John Antoniadis CV. Max-Planck-Institut für Radioastronomie. Argelander Institut für Astronomie, Auf den Hügel 69/71, Bonn, DE

Size: px
Start display at page:

Download "John Antoniadis CV. Max-Planck-Institut für Radioastronomie. Argelander Institut für Astronomie, Auf den Hügel 69/71, Bonn, DE"

Transcription

1 John Antoniadis CV Max-Planck-Institut für Radioastronomie & Argelander Institut für Astronomie, Auf den Hügel 69/71, Bonn, DE +49 (0) antoniadisjohn.com ORCID: last modified: October 2018 Biographical Information Name: John (Ioannis) Antoniadis Birthday: August 11, 1986 Place of Birth: Didymoteicho, Greece Citizenship: Greek, Cypriot Research Interests Formation and evolution of compact stars, binary neutron stars, radio pulsars, tests of fundamental physics, equation-of-state of nuclear matter, peculiar optical transients Employment History Postdoctoral Research Fellow Max-Planck-Institut für Radioastronomie 2017 now Bonn, DE Dunlap Fellow Dunlap Institute for Astronomy & Astrophysics, Toronto, CA Postdoctoral Research Fellow Max-Planck-Institut für Radioastronomie Bonn, DE Education Doctor of Natural Sciences University of Bonn Bonn, DE suma cum laude Thesis: Multi-wavelength studies of pulsars and their companions Supervisor: Prof. Dr. Michael Kramer Diploma in Physics Aristotle University of Thessaloniki Thessaloniki, GR magna cum laude Thesis: Transits of extrasolar planets Supervisor: Prof. Dr. John H. Seiradakis Awards and Fellowships John Charles Polanyi Prize in Physics 2016 Government of Ontario TalentEdge Fellowship 2015 Ontario Centres of Excellence Dunlap Fellowship Dunlap Institute for Astronomy & Astrophysics Springer Thesis Award 2013 Springer-Verlag 1/6

2 Otto Hahn Medal for Physics 2014 Max Planck Society Citation: For the study of pulsars and their companions and the resulting new insights for gravitational physics and the equation of state of matter at super-nuclear densities Best Thesis in nuclear, atomic and gravitational physics 2014 German Physics Society University of Bonn 2013 Best Thesis Award IMPRS Fellowship International Max-Planck Research School for Astronomy & Astrophysics Professional Associations International Astronomical Union Junior Member European Astronomical Society Ordinary Member Hellenic Astronomical Society Ordinary Member 2018 now 2014 now 2014 now Teaching and Mentoring Courses and Labs Optical Spectroscopy Lab 2015 Dunlap Instrumentation Summer School Role: Tutor Introduction to Astronomy 2006, 2007 Aristotle University of Thessaloniki Role: Teaching Assistant Student Mentorship Graduate Students Tasha Gautam 2018 now Project: Mass measurements of millisecond pulsars Tilemachos Athanasiadis Project: Targeted pulsar surveys Master Students Savvas Chanlaridis Project: Evolution of ultra-stripped helium stars towards core collapse Undergraduate Students 2017 now 2018 now Abhinav Jindal 2017 Project: Pulsar timing constraints on the masses and orbits of objects in the outer solar system Summer Undergraduate Research Program in Astrophysics at the Shannon Brown 2017 Project: High-cadence Multi-color Observations of the Dwarf Nova KSP-OT a Summer Undergraduate Research Program in Astrophysics at the Nicole Mateo 2015, 2016 Project: Optical Photometry of the companion to PSR J Summer Undergraduate Research Program in Astrophysics at the Chris Peacock 2015 Project: Cooling of irradiated white dwarfs Summer Undergraduate Research Program in Astrophysics at the 2/6

3 Training Didactics at the University 2018 MPIfR; 1-2 October 2018 Two-day training seminar on university didactic methods; Lecturer: Alexandra Bergedick Conference Organizing 13th BONN workshop on the formation and evolution of neutron stars 2018 December 10, 2018 Role: Chair of the SOC 12th BONN workshop on the formation and evolution of neutron stars 2018 May 14, 2018 Role: Chair of the SOC Extreme Astrophysics in an Ever-changing Universe 2014 Ierapetra, Crete; June Role: main organizer (with Dr. Emmanouil Angelakis) Invited Talks (selected) Radio millisecond pulsars as probes of binary evolution th BONN workshop on the formation and evolution of neutron stars Bonn, Germany Optical observations of pulsar companions and the nuclear matter equation-of-state 2015 The many faces of neutron stars Garching, Germany The millisecond pulsar mass distribution th Marcel Grosmann Meeting Rome, Italy Pulsar - white dwarf binaries as gravity labs th Marcel Grosmann Meeting Rome, Italy Compact binary pulsars as laboratories for fundamental physics rd Session of the Saint Cugat Forum on Astrophysics: Gravitational Waves Astrophysics Sait Cugat, Spain The compact relativistic binary PSR J Physical Applications of Millisecond Pulsars Aspen, USA Testing strong-field gravity with a massive pulsar th Quantum-to-Cosmos meeting Bensberg, Germany Administration Duties and Service to Profession University Chair of the Summer University Research Program in Astrophysics Scientists representative in the Astronomy Faculty Committee 2015 Member of the DAA/DI/CITA graduate admissions committee 2015 Community Regular referee for: the Astrophysical Journal, the Astrophysical Journal Letters, Monthly Notices of the Royal Astronomical Society, Nature Physics and others Referee for the time allocation committees of: GMRT, China Telescope Access Programme (Gemini) Grand proposal reviewer for the Czech Science Foundation 3/6

