... H.I.T.M.A.N. is a program that I have written to analyze transient host galaxies and obtain charateristics and properties of them. ... It determines physical, photometric, and cosmological properties of the host galaxies and can also correlate with transient properties. ... Any routine can be done stand alone instead of the full routine. ... The full details of the program will be described in Tucker et al 09a, and Tucker et al 09b, in prep. ...

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• Supernovae
• Brad's Research
• The Music of the Spheres

lsst.coordConv љ unknown . ... Classes . ... coordConv::OtherCoordSys Class Reference . ... OtherCoordSys (std::string const &name, double date=0, DateTypeEnum dateType= DateType_None , bool isMean =false) . ... virtual Coord љ . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom ( CoordSys const &fromCoordSys, Coord const &fromCoord, Site const &site, double tai=0) const . ... virtual Coord coordConv::OtherCoordSys::removePM . ...

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• lsst.coordConv: coordConv::ObsCoordSys Class Reference
• lsst.coordConv: coordConv::AppTopoCoordSys Class Reference
• lsst.coordConv: coordConv::FK4CoordSys Class Reference

... We have compiled the Catalogue of extragalactic supernovae using the GCVS card catalogue. ... Doubtful (?), or rejected (-) SN 8 A1 --- RemFlag [*] The '*' indicates a remark in sn_rem.dat 10- 19 A10 --- Gal Parent galaxy designation 21- 22 I2 h RAh Right Ascension 1950 of Parent galaxy 23- 24 I2 min RAm Right Ascension 1950 (minutes) 25- 28 F4.1 s RAs Right Ascension 1950 (seconds) 29 A1 --- DE- Declination 1950 (sign) 30- 31 I2 deg DEd Declination 1950 of Parent ...

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... Bad Astronomy . ... Bitesize Astronomy . ... Hey, it's either this or one of those really irritating PayPal donation buttons here. ... I have always loved supernovae, stars that explode. ... Late in the evening of February 23 rd /24 th * , 1987, an astronomer named Ian Shelton was taking images of the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way. ... Shortly thereafter, Ian Shelton developed the plates he had been taking of the LMC and immediately saw the new star. ...

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• Phil Plait's Bad Astronomy: Mad Science

... M51 plus Supernova 2011dh . This image of the Whirlpool galaxy M51 and the supernova 2011dh was taken at the Clubhouse after the Friday evening "Introduction to Astronomy DVD class". ... The type IIP supernova was discovered on May 30-31 by Amedee Riou and credit given to Tom Reiland, Amedee Riou, Thomas Griga, and Stephane Lamotte Bailey. 16 images x 240-seconds subframe, Total= 1 hr. 4 minutes. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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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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• Обсерватория
• List of Supernovae discovered by MASTER Net

... Class . ... FIELD | ... METHOD . ... java.lang.Object ij.plugin.filter.LineGraphAnalyzer . ... This method is called once when the filter is loaded. ... This method is called once when the filter is loaded. 'arg', which may be blank, is the argument specified for this plugin in IJ_Props.txt or in the plugins.config file of a jar archive containing the plugin. 'imp' is the currently active image. ... ImageJ will lock the image before calling this method and unlock it when the filter is finished. ...

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• Filler (ImageJ API)
• FFTCustomFilter (ImageJ API)
• Functions (ImageJ API)

... Seminar archive . ... Seminar archive 2013 19 July . ... Wide-field transient surveys and supernova shock breakout . ... Many transient surveys are performed intensively in these days and time-domain astronomy comes under the spotlight. ... The shock breakout is the bolometrically brightest phenomenon in supernovae but it is difficult to observe the shock breakout due to the short duration and X-ray/ultraviolet-peaked spectra. ... All seminars: . ...

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• SAI Space Monitoring Laboratory

... V.S. Beskin (Russia) "Axisymmetric Stationary Flows in Astrophysics" . S. Blinnikov (Russia) "Supernova Light and Ejecta" . ... D. Galtsov (Russia) "New string inspired models in gravitation and cosmology" . ... M. Khlopov (Russia) "Cosmoparticle physics: the physical cosmology of the XXI Century" . ... I.D. Novikov (Denmark-Russia) "Gamow and discovery of CMB" . ... R. Ruffini (Italy) " George Gamow and the URCA process: the case or URCA1 and URCA2" . ... J. Soda (Japan) "Braneworld Cosmology" . ...

