PPT-Multiple images of a highly magnified supernova formed by an early type cluster galaxy
Author : altigan | Published Date : 2020-06-15
Patrick L Kelly et al 2014 arXiv14116009 submitted to Nature Summarised by Poonam Chandra February 18 2015 Poonam Chandra 1 Punch line Discovery of the first
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Multiple images of a highly magnified supernova formed by an early type cluster galaxy: Transcript
Patrick L Kelly et al 2014 arXiv14116009 submitted to Nature Summarised by Poonam Chandra February 18 2015 Poonam Chandra 1 Punch line Discovery of the first multiplyimaged gravitationallylensed supernova. Anja. von . der. Linden et al., 2007, MNRAS, 379, 867. On the prevalence of radio-loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flows. P. N. Best et al., 2007, MNRAS, 379, 894. Supernovae . J081659.74+511233.7 . and . J07285387+3349106. . with . the BSU . Observatory. Benjamin . Lombard and Sarah Peck . (Mentor: Professor Jamie Kern). Bridgewater State University. Abstract. Original source: Arnett. , W.D.; et al. (1989). "Supernova 1987A". . Annual Review of Astronomy and Astrophysics. . 27. : 629–700. .. From Wikipedia article, downloaded 9/8/14, . http. ://. en.wikipedia.org/wiki/SN_1987A. . Chris Haines . (Universidad de Chile). Paula . Merluzzi. , Gianni . Busarello. , . Amata. . Mercurio. . (Naples). , . Nobuhiro. Okabe . (IPMU). , Luis . Campusano. . (. U.Chile. ). ESO: Dissecting Galaxies Near and Far, 26th March 2015. F. Abe. Nagoya University. 20th. Microlensing Workshop, IAP, Paris, . 15th. Jan 2016. Contents. Introduction. Lensing configuration and . the problem. Matrix expression. Successive approximation. Flow of the calculation (Random number algorithm). Physics Opportunities with. Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Sanduleak -69 202. Sanduleak . -. 69 202. Large Magellanic Cloud . Distance 50 kpc . (160.000 light years). Lenses. A . convex lens. (or a . converging lens. ) converges parallel light rays passing through it.. Various shapes of convex lenses. Terms for describing lenses. Optical centre. is the centre of a lens.. National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . SCIENCE. . PEOPLE TECHNOLOGY. Scientists Discover Galaxy that is 99.99 Percent Dark Matter. Instrument Chemistries for each step in the decontamination process. Pre-cleaning. Manual cleaning. Automated cleaning. Case Solutions. CSR Ink and adhesive remover. SchmutzOff stainless steel, acid based re-conditioner and . Kelsey McCabe. University of Arizona. Advisor: Dennis . Zaritsky. . Department of Astronomy. University of Arizona. Arizona Space Grant . Symposium. Arizona State University. Tempe. , AZ. Outline. A Brief Overview. 1. st. meeting: July 1992;. Globular Clusters Within the Context of Their Parent Galaxies. 2. nd. meeting: July 2011;. KraftFest. 2011. 3. rd. meeting: July 2030 . (subtitle to be decided at a later date). GUViCS. ). IV. The role of the cluster environment on galaxy evolution. Speaker: Xinkai Chen. Sample. Sample:. Extended Source . Catalogue of Voyer+14. recessional . velocity < . 3500kms-1. , Virgo cluster region. What is the brand?. 10 points. 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. Flags. 10 points. National Flags. 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. Name the Mr Men?. 10 points. 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. What is magnified?. Let’s us predict mathematically the properties of an image produced by a lens. Defining Variables. f = focal length, distance from the focus to the optical centre (F and F’ are the same distance from O)..
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