... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Parkes | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... The first claim that HI could be associated with a dSph-like system was for the dIrr/dSph system Phoenix (Carignan, Demers & CУДtУ? ...

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• User Parameters - Data Location & Beam Selection CentralProcessor 0.11
• Determining Calibration Solutions
• ASKAPsoft processing of BETA data CentralProcessor 0.11 documentation

... Figure 8: Can you detect the motion of the near-Earth asteroid 2000PH against the background stars during its close approach to Earth around 27 July 2004? ... Down) observed and imaged the unusual near-Earth asteroid 2000PH during its close approach to the Earth around 27 July 2004. The observations were carried out remotely using the new 2m aperture Faulkes telescope situated on the 10,000-foot summit of Haleakala, on the island of Maui in Hawaii. ...

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• Armagh Observatory Preprint No. 306
• First CCD Observations of Asteroids from Armagh
• Introduction

... General information . ... Staff . Research staff . Technical, administrative & librarian staff . ... Staff in alphabetic order . Research . ... Technical reports . Projects . ... General interest seminars . ... IT Services . ... Information . Resources and catalogs . ... Historical highlights . Historical research . Historical archive . ... Projects and events . Online resources . ...

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• Program parameters
• ISOGAL YSO Candidates (Abstract)
• Algorithm

... Bojan Nikolic web pages (r. 329) . ... From astromap version 1.5b3, the OOF software supports deconvolution of an observation of a planet to retrieve the assumed Gaussian parameters of the beam. This deconvolution can be useful for empirical monitoring of telescope beams over time over which the planets used as sources vary significantly in size. ... Bojan Nikolic <b.nikolic@mrao.cam.ac.uk> # Initial version 2005. ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA
• OOF Reduction Software
• Some first attempts at casata scripts Bojan Nikolic web pages (r. 329)

... R2218 Date Received: 2006-Feb-06 17:47:49 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: As a follow-up to our ongoing main-belt asteroid observations to correlate the hydration state of low-albedo main-belt asteroids with their radar properties, We propose to make rotationally resolved observations of asteroid ~ 554Peraga. ... Part of the observing run. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/ShepardtagR2096tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/ShepardtagR2319tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/ShepardtagR2096tp.ps

. Update is coming soon.

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• Examples of editing previous command lines
• Editing a previous command line
• Our observations: 970311

Next: Sample Properties Up: Sample Identification Previous: Comments on Individual Sources . Previously known serendipitous sources were selected by cross-correlating WGACAT with a variety of optical and radio catalogs, including the Ver?n-Cetty & Ver?n (1996) and Hewitt & Burbidge (1993) quasar catalogs, the 1 Jy (Stickel et al. 1994) and S4 (Stickel & K?hr 1994) radio catalogs, and the BL Lac catalog of Padovani & Giommi (1995b). ... Details of these 97 objects are given in Table 6. ...

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• Previous Institutions
• ESO - FORS2 and UVES Science Verification
• PAM Bulletin

Next: Filtering ROSAT HRI data Up: ROSAT HRI Recipes Previous: Correlating Spectral Data with . Although the spatial variation of the quantum efficiency across the HRI is nominally within 10% for most of the detector, occasionally it may be desirable to flat-field a map with preflight calibration measurements. ... Store the new gain map image using ``blink" in SaoImage. ... The quantum efficiency correction (QEC) is the inverse of the intensity determined from the QE map at the source position. ...

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• A Preliminary Investigation
• Stars with Highly Secure Periods
• Correlating Spectral Data with Spatial Gain Variations

... Previous: Generalized Linear Multi-Frequency Imaging in VLBI . ... At Astronomical Observatory of Valencia University (OAUV), CCD observations of asteroids and big planets satellites are obtained since 2001 with a big format camera and several telescopes. ... Software for comparison of single and overlapped CCD fields obtained at different epochs has been developed. ... After images measurement in CCD field, catalogue stars are identified and adjusted with images. ...

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• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• See Spike Run... Run, Spike, Run
• Distributed Software for Observations in the Near Infrared

2007 Jan 08) Bright comet C/2006 P1 (McNaught) . 2005 Jan 20) Tornado near Coonabarabran . 2005 Jan 16) Major upgrade in progress . 2005 Jan 16) Near Earth Comet 162P/Siding Spring . 2004 Apr) 2004 CB identified as a comet . 2004 Apr) Systematic surveying commenced 2004 March 16 . 2004 Apr) Media Releases on commencement of survey . 2004 Jan) 'Accidental' discovery of 2003 XB22 . ... Siding Spring Survey Main Page . ... Previous News Items . ...

