Title: X-Raying%20the%20Hot%20Universe%20John%20P.%20Hughes%20Rutgers%20University
1X-Raying the Hot UniverseJohn P. HughesRutgers
University
- Astrophysical Studies of Supernova Remnants and
Clusters of Galaxies
2Group 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.
3Job 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
4Principal 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
5Principal Facilities Used (cont.)
- XMM-Newton
- ESA X-ray Multi-Mirror Mission
- Launched 10 December 1999
- Large collecting area
- Nominal 10 year lifetime
6Principal 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
7Recent 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.
8On-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
9Gravitational 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
10Mass-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)
11Imminent 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
12Imminent 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
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14SALT
15Longer 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)
16Summary
- Well-defined, interesting thesis projects
- Financial support from NASA and NSF
- Good long term prognosis for astrophysics
research in the US