The Dynamic Radio Sky
|
|
- Ami Nash
- 6 years ago
- Views:
Transcription
1 The Dynamic Radio Sky Exoplanet Bursts, Lunar Neutrinos, and other Exotica Joseph Lazio (Naval Research Laboratory SKA Program Development Office)
2 Who Cares? Radio transients are like butterfly collecting is the 200 th anniversary of the birth of Charles Darwin (1809 February 12) Astronomy is an observational science As is evolutionary biology Yet collecting has led to the development of evolutionary relationships.
3 Who Cares? Transient radio sources are necessarily compact Locations of explosive or dynamic events Probe fundamental physics and astrophysics Radio signals modified by intervening media and are powerful probes of those media Dispersion Scattering Faraday rotation
4 The RadioTransient Sky Science Planets Solar(!) Extrasolar Brown Dwarfs New behavior from old friends Neutron stars Radio-wave scattering Lunar neutrinos Exotica ETI Exploding black holes Technology Time Domain Observations Confusion RFI Flexible scheduling Frequency agility Data Management
5 Solar Planetary Radio Emission Solar wind loading of magnetosphere produces radio emission 1% of auroral input energy into electron cyclotron radio emission ν < 40 MHz Accurate position of radio emission remains poorly unknown, even today! viz. LOFAR observations Basic plasma physics Model for stars, brown dwarfs, other planets, Jupiter
6 Extrasolar Planetary Radio Emission HD M = 3.32 M J P = 267 d (a = AU) e = 0.23 Discovery of extrasolar planets! ~ 400 extrasolar planets Indirect detection via optical signature Detecting characterizing: What are their properties? Can we detect planets at other wavelengths? IR thermal emission detected? Magnetospheric radio (viz. Jupiter) Implications for habitability?
7 Lighthouse-like Brown Dwarfs M9 dwarf P = hr Brown dwarf magnetosphere / emission mechanism Connection to pulsar magnetosphere? Current work typically at 5 and 8 GHz Largely unexplored ~ 1 GHz TVLM (Hallinan et al. 2007)
8 Dwarf Stars Radio emission from nearby dwarf stars E.g., AD Leo with Arecibo (~ 1.5 GHz) Structure on millisecond time scales Magnetized plasma processes in stellar coronae E.g., cyclotron maser AD Leo (Osten & Bastian) Living with a Star Real world application of
9 Transient Pulsars Long-term On-off transition < 10 s Off ~ 30 days Intrinsic Pulsar wind and emission mechanism (or ETI?) ~ 1 GHz s/s s/s PSR B Modified Julian Date (Kramer et al. 2006)
10 RRATs On ~ 10 ms Off >~ 1 hr Intrinsic Pulsar emission mechanism and/or magnetosphere Frequency (MHz) Amplitude (mjy) Time J ~ 1.4 GHz (McLaughlin et al. 2005)
11 Propagation Effects Extreme scattering events are one manifestation Months to years Extrinsic Probe of intervening medium(a) Flux Density (mjy) Date J (Maitia et al. 2003)
12 Giant and Nano-giant Pulses On ~ 2 ns duration Off ~ 10 min. T B > K Brightest objects in the Universe Probes pulsar emission mechanism scattering environment? Crab pulsar (Hankins et al. 2003) 5.5 & 8.6 GHz
13 Probing the Local Group Power-law distribution of pulse strengths Longer observations means stronger pulses Majority of Local Group medium ionized ( missing baryons ) Possible probe of local intergalactic medium? Cf. FUSE, Chandra probes of tracer species (O VI, O VII, etc.)
14 Lunar Neutrinos Moon as a beam dump Ultra-high energy ν initiates particle shower E ν ~ ev (or higher?) Negative charge excess develops Coherent radio pulse Askar yan effect Hyper-GZK probe of Universe GZK effect limits our view of Universe (HiRes experiment; arxiv:astro-ph/ ) How Do Cosmic Accelerators Work? (Quarks to Cosmos) γ HiRes ν
15 GCRT J A monitoring campaign of the Galactic center λ 1 meter Roughly 20 epochs Time samplings from ~ 1 week to 1 decade Observations with Very Large Array (most) Giant Metrewave Radio Telescope Hymanet al. 2005
16 Exotica Rees (1977) predicts primordial black holes will produce radio pulses Series of searches 40 MHz 430 MHz (= 1.8 µev, Phinney & Taylor) ~ 1 TeV (Linton et al.) Interest in Fermi/GLAST searches (e.g., Dingus et al.)
