ASKAP Source Finding and Quality Evalua*on Ma#hew Whi*ng Credit: Alex Cherney/terrastro.com CSIRO ASTRONOMY & SPACE SCIENCE Data Flow in the ASKAP System ASKAP Source Finding & Quality Evalua@on | Astroinforma@cs 2013 | ... December 13, 2013 Model flux Source- finder evalua*on ASKAP Source Finding & Quality Evalua@on | ... December 13, 2013 Alterna*ve flux error analysis Flux error Rela@ve flux error [%] ASKAP Source Finding & Quality Evalua@on | ...

Russian . ... text in Russian) . ... The Behaviour of the Bz Component of the Magnetic Field in Coronal Mass Ejections . ... Cooperation of IZMIRAN and Sternberg Astronomical Institute in the Study of the Sublimational Component of the Solar Coronal Radiation . ... Solar Wind and Magnetic Storms in the 24th Solar Activity Cycle . ... text in English) . ... The Solar Corona in the Light of TRACE Observations . ... Expeditions of Irkutsk Astronomers to Total Solar Eclipses in 1981--2012 . ...

Detected Supernovae . The search have produced till now the detections of 4 SNe. ... This result highlights the power of infrared monitoring in detecting Obscured SNe and indicates that optical surveys are probably missing a significant fraction of SNe, especially in obscured systems such as starburst galaxies. ... In Fig. we show the archival SOFI image of NGC3256 (left) and the first image obtained in 2001 (right) where SN2001db has been detected. ...

... 2015 December 15 . Colorful Arcs over Buenos Aires . ... Explanation: What are those colorful arcs in the sky? Like rainbows that are caused by rain, arcs of sunlight broken up into component colors can also result when ice crystals floating in Earth's atmosphere act together as a gigantic prism . The top color arc is more typical as it is part of the 22 degree halo surrounding the Sun when hexagonal ice crystals refract sunlight between two of the six sides. ... About APOD | ...

Astronomy Picture of the Day . ... 21.07.2014 . ... July 2014 . ... 2013 2014 . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... A service of: LHEA at NASA / GSFC . ... U. Based on Astronomy Picture Of the Day . Publications with keywords: comet . Publications with words: comet . ... Close Comet and the Milky Way . Close Comet and Large Magellanic Cloud . Comet 67P from Spacecraft Rosetta . ... Comets and Bright Star . ...

... On December 10th, 2005 the Technical Management Meeting was held, at which the decision had been taken to fill the Progress M-55 vehicle Propulsion System with the propellant components and compressed gases. On December 12th, 2005 Progress M-55 transport cargo vehicle was filled with the propellant components and compressed gases. ...

SKA-3 instrument consists of two energy-angle ( EA ) electrostatic analyzers and two energy-mass ( EM ) time-of-flight analyzers. ... Here you can find more details about SKA-3 instrumentation set. ... Case 218 . ... satellite's trajectory in geomagnetic frame ( blue coloured), UFSIPS scan location and observation moment ( red coloured), interval of the SKA-3 observations ( green coloured) . ... a view of the Nothern polar region at the moment of UFSIPS observations, the scan location is red coloured. ...

Next: Generation from Ground Calibration Up: BORESIGHT Previous: BORESIGHT Contents . This CCF component is used by QLA and the SAS. A copy of this CCF component is also used by the PHS tools. ... It is used in mission planning to predict the position of Field Acquisition Stars and targets. ... The reference point for the boresight in the OM detector is defined as the lower left edge of pixel (1025,1025) in the V-filter. Here it is assumed that the pixels are numbered starting with 1.) ...

... Weidong Li, University of California - Berkeley . ... Abstract . ... Binaries in the Kuiper Belt: Probes of Solar System Formation and Evolution . ... Asteroseismology of Extrasolar Planet Host Stars . ... Hubble Investigation of Asteroid 21 Lutetia in Support of the Rosetta Mission Flyby . ... The present program aims to use the Fine Guidance Sensors on HST to measure the pulsational modes in the star HD 17156, an 8th magnitude G-type subgiant at a distance of ~ 78 parsecs from the Sun. ...

... Archives . ... The PCA and ICA is used for separating mixed components with some assumptions. ... The need of source separation methods in astronomy has led various adaptations of decomposition methods available. ... I rarely come up with a paper which gathered and summarized component separation methods applicable to astronomical data. In that regards, the following paper seems useful to overview methods of reducing dimensionality for astronomers. [arxiv:0805.0269] . ... Chandra Blog . ...

... 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. The NOAO Pip eline Data Manager R. Hiriart, F. Valdes, F. Pierfederici, C. Smith and M. Miller National Optical Astronomy Observatories, Tucson, AZ 85719 Abstract. The Data Manager for NOAO Pipeline system is a set of interrelated components that are being developed to fulfill the pipeline system data needs. ... The Data Manager is a subsystem of the NOAO Pipeline that provides several data management services to the system. ...

... Among the objectives of Principal Components Analysis are the following. dimensionality reduction; љ . the determining of linear combinations of variables; љ . ... identification of groups of objects or of outliers. ... Finding a set of principal axes allows the objects to be adequately characterised on a smaller number of (artificial) variables. ... Reduction of dimensionality is practicable if the first new axes account for approximately 75 % or more of the variance. ...

... Bojan Nikolic web pages (r. 329) . ... SCons user manual http://www.scons.org/doc/1.2.0/HTML/scons-user/book1.html . SCons man page (on web at http://www.scons.org/doc/HTML/scons-man.html , or man scons ) . ... SCons is a tool to build compile source code into (closer-to) executable format. ... Curiously, the shared-library SCons builder will accept multiple identical sources and pass them all to the linker, which will normally lead to ?multiple definition? errors. ... Introduction to SCons . ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

... 8, ``Celestial Mechanics'', 2002 Regularity and chaos for planetary orbits in binaries D. Benest Observatoire de Nice, Nice, France 1. ... Previous papers showed that stable planetary orbits, around either the lightest or the heaviest component of several nearby binary systems, exist up to distances from their primary of the order of more than half the binary's periastron sep­ aration. ... Chaos: bounded or sticky? It is now well­known that planetary dynamics may include some proportion of chaos. ...

... QC1 database . ... The quality information is derived in form of QC1 parameters. ... The Health Check monitor collects QC1 parameters and their scores. ... The results are presented in two views: the graphical HEALTH CHECK monitor with the full trending reports, and the QUICK-LOOK monitor with scores. ... The Health Check Monitor is a joint effort of the Quality Control Group in Garching and of Paranal Science Operations. ... You can download the QC1 parameters, and also connect to the QC1 database....

Communications For Your Astronomy Event . Articles | ... John Huggins, December 19, 2005 . ... Citizens Band Radio - The original . Multi-Use Radio Service . Family Radio Service (FRS) . General Mobile Radio Service . Hybrid Radios . Amateur Radio Service . ... Does your event need communications? ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

This all-sky image shows the spatial distribution over the whole sky of the galactic haze at 30 and 44 GHz, extracted from the Planck observations. In addition to this component, other foreground components such as charged particles accelerated radially, known as synchrotron radiation, thermal dust, spinning dust, and extragalactic point sources contribute to the total emission detected by Planck at these frequencies. ... ESA/Planck Collaboration ...

. Comment on J0834+5534 . A compact symmetric object (CSO) with ~160 mas separation between components, as shown by 1.6 GHz VLBI observations (Polatidis et al. 1995). The weaker component is not detected in our survey (see also Pearson & Readhead 1988). VLBApls home page . Last modified: 16 Oct 2000

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...