The supernova zoo HUJI winter school #35

Slides:



Advertisements
Similar presentations
Pair-Instability Explosions: observational evidence Avishay Gal-Yam, Weizmann Institute Nikko 2012.
Advertisements

Insights from Radio Wavelengths into Supernova Progenitors Laura Chomiuk Jansky Fellow, Michigan State University.
The Calán/Tololo Supernova Survey
The Physics of Supernovae
Chelsea Braun Credit: Artist illustration ESO, content/uploads/2006/12/ supernova.jpg.
Supernovae Josefine Selj, Dmitry Sharapov, Auni Somero, Linda Östman supervisor: Jesper Sollerman NORDFORSK Summer School on Observational Astrophysics.
The Flavours of SN II Light Curves Iair (“ya-eer”) Arcavi Advisor: Avishay Gal-Yam.
Exploding stars László Kiss, School of Physics, University of Sydney.
SN 2012fr in NGC 1365 Mark M. Phillips, Carlos Contreras, Eric Hsiao, Nidia Morrell, Kevin Krisciunas, Peter Brown, and Max Stritzinger.
A Chandra view to Exploding Stars SN2014J R. Margutti Harvard nothing.
ASTR Fall Semester Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture14]
From Progenitor to Afterlife Roger Chevalier SN 1987AHST/SINS.
Supernovae from Massive Stars: light curves and spectral evolution Bruno Leibundgut ESO.
Observational techniques meeting #10. Spectroscopy (Cont.)
Light Echoes from Historic Supernovae
The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different.
Supernovae Historically: “new stars” in sky Seen in 1006, 1054, 1181, 1572, 1604, 1680 SN 1054 visible in daytime sky for many months (Chinese records)
1 SDSS-II Supernova Survey Josh Frieman Leopoldina Dark Energy Conference October 8, 2008 See also: poster by Hubert Lampeitl, talk by Bob Nichol.
Observed properties of SN From Woosley Lecture 16 See also Filippenko (1997; ARAA 35, 309) See also
A Broader Perspective on the GRB-SN Connection Alicia M. Soderberg Caltech Schramm Symposium, Dec
The Transient Universe: AY 250 Spring 2007 Future Observations of SN IA Geoff Bower.
Measuring Distances. Introduction Trigonometric Parallax Spectroscopic Parallax Cepheid Variables Type Ia Supernovae Tully-Fisher Relationship Hubble’s.
Type Ia Supernovae: standard candles? Roger Chevalier.
Radio studies of mysterious Type IIn supernovae Poonam Chandra National Centre for Radio Astrophysics Tata Institute of Fundamental Research Collaborators:
Natalie RoeSNAP/SCP Journal Club “Identification of Type Ia Supernovae at Redshift 1.3 and Beyond with the Advanced Camera for Surveys on HST” Riess, Strolger,
Chapter 17: Evolution of High-Mass Stars. Massive stars have more hydrogen to start with but they burn it at a prodigious rate The overall reaction is.
SNLS : Spectroscopy of Supernovae with the VLT (status) Grégory Sainton LPNHE, CNRS/in2p3 University Paris VI & VII Paris, France On behalf of the SNLS.
Weidong Li Jesse Leaman Alex Filippenko Department of Astronomy University of California, Berkeley Nearby Supernova Rates from the Lick Observatory Supernova.
Chapter 27 Hubble’s Law and the Distance Scale Revised 2007.
Type and redshift distributions 65 candidates have been observed between June 2003 and May Redshift is measured by using emission and/or absorption.
Recent results on supernova cosmology Bruno Leibundgut.
Recent Observations of GRB-Supernovae Bethany Elisa Cobb The George Washington University IAU Symposium 279 March 13, 2012.
I'm thinking of a number. 12 is a factor of my number. What other factors MUST my number have?
Zorro and the nature of SNe Ia Paolo A. Mazzali Max-Planck Institut für Astrophysik, Garching Astronomy Department and RESearch Centre for the Early Universe,
Different Kinds of “Novae” I. Super Novae Type Ia: No hydrogen, CO WD deflagration --> detonation Type Ia: No hydrogen, CO WD deflagration --> detonation.
5-9 Nov 2012Tsinghua Transient Workshop Light curves and Spectra.
Hunting youngest Type Ia SNe in the intermediate Palomar Transient Factory Yi Cao (Caltech) On behalf of the intermediate Palomar Transient Factory collaboration.
Spectroscopic signatures of SN Ia progenitors A talk not about the Palomar Transient Factory Avishay Gal-Yam, Weizmann Institute of Science Leiden workshop.
SUPERNOVA! SN 1994D in NGC 4526, NASA / ESA / Hubble Key Project Team / High-Z Supernova Search Team
Chapter 24 Galaxies  Nick Devereux Birr Telescope - Ireland.
Ay 123 Lecture 11 - Supernovae & Neutron Stars Timescales for HS Burning faster and faster..
Radio and X-ray observations of SN 2009ip Poonam Chandra National Centre for Radio Astrophysics January 4, 2013 Collaborators: Raffaella Margutti (Harvard),
Lecture 16 Supernova Light Curves and Observations.