17 Extraterrestrial Intelligence Radio signals can cross the Galaxy essentially unimpeded. CP 1919 was L.G.M 1 When we least expect it? Fortune favors the prepared mind The Universe is full of magical things, patiently waiting for our wits to grow sharper. Eden Phillpotts Ardipithecus ramidus Jocelyn Bell, 1967 Modified Julian Date
18 Transient Phase Space Physics: SD 2 = 2kT B (tν) 2 Raleigh-Jeans law S = 2kT B /λ 2 * Ω Observational: S = (2kT B /c 2 ) Ω ν 2 (and time res., cadence, ) Non-imaging Extension of typical pulsar processing Imaging Visibilities, sky models, residual images,
19 Transient Phase Space νw = dimensionless pulse width, uncertaintylike relation SD 2 = pseudoluminosity J. Cordes
20 Transient Phase Space Observational / empirical approach How does a telescope (SKA) compare with existing & previous searches? Arecibo, ATA, LOFAR, E VLA, LOFAR ATA Fly s Eye Gain (K/Jy) Field of View (arcminutes) 278 deg deg EVLA Fly s Eye Frequency (MHz)
21 Long Wavelength Demonstrator Array MHz 16-element dipole station At VLA site in NM Existence proof for transient detection with (sparse) aperture arrays
22 Radio Transients More than butterfly collecting! Probe fundamental physics and astrophysics Probe intervening media Increasing opportunities Both scientific & technical Imaging & non-imaging! Both A/T and Ω are important!
Radio Aspects of the Transient Universe
Radio Aspects of the Transient Universe Time domain science: the transient sky = frontier for all λλ Less so at high energies BATSE, RXTE/ASM, Beppo/Sax, SWIFT, etc. More so for optical, radio LSST = Large
More informationPulsars 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 informationThe Dynamic Radio Sky: An Opportunity for Discovery
The Dynamic Radio Sky: An Opportunity for Discovery J. Lazio 1 (NRL), J. S. Bloom (UC Berkeley), G. C. Bower (UC Berkeley), J. Cordes (Cornell, NAIC), S. Croft (UC Berkeley), S. Hyman (Sweet Briar), C.
More informationWhat we (don t) know about UHECRs
What we (don t) know about UHECRs We know: their energies (up to 10 20 ev). their overall energy spectrum We don t know: where they are produced how they are produced what they are made off exact shape
More informationThe Eight-meter-wavelength Transient Array
The Eight-meter-wavelength Transient Array Steve Ellingson Cameron Patterson John Simonetti Dept. of Electrical & Computer Engineering Dept. of Electrical & Computer Engineering Dept. of Physics Virginia
More informationThe Dynamic Radio Sky: On the path to the SKA. A/Prof Tara Murphy ARC Future Fellow
The Dynamic Radio Sky: On the path to the SKA A/Prof Tara Murphy ARC Future Fellow What causes radio variability? 1. Explosions - e.g. supernovae, gamma-ray bursts, orphan afterglows 2. Propagation - e.g.
More informationPoS(ISKAF2010)083. FRATs: a real-time search for Fast Radio Transients with LOFAR
FRATs: a real-time search for Fast Radio Transients with LOFAR Radboud University Nijmegen (Department of Astrophysics) E-mail: s.terveen@astro.ru.nl H. Falcke Radboud University Nijmegen (Department of
More informationFast Radio Bursts. Laura Spitler Max-Planck-Institut für Radioastronomie 11. April 2015
Fast Radio Bursts Laura Spitler Max-Planck-Institut für Radioastronomie 11. April 2015 Lorimer Burst Bright burst discovered in the reprocessing of archival data from a pulsar survey A Bright Millisecond
More informationThoughts on LWA/FASR Synergy
Thoughts on LWA/FASR Synergy Namir Kassim Naval Research Laboratory 5/27/2003 LWA-FASR 1 Ionospheric Waves 74 MHz phase 74 MHz model Ionosphere unwound (Kassim et al. 1993) Ionospheric
More informationHOW TO GET LIGHT FROM THE DARK AGES
HOW TO GET LIGHT FROM THE DARK AGES Anthony Smith Lunar Seminar Presentation 2/2/2010 OUTLINE Basics of Radio Astronomy Why go to the moon? What should we find there? BASICS OF RADIO ASTRONOMY Blackbody
More informationPlanetary Magnetic Fields: Planetary Interiors and Habitability
Planetary Magnetic Fields: Planetary Interiors and Habitability W. M. Keck Institute for Space Studies (KISS) Study Joseph Lazio, Evgenya Shkolnik, Gregg Hallinan on behalf of the KISS Study team 2017