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• Cosmic Rays
• The Origin of the Solar System

... We address a question if globular clusters (GC) in a protogalaxy could for some time evolve chemically as isolated systems, enriching themselves with heavy elements produced in first supernova events that follow initial star formation. We determine both the critical mass of a protoglobular cluster that is needed to retain the ejecta of the very first supernova, and the critical energy (i.e., number of supernovae) that is needed to expel the residual gas from a cluster of a given mass. ...

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... One of the objectives of this work is to derive radial distribution of supernova remnant surface densities in spiral galaxies. ... Other objectives include the comparison of the SNR radial distribution with the radial distribution of HII regions to look for any association between Type II progenitors and the SNRs and comparison of the SNR distribution to the spiral arm patterns. ... Knowing the positions of the SNRs, we can compare their distributions relative to HII regions and spiral arms. ...

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• Results scientific researchs LRS
• Results scientific researchs 20
• Results scientific researchs 9

... P2531 Date Received: 2009-Oct-01 11:50:25 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 2.5 Hours 2.5 A deep search for a pulsar in the supernova remnant G64.5+0.9 We request 2.5 hours to search for radio pulsations from the recently discovered shell supernova remnant G64.5+0.9 using the ALFA receiver. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/DonovantagP2112tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/LorimertagP1683tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/DonovantagP1881tp.ps

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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... Future seminars . P a s t seminars . ... E.G. Berezhko (Yu.G.Shafer Institute of Cosmophysical Research and Aeronomy) . ... CR acceleration (generation) at the shocks, produced by supernova explosions, and the properties of nonthermal emission generated by CRs accelerated in supernova remnants are detaily discussed. ... Due to magnetic field amplification CR acceleration in supernova remnants provide the formation of the observed galactic CR spectrum up to the energy 10**17 eV. ...

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• Rayos Cosmicos

... According to modern views on the evolution and origin of stars, most of the stars are members of binary systems. ... After the second explosion, the pairs tend to break up and neutron stars and/or black holes fly apart. High velocities of radio pulsars are apparently largely due to this effect. ... For all possible pairs the probability of trajectory approach at small distances for the epoch, corresponding to the age of the younger pulsar have been evaluated. ... Pulsars J0543+2329 and J0528+2200. ...

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• Galaxy sector, archive 2008

. -!> download . Left: Consequtive explosion of 20 supernovae during 30 Myr. Right: Single hypernova (GRB) explosion with the total energy equivalent to 20 supernovae. The simulation was performed using a 2D Eulerian hydro code. The animation was done using IDL. -!>

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. Last updated: January, 2005.

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КАЛЕНДАРЬ КОНФЕРЕНЦИЙ First Announcement Workshop Presupernovae, Supernovae and Supernova Remnants Pushchino June 3 -- 7, 1996 The purpose of the Workshop is to give an opportunity for both astronomers and theoretical astrophysicists to meet together for a critical discussion of the hot problems of physics of supernovae and their impact on the surrounding medium from both the points of view --- observational and theoretical. ... Stellar remnants of supernovae (neutron stars, black holes). ...

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Next: Large Scale Clustering in the Universe - A Package of Codes . ... The discovery of a correlation between the light curve shape and intrinsic brightness has made Type Ia supernovae exceptionally accurate distance indicators out to cosmologically interesting redshifts. ... But supernovae are relatively rare events. ... Type Ia supernovae make excellent distance indicators, so these events at high redshift can be used to map out the history of the expanding Universe. ...

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• ADASS 2000 Conference Proceedings
• ADASS 2002 Conference Proceedings
• A Pipeline Tool for CCD Image Processing

... Meta Index / Home Page / Description / Soft flare rejection for . In this version of epreject only the boxcar method for screening the soft flares has been implemented. ... In order to perform the soft flare event selection the program generates a lightcurve in 0.1 sec bins in the specified PHA range using the rawevents obtained from the epframes procedure. ... This smoothed lightcurve is then used to help perform the soft flare event selection. ... This column can the be used to screen the data. ...

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• An additional layer over the DAL which implements some short cuts