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. ...

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• K-band Arcetri Obscured Supernova Search - What is the KAOSS Projrect?
• K-band Arcetri Obscured Supernova Search - Home page

We report far-infrared and submillimeter observations of supernova 1987A, the star whose explosion was observed on 23 February 1987 in the Large Magellanic Cloud, a galaxy located 160,000 light years away. ... The intensity and spectral energy distribution of the emission suggest a dust mass of about 0.4 to 0.7 times the mass of the Sun. ... Our observations imply that supernovae can produce the large dust masses detected in young galaxies at very high redshifts. ... ADS Citation Query . ...

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• Detection of a Massive Dust Shell around the Type II Supernova SN 2002hh

Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...

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• APOD: 2001 April 4 - Distant Supernova, Dark Energy
• APOD: 2002 May 17 - Gamma Ray Burst, Supernova Bump
• SAI Supernova catalog

2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...

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• Abstract
• G338.1+0.4

... A Gamma Ray Burst Supernova Connection . ... Credit: Al Kelly ( JSCAS / NASA ) Arne Henden ( Flagstaff / USNO ) Explanation: New evidence has emerged that a mysterious type of explosion known as a gamma ray burst is indeed connected to a supernova of the type visible in the above image . ... Type II Supernovas might not appear coincident with gamma-ray bursts , however, when the gamma-ray beam goes in another direction. ... Publications with keywords: GRB 030329 - gamma-ray burst - supernova - GRB ....

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• Hot Gas Halo Detected Around Galaxy NGC 4631
• Distant Supernova Dark Energy
• Gamma Ray Burst, Supernova Bump

Here are two images of SN 1998ey in NGC 7080. The discovery image (Dec.5th) was stretched quite a lot and only just visible above the noise. It was a 30 sec. exposure with a 30cm f/6.3 SCT and Starlight Xpress ccd in bright Moonlight and mist. I was very lucky to have detected it under these conditons as it was at mag. 17.0 or a little fainter. ... Back to 1998ey . Back to Bright Supernovae David Bishop Last modified: Sat Dec 26 16:42:45 EST 1998 ...

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• Supernova 1999ab in anonymous galaxy
• Supernova 2000ch in NGC 3432
• Bright Supernova Bright Supernova

... Original paper: E.Churazov, R.Sunyaev, J.Isern, J.KnЖdlseder, P.Jean, F.Lebrun, N.Chugai, S.Grebenev, E.Bravo, S.Sazonov, M.Renaud, "56CO -ray emission lines fro m the type Ia supernova SN 2014J", Nature, 512, 406, 2014, http://dx.doi.o rg/10.1038/nature13672 Fig 1. ... Microsatellite "Chibis-M" was developed on the plat form originally designed at the Specia l Engineering Depart ment of Space Research Institute of Russian Academy of Sciences in 2011. ... 1 Fig .1. ... 2014, 52, 2, . ...

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True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... Chandra Proposer's Guide pile up section ] During frame readout, the ACIS CCDs take 40 microsec to (parallel) transfer the charge by one pixel. As a result of this, each frame readout, each pixel is exposed for 40 microsec to a source (plus cosmic X-ray background) at each location along its column. ... Note also that the image does not just trail, it extends along the whole column. ... Chandra Supernova Remnant Catalog . ...

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• The Diffuse X-Ray Background
• PAUL J. GREEN - Research Page
• Pat Slane: Pulsar Papers

. While studying the dust content of the Crab Nebula with the Herschel Space Observatory, astronomers have detected emission lines from argon hydride, a molecular ion containing the noble gas argon. This is the first detection of a noble-gas based compound in space. This image shows a composite view of the supernova remnant as viewed by the Herschel and the Hubble Space Telescope. ESA/Herschel/PACS/MESS Key Programme Supernova Remnant Team; NASA/ESA/A. Loll/J. Hester (Arizona State University)

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• Black hole outflows from Centaurus A detected | Astronomy.com
• Has dark matter ever been detected in or around the Milky Way Galaxy? |
• Precisely measuring velocity of a supernova shock wave | Astronomy.com

... This supernova was discovered on April 6, 1998 on spectra obtained with 6m telescope of Special Astrophysical Observatory RAS (Kniazev et al. ... BVRI and H images were taken with the 1.52m EOCA telescope at Calar Alto on April 24, 1998. ... The available spectra for the SN, from April 6 and 19 taken with the 6m SAO Russian telescope and from May 26 with the NOT are shown in Figure 2. ... The spectra are typical of a type II supernova. ...