More informationETA Observations of Crab Pulsar Giant Pulses
ETA Observations of Crab Pulsar Giant Pulses John Simonetti,, Dept of Physics, Virginia Tech October 7, 2005 Pulsars Crab Pulsar Crab Giant Pulses Observing Pulses --- Propagation Effects Summary Pulsars
More informationRadio Transients, Stellar End Products, and SETI Working Group Report
Radio Transients, Stellar End Products, and SETI Working Group Report J. Lazio (chair), D.Backer,J.Cordes,J.Jonas,M.Kramer,M.Rupen,J.Tarter March 22, 2002 1 Science Projects This WG has identified the
More informationRadio Transient Surveys with The Allen Telescope Array & the SKA. Geoffrey C Bower (UC Berkeley)
Radio Transient Surveys with The Allen Telescope Array & the SKA Geoffrey C Bower (UC Berkeley) Transient Science is Exploding New Phenomena An Obscured Radio Supernova in M82 Discovered serendipitously
More informationSEARCH FOR RADIO EMISSIONS FROM EXTRASOLAR PLANETS: THE OBSERVATION CAMPAIGN
SEARCH FOR RADIO EMISSIONS FROM EXTRASOLAR PLANETS: THE OBSERVATION CAMPAIGN D. Winterhalter, T. Kuiper, W. Majid, I. Chandra, J. Lazio, P. Zarka, C. Naudet, G. Bryden, W. Gonzalez, and R. Treumann Abstract
More informationWhat are the Big Questions and how can Radio Telescopes help answer them? Roger Blandford KIPAC Stanford
What are the Big Questions and how can Radio Telescopes help answer them? Roger Blandford KIPAC Stanford Radio Astronomy in 1957 ~100 MHz ~100 Jy ~100 sources ~100 arcseconds 2 Radio Astronomy in 2007
More informationAASTCS 5: Radio Exploration of Planetary Habitability 7 12 May, 2017
AASTCS 5: Radio Exploration of Planetary Habitability 7 12 May, 2017 Sunday 7 May, 2017 3:00 pm 7:00 pm 6:00 pm 7:30 pm Registration and Speaker Ready, Tuscany Foyer Opening Reception, Miramonte Green
More informationGravity 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 informationFlaring Stars and the Long Wavelength Array
Flaring Stars and the Long Wavelength Array Rachel Osten 1,2 February 14, 2008 1. Introduction Coherent emission appears to be a common phenomenon on radio-active late-type stars. Solar radio flare emissions
More informationSEARCH FOR RADIO EMISSIONS FROM EXTRASOLAR PLANETARY MAGNETOSPHERES
SEARCH FOR RADIO EMISSIONS FROM EXTRASOLAR PLANETARY MAGNETOSPHERES Daniel Winterhalter, Walid Majid, Tom Kuiper, and Joe Lazio Jet Propulsion Laboratory, California Institute of Technology, Pasadena,
More informationAASTCS 5: Radio Exploration of Planetary Habitability 7 12 May, 2017
AASTCS 5: Radio Exploration of Planetary Habitability 7 12 May, 2017 Sunday 7 May, 2017 3:00 pm 7:00 pm 6:00 pm 7:30 pm Welcome Reception Miramonte Green Monday 8 May, 2017 8:00 am Stellar Activity and
More informationFast Radio Bursts. The chase is on. Sarah Burke Spolaor National Radio Astronomy Observatory
Fast Radio Bursts The chase is on. Sarah Burke Spolaor National Radio Astronomy Observatory with C. Law, G. Bower, B. Butler, P. Demorest, J. Lazio, M. Rupen, many others S P A C E S P A C E f At source
More informationAlexey Kuznetsov. Armagh Observatory
Alexey Kuznetsov Armagh Observatory Outline of the talk Solar radio emission History Instruments and methods Results of observations Radio emission of planets Overview / history / instruments Radio emission
More informationDetecting High Energy Cosmic Rays with LOFAR
Detecting High Energy Cosmic Rays with LOFAR Andreas Horneffer for the LOFAR-CR Team LOFAR CR-KSP: Main Motivation Exploring the sub-second transient radio sky: Extensive Air showers as guaranteed signal
More informationPulsar 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 informationPulsars. Table of Contents. Introduction
Pulsars Table of Contents Introduction... 1 Discovery...2 Observation...2 Binary Pulsars...3 Pulsar Classes... 3 The Significance of Pulsars... 3 Sources...4 Introduction Pulsars are neutron stars which
More informationAstronomy 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 informationMonitoring nearly 4000 nearby stellar systems with the OVRO-LWA in search of radio exoplanets
