Laurie Duncan Shaw. Research Positions. Education
|
|
|
- Estella Hall
- 7 years ago
- Views:
Transcription
1 Laurie Duncan Shaw 122 Foster Street New Haven Connecticut USA, Nationality: British Date of birth: 15 March 1981 Phone : Fax : laurie.shaw@yale.edu lds4/ Research Positions 09/ Yale University present Postdoctoral Associate, Yale Centre for Astronomy and Astrophysics Postdoctoral Mentor: Prof. Daisuke Nagai 11/ McGill University 08/2009 Postdoctoral Research Fellow, Department of Physics Postdoctoral Mentor: Prof. Gil Holder Education University of Cambridge, UK Ph.D. Institute of Astronomy Thesis Advisor: Prof. Jeremiah P. Ostriker (since 7/2004 Princeton University) Thesis Title: Analysing Bound Structures in Cosmological N-body Simulations Imperial College, London, UK Msci. Physics, 1st Class with Honours Diploma Thesis: Constraining the Jovian Magnetodisc Parameters Thesis Advisor: Dr. Michelle Dougherty Research Interests Cosmological structure formation Hydrodynamical simulations of galaxy clusters Sunyaev-Zel dovich surveys and observations of galaxy clusters The cosmic microwave background and secondary anisotropy signals The origins of the cosmic infrared background The epoch of reionization Scholarships and Awards Postdoctoral Fellowship, McGill University, Oct 2006-Sep 2009 PPARC Graduate Student Fellowship, Oct ASH Scholarship, Imperial College London, Oct 1999 Astronomy R international essay-writing competition, runner up, May 1998
2 Laurie Duncan Shaw (2 of 5) Funding Proposals Precision Modeling for Sunyaev-Zel dovich surveys, NSF Extragalactic Astronomy and Cosmology Program, $717,204, (PI: D. Nagai, Yale) Observing Proposals Measuring the kinetic SZ signal from Reionization Awarded 79 hours of Herschel time to map 100 deg 2 at priority 1 (PI: J. Carlstrom, Chicago), 2010 The SPT-Spitzer Deep Field Awarded time to survey 100 deg 2 with Spitzer (PI: S. Stanford, UC Davis), 2011 IRAC Imaging of SPT Clusters Awarded time to observe 84 high-redshift clusters (PI: M. Brodwin, CfA), 2009 Professionol Activities Referee, ApJ, MNRAS, A&A, JCAP Student Supervision Pearson Miller, Yale Undergrad I currently supervise Pearson, who is working with me investigating spatial correlations between the cosmic infrared background and the thermal SZ signal. Camille Avestruz, Yale Grad During 2009 I supervised Camille on her project to develop source-extraction algorithms for detecting clusters via their thermal SZ signal. Adele Plunkett, Yale Grad supervised Adele for her graduate theory project. For this project, Adele helped apply a semi-analytic model for the intra-cluster medium to clusters identified in an N-body simulation and compared the results to those from hydrodynamical simulations. Nathalie Ouellette, McGill undergrad co-supervised summer student Nathalie Ouellette for her research project, which involved running and analysing cosmological simulations with the RAMSES hydrodynamics code. Teaching Experience and Student Supervision Lecturing, Covering lecturer for Prof. Tracey Webb and Prof. Gil Holder lecturing second and third year undergraduate courses Introduction to Astrophysics & Classical Mechanics. Supervisor, Part 1A Mathematics, undergraduate Natural Sciences, Cambridge, Topics: algebra and calculus of both scalar and vector functions, ordinary and partial differential equations, Fourier series, matrices, complex numbers, statistics and elementary computational techniques. Observing Experience NTT, EMMI, identification of planetary nebulae in galaxy NGC 5128 using narrow band on/off imaging of the O3 emission line.