4 Telescope Observing Proposals (selected) The European Pulsar Interior Composition Survey [PI] now Effelsberg Radio Telescope 130+ hours The transitional millisecond pulsar PSR J [PI] 2015 Kepler K2 - C11 Program GO11901 (Short-cadence mode) Spectroscopic follow-up of infant supernovae discovered by KMTNet [PI] 2015 Gemini South 14 hours in rapid response mode Probing the properties of the double pulsar emission at low frequencies [PI] 2015 Giant Metrewave Radio Telescope 10 hours Mass determination of an eclipsing binary pulsar using X-Shooter [PI] nights; Programme 093.D-0580 Mass determination of the first eccentric binary pulsar with a white-dwarf companion [PI] hours; Programme 093.D-0108 Photometry of the massive relativistic binary pulsar PSR J [PI] 2012 William Herschel Telescope/ULTRACAM 5 hours The properties for the pulsar - white dwarf system with the shortest orbital period [PI] nights; Programme 088.D-0138 Deep imaging of the white dwarf companion of an extremely low mass neutron star candidate [PI] hours; Programme 087.D-0898 Outreach and Media Press releases Dunlap Fellow Dr. John Antoniadis Awarded Prestigious 2016 Polanyi Prize in Physics 2016 Dunlap Institute for Astronomy & Astrophysics, UofT Amateur Astronomer Helps Uncover Secrets of Unique Pulsar Binary System 2016 Dunlap Institute for Astronomy & Astrophysics, UofT Excellent Pulsar Research 2014 Max-Planck-Institut für Radionastronomie A heavyweight for Einstein 2013 Max-Planck-Gesellschaft & Max-Planck-Institut für Radionastronomie Record-breaking pulsar takes tests of general relativity into new territory 2013 European Southern Observatory Einstein s Gravity Theory Passes Toughest Test Yet 2013 National Radio Astronomy Observatory Arecibo Telescope Used to Study Neutron Star Twice as Massive as the Sun 2013 Arecibo Telescope, Universities Space Research Association A heavyweigt for Einstein: Probing gravity where no one has done it before 2013 European Research Council Bizarre binary star system pushes study of relativity to new limits 2013 [In German]Kosmisches Schwergewicht gibt Einstein Recht 2013 University of Bonn 4/6

5 Interviews [in Greek] Looking for Einstein s Achilles heel 2013 newspaper To Vima Podcast Interview for Science Online 2013 Science (vol. 340, n. 6131) Media Coverage (selected) An amateur astronomer just made a stellar discovery about pulsars 2016 Astronomy.com A pulsar and a white dwarf in an unexpected orbit 2016 Nova; AAS Highlights Black hole binge could test general relativity 2013 New Scientist, Issue: 2915 Extreme binary pulsar shows no deviation from general relativity 2013 Physics Today, Vol. 66, Issue 7 Massive double star is latest test for Einstein s gravity theory 2013 Nature, Issue: Exotic Objects Test Einstein s Theory 2012 Sky & Telescope [in German] Auf der Suche nach extrasolaren Transitplaneten 2010 Sterne und Weltraum Ten Most Significant Publications A detailed publication list is available upon request 1 J. Antoniadis. On the Formation of Eccentric Millisecond Pulsars with Helium White-dwarf Companions. the Astrophysical Journal Letters, 797:L24, December J. Antoniadis, P. C. C. Freire, N. Wex, T. M. Tauris, R. S. Lynch, M. H. van Kerkwijk, M. Kramer, C. Bassa, V. S. Dhillon, T. Driebe, J. W. T. Hessels, V. M. Kaspi, V. I. Kondratiev, N. Langer, T. R. Marsh, M. A. McLaughlin, T. T. Pennucci, S. M. Ransom, I. H. Stairs, J. van Leeuwen, J. P. W. Verbiest, and D. G. Whelan. A Massive Pulsar in a Compact Relativistic Binary. Science, 340:448, April J. Antoniadis, D. L. Kaplan, K. Stovall, P. C. C. Freire, J. S. Deneva, D. Koester, F. Jenet, and J. G. Martinez. An Eccentric Binary Millisecond Pulsar with a Helium White Dwarf Companion in the Galactic field. the Astrophysical Journal, 830:36, October J. Antoniadis, D.-S. Moon, Y. Q. Ni, D.-J. Kim, Y. Lee, and H. Neilson. Discovery of a Rapid, Luminous Nova in NGC 300 by the KMTNet Supernova Program. the Astrophysical Journal, 844:160, August J. Antoniadis, T. M. Tauris, F. Ozel, E. Barr, D. J. Champion, and P. C. C. Freire. The millisecond pulsar mass distribution: Evidence for bimodality and constraints on the maximum neutron star mass. ArXiv e-prints, May J. Antoniadis, M. H. van Kerkwijk, D. Koester, P. C. C. Freire, N. Wex, T. M. Tauris, M. Kramer, and C. G. Bassa. The relativistic pulsar-white dwarf binary PSR J I. Mass determination and evolutionary history. Monthly Notices of the Royal Astronomical Society, 423: , July P. C. C. Freire, N. Wex, G. Esposito-Farèse, J. P. W. Verbiest, M. Bailes, B. A. Jacoby, M. Kramer, I. H. Stairs, J. Antoniadis, and G. H. Janssen. The relativistic pulsar-white dwarf binary PSR J II. The most stringent test of scalar-tensor gravity. Monthly Notices of the Royal Astronomical Society, 423: , July A. G. Istrate, T. M. Tauris, N. Langer, and J. Antoniadis. The timescale of low-mass proto-helium white dwarf evolution. Astronomy & Astrophysics, 571:L3, November /6

6 9 T. M. Tauris, M. Kramer, P. C. C. Freire, N. Wex, H.-T. Janka, N. Langer, P. Podsiadlowski, E. Bozzo, S. Chaty, M. U. Kruckow, E. P. J. van den Heuvel, J. Antoniadis, R. P. Breton, and D. J. Champion. Formation of Double Neutron Star Systems. the Astrophysical Journal, 846:170, September A. D. van Staden and J. Antoniadis. An Active, Asynchronous Companion to a Redback Millisecond Pulsar. the Astrophysical Journal Letters, 833:L12, December /6

The Hunt for New Pulsars with the Green Bank Telescope

The Hunt for New Pulsars with the Green Bank Telescope The Hunt for New Pulsars with the Green Bank Telescope Ryan Lynch Postdoctoral Fellow McGill University What we'll talk about... Two most recent large-area GBT pulsar surveys the 350 MHz Drift Scan Survey

More information

Pulsar Key Science with the SKA

Pulsar Key Science with the SKA Pulsar Key Science with the SKA Strong-field tests of gravity using Pulsars and Black Holes Michael Kramer Krabi, April 2007 Pulsar Key Science with the SKA Strong-field tests of gravity using Pulsars