Monitoring nearly 4000 nearby stellar systems with the OVRO-LWA in search of radio exoplanets Marin M Anderson Caltech AASTCS 5: Radio Habitability May 11, 2017 OVRO-LWA 1 CME CME Mass Mass Understanding
More informationTransient Phenomena: Opportunities for New Discoveries
Transient Phenomena: Opportunities for New Discoveries T. Joseph W. Lazio Abstract Known classes of radio wavelength transients range from the nearby (stellar flares and radio pulsars) to the distant Universe
More informationDesign Reference Mission for SKA1 P. Dewdney System Delta CoDR
Phasing of SKA science: Design Reference Mission for SKA1 P. Dewdney System Delta CoDR Feb. 23, 2011 21 st Century Astrophysics National Aeronautics and Space Administration Jet Propulsion Laboratory California
More informationProject RISARD. - the story so far. Marcin P. Gawroński (Toruń Centre for Astronomy)
Project RISARD - the story so far credit : wiki Marcin P. Gawroński (Toruń Centre for Astronomy) in collaboration with K. Goźdzewski, K. Katarzyński, G. Rycyk (TCfA) Overview RISARD motivation and current
More informationStarlight 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 informationGregg Hallinan National Radio Astronomy Observatory & University of California Berkeley
Donati et al. 2006 Hallinan et al. 2007 Clarke et al. 1998 Gregg Hallinan National Radio Astronomy Observatory & University of California Berkeley Southern Cross Astrophysics Conference Series Kiama 10
More informationFinal States of a Star
Pulsars Final States of a Star 1. White Dwarf If initial star mass < 8 MSun or so. (and remember: Maximum WD mass is 1.4 MSun, radius is about that of the Earth) 2. Neutron Star If initial mass > 8 MSun
More informationPulsar Surveys Present and Future: The Arecibo-PALFA Survey and Projected SKA Survey
Pulsar Surveys Present and Future: The Arecibo-PALFA Survey and Projected SKA Survey Arecibo Telescope SKA concept design Julia Deneva,, Cornell University, USA 15 May 2006 363 rd Heraeus Seminar, Bad
More informationCitation for published version (APA): Lazio, J. (2009). The Square Kilometre Array. In EPRINTS-BOOK-TITLE Groningen: University of Groningen.
University of Groningen The Square Kilometre Array Lazio, Joseph Published in: EPRINTS-BOOK-TITLE IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite
More informationAstronomy Ch. 22 Neutron Stars and Black Holes. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
Name: Period: Date: Astronomy Ch. 22 Neutron Stars and Black Holes MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) In a neutron star, the core
More informationFRB : A Repeating Fast Radio Burst. Laura Spitler 20. June 2016 Bonn Workshop IX
FRB 121102: A Repeating Fast Radio Burst Laura Spitler 20. June 2016 Bonn Workshop IX 1 Fast Radio Bursts (FRB): An Overview 17 Published Sources Parkes (15) Arecibo (1) GBT (1) Broadband radio pulses
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
HW3 Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) A surface explosion on a white dwarf, caused by falling matter from the atmosphere of
More informationThe Mystery of Fast Radio Bursts and its possible resolution. Pawan Kumar
The Mystery of Fast Radio Bursts and its possible resolution Outline Pawan Kumar FRBs: summary of relevant observations Radiation mechanism and polarization FRB cosmology Wenbin Lu Niels Bohr Institute,
More informationThe Search for Extraterrestrial Intelligence (SETI) What can SETI
The Search for Extraterrestrial Intelligence (SETI) What can SETI Mike Garrett researchers learn Sir Bernard Lovell Chair, Prof. of Astrophysics. from FRBs Director Jodrell Bank Centre for Astrophysics
More informationThe Stellar Graveyard
Life and Death of High Mass Stars (M > 8 M sun ) AST 101 Introduction to Astronomy: Stars & Galaxies Last stage: Iron core surrounded by shells of increasingly lighter elements. Announcements MIDTERM #2
More informationRotating RAdio Transients (RRATs) ApJ, 2006, 646, L139 Nature, 2006, 439, 817 Astro-ph/
Rotating RAdio Transients (RRATs) ApJ, 2006, 646, L139 Nature, 2006, 439, 817 Astro-ph/0608311 Introduction 11 Rotating RAdio Transients (RRATs) (Mclaughlin et al 2006) Repeated, irregular radio bursts