3 Laurie Duncan Shaw (3 of 5) Referees Prof. Jeremiah P. Ostriker Prof. Gilbert Holder Department of Astrophysical Sciences Department of Physics Princeton University McGill University Peyton Hall - Ivy Lane 3600 rue University Princeton, NJ Montreal H3A 2T8 USA. QC, Canada ostriker@princeton.edu gil.holder@gmail.com tel: +1 (609) tel: Prof. Daisuke Nagai Prof. John Carlstrom Department of Physics Kavli Institute for Cosmological Physics Yale University University of Chicago J. W. Gibbs Laboratory, 260 Whitney Avenue 933 East 56th Street Yale, CT Chicago, IL USA. USA daisuke.nagai@yale.edu jc@kicp.uchicago.edu tel: +1 (203) Tel. +1 (773)
4 Laurie Duncan Shaw (4 of 5) Publication Statistics As of 26th September, 2011 (and since 2005) 22 papers published plus two submitted First author on 7 papers total of 763 citations (195 for first-authored papers) h-index of 18 Refereed Publications 1. L.D. Shaw, D.H. Rudd, D. Nagai, Deconstructing the kinetic SZ Power Spectrum, 2011, submitted to ApJ, (ArXiv: ) 2. R. Williamson, B.A. Benson, F.W. High,..., L.D. Shaw, et al., A Sunyaev-Zel dovich-selected Sample of the Most Massive Galaxy Clusters in the 2500 deg 2 South Pole Telescope Survey, 2011, ApJ, 738, K. Andersson, B.A. Benson,..., L.D. Shaw, et al., X-Ray Properties of the First Sunyaev- Zel dovich Effect Selected Galaxy Cluster Sample from the South Pole Telescope, 2011, ApJ, 738, E. Shirkoff, C.L. Reichardt, L.D. Shaw, et al., Improved Constraints on Cosmic Microwave Background Secondary Anisotropies from the Complete 2008 South Pole Telescope Data,2011, ApJ, 736, K. Storey,..., L.D. Shaw, et al., South Pole Telescope Detections of the Previously Unconfirmed Planck Early SunyaevZel dovich Clusters in the Southern Hemisphere,2011, ApJ, 735, 36, 6. R. Keisler, C.L. Reichardt,..., L.D. Shaw, et al., A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope, 2011, submitted to ApJ, (ArXiv: ) 7. R.J. Foley, K. Andersson, G. Bazin,..., L.D. Shaw, et al., Discovery and Cosmological Implications of SPT-CL J , the Most Massive Known Cluster at z > 1, 2011, ApJ, 731, M. Millea, O. Dore, J. Dudley, G.P. Holder, L. Knox, L. Shaw, Y-S. Song, O. Zahn, Modeling Extragalactic Foregrounds and Secondaries for Unbiased Estimation of Cosmological Parameters From Primary CMB Anisotropy, 2011, submitted to ApJ, ArXiv L.D. Shaw, D. Nagai, S. Bhattacharya, E.T. Lau, Impact of Cluster Physics on the Sunyaev- Zel dovich Power Spectrum, 2010, ApJ, 725, F.W. High, B. Stalder, Song.J,..., L.D. Shaw, et al.,optical Redshift and Richness Estimates for Galaxy Clusters Selected with the Sunyaev-Zel dovich Effect from 2008 South Pole Telescope Observations, 2010, ApJ, 723, 1736
5 Laurie Duncan Shaw (5 of 5) 11. K. Vanderlinde, T.M. Crawford, T. de Haan, J. Dudley, L.D. Shaw et al., Galaxy Clusters Selected with the Sunyaev-Zel dovich Effect from 2008 South Pole Telescope Observations,2010, ApJ, 722, M. Brodwin, J. Ruel,..., L.D. Shaw, et al., SPT-CL J : A Massive z 1 Galaxy Cluster Selected Via the Sunyaev-Zel dovich Effect with the South Pole Telescope,2010, ApJ, 721, M. Lueker, C.L. Reichardt, K.K. Schaffer,..., L.D. Shaw, et al., Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope,2010, ApJ, 719, J.D. Vieira, T.M. Crawford, E.R. Switzer,..., L.D. Shaw, et al, Extragalactic Millimeter-wave Sources in South Pole Telescope Survey Data: Source Counts, Catalog, and Statistics for an 87 Square-degree Field,2010, ApJ, 719, N.R. Hall, R. Keisler, L. Knox,..., L.D. Shaw, et al., Angular Power Spectra of the Millimeterwavelength Background Light from Dusty Star-forming Galaxies with the South Pole