Supernovae 2016adj in NGC 5128 . This page is devoted to information on Supernova 2016adj in NGC 5128 (= Centarus A). ... Discovered by Peter Marples and Greg Bock ( BOSS ) (Australia). ... TNS 2016adj . TNS 2016adj spectra . ... 2016/01/20.000 . ... 2016/01/21.360 . ... 2016/01/22.329 . ... 2016/01/29.277 . ... Prediscovery . ... Prediscovery Color, Wow without inset Black and White version . ... Peter Marples and Greg Bock . ... Peter Marples . ... Back to Bright Supernovae - 2016 . ...

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• Supernova 2008ha in UGC 12682
• Supernova 2006fo in UGC 2019
• Supernova 2005ch in anonymous

Supernova 2004ey in UGC 11816 . This page is devoted to information on Supernova 2004ey in UGC 11816 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. ... Click on the name in the "Image Credit" column to see the image. ... 2004/10/14.23 . ... Light curves and Spectra: . ... VSNET Light curve. ...

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• Supernova 2011ja in NGC 4945
• Supernova 2006jc in UGC 4904
• Supernova 2005bf in MCG +00-27-5

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... 1997, ADNDT, 67, 225 %Comment: the theoretical energies from Palmeri et al. have been used as experimental ones when the latter were unavailable % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi - Feb 2005 . ...

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... Radio Catalog . The corrections in NVSS fluxes leading to the corrected Version 1.1 also result in changes to some of the figures and tables in Kimball Ivezi? ... The results are qualitatively the same. ... The new versions of the figures, along with the original versions (in high resolution), are available here . ... These figures, along with Table 4, continue to motivate t = 0.35 as the optimal separator between "simple" and "complex" sources). ... Complex Sources . ... t NVSS . ... galaxy . ...

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• Australia-Japan Collaborative Workshops
• ESO Collaboration
• Final Comments

... Credit Copyright: NASA , DOE , Fermi LAT Collaboration Explanation: A tremendous explosion has occurred in the nearby universe and major telescopes across Earth and space are investigating. ... Within three minutes, the half-meter ISON telescope in New Mexico found the blast in visible light, noted its extreme brightness, and relayed more exact coordinates. ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... Bright Supernova in M82 . ... M95 with Supernova . ...

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• The Pulsar Powered Crab
• XWare > APOD
• Journal "Peremennye Zvezdy"

... HST . ... APT . ... HST Overview . Overview . ... Phase I Proposing . ... Cycle 24 Announcement . ... Phase II Cycle 23 . ... Documents . ... After you have brought up APT you will see a "Help" menu on the top menu bar. From here you can also bring up the documents that will help you to learn APT. Phase I: You can bring up Phase I Specific APT Training Materials to learn about using APT to submit your Phase I proposal. ... These are the same documents you will find on the HST Website. ...

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• RPS2 Demonstration
• Reporting Problems
• GHRS Instrument Handbook

... Solar System . ... European astronomers have discovered a planet with about the mass of the Earth orbiting a star in the Alpha Centauri system тАФ the nearest to Earth. ... Alpha Centauri is one of the brightest stars in the southern skies and is the nearest stellar system to our Solar System тАФ only 4.3 light-years away. ... The European team detected the planet by picking up the tiny wobbles in the motion of the star Alpha Centauri B created by the gravitational pull of the orbiting planet [2] . ...

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• DFS Problem Reporting rules and recommendations
• Bright supernova in the LMC | ESO
• The bright star Fomalhaut in the constellation of Piscis Austrinus | ESO

Comment on J0513-2159 . Our image shows an extension to about 5 mas SE from the brightest feature. The EVN 8 GHz image by Dallacasa et al. (1998), with about five times larger resolution, shows an extension from the brightest feature roughly opposite to our direction. As noted by Dallacasa et al. (1998), the structure detected has a highly inverted spectrum, which, together with the reported variability in the source, could explain the structural disagreement. ...

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README for XFree86 on OS/2 : Bug Reports for This Document . Previous: What and Where is XFree86? . Next: Hardware and Software Requirements . Send email to Holger.Veit@gmd.de (Holger Veit) or XFree86@XFree86.org if you have comments or suggestions about this file and we'll revise it. README for XFree86 on OS/2 : Bug Reports for This Document . Previous: What and Where is XFree86? . Next: Hardware and Software Requirements

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• Album: Reports from various events

... 81Trushkin+ The results of the multi-frequency radio observations of fourteen supernova remnants (SNRs) made with the RATAN-600 radio telescope in 1985 are reported. Flux densities of these SNRs are measured at least at two wavelengths: 31.3 and 7.6 cm. The radio spectra of some SNRs are precised. ... The radio sources detected inside or near the SNRs with the flux densities measured in the most sensitive 7.6-cm radiometer. The spectra of some point sources are discussed. ...

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• ESO-MIDAS Problem report Form
• COMPACT RADIO
• Support and Information Services

... Next: Object Detection Using Up: Object Detection and Previous: Automated Classification of . ... A status report of the The GSC Object Classifier (GOC) project is presented. ... The GSC contains multiple entries for some objects due to plate overlap. It classifies objects as stars, non-stars, galaxies, blends and potential artifacts; the latter three classifications are rare, and only exist in GSC version 1.1, to which they were added manually. ... star, . ... non-star, . ...