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• Philip Lah's Research
• Emma Kirby - Outreach
• Spectroscopy

Next: Navigation Pre-Observation Products . ... SRT (Space Radio Telescope) Schedule (SRS) File . ... What: GOCG generates the Space Radio Telescope (SRT) schedule file, or SRS file, from current GSTS file. The SRS file has more precise time stamps than long-term schedules, and also designates which GTS will be used when. ... The SRS file also serves as the antenna pointing schedule file, as it describes the planned orientation of the spacecraft (and solar panels) as a function of time. ...

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• RSOG Pre-Observation Products
• DPC Post-Observations Products
• Correlator Products

... Variation of systematic errors for USNO A2 (in mas per year) 23 .914 0.082 0.250 0.418 0.586 0.753 0.921 1.089 1.257 1.425 1.593 4 4. 3. 3. 3. 3. 3. 3. 3. 3. 3. 15 ? 7? 1? 3? 3? 10 ? 10 ? 11 ? 6? 10 ? 12 ? and their errors USNO UCAC USNO UCAC A2.0 2 3 B1.0 4 (1998) (2006) (2003) (2012) 37 27 11 4 732 529 778 501 050 078 775 387 (34 610 829) (17 209 447) (9 744 401) () Distribution of observations ( ...

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• http://www.gao.spb.ru/russian/lg/dbase/comztf_eng.doc
• http://www.gao.spb.ru/english/as/j2014/presentations/filippova.pdf

Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

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• Second Spectrum-RG/eROSITA Conference
• Пширков Максим Сергеевич (ПРАО АКЦ ФИАН)
• Титарчук Лев Григорьевич (NRL)

. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 20/08 Nijo castle (ancient shogun palace). Assembly opening. Maiko . Up . << Prev . This shot is slightly better than previous. Next >> . Album created by album tool a Marginal Hack by David Ljung on Tue Jun 23 14:46:12 2015 .

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• Image: Harvard Medical School, view from the previous building
• Image: Same shot. Slightly worse than previous.
• Notation

... Let us first find out which way -- rise in spectral resolution with some loss in the S/N ratio or increase in the S/N ratio with a fixed spectral resolution -- is better for the purpose of reduction of equivalent width determination errors. ... N -- number of counts for 1 ? ... line equivalent width, . ... Thus if the spectral resolution is managed to be increased (i.e. to decrease )without loss in the number of counts falling at 1 ?, the equivalent width measurement error is then proportional to . ...

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• Observations and spectra reduction
• The spectrograph design and the observing procedure
• Introduction

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

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ASTEROIDAL DAMAGE TO THE EARTH: IMPLICATIONS BY ASTEROIDS ґ RUBBLE PILES. ... 13, Moscow 119892, Russia, E-mail:san@sai.msu.ru In the cause of asteroids ґ rubble piles its effective cross-section of collision to the Earth is determined not by consolidated body, but by cluster of its fragments. Since the stage of rubble ґ piles may be ~108 years (see our communication at previous symposium), it may be significant for estimation the asteroidal damage to the Earth. ...

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• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms38/ms080.pdf

... I have always heard that everything we see is "star stuff" from previous stars that died after converting their hydrogen into heavier elements. So how is there any hydrogen left for the Sun and planets? ... Hydrogen is the main source of fuel for stars like the Sun. ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...

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• Previously understood that magnetic fields were directly related to rotation,
• Kepler stars and planets are bigger than previously thought | Astronomy.com
• Space telescopes reveal previously unknown brilliant X-ray explosion in Milky

... Laboratory and theoretical modelling of the UV bump on the interstellar extinction curve is a very popular topic in dusty investigations. ... feature is illustrated by Fig. 10 where the profiles were calculated using the model of graphite spheres. Figure 10: Normalized extinction efficiencies for graphite spheres. ... The lower panel shows the summary extinction of two graphite spheres with radii and (from upper panel) taken in equal proportions. ...

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• Linear polarization: wavelength dependence
• Introduction
• Extinction properties (transmitted radiation)

375: Candidate Quark Star . ... Credit Copyright: M. van Kerkwijk ( Institute of Astronomy, Utrecht ), S. Kulkarni ( Caltech ), VLT Kueyen, ESO Explanation: Why is RJX J185635-375 so cool and so dim? Previously, this compact star held claim to being the closest neutron star -- only 150 light-years away. ... One hypothesized solution holds hope a RJX J185635-375 is actually a not a neutron star but a quark star -- something new. ... NASA Web Site Statements, Warnings, and Disclaimers . ...

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• Астронет > 375: Candidate Quark Star
• A Lonely Neutron Star
• Астронет > A Lonely Neutron Star