Telescope,2010, ApJ, 718, L.D. Shaw, G.P. Holder, J. Dudley, Non-Gaussian Scatter in Cluster Scaling Relations, 2010, ApJ, 718, T. Plagge, B.A. Benson,..., L.D. Shaw, et al., Sunyaev-Zel dovich Cluster Profiles Measured with the South Pole Telescope, 2010, ApJ, 716, L. D. Shaw, O. Zahn, G.P. Holder, O. Dore Sharpening the Precision of the Sunyaev-Zel dovich Power Spectrum, 2009, ApJ, 702, Staniszewski Z.,..., L.D. Shaw, et al., Galaxy Clusters Discovered with a Sunyaev-Zel dovich Effect Survey, 2009, ApJ, 701, L.D. Shaw, Holder G., Bode, P., The Impact of Halo Properties, Energy Feedback, and Projection Effects on the Mass-SZ Flux Relation, 2008, ApJ, 686, Bode P., Ostriker J. P., Weller J., Shaw, L. D., Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback, ApJ, 663, 139 (2007) 22. L.D. Shaw, Weller J., Ostriker J. P., Bode P., The Bound Mass of Substructures in Dark Matter Halos, ApJ, 659, 1082 (2007) 23. L.D. Shaw, Weller J., Ostriker J. P., Bode P., The Statistics of Physical Properties of Dark Matter Clusters, ApJ, 646, 815 (2006) 24. Weller J., Ostriker J. P., Bode P., L.D. Shaw, Fast Identification of Bound Structures in Large N-body Simulations, MNRAS, 364, 823 (2005)
Cosmological Analysis of South Pole Telescope-detected Galaxy Clusters
Cosmological Analysis of South Pole Telescope-detected Galaxy Clusters March 24th Tijmen de Haan (McGill) - Moriond 2014 Photo credit: Keith Vanderlinde Outline The galaxy cluster sample Calibrating the
Summary of Data Management Principles South Pole Telescope
Summary of Data Management Principles South Pole Telescope Experiment description - Where it is: The South Pole Telescope (SPT) is a 10-meter-diameter telescope located at the Amundsen-Scott South Pole
1 Personal. Name: Graça Maria Moreira de Sousa Teixeira da Rocha. Nationality: Portuguese.
Curriculum Vitae Graça Rocha 1 Personal Name: Graça Maria Moreira de Sousa Teixeira da Rocha. Nationality: Portuguese. Work address: Cavendish Astrophysics Group Cavendish Laboratory Madingley Road Cambridge
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion σ v and X-Ray Y X Measurements
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion σ v and X-Ray Y X Measurements The Harvard community has made this article openly available. Please
The Science Education System in Oxford and the UK. David Andrews
The Science Education System in Oxford and the UK David Andrews 1 Outline of this talk High school education (brief) Undergraduate education Oxford Physics Other sciences at Oxford Other universities Postgraduate
University of Wisconsin - Madison B.S., May 2003, Astronomy-Physics (with Comprehensive Honors), Physics, French
EDUCATION TABASGO Postdoctoral Fellow Department of Physics, Mail Code 9530 University of California, Santa Barbara, CA 93106 Tel 805.893.3189 Fax 805.893.3307 mkpresco@physics.ucsb.edu University of Arizona
WIMP dark matter and the isotropic radio signal Roberto A. Lineros R. Instituto de Física Corpuscular - CSIC/U. Valencia @Roberto_Lineros Outline Introduction Cosmic ray propagation Synchrotron emission
Physics Department Phone: (541)357-9284 Center of High Energy Physics Fax: (541)346-5217
Spencer Chang Curriculum Vitae Contact Information Research Positions Education Awards Teaching Physics Department Phone: (541)357-9284 Center of High Energy Physics Fax: (541)346-5217 University of Oregon
Galaxy clusters, in the light of Planck. Nabila Aghanim, Institut d'astrophysique Spatiale, CNRS-Univ. Paris Sud
Galaxy clusters, in the light of Planck Nabila Aghanim, Institut d'astrophysique Spatiale, CNRS-Univ. Paris Sud Galaxy clusters in the cosmic web CLEF-SSH hydro simulation, Kay et al. '06 Cluster components