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• A 10-GHz Radio Continuum Survey
• Upper Limits for Sources not Detected
• Results of observations

Interaction of the Supernova Remnant S 147 . ... Based on RATAN-600 21-cm HI line observations with an angular resolution of 2.4', we study the neutral-hydrogen distribution in the region of the supernova remnant ( SNR ) S 147 ( G180.0-1.7 ). ... FIGURE CAPTIONS . ... The distribution of HI emission features in the vicinity of S 147 after the subtraction of the extended background. ... The distribution of HI emission features, as constructed from the survey data by Westerhout and Wendlandt ( 1982 ). ...

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This source is hiding behind our Galaxy at a distance of ~18 Mpc, located at a galactic latitide of 0 degrees. ... As we look towards longer wavelengths, 60 micron, to try and penetrate the Galactic Plane, we still see confusion from galactic sources. ... If the image seems some what confusing that is because the MOST is a continuum radio telescope and when it looks in the direction of our Galaxy it detects radiation from sources within our Galaxy and from sources that may lie behind our Galaxy. ...

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• Figure 2 - Supernova search coverage map.
• Optical and other high energy emission
• Searching For Supernova Remnants

home publications > mercury . SEARCH ASP SITE: Match ALL words Match ANY word . ... ASP Conference Series . ... Publications of the ASP (PASP) . ... The Gamma-Ray Burst/Supernova Connection . ... After 30 years of bewilderment, astronomers finally know that collapsing massive stars generate most gamma-ray bursts. Gamma-ray bursts (GRBs) were first detected in the late 1960s by American military satellites designed to monitor Soviet compliance with the Nuclear Test Ban Treaty. ...

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... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dust in the Crab Nebula Supernova Remnant . ... Data Handling and Products . ... Science Data Products Forum . ... The Crab Nebula supernova remnant, NGC 1952, is the remains of a massive star that underwent a supernova explosion in AD 1054 (see the HST image ). ... A thesis topic to study in detail the properties of the dust features in the Crab Nebula is outlined. ...

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• ESO - Why do I get the message that "no slits could be detected", even though
• Black hole outflows from Centaurus A detected with APEX | ESO
• Black hole outflows from Centaurus A detected with APEX | ESO United Kingdom

... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...

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• X-rays binary Cyg X-3
• V1494
• Galaxy sector, archive 2008

Astronomers Detect Coolest Radio Star . ... The new radio-star is much smaller and colder than our Sun.€а With a surface temperature not much higher than that of a giant planet, and a size comparable to JupiterтАЩs, it is scarcely visible in optical light.€а Yet the radio flares seen at Arecibo show it must have a strong magnetic field, implying that the same could be true of other similar stars. ...

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• Astronomers Detect Coolest Radio Star National Astronomy and Ionosphere Center
• HI Self-Absorption in the Canadian Galactic Plane Survey: First Results
• Solar System Studies at AO

Next: Radiopulsars as Sources of Up: Cosmic Rays and Evolution Previous: Cosmic Rays and Evolution . Presently, there is little doubt that galactic CR can be generated at rapidly expanding shock fronts produced by supernova explosions. ... Statistical properties of radiopulsars in our Galaxy indicate a formation rate of NS of about 1 per 10-20 years in the present cosmological epoch, while direct astronomical observations have so far not detected supernova explosions at this high rate. ...

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• #tex2html_wrap_inline12527#-#tex2html_wrap_inline12529# for Supernova...
• Seminars
• Evolution of Supernova Explosion Rates in the Universe

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

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Astronomy Discussion Forums . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... SETI Assumes ET Doesnot Care About Can Being Detected What If . ... Post Message | ... My search on how to go undetected in space and SETI Search for Extraterrestrial Intelligence SETI. ... www.astronomy.net . About Astronomy Net | Advertise on 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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... MASTER Net is 56 square degrees per 1 exposition . ... 06 Dec 2015: GRB 151205B: MASTER-NET early optical observations GCN18665 . ... 18 Nov 2015: GRB 151118A: MASTER-NET optical observations GCN18613 . ... 12 Nov 2015: GRB 151112A: MASTER-NET optical limit GCN18591 . ... 07 Nov 2015: GRB 151107A: MASTER-NET optical observations GCN18565 . ... 31 Oct 2015: Five OTs detected by Global Robotic MASTER Net ATel8232 . ... 02 Oct 2015: GRB 151001B: MASTER-NET early optical observations GCN18380 . ...

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