More informationThe Square Kilometre Array and the radio/gamma-ray connection toward the SKA era
The Square Kilometre Array and the radio/gamma-ray connection toward the SKA era Marcello Giroletti INAF Istituto di Radioastronomia 12th AGILE Workshop Roma, 8/5/2014 What s in this talk: SKA basics and
More informationPulsars with LOFAR The Low-Frequency Array
Pulsars with LOFAR The Low-Frequency Array Ben Stappers ASTRON, Dwingeloo With assistance from Jason Hessels,, Michael Kramer, Joeri van Leeuwen and Dan Stinebring. Next generation radio telescope Telescope
More informationExoplanet searches in Radio : Theory & Observations from UTR-2 to LOFAR/SKA
Exoplanet searches in Radio : Theory & Observations from UTR-2 to LOFAR/SKA P. Zarka LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris Diderot, 92190 Meudon, philippe.zarka@obspm.fr Jupiter LF
More informationRecent Radio Observations of Pulsars
Recent Radio Observations of Pulsars R. N. Manchester Australia Telescope National Facility, CSIRO Sydney Australia Summary A pulsar census Recent pulsar surveys Pulse modulation and drifting subpulses
More informationThe (obscene) Challenges of Next-Generation Pulsar Surveys
The (obscene) Challenges of Next-Generation Pulsar Surveys Scott Ransom NRAO / Univ. of Virginia Charlottesville, VA Haslam 408MHz Survey Summary: The Pulsar Search Problem Pulsars are faint we are sensitivity
More informationProbing the Cosmos with light and gravity: multimessenger astronomy in the gravitational wave era
Utah State University DigitalCommons@USU Colloquia and Seminars Astrophysics 9-7-2011 Probing the Cosmos with light and gravity: multimessenger astronomy in the gravitational wave era Shane L. Larson Utah
More informationSearching for Other Worlds: The Methods
Searching for Other Worlds: The Methods John Bally 1 1 Center for Astrophysics and Space Astronomy Department of Astrophysical and Planetary Sciences University of Colorado, Boulder The Search Extra-Solar
More informationEnhancing Our Understanding of Ultracool Dwarfs with Arecibo Observatory
Enhancing Our Understanding of Ultracool Dwarfs with Arecibo Observatory Arecibo Observatory has recently been involved in searches for bursts of radio emission from ultracool dwarfs, which bridge the
More information- Synchrotron emission: A brief history. - Examples. - Cyclotron radiation. - Synchrotron radiation. - Synchrotron power from a single electron
- Synchrotron emission: A brief history - Examples - Cyclotron radiation - Synchrotron radiation - Synchrotron power from a single electron - Relativistic beaming - Relativistic Doppler effect - Spectrum
More informationMike Garrett. Sir Bernard Lovell Chair, Prof. of Astrophysics. Director Jodrell Bank Centre for Astrophysics
The Search for Extraterrestrial Intelligence (SETI) All-sky Radio Mike Garrett SETI Sir Bernard Lovell Chair, Prof. of Astrophysics. Director Jodrell Bank Centre for Astrophysics Mike Garrett Sir Bernard
More informationSquare Kilometre Array: World s Largest Radio Telescope Design and Science drivers
Square Kilometre Array: World s Largest Radio Telescope Design and Science drivers Miroslava Dessauges Geneva Observatory, University of Geneva With my thanks to Philip Diamond (SKA director-general),
More informationHistory of Radioastronomy from 1800 to 2007
History of Radioastronomy from 1800 to 2007 (a personal selection) Steve Torchinsky Observatoire de Paris History of radio astronomy, Steve Torchinsky Goutelas, 4 June 2007 1 Herschel discovers invisible
More informationarxiv:astro-ph/ v1 10 Nov 1999
Pulsar Astronomy 2000 and Beyond ASP Conference Series, Vol. e iπ + 1, 2000 M. Kramer, N. Wex, and R. Wielebinski, eds. The Parkes Multibeam Pulsar Survey arxiv:astro-ph/9911185v1 10 Nov 1999 F. Camilo
More informationCherenkov Telescope Array ELINA LINDFORS, TUORLA OBSERVATORY ON BEHALF OF CTA CONSORTIUM, TAUP
Cherenkov Telescope Array A SENSITIVE PROBE OF EXTREME UNIVERSE ELINA LINDFORS, TUORLA OBSERVATORY ON BEHALF OF CTA CONSORTIUM, TAUP 2015 1 The CTA Observatory SST ( 4m) LST ( 23m) MST ( 12m) South North