More information

In Search of New MSPs for Pulsar Timing Arrays. Kevin Stovall, NRAO Socorro NANOGrav Collaboration

In Search of New MSPs for Pulsar Timing Arrays. Kevin Stovall, NRAO Socorro NANOGrav Collaboration In Search of New MSPs for Pulsar Timing Arrays Kevin Stovall, NRAO Socorro NANOGrav Collaboration NRAO Postdoc Symposium, March 27, 2017 NANOGrav = US/Canada-based collaboration working to detect nhz GW

More information

High Precision Pulsar Timing at Arecibo Observatory

High Precision Pulsar Timing at Arecibo Observatory High Precision Pulsar Timing at Arecibo Observatory What are pulsars? When the cores of massive stars run out of nuclear fuel they collapse catastrophically. Their immense gravitational field, now unopposed,

More information

Gravity with the SKA

Gravity with the SKA Gravity with the SKA Strong-field tests of gravity using Pulsars and Black Holes Michael Kramer Jodrell Bank Observatory University of Manchester With Don Backer, Jim Cordes, Simon Johnston, Joe Lazio

More information

Curriculum Vitae. Prof. Dr. Thomas Henning

Curriculum Vitae. Prof. Dr. Thomas Henning Curriculum Vitae Prof. Dr. Thomas Henning Max Planck Institute for Astronomy Königstuhl 17 69117 Heidelberg Germany Phone: +49-6221-528-200 Fax: +49-6221-528-339 Position: Director E-mail: henning@mpia.de

More information

CURRICULUM VITAE. Natalia Ivanova

CURRICULUM VITAE. Natalia Ivanova CURRICULUM VITAE Natalia Ivanova Assistant Professor of Physics Email: nata.ivanova@ualberta.ca Dept. of Physics Office: +1 (780) 248-1899 University of Alberta FAX: +1 (780) 492-0714 CEB, 11322-89 Ave

More information

Bernard Frederick Schutz

Bernard Frederick Schutz 1 of 5 29/01/2007 18:13 Homepage of Bernard Schutz 14 / 24 Bernard Frederick Schutz Director, Max Planck Institute for Gravitational Physics Born 11 August 1946, Paterson, NJ, USA Nationality: USA (by

More information

Starlight in the Night: Discovering the secret lives of stars

Starlight in the Night: Discovering the secret lives of stars Utah State University DigitalCommons@USU Public Talks Astrophysics 8-2-2008 Starlight in the Night: Discovering the secret lives of stars Shane L. Larson Utah State University Follow this and additional

More information

Gravity Tests with Radio Pulsars

Gravity Tests with Radio Pulsars Gravity Tests with Radio Pulsars Norbert Wex Paris, June 21 st, 2010 Regimes of Gravity Tests (1) Quasi-stationary weak-field regime Solar system experiments (2) Quasi-stationary strong-field regime (3)

More information

Astronomy. Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes

Astronomy. Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes Astronomy Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes are hot, compact stars whose mass is comparable to the Sun's and size to the Earth's. A. White dwarfs B. Neutron stars

More information

Measurements of Neutron Star Masses with a strong emphasis on millisecond binary radio pulsar timing

Measurements of Neutron Star Masses with a strong emphasis on millisecond binary radio pulsar timing Measurements of Neutron Star Masses with a strong emphasis on millisecond binary radio pulsar timing David Nice, Lafayette College Physics of Neutron Stars 2014, Saint Petersburg 1. Motivation 2. How to

More information

Five and a half roads to from a millisecond pulsar. Thomas Tauris AIfA, University of Bonn Max-Planck-Institut für Radioastronomie, Bonn

Five and a half roads to from a millisecond pulsar. Thomas Tauris AIfA, University of Bonn Max-Planck-Institut für Radioastronomie, Bonn Five and a half roads to from a millisecond pulsar Thomas Tauris AIfA, University of Bonn Max-Planck-Institut für Radioastronomie, Bonn Evolution of Compact Binaries, ESO Chile, March 6-11, 2011 Millisecond

More information

Long-term radio observations of orbital phase wander in six eclipsing pulsar binaries. Brian Prager Department of Astronomy University of Virginia

Long-term radio observations of orbital phase wander in six eclipsing pulsar binaries. Brian Prager Department of Astronomy University of Virginia Long-term radio observations of orbital phase wander in six eclipsing pulsar binaries. Brian Prager Department of Astronomy University of Virginia Collaborators: Scott Ransom (NRAO), Phil Arras (UVa),

More information

Measurements of binary pulsar masses and a study on the nature of gravitational waves

Measurements of binary pulsar masses and a study on the nature of gravitational waves Measurements of binary pulsar masses and a study on the nature of gravitational waves Paulo C. C. Freire Max-Planck-Institut für Radioastronomie Bonn, Germany 2016 November 2, ``Compact Stars and Gravitational

More information

EWASS Thomas Tauris Argelander-Institut für Astronomie - Universität Bonn Max-Planck-Institut für Radioastronomie

EWASS Thomas Tauris Argelander-Institut für Astronomie - Universität Bonn Max-Planck-Institut für Radioastronomie EWASS 2015 Thomas Tauris Argelander-Institut für Astronomie - Universität Bonn Max-Planck-Institut für Radioastronomie Collaborators on Pulsars / Compact Binaries / SNe research John Antoniadis Hai-Liang

More information

The Hertzprung-Russell Diagram. The Hertzprung-Russell Diagram. Question

The Hertzprung-Russell Diagram. The Hertzprung-Russell Diagram. Question Key Concepts: Lecture 21: Measuring the properties of stars (cont.) The Hertzsprung-Russell (HR) Diagram (L versus T) The Hertzprung-Russell Diagram The Stefan-Boltzmann Law: flux emitted by a black body

More information

Pulsar Overview. Kevin Stovall NRAO

Pulsar Overview. Kevin Stovall NRAO Pulsar Overview Kevin Stovall NRAO IPTA 2018 Student Workshop, 11 June, 2018 Pulsars Pulsars ~2,700 pulsars known Act as clocks, therefore provide a means for studying a variety of physical phenomena Strongly

More information

Postdoctoral researcher, ASTRON Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, Supervisor: Dr. Joeri van Leeuwen.