Jeremy Sakstein Curriculum Vitae
Contact Information University of Portsmouth Dennis Sciama Building Burnaby Road Portsmouth PO1 3FX Email: jeremy.sakstein@port.ac.uk Website: jeremysakstein.com www.icg.port.ac.uk/author/saksteij/ Academic
NASA's Postdoctoral Fellowship Programs
NASA's Postdoctoral Fellowship Programs Einstein Fellowships Dr. Charles A. Beichman & Dr. Dawn M. Gelino NASA Exoplanet Science Institute Dr. Ron Allen Space Telescope Science Institute Dr. Andrea Prestwich
Malcolm S. Longair. Galaxy Formation. With 141 Figures and 12 Tables. Springer
Malcolm S. Longair Galaxy Formation With 141 Figures and 12 Tables Springer Contents Part I Preliminaries 1. Introduction, History and Outline 3 1.1 Prehistory 3 1.2 The Theory of the Expanding Universe
Curriculum Vitae: Kazuya Koyama
Curriculum Vitae: Kazuya Koyama Personal Record PERSONAL INFORMATION Kazuya Koyama Reader in Cosmology in the Institute of Cosmology and Gravitation at the University of Portsmouth Dennis Sciama Building,
The Crafoord Prize 2005
I N F O R M A T I O N F O R T H E P U B L I C The Royal Swedish Academy of Sciences has decided to award the Crafoord Prize in Astronomy 2005 to James Gunn, Princeton University, USA, James Peebles, Princeton
Physical Self-Calibration of X-ray and SZ Surveys
Physical Self-Calibration of X-ray and SZ Surveys Greg L. Bryan, Zoltan Haiman (Columbia University) and Joshua D. Younger (CfA) 1. Cluster Surveys and Self-Calibration Clusters of galaxies form at the
Astronomy & Physics Resources for Middle & High School Teachers
Astronomy & Physics Resources for Middle & High School Teachers Gillian Wilson http://www.faculty.ucr.edu/~gillianw/k12 A cosmologist is.... an astronomer who studies the formation and evolution of the
8 Radiative Cooling and Heating
8 Radiative Cooling and Heating Reading: Katz et al. 1996, ApJ Supp, 105, 19, section 3 Thoul & Weinberg, 1995, ApJ, 442, 480 Optional reading: Thoul & Weinberg, 1996, ApJ, 465, 608 Weinberg et al., 1997,
Cosmological constraints from large scale structure Relationship between galaxies and dark matter halos Cosmological neutrinos
Beth Ann Reid Contact Information Research Interests Education Lawrence Berkeley National Laboratory 1 Cyclotron Road MS 50R5008 Berkeley, CA 94720 Cosmological constraints from large scale structure Relationship
Einstein Rings: Nature s Gravitational Lenses
National Aeronautics and Space Administration Einstein Rings: Nature s Gravitational Lenses Leonidas Moustakas and Adam Bolton Taken from: Hubble 2006 Science Year in Review The full contents of this book
Top 10 Discoveries by ESO Telescopes
Top 10 Discoveries by ESO Telescopes European Southern Observatory reaching new heights in astronomy Exploring the Universe from the Atacama Desert, in Chile since 1964 ESO is the most productive astronomical
Software challenges in the implementation of large surveys: the case of J-PAS
Software challenges in the implementation of large surveys: the case of J-PAS 1/21 Paulo Penteado - IAG/USP pp.penteado@gmail.com http://www.ppenteado.net/ast/pp_lsst_201204.pdf (K. Taylor) (A. Fernández-Soto)
Perspective of discoveries from Intergalactic Space. Matteo Viel INAF/OATS & INFN/TS Off-the-beaten-track workshop ICTP Trieste - 14 th April 2015
Perspective of discoveries from Intergalactic Space Matteo Viel INAF/OATS & INFN/TS Off-the-beaten-track workshop ICTP Trieste - 14 th April 2015 1 OFF-THE-BEATEN-TRACK TOPIC #1: MASSIVE NEUTRINOS 2 COSMOLOGICAL