More informationNeutron Stars. Neutron Stars Mass ~ 2.0 M sun! Radius ~ R sun! isolated neutron stars first seen only recently (1997)
Neutron Stars 1 2 M core > 1.4 M - collapse past WD! sun nuclei packed tightly together! protons absorb electrons; only neutrons left! collapse halted by neutron degeneracy pressure How do you find something
More informationSETI with SKA1 and SKA2
SETI with SKA1 and SKA2 Alan Penny1, Heino Falcke2, Mike Garrett3 1 University of St Andrews and South African Astronomical Observatory PI: LOFAR Early Access Program LEA070 'A SETI Pilot Program' 2 Raboud
More informationMulti-wavelength Astronomy
astronomy Multi-wavelength Astronomy Content What do we measure Multi-wavelength approach Data Data Mining Virtual Observatory Hands on session Larmor's formula Maxwell's equations imply that all classical
More informationFuture Radio Observatories for Pulsar Studies
Future Radio Observatories for Pulsar Studies Michael Kramer University of Manchester Jodrell Bank Observatory 17 th August 2006 Many new facilities Many new facilities LOFAR EMBRACE LFD LWA KAT xntd SKA
More informationHI Galaxy Science with SKA1. Erwin de Blok (ASTRON, NL) on behalf of The HI Science Working Group
HI Galaxy Science with SKA1 Erwin de Blok (ASTRON, NL) on behalf of The HI Science Working Group SKA1 HI Science Priorities Resolved HI kinematics and morphology of ~10 10 M mass galaxies out to z~0.8
More informationSolar Radiophysics with HF Radar
Solar Radiophysics with HF Radar Workshop on Solar Radiophysics With the Frequency Agile Solar Radiotelescope (FASR) 23-25 May 2002 Green Bank, WV Paul Rodriguez Information Technology Division Naval Research
More informationDiscovery of fast radio transients at very low frequencies
Discovery of fast radio transients at very low frequencies Yogesh Maan National Centre for Radio Astrophysics (NCRA), Pune, INDIA June 02, 2015 Yogesh Maan (NCRA) June 02, 2015 1 / 22 Overview 1 Motivations
More informationRadio Probes of Extrasolar Space Weather
Radio Probes of Extrasolar Space Weather Rachel Osten Space Telescope Science Institute Radio Stars: from khz to THz Haystack Observatory November 2, 2017 Star s magnetic field helps to set the environment
More informationFAST RADIO BURSTS. Marta Burgay
FAST RADIO BURSTS Marta Burgay 1967: THE FIRST FAST RADIO BURSTS' Jocelyn Bell set the field going in 1967 by discovering pulsars through their time-variable bursts of emission SEARCHES FOR PSRS AND FAST
More informationStellar radio emission in the SKA era: the SCORPIO project
Stellar radio emission in the SKA era: Grazia Umana the SCORPIO project INAF-OAC C. Trigilio, R. Norris, T. Franzen, A. Ingallinera, C. Agliozzo P. Leto, C. Buemi, E. Budding, B. Slee, G. Ramsay, G. Doyle,
More informationTHE 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 informationTransient Cosmic Phenomena and their Influence on the Design of the SKA Radio Telescope
Transient Cosmic Phenomena and their Influence on the Design of the SKA Radio Telescope Research Review Curtin Institute of Radio Astronomy 5 May 2009 ToC Parameter space Discovering phenomena ASKAP &
More informationGregg Hallinan National Radio Astronomy Observatory & UC Berkeley
Gregg Hallinan National Radio Astronomy Observatory & UC Berkeley E-mail: gregg@astro.berkeley.edu Stephen White University of Maryland The EVLA: A New Era in Stellar Radio Astronomy EVLA Continuum point-source
More informationProbing Into The Dark Ages with a Low Frequency Interferometer on the Moon
Probing Into The Dark Ages with a Low Frequency Interferometer on the Moon Jack Burns Center for Astrophysics and Space Science University of Colorado, Boulder (with contributions from A. Loeb, J. Hewitt,
More informationThe Stellar Graveyard Neutron Stars & White Dwarfs
The Stellar Graveyard Neutron Stars & White Dwarfs White Dwarfs White dwarfs are the remaining cores of low-mass (M < 8M sun ) stars Electron degeneracy pressure supports them against gravity Density ~
More informationSUPERNOVA! What is a supernova? How dangerous are they to life on Earth? How would the universe be different without supernovae?