Postdoctoral researcher, ASTRON Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, Supervisor: Dr. Joeri van Leeuwen. Emily Petroff PhD, Astrophysics ASTRON Netherlands Institute for Radio Astronomy Oude Hoogeveensedijk 4 7995 PD Dwingeloo, Netherlands (+31) 0611 201 941 (+31) 0521 595 794 ebpetroff@gmail.com www.ebpetroff.com

More information

Pulsars. in this talk. Pulsar timing. Pulsar timing. Pulsar timing. Pulsar timing. How to listen to what exotic. are telling us! Paulo César C.

Pulsars. in this talk. Pulsar timing. Pulsar timing. Pulsar timing. Pulsar timing. How to listen to what exotic. are telling us! Paulo César C. How to listen to what exotic Pulsars are telling us! in this talk 1. 2. 3. Test of gravitational theories using binary pulsars 4. Probing the equation of state of super-dense matter Paulo César C. Freire

More information

CURRICULUM VITAE. Christian Wolf Department of Mathematics Wichita State University. Wichita, KS Citizenship: Germany, Permanent Resident: USA

CURRICULUM VITAE. Christian Wolf Department of Mathematics Wichita State University. Wichita, KS Citizenship: Germany, Permanent Resident: USA CURRICULUM VITAE Christian Wolf Department of Mathematics Wichita State University Wichita, KS 67260 Citizenship: Germany, Permanent Resident: USA e mail: cwolf@math.wichita.edu Phone #: Office: 316 978

More information

arxiv: v1 [gr-qc] 28 Oct 2012

arxiv: v1 [gr-qc] 28 Oct 2012 Neutron Stars and Pulsars: Challenges and Opportunities after 80 years Proceedings IAU Symposium No. 291, 2012 c 2012 International Astronomical Union J. van Leeuwen, ed. DOI: 00.0000/X000000000000000X

More information

Supernova-accelerated Electrons to Dark Matter: A Career in Radio Astronomy. Professor Dr Uli Klein

Supernova-accelerated Electrons to Dark Matter: A Career in Radio Astronomy. Professor Dr Uli Klein Supernova-accelerated Electrons to Dark Matter: A Career in Radio Astronomy Professor Dr Uli Klein SUPERNOVA-ACCELERATED ELECTRONS TO DARK MATTER: A CAREER IN RADIO ASTRONOMY Considering we didn t know

More information

AN INTRODUCTIONTO MODERN ASTROPHYSICS

AN INTRODUCTIONTO MODERN ASTROPHYSICS AN INTRODUCTIONTO MODERN ASTROPHYSICS Second Edition Bradley W. Carroll Weber State University DaleA. Ostlie Weber State University PEARSON Addison Wesley San Francisco Boston New York Cape Town Hong Kong

More information

arxiv: v1 [astro-ph.im] 30 Oct 2012

arxiv: v1 [astro-ph.im] 30 Oct 2012 Neutron Stars and Pulsars: Challenges and Opportunities after 80 years Proceedings IAU Symposium No. 291, 2012 c 2012 International Astronomical Union J. van Leeuwen, ed. DOI: 00.0000/X000000000000000X

More information

PoS(SSC2015)051. Multi-tomography of polars from SALT spectroscopy

PoS(SSC2015)051. Multi-tomography of polars from SALT spectroscopy from SALT spectroscopy Stephen B. Potter 1 South African Astronomical Observatory Cape Town, South Africa E-mail: sbp@saao.ac.za Enrico J. Kotze South African Astronomical Observatory and Astrophysics,

More information

PhD student University of Florence, Italy Advisor: Prof. Franco Pacini Thesis: Particle acceleration and transport in Pulsar Wind Nebulae

PhD student University of Florence, Italy Advisor: Prof. Franco Pacini Thesis: Particle acceleration and transport in Pulsar Wind Nebulae Elena Amato INAF-Osservatorio Astrofisico di Arcetri Largo E. Fermi, 5 50125 - Firenze, Italy Office: +39 055 2752 236 Fax: +39 055 220039 E-mail: amato@arcetri.astro.it ACADEMIC TRAINING 2001, Ph.D. in

More information

ASTR2050: Introductory Astronomy and Astrophysics Syllabus for Spring 1999 January 4, 1999

ASTR2050: Introductory Astronomy and Astrophysics Syllabus for Spring 1999 January 4, 1999 ASTR2050: Introductory Astronomy and Astrophysics Syllabus for Spring 1999 January 4, 1999 This is a working document and will change periodically. It outlines the topics that will be covered during the

More information

Stellar-Mass Black Holes and Pulsars

Stellar-Mass Black Holes and Pulsars Stellar-Mass Black Holes and Pulsars Anthony Rushton Work group 2 leader (ESO ALMA fellow) 2010-06-24 Overview of Work Group 2 Stellar-mass black holes and pulsars Two work group leaders: Anthony Rushton

More information

Robert C. Morehead Curriculum Vitae

Robert C. Morehead Curriculum Vitae Robert C. Morehead Curriculum Vitae Department of Physics & Astronomy Texas Tech University Box 41051 Lubbock, TX 79409-1051 www.robertmorehead.com robert.morhead@ttu.edu (806) 834 7940 Education Doctoral

More information

DEPARTMENT OF ASTRONOMY

DEPARTMENT OF ASTRONOMY Department of Astronomy 1 DEPARTMENT OF ASTRONOMY 567 Sears Library Building http://astronomy.case.edu/ Phone: 216.68.278 Stacy S. McGaugh, Department Chair dept@astroweb.case.edu The Department of Astronomy

More information

Lecture 13: Binary evolution

Lecture 13: Binary evolution Lecture 13: Binary evolution Senior Astrophysics 2017-04-12 Senior Astrophysics Lecture 13: Binary evolution 2017-04-12 1 / 37 Outline 1 Conservative mass transfer 2 Non-conservative mass transfer 3 Cataclysmic