HIGHLIGHTS OF RECENT RESULTS FROM THE VERITAS GAMMA-RAY OBSERVATORY TAUP-2015 TORINO. Lucy Fortson. VERITAS Collaboration. Fortson, TAUP 2015, Torino
HIGHLIGHTS OF RECENT RESULTS FROM THE VERITAS GAMMA-RAY OBSERVATORY TAUP-2015 TORINO Lucy Fortson forlucy the VERITAS Collaboration Fortson, TAUP 2015, Torino 1 499 PMTs 3.5o field of view 0.15o spacing
Self Calibration of Cluster Counts: Observable-Mass Distribution. Wayne Hu Kona, March 2005
Self Calibration of Cluster Counts: Observable-Mass Distribution Wayne Hu Kona, March 2005 Self Calibration of Cluster Counts: Observable-Mass Distribution Wayne Hu Kona, August 2004 Scattered Forecasts
Undergraduate Studies Department of Astronomy
WIYN 3.5-meter Telescope at Kitt Peak near Tucson, AZ Undergraduate Studies Department of Astronomy January 2014 Astronomy at Indiana University General Information The Astronomy Department at Indiana
Neil D. Christensen CV 1
Neil D. Christensen CV 1 Neil D. Christensen Department of Physics University of Wisconsin - Madison 5213 Chamberlin Hall Madison, WI 53706 Phone: (608) 890-1001 Fax: (608) 262-8628 Email: neil@hep.wisc.edu
PhD School of Physics University of Trieste
PhD School of Physics University of Trieste Scientific Council Meeting REPORT OF THE SCIENTIFIC COUNCIL December 2011 1 Scientific Council Report. 1. Introduction. The objective of the present report is
Galaxy Survey data analysis using SDSS-III as an example
Galaxy Survey data analysis using SDSS-III as an example Will Percival (University of Portsmouth) showing work by the BOSS galaxy clustering working group" Cosmology from Spectroscopic Galaxy Surveys"
Description of the Dark Energy Survey for Astronomers
Description of the Dark Energy Survey for Astronomers May 1, 2012 Abstract The Dark Energy Survey (DES) will use 525 nights on the CTIO Blanco 4-meter telescope with the new Dark Energy Camera built by
ASTRONOMY and ASTROPHYSICS
UNDERGRADUATE CURRICULUM B. S. PROGRAM ASTRONOMY and ASTROPHYSICS MICHIGAN STATE UNIVERSITY February 2013 Prof. Daniel Stump Undergraduate Program Director Department of Physics and Astronomy Michigan
CURRICULUM VITAE. Marcos Lima
CURRICULUM VITAE Marcos Lima Current Address Department of Physics & Astronomy Tel: (215) 898-0790 University of Pennsylvania Fax: (215) 898-2010 209 South 33rd St., DRL 4N4 mlima@sas.upenn.edu Philadelphia,
Orfeas Kypris. Curriculum Vitae. Personal Statement. Experience. Academic. Miscellaneous
Orfeas Kypris Curriculum Vitae Personal Statement I m a postdoctoral research associate in the Sensor Networks group at the Department of Computer Science at the University of Oxford, and my research focus
The Search for Dark Matter, Einstein s Cosmology and MOND. David B. Cline
The Search for Dark Matter, Einstein s Cosmology and MOND David B. Cline Astrophysics Division, Department of Physics & Astronomy University of California, Los Angeles, CA 90095 USA dcline@physics.ucla.edu
arxiv:1007.4101v1 [astro-ph.co] 23 Jul 2010
![arxiv:1007.4101v1 [astro-ph.co] 23 Jul 2010](/thumbs/39/20204778.jpg "arxiv:1007.4101v1 [astro-ph.co] 23 Jul 2010")
arxiv:1007.4101v1 [astro-ph.co] 23 Jul 2010 Trumpeting the Vuvuzela: UltraDeep HI observations with MeerKAT Benne Willem Holwerda Astrophysics, Cosmology and Gravity Centre (ACGC), Astronomy Department,
Spettrometria Differenziale nel millimetrico e sub/mm
Spettrometria Differenziale nel millimetrico e sub/mm Paolo de Bernardis Dipartimento di Fisica, Università La Sapienza Workshop Studi di Osservazione dell Universo 26 Marzo 2009 WP2420 26/03/2009 1 Diversi
UNIVERSITY OF HAWAI I AT MĀNOA ASTRONOMY & ASTROPHYSICS. The University of Hawai i is an equal opportunity/affirmative action institution.