SUPERNOVA! What is a supernova? How dangerous are they to life on Earth? How would the universe be different without supernovae? 1 Stellar Evolution: The Deaths of Stars A hundred years ago, we believed
More informationAstrophysics Enabled by the Return to the Moon
Astrophysics Enabled by the Return to the Moon One s Destination is never a place but rather a new way of looking at things. Henry Miller Mario Livio Space Telescope Science Institute BRIEF OUTLINE What
More informationGamma-ray Astrophysics with VERITAS: Exploring the violent Universe
Gamma-ray Astrophysics with VERITAS: Exploring the violent Universe K. Ragan McGill University Soup & Science 11-Jan-2008 Soup & Science Jan. '08 1 How do we know about the Universe? Historically, all
More informationPulsars - a new tool for astronomy and physics
1 Reading: Chapter 24, Sect. 24.5-24.6; Chap. 20, Chap. 25, Sec. 25.1 Exam 2: Thursday, March 22; essay question given on Tuesday, March 20 Last time:death of massive stars - supernovae & neutron stars
More informationWide-field Near-real-time Radio Transient Surveys
Photo by D. Medlin, NRAO/AUI/NSF Wide-field Near-real-time Radio Transient Surveys Kunal Mooley (Oxford) Gregg Hallinan, Shri Kulkarni (Caltech), Steven Myers, Dale Frail, Preshanth Jagannathan (NRAO),
More informationThe Square Kilometre Array
Cosmology, Galaxy Formation and Astroparticle Physics on the pathway to the SKA Klöckner, H.-R., Rawlings, S., Jarvis, M. & Taylor, A. (eds.) April 10th-12th 2006, Oxford, United Kingdom The Square Kilometre
More informationThe VLA Sky Survey. Claire Chandler (on behalf of the VLASS Project Office and the Survey Science Group)
The VLA Sky Survey Claire Chandler (on behalf of the VLASS Project Office and the Survey Science Group) 1 NM Symposium, Nov 4, 2016 What is the VLA Sky Survey? With the completion of the Expanded VLA construction
More informationFermi Large Area Telescope:
Fermi Large Area Telescope: Early Results on Pulsars Kent Wood Naval Research Lab kent.wood@nrl.navy.mil for the Fermi LAT Collaboration Tokyo Institute of Technology 7 March 2009 K. Wood (NRL) 1/30 Fermi
More informationMagnetic Fields in Evolving Spiral Galaxies and their Observation with the SKA
Magnetic Fields in Evolving Spiral Galaxies and their Observation with the SKA Rainer Beck MPIfR Bonn & SKA Science Working Group Fundamental magnetic questions When and how were the first fields generated?
More informationPERSPECTIVES of HIGH ENERGY NEUTRINO ASTRONOMY. Paolo Lipari Vulcano 27 may 2006
PERSPECTIVES of HIGH ENERGY NEUTRINO ASTRONOMY Paolo Lipari Vulcano 27 may 2006 High Energy Neutrino Astrophysics will CERTAINLY become an essential field in a New Multi-Messenger Astrophysics What is
More informationThe Main Point(s) Lecture #36: Planets Around Other Stars. Extrasolar Planets! Reading: Chapter 13. Theory Observations
Lecture #36: Planets Around Other Stars Extrasolar Planets! Theory Observations Detection methods Results to date... Implications for "Habitable Zones" Reading: Chapter 13 Astro 102/104 1 The Main Point(s)
More informationCoherent and continuous radio emission from Magnetic Chemically Peculiar stars
Coherent and continuous radio emission from Magnetic Chemically Peculiar stars C. Trigilio 1 P. Leto 1, G. Umana 1, C.Buemi 1, F.Leone 2 1 INAF-OACT, 2 UNICT Magnetic Chemically Peculiar stars MS B-A type
More informationMass loss from stars
Mass loss from stars Can significantly affect a star s evolution, since the mass is such a critical parameter (e.g., L ~ M 4 ) Material ejected into interstellar medium (ISM) may be nuclear-processed:
More informationDark Matter ASTR 2120 Sarazin. Bullet Cluster of Galaxies - Dark Matter Lab
Dark Matter ASTR 2120 Sarazin Bullet Cluster of Galaxies - Dark Matter Lab Mergers: Test of Dark Matter vs. Modified Gravity Gas behind DM Galaxies DM = location of gravity Gas = location of most baryons
More informationMilky Way SKA: the ISM, star formation and stellar evolution with the SKA. Mark Thompson, Grazia Umana, and the Our Galaxy SWG