More information

Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003

Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003 Name: Seat Number: Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003 Do not open the test until instructed to begin. Instructions: Write your answers in the space provided. If you need additional

More information

Dr. Bailey E. Tetarenko Department of Physics University of Alberta Edmonton, Canada

Dr. Bailey E. Tetarenko Department of Physics University of Alberta Edmonton, Canada Education Dr. Bailey E. Tetarenko Department of Physics University of Alberta Edmonton, Canada Email: btetaren@ualberta.ca Ph.D., Physics September 2014-August 2018 Supervisor: Gregory R. Sivakoff Thesis

More information

The timescale of low-mass proto-helium white dwarf evolution

The timescale of low-mass proto-helium white dwarf evolution Astronomy & Astrophysics manuscript no. itla14 c ESO 2014 October 22, 2014 Letter to the Editor The timescale of low-mass proto-helium white dwarf evolution A. G. Istrate 1,, T. M. Tauris 1,2 N. Langer

More information

Student Review Investigations in Earth and Space Science Semester A 2015 Examination

Student Review Investigations in Earth and Space Science Semester A 2015 Examination Investigations in Earth and Space Science Semester A Examination Test Description Length: 2 hours Items: 56 SR (85%), 2 BCRs (15%) Unit Approximate Number of Selected Response Items IESS Skills and Processes

More information

Astronomy Today. Eighth edition. Eric Chaisson Steve McMillan

Astronomy Today. Eighth edition. Eric Chaisson Steve McMillan Global edition Astronomy Today Eighth edition Eric Chaisson Steve McMillan The Distance Scale ~1 Gpc Velocity L Distance Hubble s law Supernovae ~200 Mpc Time Tully-Fisher ~25 Mpc ~10,000 pc Time Variable

More information

Black holes in dormant X-ray transients

Black holes in dormant X-ray transients Mem. S.A.It. Vol. 83, 213 c SAIt 2012 Memorie della Black holes in dormant X-ray transients J. Ziółkowski Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warszawa, Poland e-mail: jz@camk.edu.pl

More information

MILLISECOND PULSAR POPULATION

MILLISECOND PULSAR POPULATION MILLISECOND PULSAR POPULATION on Formation and Evolution Of Neutron Stars 11/12/2017 COMPANY NAME Outline 1. Millisecond Pulsars 2.Current Population 3.Applications 4.Future Prospects 4.1.Potential Science

More information

Stars. The composition of the star It s temperature It s lifespan

Stars. The composition of the star It s temperature It s lifespan Stars Stars A star is a ball of different elements in the form of gases The elements and gases give off electromagnetic radiation (from nuclear fusion) in the form of light Scientists study the light coming

More information

Life as an Astronomer:

Life as an Astronomer: 1. What do Astronomers Study? Planets Solar System Stars Star Stuff (Interstellar Medium) Galaxies AGN/Quasars Clusters Universe 1 1. What do Astronomers Study? Solar System Sun Solar Wind Planets Moons

More information

Assistant Professor of Physics, Division of Astrophysics

Assistant Professor of Physics, Division of Astrophysics (JANUARY 2012) Walter Breitinger Anna Frebel Assistant Professor of Physics, Division of Astrophysics Professor Anna Frebel s broadly cover the chemical and physical conditions of the early Universe, and

More information

Planet-like Companion to a Brown Dwarf

Planet-like Companion to a Brown Dwarf National Aeronautics and Space Administration Planet-like Companion to a Brown Dwarf Taken from: Hubble 2010: Science Year in Review Produced by NASA Goddard Space Flight Center and the Space Telescope

More information

Ben K. D. Pearce benkdpearce.com

Ben K. D. Pearce benkdpearce.com Ben K. D. Pearce benkdpearce.com Research Interests Contact Information -Origins of life McMaster University -Prebiotic chemistry ABB-253, 1280 Main St. W -The RNA world Hamilton, ON, Canada L8S 4M1 -Meteoritic

More information

Logistics. Test 3 will be 4/24 MRS 2 due Thursday 4/17

Logistics. Test 3 will be 4/24 MRS 2 due Thursday 4/17 Stellar Evolution Logistics Test 3 will be 4/24 MRS 2 due Thursday 4/17 GTA Award The Graduate Teaching Assistant Excellence Award is an internal initiative which is intended to promote, recognize, and

More information

Pulsars and Radio Transients. Scott Ransom National Radio Astronomy Observatory / University of Virginia

Pulsars and Radio Transients. Scott Ransom National Radio Astronomy Observatory / University of Virginia Pulsars and Radio Transients Scott Ransom National Radio Astronomy Observatory / University of Virginia TIARA Summer School on Radio Astronomy 2016 Radio Transients Non-thermal emission Emission types

More information

Visiting Assistant Professor at Space Science Institute, Macau University of Science and Technology, December 2015 October 2016

Visiting Assistant Professor at Space Science Institute, Macau University of Science and Technology, December 2015 October 2016 Academic Staff Resume Name: Chih-Hao Hsia Title: Research Fellow Space Science Institute Office:A 505 Tel.:+853-8897 3350 E-mail:chhsia@must.edu.mo Photo Academic Qualification: Ph.D. in Astronomy, Graduate

More information

Chapter 21: Stars Notes

Chapter 21: Stars Notes Branches of Earth Science Chapter 21: Stars Notes Astronomy: The study of planets, stars, and other objects in space. Lithosphere: the land masses of earth o Litho means rock Hydrosphere: waters of the

More information

Bringing Real-time Astronomical Observations into the Classroom

Bringing Real-time Astronomical Observations into the Classroom Bringing Real-time Astronomical Observations into the Classroom Prof. Lynn Cominsky Sonoma State University Department of Physics and Astronomy and NASA Education and Public Outreach Group Why do astronomical

More information

New Insights from the Optical Study of Spiders

New Insights from the Optical Study of Spiders New Insights from the Optical Study of Spiders Rene Breton University of Manchester with many collaborators (V. Dhillon, J. Hessels, M. van Kerkwijk, M. Roberts, ) EWASS 25 June 2015 SDO/AIA/AEI Why Do

More information

Charli Sakari. 2014, Post-doctoral Research Associate Department of Astronomy, University of Washington

