The Nearby Supernova Factory

The Nearby Supernova Factory

The Nearby Supernova Factory Benjamin Alan Weaver HPWREN Users Meeting 3 November 2006 B. A. Weaver HPWREN 2006-11-03 1 SNF Collaboration ● Lawrence Berkeley National Laboratory: G. Aldering, C. Aragon, S. Bailey, S. Bongard, M. J. Childress, S. Koshy, S. Loken, P. Nugent, S. Perlmutter, K. Runge, R. Scalzo, R. C. Thomas, B. A. Weaver ● Yale University: C. Baltay, A. Bauer, D. Herrera, D. Rabinowitz ● Kavli Institute for Cosmological Physics, Chicago: R. Kessler ● Laboratoire de Physique Nucléaire et de Haute Energies de Paris: P. Antilogus, S. Gilles, R. Pain, R. Pereira ● Centre de Recherche Astronomique de Lyon: E. Pécontal, G. Rigaudier ● Institut de Physique Nucléaire de Lyon: C. Buton, Y. Copin, E. Gangler, G. Smadja B. A. Weaver HPWREN 2006-11-03 2 Background ● Accelerating Expansion discovered ~1999 ● 70% of the Universe is Anybody©s Guess ● Distant supernovae easier to find B. A. Weaver HPWREN 2006-11-03 3 SNF Overview ● Find & study supernovae in nearby galaxies ● Search on Mt. Palomar (Oschin 48 inch Schmidt) ● Follow-up on Mauna Kea (UH 88 inch) ● High performance networking critical ● Create public database of supernova spectra ● Deeper understanding of Type Ia physics & cosmology B. A. Weaver HPWREN 2006-11-03 4 SNF Data Flow HPWREN ~35000 images/night ~50 GB/night Palomar 48 inch Schmidt NEAT/QUEST Data HPSS Mass Storage SN2004dt Supernovae! NERSC PDSF Compute Cluster B. A. Weaver HPWREN 2006-11-03 5 SN2005gj ● G. Aldering et al., ªNearby Supernova Factory Observations of SN 2005gj: Another Type Ia Supernova in a Massive Circumstellar Envelopeº, Astrophys. J. 650, 510 (2006). ● ªHybridº SN Ia/II similar to SN2002ic ● Found in anonymous low-metallicity galaxy ● Type Ia surrounded by large cloud of gas. B. A. Weaver HPWREN 2006-11-03 6 SN2006D ● R. C. Thomas et al., ªNearby Supernova Factory Observations of SN 2006D: On Sporadic Carbon Signatures in Early Type Ia Supernova Spectraº, Astrophys. J. Lett. submitted. ● Observation of C II (ionized carbon) features. ● Evidence of unburned white-dwarf star material. ● Constraints on white-dwarf explosion models. B. A. Weaver HPWREN 2006-11-03 7 Conclusion ● Current search very successful ● Smoothly handling increased NEAT/QUEST data ● Continuous improvement ● Further information at http://snfactory.lbl.gov B. A. Weaver HPWREN 2006-11-03 8.

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    8 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us