Milky Way SKA: the ISM, star formation and stellar evolution with the SKA Mark Thompson, Grazia Umana, and the Our Galaxy SWG Uncovering the ecology of baryons Graphic courtesy Naomi McClure- Griffiths
More information3/1/18 LETTER. Instructors: Jim Cordes & Shami Chatterjee. Reading: as indicated in Syllabus on web
Astro 2299 The Search for Life in the Universe Lecture 9 Last time: Star formation Formation of protostars and planetary systems This time A few things about the epoch of reionization and free fall times
More informationAstronomy 110: SURVEY OF ASTRONOMY. 11. Dead Stars. 1. White Dwarfs and Supernovae. 2. Neutron Stars & Black Holes
Astronomy 110: SURVEY OF ASTRONOMY 11. Dead Stars 1. White Dwarfs and Supernovae 2. Neutron Stars & Black Holes Low-mass stars fight gravity to a standstill by becoming white dwarfs degenerate spheres
More informationSKA Precursors and Pathfinders. Steve Torchinsky
SKA Precursors and Pathfinders Steve Torchinsky steve.torchinsky@obspm.fr A square kilometre of collecting area for each of three frequency bands SKA Low frequency 50MHz to 450MHz to be built in Western
More information=> most distant, high redshift Universe!? Consortium of international partners
LOFAR LOw Frequency Array => most distant, high redshift Universe!? Consortium of international partners Dutch ASTRON USA Haystack Observatory (MIT) USA Naval Research Lab `best site = WA Novel `technology
More informationFast Transients: A Tutorial. Dale A. Frail NRAO
Fast Transients: A Tutorial Dale A. Frail NRAO Tutorial Outline 1. Fast transients What are they and why are they interesting now? 2. Optimal Search Strategies The problem and some recent progress 3. Fast
More informationRadio followup of ransient sources: Feasibility and practicality
Radio followup of ransient sources: Feasibility and practicality C. H. Ishwara Chandra National Centre for Radio Astrophysics Tata Institute of Fundamental Research Pune University Campus, Pune - India
More informationASTR Midterm 2 Phil Armitage, Bruce Ferguson
ASTR 1120-001 Midterm 2 Phil Armitage, Bruce Ferguson SECOND MID-TERM EXAM MARCH 21 st 2006: Closed books and notes, 1 hour. Please PRINT your name and student ID on the places provided on the scan sheet.
More informationNeutron Stars. We now know that SN 1054 was a Type II supernova that ended the life of a massive star and left behind a neutron star.
Neutron Stars Neutron Stars The emission from the supernova that produced the crab nebula was observed in 1054 AD by Chinese, Japanese, Native Americans, and Persian/Arab astronomers as being bright enough
More informationRob Fender, Ben Stappers and Ralph Wijers on behalf of LOFAR and the Transients Key Science Project
Quiquid variat notandum Rob Fender, Ben Stappers and Ralph Wijers on behalf of LOFAR and the Transients Key Science Project RAMJW 1 LOFAR: surveyor and transient monitor (SCUBA-2, ALMA fields of view smaller
More informationCherenkov Telescope Array Status Report. Salvatore Mangano (CIEMAT) On behalf of the CTA consortium
Cherenkov Telescope Array Status Report Salvatore Mangano (CIEMAT) On behalf of the CTA consortium Outline Very-High-Energy Gamma-Ray Astronomy Cherenkov Telescope Array (CTA) Expected Performance of CTA
More informationSKADS Virtual Telescope: Pulsar Survey IV: Globular Cluster Pulsars
SKADS Virtual Telescope: Pulsar Survey IV: Globular Cluster Pulsars PI: S. Ransom Co-I: M. Kramer We propose to use the SKADS Virtual Telescope (SVT) to search Globular clusters for fast rotating pulsars
More informationRadio emission from Supernova Remnants. Gloria Dubner IAFE Buenos Aires, Argentina
Radio emission from Supernova Remnants Gloria Dubner IAFE Buenos Aires, Argentina History Before radio astronomy, only 2 SNRs were known: Crab and Kepler s SNR 1948: Ryle and Smith detected an unusually
More informationRAL Configuration Science Requirements for the Allen Telescope Array
RAL Configuration Science Requirements for the Allen Telescope Array Douglas Bock March 26, 2001 (with minor emendations, but not updates, February 5, 2002) Purpose This document describes the science
More information