Charli Sakari. 2014, Post-doctoral Research Associate Department of Astronomy, University of Washington Charli Sakari Department of Astronomy Box 351580, U.W. Seattle, WA 98195-1580 Email: sakaricm@u.washington.edu 3108 NE 55 th Street Seattle, WA 98105 (541) 914-3861 Citizenship: http://www.faculty.washington.edu/sakaricm

More information

CURRICULUM VITAE Roman V. Krems

CURRICULUM VITAE Roman V. Krems CURRICULUM VITAE Roman V. Krems POSTAL ADDRESS: Department of Chemistry, University of British Columbia 2036 Main Mall, Vancouver, B.C. Canada V6T 1Z1 Telephone: +1 (604) 827 3151 Telefax: +1 (604) 822

More information

PoS(ISKAF2010)080. The European Pulsar Timing Array. Roy Smits. The EPTA collaboration

PoS(ISKAF2010)080. The European Pulsar Timing Array. Roy Smits. The EPTA collaboration The University of Manchester, School of Physics and Astronomy, Jodrell Bank Netherlands Institute for Radio Astronomy (ASTRON), Dwingeloo, The Netherlands E-mail: rsmits@jb.man.ac.uk The EPTA collaboration

More information

Yale Center for Astronomy and Astrophysics, New Haven, USA YCAA Prize Fellowship

Yale Center for Astronomy and Astrophysics, New Haven, USA YCAA Prize Fellowship Pascal A. Oesch Yale Center for Astronomy and Astrophysics, JWG 469, P.O. Box 208120, New Haven, CT 06520 Phone: +1 203 432 1265! E-Mail: pascal.oesch@yale.edu Web: www.astro.yale.edu/poesch Research Interests

More information

imin...

imin... Pulsar Timing For a detailed look at pulsar timing and other pulsar observing techniques, see the Handbook of Pulsar Astronomy by Duncan Lorimer and Michael Kramer. Pulsars are intrinsically interesting

More information

ASTRONOMY FACULTY UNDERGRADUATE PROGRAM DEPARTMENTAL ADVISING EXPERTS. Astronomy 1

ASTRONOMY FACULTY UNDERGRADUATE PROGRAM DEPARTMENTAL ADVISING EXPERTS. Astronomy 1 Astronomy 1 ASTRONOMY The Wesleyan Astronomy Department provides outstanding opportunities for undergraduates who wish to major in this fascinating subject, either in preparation for graduate school or

More information

Masses, Radii, and Equation of State of Neutron Stars

Masses, Radii, and Equation of State of Neutron Stars Masses, Radii, and Equation of State of Neutron Stars arxiv:1603.02698v1 [astro-ph.he] 8 Mar 2016 Xxxx. Xxx. Xxx. Xxx. YYYY. 00:1 39 This article s doi: 10.1146/((please add article doi)) Copyright c YYYY

More information

The Formation of the Most Relativistic Pulsar PSR J

The Formation of the Most Relativistic Pulsar PSR J Binary Radio Pulsars ASP Conference Series, Vol. 328, 2005 F. A. Rasio and I. H. Stairs The Formation of the Most Relativistic Pulsar PSR J0737 3039 B. Willems, V. Kalogera, and M. Henninger Northwestern

More information

Supernova Explosions. Novae

Supernova Explosions. Novae Supernova Explosions Novae Novae occur in close binary-star systems in which one member is a white dwarf. First, mass is transferred from the normal star to the surface of its white dwarf companion. 1

More information

Academic profile of the faculty member

Academic profile of the faculty member Academic profile of the faculty member 1. Name: PRAVEEN SINGH NEGI. 2. Father s Name: Late. Mr. B. S. NEGI. 3. Date of birth: 10/01/1963 (10 JANUARY 1963). 4. Marital status: Married. 5. Affiliated Institution:

More information

NS masses from radio timing: Past, present and future. Paul Demorest (NRAO) Symposium on Neutron Stars, Ohio U., May 2016

NS masses from radio timing: Past, present and future. Paul Demorest (NRAO) Symposium on Neutron Stars, Ohio U., May 2016 NS masses from radio timing: Past, present and future Paul Demorest (NRAO) Symposium on Neutron Stars, Ohio U., May 2016 Overview Review of how to measure neutron star masses via radio pulsar timing. Summary

More information

Testing General Relativity with Relativistic Binary Pulsars

Testing General Relativity with Relativistic Binary Pulsars Testing General Relativity with Relativistic Binary Pulsars Ingrid Stairs UBC GWPAW Milwaukee Jan. 29, 2011 Green Bank Telescope Jodrell Bank Parkes Arecibo Outline Intro to pulsar timing Equivalence principle

More information

Santiago del Palacio. Academic Formation. Fellowships. PhD Courses

Santiago del Palacio. Academic Formation. Fellowships. PhD Courses Santiago del Palacio Academic Formation PhD in Astronomy, Faculty of Astronomical and Geophysical Sciences, La Plata National University., La Plata. 2008 2014 Ms.S. in Astronomy, Faculty of Astronomical

More information

Probing Relativistic Gravity with the Double Pulsar

Probing Relativistic Gravity with the Double Pulsar Probing Relativistic Gravity with the Double Pulsar Marta Burgay INAF Osservatorio Astronomico di Cagliari The spin period of the original millisecond pulsar PSR B1937+21: P = 0.0015578064924327 ± 0.0000000000000004

More information

Testing Gravity and Extreme Physics with Pulsars

Testing Gravity and Extreme Physics with Pulsars Testing Gravity and Extreme Physics with Pulsars John Rowe Animation Australia Telescope National Facility, CSIRO René Breton School of Physics & Astronomy The University of Manchester Liverpool Physics

More information

The Milky Way Galaxy. Some thoughts. How big is it? What does it look like? How did it end up this way? What is it made up of?

