Carnegie Mellon University
Scientific Program

Scientific Program

In keeping with the goal of encouraging the broadest possible participation from young researchers in Great Lakes institutions, the detailed scientific program has been largely driven by the topics which participants choose to present. The detailed program is below. It is preferred that presentations at GLCW9 be directly relevant to one of the following topics:

  • Large Scale Structure (including CMB and galaxy clusters)
  • Cosmological Simulations
  • Cosmological Data Analysis (including dark matter detection)
  • Astroparticle/Early Universe

Contributed talks will be limited to 12 minutes, plus an additional 3 minutes for questions. In addition, contributed talks will be supplemented by slightly longer (25+5 min) talks from distinguished faculty of several Great Lakes Institutions.

Talks are grouped into ten ~1.5 hour sessions comprising both  contributed talks by GLCW9 participants and talks by invited speakers.  In order to ensure compliance with the schedule, time limits will be strictly enforced, so we request that you plan accordingly. There will also be a poster session.
 
Copies of the talks (slides only) presented at GLCW9 will be made available on-line at this web site.

Plenary speakers include:

 John Beacom (Ohio State University) , Rachel Bean (Cornell University), Cliff Burgess (Perimeter), Jane Charlton (Pennsylvania State University), Douglas Clowe (Ohio University), August Evrard (University of Michigan), Joshua Frieman (Fermilab/Chicago), Lev Kofman (CITA), Bhuvnesh Jain (University of Pennsylvania), Jeffrey Newman (University of Pittsburgh), Ue-Li Pen (CITA), David Weinberg (Ohio State University), Michael Wood-Vasey (Harvard, University of Pittsburgh)

Location

The workshops will take place in the Carnegie Mellon University Center. Unless posted otherwise, all talks will be held in the Rangos rooms on the second floor.
 

Schedule

Sunday June 8
6-9 p.m.: Registration / Reception - Rangos Auditorium
A buffet meal will be provided at the reception.

Monday June 9

9-10:30 a.m.: Session I
10:30-11 a.m.: Coffee Break
11 a.m.-12:45 p.m.: Session II
12:30-2:30 p.m.: Lunch Break
2:30-4 p.m.: Session III
4-4:30 p.m.: Coffee Break
4:30-6 p.m.: Session IV

Tuesday June 10
9-10:30 a.m.: Session V
10:30-11 a.m.: Coffee Break
11 a.m.-12:45 p.m.: Session VI
12:30-2:30 p.m.: Lunch Break
2:30-4 p.m.: Session VII
4-4:30 p.m.: Coffee Break
4:30-6 p.m.: Session VIII
6:30-9:30 p.m.: GLCW9 Banquet - Carnegie Museum

Wednesday June 11
9-10:30 a.m.: Session IX
10:30-11 a.m.: Coffee Break
11 a.m.-12:45 p.m.: Session X

Oral presentation program

(*=30 min talks, others 15 min) 

Session  1 Mon 9am-10:30am  (Chair: Ryan Scranton)

Fred Gilman, CMU, Welcoming remarks

*August Evrard, Michigan, Challenges for Galaxy Cluster Cosmology

*Bhuvnesh Jain, Penn, Tests of dark energy and gravity with lensing

 Xinghai Zhao,  Notre Dame, Effects of Structure Formation on the Apparent Expansion Rate of the Universe

 Graziano Rossi, Penn, Peak Statistics in the WMAP Sky:  Non-Gaussianity?

Session  2 Mon 11am-12:45pm (Chair: Jeff Newman)

*Josh Frieman, Fermilab/UChicago, First Results from the SDSS Supernova Survey  

*Michael Wood-Vasey Harvard/Pitt, Supernova Cosmology from Today and Tomorrow to the Future,
Infinity, and Beyond 

Matt Kistler, Ohio State, What's the Deal with Supernovae?

Christopher Genovese, CMU, Nonparametric Inference for the Dark Energy Equation of State using Type Ia Supernova 

Suman Bhattacharya, Pitt, Measuring Mean Pairwise Velocity from LSST Supernovae Survey

Session  3 Mon 2:30pm-4pm (Chair Rich Holman)

*Cliff Burgess, McMaster/Perimeter/CERN String Inflation

*Lev Kofman, CITA,TBA

 Cristian Armendariz-Picon, Syracuse, Preheating with Derivative Couplings

 Jimmy Hutasoit, CMU, Non-linear Dynamics in Axionic Inflation

Session  4 Mon 4:30pm-6pm (Chair: Arthur Kosowsky)

*Rachel Bean, Cornell, Observational signatures of brane inflation.
 