Formation of Dust in Various Types of Supernovae Takaya Nozawa IPMU (Institute for the Physics and Mathematics of the Universe, Univ. of Tokyo) Collaborators.
Observational Properties and Modelling of Hypernovae Jinsong Deng National Astronomical Observatories of China Collaborators: P. A. Mazzali (Trieste Obs.
Searching High-z Supernovae with HSC and WFMOS
Progenitor stars of supernovae Poonam Chandra Royal Military College of Canada.
Study of the type IIP supernova 2008gz Roy et al. 2011, MNRAS accepted.
Lessons from Spectral Evolution and High-Velocity Features in Core-Normal Type Ia J. Craig Wheeler On Behalf of the Austin Mafia: Howie Marion (+CfA),
Chapter 15.2 The classification of Supernovae. Types of Supernova.
Announcements Exam 3 is scheduled for Wednesday April 8. Will be pushed back to Monday April 13 Tentatively will cover the rest of Chapter 4, all of Chapters.
1 Observations of Cosmic Explosions Review, and results from the Palomar Transient Factory Avishay Gal-Yam | Weizmann Institute of Science Avishay Gal-Yam.
Single versus Binary Star Progenitors of Type IIb Supernovae
The monitoring of supernovae with the 6-meter telescope of SAO RAS
A photometric method to classify high-z supernovae found with HSC
The Caltech Core-Collapse Program (CCCP)
Keck Observations of Two Supernovae Hours After Explosion Shock-Breakout Flash Spectroscopy as a New Window into the Evolution and Death of Massive Stars.
Radio Emission from Embryonic Super-Luminous Supernova Remnants
Supernova Panel Discussion
Supernovae and Gamma-Ray Bursts
RADIO EMISSION FROM SNe & GRBs, AND THE NEED FOR SKA
GRB-Supernova observations: State of the art
Supernovae as sources of dust in the early universe
Single Vs binary star progenitors of Type Iib Sne
Supernovae Josefine Selj, Dmitry Sharapov, Auni Somero, Linda Östman
Observational techniques meeting #9
“What do you see. What do you think about that
Transient emission associated with the birth of neutron stars
Formation and evolution of dust in hydrogen-poor supernovae
Predicted Light Curves and Spectra
Presentation transcript:

The supernova zoo HUJI winter school #35 My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Supernova Classification The classification of supernovae is based almost entirely on peak visible-light spectra. This classification method was first proposed by Minkowski (1941; Type I/Type II) and developed since. Filippenko (1997) provided the classical review of this subject. The chapter “observational and physical classification of supernovae” in the “SN Handbook” (Gal-Yam 2016) provides a modern reference. My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type I supernovae (no hydrogen) My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ia My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ia - peculiars My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ia family – early, peculiar My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ia family – nebular, interacting My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ib/c supernovae (no hydrogen) My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ib My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Peculiar Type Ib My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Interacting Type Ibn My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ic My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type Ic-BL My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type I – nebular – Ca rich Ib My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type I – nebular – interactors My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Quantitative separation of Type I SNe Sun & Gal-Yam 2017 My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Hydrogen in SNe Ib My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type I – light curve outliers Taddia My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe De

Hydrogen rich Sne: Type II My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type II - regular My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type II - evolution My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type IIb - transitional My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Type IIn - interacting My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

SLSNe Superluminous SNe My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

SLSNe - peak My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

SLSNe - late My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Summary My name is … I’m so glad to end this evening and have the opportunity to share with you some of our wonder at the universe

Thanks