The Milky Way Galaxy. Some thoughts. How big is it? What does it look like? How did it end up this way? What is it made up of? Some thoughts The Milky Way Galaxy How big is it? What does it look like? How did it end up this way? What is it made up of? Does it change 2 3 4 5 This is not a constant zoom The Milky Way Almost everything

More information

David B Fisher Curriculum Vitae

David B Fisher Curriculum Vitae David B Fisher Curriculum Vitae Contact Current e-mail: dbfisher@astro.umd.edu CARMA Postdoctoral Fellow (2010-present) University of Maryland Joint Space Science Institute Scientist Education University

More information

Death of Stars Part II Neutron Stars

Death of Stars Part II Neutron Stars Death of Stars Part II Neutron Stars 1 REMEMBER THIS!? 2 Guiding Questions 1. What led scientists to the idea of a neutron star? 2. What are pulsars, and how were they discovered? 3. How did astronomers

More information

Lecture Outlines. Chapter 22. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 22. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 22 Astronomy Today 8th Edition Chaisson/McMillan Chapter 22 Neutron Stars and Black Holes Units of Chapter 22 22.1 Neutron Stars 22.2 Pulsars 22.3 Neutron-Star Binaries 22.4 Gamma-Ray

More information

General Relativity Tests with Pulsars

General Relativity Tests with Pulsars General Relativity Tests with Pulsars Ingrid Stairs UBC Rencontres de Moriond La Thuile March 25, 2011 Green Bank Telescope Jodrell Bank Parkes Arecibo Outline Intro to pulsar timing Equivalence principle

More information

A Pulsar Timing Array for Gravitational Wave Detection. Paul Demorest, NRAO

A Pulsar Timing Array for Gravitational Wave Detection. Paul Demorest, NRAO A Pulsar Timing Array for Gravitational Wave Detection Paul Demorest, NRAO About 10% of known radio pulsars are recycled millisecond pulsars (MSPs). These are spun up by accreting matter from a companion

More information

Alex Gianninas Mukremin Kilic, Warren Brown, & J.J. Hermes December 9 th, th Texas Symposium

Alex Gianninas Mukremin Kilic, Warren Brown, & J.J. Hermes December 9 th, th Texas Symposium Alex Gianninas Mukremin Kilic, Warren Brown, & J.J. Hermes December 9 th, 2013 27th Texas Symposium White Dwarf Properties M ~ 0.6 M R ~ 0.01 R ~ 1 R ~ 10 6 log g ~ 8.0 (log g = 4.4) T eff ~ 150,000 3000

More information

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 9

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 9 Phys 0 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 9 MULTIPLE CHOICE 1. We know that giant stars are larger in diameter than the sun because * a. they are more luminous but have about the

More information

Neutron Stars. Properties of Neutron Stars. Formation of Neutron Stars. Chapter 14. Neutron Stars and Black Holes. Topics for Today s Class

Neutron Stars. Properties of Neutron Stars. Formation of Neutron Stars. Chapter 14. Neutron Stars and Black Holes. Topics for Today s Class Foundations of Astronomy 13e Seeds Phys1403 Introductory Astronomy Instructor: Dr. Goderya Chapter 14 Neutron Stars and Black Holes Cengage Learning 2016 Topics for Today s Class Neutron Stars What is

More information

Measuring the Masses of Neutron Stars

Measuring the Masses of Neutron Stars Measuring the Masses of Neutron Stars Lex Kaper Arjen van der Meer Marten van Kerkwijk 2 Ed van den Heuvel Visualisation: B. Pounds Astronomical Institute Anton Pannekoek and Centre for High Energy Astrophysics,

More information

Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical

Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical Trigonometry p. 9 The Earth p. 12 The Celestial Sphere p. 14 The

More information

FORMATION AND EVOLUTION OF COMPACT BINARY SYSTEMS

FORMATION AND EVOLUTION OF COMPACT BINARY SYSTEMS FORMATION AND EVOLUTION OF COMPACT BINARY SYSTEMS Main Categories of Compact Systems Formation of Compact Objects Mass and Angular Momentum Loss Evolutionary Links to Classes of Binary Systems Future Work

More information

29:50 Stars, Galaxies, and the Universe Second Hour Exam November 10, 2010 Form A

29:50 Stars, Galaxies, and the Universe Second Hour Exam November 10, 2010 Form A 29:50 Stars, Galaxies, and the Universe Second Hour Exam November 10, 2010 Form A There are 20 questions (Note: There will be 32 on the real thing). Read each question and all of the choices before choosing.

More information

HSIN-YU CHEN. ERC 454, 5640 South Ellis Ave. Chicago, IL (515)

HSIN-YU CHEN. ERC 454, 5640 South Ellis Ave. Chicago, IL (515) HSIN-YU CHEN ERC 454, 5640 South Ellis Ave. Chicago, IL 60637 (515) 817 3082 hsinyuchen@uchicago.edu EDUCATION The University of Chicago 2010 - present Ph.D. in Astronomy and Astrophysics Thesis advisor:

More information

The surface gravitational redshift of the neutron star PSR B

The surface gravitational redshift of the neutron star PSR B Bull. Astr. Soc. India (2013) 41, 291 298 The surface gravitational redshift of the neutron star PSR B2303+46 Xian-Feng Zhao 1 and Huan-Yu Jia 2 1 College of Mechanical and Electronic Engineering, Chuzhou

More information

Pulsar timing and its applications

Pulsar timing and its applications Journal of Physics: Conference Series PAPER OPEN ACCESS Pulsar timing and its applications To cite this article: R N Manchester 2017 J. Phys.: Conf. Ser. 932 012002 Related content - The European Pulsar

More information

ASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS. Spring, This is a one quarter course dealing chiefly with:

ASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS. Spring, This is a one quarter course dealing chiefly with: This is a one quarter course dealing chiefly with: ASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS Spring, 2015 http://www.ucolick.org/~woosley a) Nuclear astrophysics and the relevant

More information

1. Star: A object made of gas found in outer space that radiates.

1. Star: A object made of gas found in outer space that radiates. 1. Star: A object made of gas found in outer space that radiates. 2. Stars produce extremely great quantities of energy through the process of. The chemical formula for nuclear fusion looks like this:

More information

Chapter 0 Introduction X-RAY BINARIES

Chapter 0 Introduction X-RAY BINARIES X-RAY BINARIES 1 Structure of this course 0. Introduction 1. Compact stars: formation and observational appearance. Mass transfer in binaries 3. Observational properties of XRBs 4. Formation and evolution

