institute, Moscow, Russia) . ... XV_VTDF <filename> - load TDF file at startup (default size) . ... The XV_VTDF operates with fixed-size satellite images in TDF format. ... Back to SMIS Home Page . ...

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... SETI@home consists of a receiving Arecibo antenna, a professional team (PT), and a two-way Internet connection between the PT and an army of S@h users, who load from the S@h server special software for digital signal processing. ... Thereby, METI@home will consist of several originators, which may load via Internet from a M@h server special software for the creation of analog and digital messages. ... ETI as a Source of Information . ... Main Internet Server . ... ETI as a Customer of Information . ...

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• Project 5 - State Program "Condenced Matter Physics"
• Project 1 - SfP - Ovsyannikov, Supersensitive high-Tc superconducting

Ron Miksa, Carl Lindenmeyer, and John Korienek, as well as Steve Bastian (all from FNL), were on site to install the new manipulator arm in the 2.5m support building. Not to break tradition, these photos are of the completed installation and those hard working folks are not pictured. Captions above photo . ... Note that the bay door is open. ... The arm swings out from the body of the manipulator, and the assembly is moved along the metal runners to position it in front of the plate cartridge. ...

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• APO Housing Form
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... The Chandra Multiwavelength Project (ChaMP) seeks to understand the nature and evolution of quasars, galaxies, and clusters of galaxies in a large, carefully constructed multi-wavelength survey. ... Recent ChaMP Papers . The Field X-ray AGN Fraction to z=0.7 from the Chandra Multiwavelength Project and the Sloan Digital Sky Survey , Haggard, D., Green, P.J., Anderson, S.F., Constantin, A., Aldcroft, T., Kim, D.-W., Barkhouse, W.A. 2010, ApJ, 723, 1447 (arXiv:1004.1638) . ... 2009, ApJ, 690, 644 . ...

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• Five-Minute-Task Time Estimate Worksheet - SAMPLE
• common tcsh completions
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... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...

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• Zen: wildspeed
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. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• Astronomy HyperText Book
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SAI VO . ... SAI CAS . ... Web Services . ... SAI Web Services . ... This Web site is provided by SAI VO Group and the use of the Web site and the services available at the Web site are subject to the following terms and conditions in this Terms of Use notice. ... SAI VO Group is constantly improving Web site and services and reserves the right to make such improvements or changes to this Web site, the materials and services provided from this Web site without prior notice as it deems necessary. ...

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• SAI CAS: About the SAI CAS project
• SAI Virtual Observatory Project - About
• SAI VO: Projects in Development

... The IVOA Data Access Layer (DAL) working group is defining a Simple Spectral Access (SSA) protocol for accessing 1D spectra and SEDs. ... The survey consists of two parts. ... Elodie: 25000 extracted Echelle spectra, resolution 42000, 4000 - 6800 ? ... ISO 1D Spectral Data: 10000 files, 2.4-197 micron, resolution 40-30000 . ... XMM-Newton 1D Spectral Data: XMM/RGS, 20000 spectra (expected), 0.35-2.5 keV, resolution 200-800; XMM/EPIC, 1.5 mio. spectra (expected), 0.35-15 keV, resolution 20-50 . ...

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• Starlink's Software Distribution System
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