LOFAR in Australia ­ A Brief Engineering Perspective By Dr Peter J Hall, CSIRO SKA/LOFAR Program Leader 6 November, 2002 Background LOFAR (LOw Frequency ARray) is a proposed radio telescope designed to operate in the approximate frequency range 10 - 250 MHz. ... In both cases, the instruments would be built and operated by international consortia; Australia is a founding member of the 11-participant SKA consortium and may join the USA and Europe in the LOFAR endeavour. ...

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• http://www.atnf.csiro.au/management/atuc/2002nov/LOFAR-technologies.pdf
• http://www.atnf.csiro.au/management/atuc/2002nov/multibeaming-demonstrator.pdf
• Australia Telescope National Facility

Science Support Status Maria Santos-Lleo EPIC calibration meeting, ESAC 9 April 2015 Overview XMM-Newton Mission extension approved for 2 more years Team moves are now frequent, thank you to those who left (excellent contribution appreciated!) and welcome to new, very motivated people! ... EPIC calibration | 9 April 2015 | Pag. ... A O 15 · Call for proposals 25 August ­ 9 October (12:00 UT) 2015 · OTAC results mid Dec 2015 · Phase II: 12 Jan ­ 5 Feb 2016 Science Operations | ...

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• http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201504/Lumb_Cal_2015.pdf
• CCD gap and bad pixel corrections
• Effective Area, Filter Transmission, Quantum Efficiency and Grating attenuation

... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

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The sky background can contribute significant Poisson noise in broad and medium band filters, and must be taken into account during noise calculations. The actual sky b1rightness depends on the heliocentric ecliptic coordinates (latitude and longitude) in a manner summarized in Table 6.3 . ... 22.4 . ... Values for other filters or sky brightnesses can be computed from Table 6.2 , Table 6.1 , Table 6.3 , and Equation 6.2. Table 6.4: Sky Count Rate per Pixel (P sky ). ...

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• WFPC2 Instrument Handbook Update
• Proceedings
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... One of the major activities going on at my Mira observatory at Sava, Italy, is to record deep sky CCD images for a personal atlas I'm currently working on. ... Images are made using a SpectraSource CCD HPC 1 camera equipped with a Texas Instrument TC215 chip, 1024 square, 12 micron pixels size, at 16 bit. ... After a 40sec exposure, the PC monitor showed a faint glow just above the camera termal noise. ... The image showed clearly a star in the galaxy core, of magnitude 14.5, some 50sec. ...

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• Contributions by amateurs: SN1996X.
• Contributions
• Contributions by amateurs: SN1995ad.

... Up: Science Data Pipelines . ... SIRTF Science Center, Caltech . The design and implementation of the data processing pipelines for the Infrared Spectrograph (IRS) onboard Space Infrared Telescope Facility (SIRTF) are presented. This includes pipeline for generating Basic Calibrated Data (BCD) in which instrument artifacts are removed, and calibration pipelines generating calibration data that allows reduction of the science data to the BCD level. ...

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• Post Operational HST Science Instrument Archives
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... Astrophysics Group . ... STFC announces бе119 million contribution to The Square Kilometre Array . ... SKA AAVS0 array . ... One of these is the Square Kilometre Array telescope . ... STFC has as well announced today a contribution of бе165 million to theб European Spallation Source and бе25 millionб to participate in the M3 Space Mission (PLATO).б  Speaking ahead of an event at Jodrell Bank Observatory Science Minister David Willetts announced the funding for the two projects. ...

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• Abstract
• XXVIIth YERAC Contributions
• Astrophysics Group Integration of the NIRSpec instrument

I'm glad you're interested in collaborating on the ConcepTests for Astronomy WWW database project! ... I'm looking forward to your contributions! ... a) high luminosity, high temperature to low luminosity, low temperature . b) high luminosity, low temperature to low luminosity, low temperature . c) high luminosity, low temperature to low luminosity, high temperature . d) high luminosity, high temperature to low luminosity high temperature. ... Back to Paul Green's Peer Instruction page. ...

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• The AstroStat Slog Blog Archive Quintessential Contributions
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... The 2018 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. ... IKI's contribution to the Pasteur rover is: . Infrared Spectrometer for ExoMars (ISEM) to be installed on the rover's beam. ... study surface composition; . study Mars's internal structure; . ... Optical module of Infrared Spectrometer for ExoMars (ISEM) for Pasteur rover (ExoMars 2018 mission) (c) IKI . Adron-RM for Pasteur rover (ExoMars 2018 mission). ...

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• MARS TOGETHER
• "Exploration" as a Classroom Resource
• Data sources

Herschel Hardware and Software . at Arcetri . Arcetri research teams have contributed to the Heterodyne Instrument for the Far Infrared (HIFI) instrument (PI: F. Helmich, SRON, Groningen, The Netherlands) and to the calibration of Photodetector Array Camera and Spectrometer (PACS) instrument (PI: A. Poglitsch, MPE, Garching, Germany). ... The photometric and spectral calibration of PACS, the 50-250 micron imager/spectrometer on board Herschel was done in collaboration with Arcetri. ...