More information

Program Request for Astronomy Minor. Department of Physics. College of Science

Program Request for Astronomy Minor. Department of Physics. College of Science Program Request for Astronomy Minor Department of Physics College of Science March 8, 2006 Astronomy Minor Sponsoring Department: Course Listings in Astronomy: PHYSICS ASTR 1050 (The Solar System) ASTR

More information

ASTRONOMY (ASTR) 100 Level Courses. 200 Level Courses. 300 Level Courses

ASTRONOMY (ASTR) 100 Level Courses. 200 Level Courses. 300 Level Courses Astronomy (ASTR) 1 ASTRONOMY (ASTR) 100 Level Courses ASTR 103: Astronomy. 3 credits. Introduction to origin of life, Earth, planets and sun, stars, galaxies, quasars, nature of space radiation, and general

More information

Prof. Clifford M. Will Parameter estimation of binary black holes mergers with Laser Interferometric Space Antenna.

Prof. Clifford M. Will Parameter estimation of binary black holes mergers with Laser Interferometric Space Antenna. Adamantios Stavridis Department of Physics Phone: +30 2310 998141 Aristotle University of Thessaloniki Fax: +30 2310 995384 54124 astavrid@astro.auth.gr Thessaloniki http://www.astro.auth.gr/~astavrid/

More information

Extrasolar Planets. to appear in Encyclopedia of Time, Sage Publishing, in preparation, H.J. Birx (Ed.)

Extrasolar Planets. to appear in Encyclopedia of Time, Sage Publishing, in preparation, H.J. Birx (Ed.) Extrasolar Planets to appear in Encyclopedia of Time, Sage Publishing, in preparation, H.J. Birx (Ed.) The term extrasolar planets or exoplanets stands for planets outside our Solar System, i.e. not orbiting

More information

ASTRONOMY (ASTRON) ASTRON 113 HANDS ON THE UNIVERSE 1 credit.

ASTRONOMY (ASTRON) ASTRON 113 HANDS ON THE UNIVERSE 1 credit. Astronomy (ASTRON) 1 ASTRONOMY (ASTRON) ASTRON 100 SURVEY OF ASTRONOMY 4 credits. Modern exploration of the solar system; our galaxy of stars, gas and dust; how stars are born, age and die; unusual objects

More information

Grégory Schehr. Citizenship : French Date of birth : March 29, First class Junior Scientist (CR1) at CNRS in Theoretical Physics.

Grégory Schehr. Citizenship : French Date of birth : March 29, First class Junior Scientist (CR1) at CNRS in Theoretical Physics. Curriculum Vitae Grégory Schehr Citizenship : French Date of birth : March 29, 1977 Current position First class Junior Scientist (CR1) at CNRS in Theoretical Physics. Professional address Laboratoire

More information

Evolution of High Mass stars

Evolution of High Mass stars Evolution of High Mass stars Neutron Stars A supernova explosion of a M > 8 M Sun star blows away its outer layers. The central core will collapse into a compact object of ~ a few M Sun. Pressure becomes

More information

Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy. Astronomy 111 Wednesday November 29, 2017

Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy. Astronomy 111 Wednesday November 29, 2017 Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy Astronomy 111 Wednesday November 29, 2017 Reminders Online homework #11 due Monday at 3pm One more lecture after today Monday

More information

Survey of Astronomy ASTRO 110-5

Survey of Astronomy ASTRO 110-5 Survey of Astronomy ASTRO 110-5 Prof. Istvan Szapudi Institute for Astronomy IfA B204/WAT 401 Phone: 956 6196 Email: szapudi@ifa.hawaii.edu Class meets TTh 12:00 to 13:15 WAT 112 Office Hours after class

More information

arxiv: v1 [astro-ph.he] 11 Nov 2016

arxiv: v1 [astro-ph.he] 11 Nov 2016 Preprint November 14, 216 Compiled using MNRAS LATEX style file v3. A Massive Millisecond Pulsar in an Eccentric Binary E. D. Barr, 1 P. C. C. Freire, 1 M. Kramer, 1 D. J. Champion, 1 M. Berezina, 1 C.

More information

Relativistic Astrophysics Neutron Stars, Black Holes & Grav. W. ... A brief description of the course

Relativistic Astrophysics Neutron Stars, Black Holes & Grav. W. ... A brief description of the course Relativistic Astrophysics Neutron Stars, Black Holes & Grav. Waves... A brief description of the course May 2, 2009 Structure of the Course Introduction to General Theory of Relativity (2-3 weeks) Gravitational

More information

The Dynamic Radio Sky

The Dynamic Radio Sky The Dynamic Radio Sky Exoplanet Bursts, Lunar Neutrinos, and other Exotica Joseph Lazio (Naval Research Laboratory SKA Program Development Office) Who Cares? Radio transients are like butterfly collecting.

More information

Post-Keplerian effects in binary systems

Post-Keplerian effects in binary systems Post-Keplerian effects in binary systems Laboratoire Univers et Théories Observatoire de Paris / CNRS The problem of binary pulsar timing (Credit: N. Wex) Some classical tests of General Relativity Gravitational

More information

Stellar Evolution: from star birth to star death and back again

Stellar Evolution: from star birth to star death and back again Stellar Evolution: from star birth to star death and back again Prof. David Cohen Dept. of Physics and Astronomy This presentation is available at: astro.swarthmore.edu/~cohen/presentations/admitted_students_2006/

More information

Directions: For numbers 1-30 please choose the letter that best fits the description.

Directions: For numbers 1-30 please choose the letter that best fits the description. Directions: For numbers 1-30 please choose the letter that best fits the description. 1. The main force responsible for the formation of the universe is: a. Gravity b. Frictional force c. Magnetic force

More information

THE HIGH TIME RESOLUTION UNIVERSE. A survey for pulsars & fast transients

THE HIGH TIME RESOLUTION UNIVERSE. A survey for pulsars & fast transients THE HIGH TIME RESOLUTION UNIVERSE A survey for pulsars & fast transients 1 REVIEW OF HTRU 2 SURVEY OVERVIEW The High Time Resolution Universe survey for pulsars and fast transients -- HTRU An ambitious

More information