Michele Fontanini, Syracuse, The Limits of Cosmological Perturbation Theory
 
Chad Fendt, Univ. Illinois at UC, Pico:  Parameters for the Impatient Cosmologist
Rahul Biswas, Univ. Illinois at UC, Bayesian Forecasting of Cosmological Parameter Constraints for Future Experiments
Peter Freeman, CMU, Nonparametric Estimation of CMB Foreground Emission

Session  5 Tue 9am-10:30am (Chair: Jeff Peterson)

*John Beacom, Ohio State, A New Era in High Energy Astronomy
Catherine Bailey, Case Western, First 5 Tower CDMS Analysis Results
Matthew Szydagis, UChicago, Spin-Dependent WIMP Limits from a Bubble Chamber
        
Sean Bryan, Case, SPIDER:  A Balloon-Borne Experiment to Measure CMB Polarization on Large Angular Scales
 
David Friedenberg, CMU, Object Detection in Arcminute-Resolution Microwave, Background Maps with Statistical Error Control

Session  6 Tue 11am-12:45pm (Chair: David Turnshek)

*Douglas Clowe, Ohio U., Cosmological Constraints from Weak Lensing Observations of Galaxy Clusters
 
Barun Dhar, UMinnesota, Reconstructing Dark Matter Distribution in Clusters of  Galaxies:  A New Approach
Zhaoming Ma, Penn Effect of Source Clustering on Weak Lensing
Ross Fadely, Rutgers, Dark and Luminous Matter in the Gravitational Lens Q0957+561
David Gilbank, Univ. Waterloo, Cosmology with the Red-sequence Cluster Survey 2 (RCS-2)

Session  7 Tue 2:30pm-4:00pm (Chair: Tiziana Di Matteo)

*David Weinberg, Ohio State, SDSS-III: Dark Energy and Near-Field Cosmology
 
James Wadsley, McMaster Univ., Stellar Feedback in Dwarf Galaxy Formation and the Structure of Dark Matter Halos
Greg Stinson, McMaster Univ. SPH Simulations of Galaxy Formation with Supernova Feedback
Silvia Bonoli, MPA,  Co-evolution of Supermassive Black Holes and Galaxies:  Models for BH Accretion and Quasars
Elena Rasia, UMichigan, The M-Yx Relation for Clusters During Extreme Mergers

Session  8 Tue 4:30pm-6pm (Chair: David Weinberg)

*Ue-Li Pen, CITA, TBA 
Tonia M. Venters, UChicago, The Extragalactic Gamma-ray Background:  Modeling Blazars to Constrain D
ark Matter 
 
Cameron McBride, Pitt, Our non-Gaussian Universe:  Higher Order Clustering in Galaxy Surveys
Neal Dalal, UToronto, Halo Assembly Bias
      
Jorge Moreno, Penn, The Creation of Dark Matter Haloes      

Session  9  Wed 9am-10:30am (Chair: Gus Evrard)

*Jeff Newman, Pitt, Calibrating Photometric Redshifts for Dark Energy Experiments with Cross-Correlation Techniques
 
Brian Nord, Michigan, Calibration of upcoming surveys in the laboratory and in silicon: Filter testing for the Dark Energy Survey 
 
Niraj Welikala, Pitt, Spatially Resolved Galaxy Star Formation and its Environmental Dependence
Tsz Yan Lam, Penn, The Probability distribution Function of Dark Matter in Real and Redshift  Space
Fred C. Adams, UMichigan, Orbits and instabilities in Triaxial Dark Matter Halos

Session  10 Wed 11am-12:45pm (Chair: Rupert Croft)

*Jane Charlton, PSU, Mapping the Gas in the Universe
 
Darren Reed, Los Alamos Nat. Lab, The Clustering of the 1st Galaxies 
 
Gabriel Altay, CMU, SPHRAY Tracing low mass galaxies with a view towards reionization
Hasan Yuksel, Ohio State, Revealing the High-Redshift Star Formation Rate with gamma-Ray Bursts
Eli Visbal CfA,Constraining Cosmological Parameters with 21cm Surveys
 
Rishi Khatri, UIllinois at UC, Fundamental Physics from the Cosmological 21 cm Radiation
 

Poster presentations

 Matthew Bayliss, Chicago, Cluster-scale gravitational lenses.

 Jonathan Dudley, McGill, Modelling the Vishniac Effect

 Felipe Marin, Chicago, Galaxy bias from the LRG 3point correlation function

 Chris Orban, OSU,  Delving deeper into the tumultuous lives of galactic dwarfs: modelling star formation histories

 Joseph W. Richards, CMU, Dimensionality Reduction and Efficient Inference for Astronomical Spectra    

 Paul Ricker, UIUC,  Expected Counts of Galaxy Cluster Radio Halos in Low-Frequency Radio Surveys
 
 Megan Roscioli, UChicago, Radio Sources in Galaxy Clusters
 
 Regina Schulte-Ladbeck, Pitt, The Dwarf Galaxies Crisis of Cosmology Continues
 
 Sijing Shen, McMaster Univ., Probing Metals in the Intergalactic Medium
 
 Alexander van Engelen, McGill Univ., Cosmological Parameters and the Promordial Power Spectrum