X-Raying%20the%20Hot%20Universe%20John%20P.%20Hughes%20Rutgers%20University - PowerPoint PPT Presentation

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X-Raying%20the%20Hot%20Universe%20John%20P.%20Hughes%20Rutgers%20University

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XMM-Newton. ESA X-ray Multi-Mirror Mission. Launched 10 December 1999 ... Chandra and XMM-Newton Observations of the Deep Lens Survey (DLS) Shear-Selected ... – PowerPoint PPT presentation

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Title: X-Raying%20the%20Hot%20Universe%20John%20P.%20Hughes%20Rutgers%20University


1
X-Raying the Hot UniverseJohn P. HughesRutgers
University
  • Astrophysical Studies of Supernova Remnants and
    Clusters of Galaxies

2
Group Members
  • Jack Hughes at RU since Sept 1996 (PhD Columbia)
    SNRs and CoGs
  • Carlos Badenes post-doc (PhD Barcelona) SNRs
  • Gamil Cassam-Chenai post-doc (PhD Saclay) SNRs
  • Jessica Warren grad student (Vassar) SNRs
  • Neelima Sehgal grad student (Yale) CoGs
  • External Collaborators Harvard-Smithsonian
    Center for Astrophysics, Pennsylvania State
    University, Princeton University, University of
    Pennsylvania, Univeristy of California, Davis.

3
Job Prospects
  • Recent RU astronomy PhD graduates obtained jobs
    in industry, teaching colleges, NASA centers,
    academic post-docs, and research universities
  • http//www.physics.rutgers.edu/ast/group-ast.html
  • American Astronomical Society Career Services
  • http//www.aas.org/career/index.htm

This figure shows the number of new job postings
each month in the AAS Job Register. There has
been a steady growth in the number of new jobs
advertised, nearly doubling every five years
4
Principal Facilities Used
  • Chandra X-ray Observatory
  • NASA Great Observatory
  • Launched 23 July 1999
  • First (and only) X-ray telescope with 1 angular
    resolution
  • Nominal 10 year lifetime

5
Principal Facilities Used (cont.)
  • XMM-Newton
  • ESA X-ray Multi-Mirror Mission
  • Launched 10 December 1999
  • Large collecting area
  • Nominal 10 year lifetime

6
Principal Facilities Used (cont.)
  • Ground-based facilities such as the Cerro Tololo
    Inter-American Obs.
  • Optical telescopes of the US National Observatory
  • 4-m, 1.5-m imaging and spectroscopy

7
Recent SNR Science Highlights
J. S. Warren, J.P. Hughes, et al. 2005, Cosmic
Ray Acceleration at the Forward Shock in Tycho's
Supernova Remnant Evidence from Chandra X-ray
Observations, ApJ, 634, 376.
J.P. Hughes, C.E. Rakowski, D.N. Burrows, and
P.O. Slane 2000, Nucleosynthesis and Mixing in
Cassiopeia A, ApJL, 528, L109.
8
On-going CoG Projects
  • Chandra and XMM-Newton Observations of the Deep
    Lens Survey (DLS) Shear-Selected Cluster Survey

Hubble Space Telescope
Deep Lens Survey/NOAO
9
Gravitational Lensing
  • Gravity bends light - a consequence of General
    Relativity
  • Strong lensing
  • Arcs, multiple images
  • Weak lensing
  • Statistical effect average over many randomly
    aligned background galaxies

10
Mass-Selected Clusters
  • Deep Lens Survey (DLS) over 20 deg2 could find
    up to 100 such clusters!

40
  • First year Survey
  • Wittman et al 2006, ApJ, in press. (Detections
    and follow-up)
  • Hughes et al 2006, ApJL, in prep. (Luminosity
    vs. temperature correlation)

11
Imminent Projects (SNRs)
  • Deep Chandra observations
  • Cas A 1 million second observation (in hand)
  • Kepler and G292.01.8 to be observed this year
  • Tycho being proposed for observation next year
  • Accepted XMM-Newton observation
  • 60 kilosec observation of young pulsar (135 ms
    period) in G292.01.8

12
Imminent Projects (CoGs)
  • Atacama Cosmology Telescope Survey for CoGs
    using the Cosmic Microwave Background with a
    custom built telescope and camera to be sited in
    Chile.
  • First observations expected later this year
  • Survey continues through 2007 and 2008
  • Main collaborators Princeton (camera) and the
    Univ. of Pennsylvania (telescope)
  • Rutgers role follow-up optical studies using the
    Southern African Large Telescope (SALT) and X-ray
    studies with Chandra and XMM-Newton

13
(No Transcript)
14
SALT
15
Longer Timescale Projects
  • Southern African Large Telescope RU has 10 of
    observing time on this 11-m telescope (one of the
    largest in the world)
  • First light in Sept 2004
  • Scientifically useful observations beginning
    later this year
  • Suzaku US/Japanese X-ray spectroscopy satellite
    (launched Aug 2005), involves visit(s) to Japan
  • Constellation X-Facility NASA follow-on mission
    to Chandra with much more collecting area and
    high spectral resolution (post 2010)

16
Summary
  • Well-defined, interesting thesis projects
  • Financial support from NASA and NSF
  • Good long term prognosis for astrophysics
    research in the US
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