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• IBIS - Flat Fielding
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Next: Armagh Observatory New TSN Up: New TSN Action Plan Previous: What We Do . ... In this way, the Observatory contributes directly to the Northern Ireland Executive's New TSN Policy and Programme for Government, especially in providing enhanced access and choice for those in education, and lifelong learning opportunities for all. Next: Armagh Observatory New TSN Up: New TSN Action Plan Previous: What We Do M.E. Bailey . ...

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• Armagh Observatory
• What We Do

... Colours of stars and galaxies hold information on intrinsic and extrinsic parameters, such as stellar temperatures and galaxy populations, selective absorption and colour changes due different dust contents and inclination angles of galaxies, as well as galaxy redshifts and evolution. ... The colour magnitude diagram of 65000 galaxies to which all above-mentioned quantities and others contribute can only be explained by comparison with simulations. ... Colours are also of technical help. ...

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• ESO - cosmology2002
• Instructions for Authors
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... Results 3. ... 2004), Escapa (2011): Hamiltonian approach, simplified elastic response. ... PАg. ... Let us recall that assuming a rheological model based in Smith (1974) , Wahr (1979) and IERS (2010) for the elastic/anelastic response of the Earth, the second order harmonic components of the redistribution potential admit a truncated development in complex spherical harmonics in the form Generalized Love Numbers, dependent on: Harmonic order, Excitation frequencies In magnitude, PАg. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/heinkelmann_swg3.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm03d.pdf
• http://www.gao.spb.ru/russian/psas/ffk2013/part-en.html

... He made observations of a supernova (literally: nova= "new star") in 1572 (we now know that a supernova is an exploding star, not a new star). ... Brahe's meticulous observations showed that the supernova did not change positions with respect to the other stars (no parallax). ... This was early evidence against the immutable nature of the heavens, although Brahe did not interpret the absence of parallax for stars correctly, as we discuss below. Brahe made careful observations of a comet in 1577. ...

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• Digital Stellar Spectra
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On' failures in the NIRSpec MEMS ST-ECF Instrument Science Report NGST 2002-02 The effects of `on' failures in a MEMS array for the NGST NIRSpec Santiago Arribas, Robert Fosbury Peter Jakobsen --1-- ST-ECF Instrument Science Report NGST 2002-02 The effects of `on' failures in a MEMS array for the NGST ... Assuming that the spectrum of a single facet uses 2000 detector pixels, only 0.01% of `on' failures is acceptable (i.e., 400 facets in a 2k в 2K MEMS array). ...

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• Space Telescope-European Coordinating Facility
• VLT First Light
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... Meade Instruments Corporation . ... Choosing the Right Microscope . ... On most microscopes the specimen glass remains fixed while the microscope's objective lens and eyepiece move as a unit up or down to focus the image. ... Eyepieces of varying powers work with objective lenses of varying powers to yield a range of microscope magnifications. ... Magnification: The effective magnification of a microscope is determined by multiplying the eyepiece power by the objective lens power . ... about meade |...

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• UHTC Coatings: Ultra High Transmission Coatings, Special Coatings, Telescopes,
• Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes
• Meade Instruments Corporation - Pictor Manual Index

GTK+ 2.0 Tutorial . Prev . Next . This document, like so much other great software out there, was created for free by volunteers. If you are at all knowledgeable about any aspect of GTK that does not already have documentation, please consider contributing to this document. If you do decide to contribute, please mail your text to Tony Gale, gale@gtk.org . Also, be aware that the entirety of this document is free, and any addition by you provide must also be free. ...

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• Fitting the Blaze Function
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• Using a Standard Star

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . The Novosibirsk Instrument-Making Plant was founded in 1905 to manufacture artillery sights for the Imperial Russian Army. ... Listed Since July 07, 2001 . ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

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... Tonight's Sky . ... Sky this Month . ... milky way . ... The Sky This Week: April 1 - 10 . ... Sky this Week . ... Astronomy for Kids . ... Sky Events . Get to Know the Night Sky . ... Is there any way photons could contribute to the mysterious dark matter? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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• Improved measurements of Sun to advance understanding of climate change |

Masses of asteroids 10 Hygiea and 152 Atala obtained by the dynamical method . ... Masses of asteroids 10 Hygiea and 152 Atala have been obtained by the dynamical method. ... m 152 = 1.34 0.27 (10 -11 Sun )]. ... Very Long Baseline Interferometry (VLBI), Small Solar System Body (SSSB), mass of asteroids 10 Hygiea, mass of asteroids 152 Atala, the dynamical method, perturbing asteroids, the additional acceleration, the Yarkovsky effect, elimination of erroneous observations, optical observations. ...

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