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... Posts tagged ?F-test? ... Therefore, with such a high percentage of having nukes, it is right to send troops to A. This episode immediately brought me a thought about astronomers? null hypothesis probability and their ways of concluding chi-square goodness of fit tests, likelihood ratio tests, or F-tests. ... Tags: cases , chi-sq , curious , degree of freedom , dof , F-test , goodness-of-fit test , Model Selection , null hypothesis probability , p-value , reduced chi-sq . ... Continue reading ?[ ...

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• The AstroStat Slog p-value
• The AstroStat Slog chi-sq
• The AstroStat Slog reduced chi-sq

MAIN PAGE . ... Nova Cygni August 1975! ... 1975/76: Comet West! ... Dr. Richard West (4th from left) & AAL members visiting SES Betzdorf on occasion of our club's 25th anniversary - October 1996 . Comet West Information . ... It was the brightest comet visible from Earth since Comet West in 1976. ... 1997: Comet Hale-Bopp! ... Thus Comet Hale-Bopp never got closer to Earth than Earth gets to the Sun. ... Comet Hale-Bopp JPL Page . ... 1999: Total solar eclipse over Luxembourg! ...

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How do I report problems I've encountered using NEdit ? ... If you have a problem which is not covered in the on-line help, in this FAQ, or in the README file specific to your system, you can report it to discuss@nedit.org (usage questions) or, develop@nedit.org (error reports). ... Below are some suggestions for information you can provide to help in diagnosing your problem. ... As of version 5.2 a summary with build information is present under 'Version' in the Help menu. ...

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• LWN: Driver porting: mutual exclusion with seqlocks
• NEdit.org
• Linux PCI-HOWTO: Reports of problems

... Bojan Nikolic web pages home . ... We have posted today three reports on ALMA phase correction performance when using the WVRGCAL program. ... Sarah F. Graves: WVRGCAL performance: early 2011 observations & smoothing, March 2012 . Marcel Clemens, The performance of wvrgcal тАФ The 4 quasar, band 9 experiment, uid A002 X2d1a7d X35b.ms , November 2011 . Marcel Clemens, The performance of wvrgcal тАФ The influence of self-cal, September 2011 . ... Copyright 2012, Bojan Nikolic feedback welcome ...

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• Supernova Remnant (SNR) Catalogue or Catalog of Galactic SNRs
• ALMA Phase Calibration Techniques at the Cavendish Astrophysics Group
• Bojan Nikolic -- Astrophysical techniques graduate course

... Armagh Observatory received many telephone and internet reports from members of the public regarding sightings of a bright meteor or fireball which crossed over Northern Ireland in the early morning of Sunday, 10th October. ... Account: I was driving on the main Armagh/Portadown Road travelling towards Richhill when the sky in front of me was lit up by a couple of very bright flashes of light which were followed by a trail of white light. ... The trail faded over approximately 20 seconds. ...

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• Terry Mosely's Bulletins
• Fireball Report from Astronomy Ireland

Astronomy Discussion Forums . ... Observation Report On Mars And .. ... Post Message | ... Despite the bad conditions we had yesterday, we couldn?t resist the Mars? ?attraction? and here it is the report. ... We disassembled the LPR filter to preserve its colour balance and we prepared a set of Ultima series eyepieces and filters. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Yes - an Astronomy Net Observation_reports Forum Message
• So Where Is Mars Now? - an Astronomy Net Observation_reports Forum Message
• Observation Report From Coyle 07/19/03 - an Astronomy Net Observation_reports

... Seminar archive . ... Type Ia Supernovae (SNe Ia) have an important role to measure a distance to an anonymous galaxy because they have a good correlation of the decline rates of the light curves with the absolute luminosity. ... First, super-Chandrasekhar SNe which have extremely high luminosity, slow decline rate of the light curves, slow expansion velocity and strong carbon features. ... As another example of diversity of SNe Ia, I would like also to introduce Type Iax SNe. ... All seminars: . ...

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... the average spectra was computed for each band. the rms/mean by channel was computed for each band. ... The rfi mask was used to compute the total power for each band. ... interim correlator 9 level sampling, 1 second spectra, 25 Mhz bw, 1024, centered at 1385. take data for 4200 seconds. rms/mean computed over the 4200 seconds and then a mask was created using a linear fit to rms/mean. total power was computed using the above mask. the spectrum of the total power was also computed. ...

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• RFI Reporting Form
• lbw 1200 Mhz tone
• a2186

Astronotes Armagh Planetarium's Stellar Blog! ... Colin Johnston . ... Our Galaxy . ... To locate it, look along the imaginary line between the two end stars on the leading edge of the PloughтАЩs blade (Merak and Dubhe) and Polaris (the North Star), the galaxy M82 (also known as the Cigar Galaxy) along with its companion M81, lies just off this line about a third of the way between the Plough and Polaris. €а€аAs usual, the supernova is far brighter than its home galaxy, appearing as an extra star. ...

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• - Part 9
• Astronotes | Armagh Planetarium's astronomy news from across the Universe -
• Will Betelgeuse bring doom in 2012? | Astronotes