UNIVERSITY OF HAWAI I AT MĀNOA ASTRONOMY & The University of Hawai i is an equal opportunity/affirmative action institution. A M E SSAG E F R O M THE PROGRAM U N D E R G R A D U AT E P R O G R A M S I
Search for Pulsed Emission in Archival VERITAS Data. Since the 2011 VERITAS discovery of very high energy (VHE; E>100 GeV) gamma rays from
Search for Pulsed Emission in Archival VERITAS Data Avery Archer * for The VERITAS Collaboration Washington University in St. Louis E-mail: a.archer@wustl.edu Since the 2011 VERITAS discovery of very high
Undergraduate Degree Programs in the Department of Physics and Astronomy
UNIVERSITY OF PITTSBURGH DIETRICH SCHOOL OF ARTS AND SCIENCES DEPARTMENT OF PHYSICS AND ASTRONOMY Undergraduate Degree Programs in the Department of Physics and Astronomy Updated 8/17/2015 This document
Probing Dark Energy with Baryon Acoustic Oscillations from Future Large Galaxy Redshift Surveys
Probing Dark Energy with Baryon Acoustic Oscillations from Future Large Galaxy Redshift Surveys Hee-Jong Seo (Steward Observatory) Daniel J. Eisenstein (Steward Observatory) Martin White, Edwin Sirko,
Program Proposal Submitted to the College of Science Curriculum Committee (COSCC)
Program Approval Form For approval of new programs and deletions or modifications to an existing program. Action Requested: Type (Check one): Create New (SCHEV approval required except for minors) B.A.
Modeling Galaxy Formation
Galaxy Evolution is the study of how galaxies form and how they change over time. As was the case with we can not observe an individual galaxy evolve but we can observe different galaxies at various stages
FIRST LIGHT IN THE UNIVERSE
FIRST LIGHT IN THE UNIVERSE Richard Ellis, Caltech 1. Role of Observations in Cosmology & Galaxy Formation 2. Galaxies & the Hubble Sequence 3. Cosmic Star Formation Histories 4. Stellar Mass Assembly
Planck Early Results: New light on Anomalous Microwave Emission from Spinning Dust Grains
Planck Early Results: New light on Anomalous Microwave Emission from Spinning Dust Grains Perseus in the optical Clive Dickinson Jodrell Bank Centre for Astrophysics (University of Manchester) On behalf
The Birth and Assembly of Galaxies: the Relationship Between Science Capabilities and Telescope Aperture
The Birth and Assembly of Galaxies: the Relationship Between Science Capabilities and Telescope Aperture Betsy Barton Center for Cosmology University of California, Irvine Grateful acknowledgements to:
The Mainz LXe TPC MC simulations for a Compton scattering experiment
The Mainz LXe TPC MC simulations for a Compton scattering experiment Pierre Sissol Johannes Gutenberg Universität Mainz 12 November 2012 1 / 24 Outline 1 Dark Matter 2 Principle of a dual-phase LXe TPC
Cover Page. The handle http://hdl.handle.net/1887/36959 holds various files of this Leiden University dissertation.
Cover Page The handle http://hdl.handle.net/1887/36959 holds various files of this Leiden University dissertation. Author: Richings, Alexander James Title: Non-equilibrium chemistry and cooling in simulations
Adaptive Optics (AO) TMT Partner Institutions Collaborating Institution Acknowledgements
THIRTY METER TELESCOPE The past century of astronomy research has yielded remarkable insights into the nature and origin of the Universe. This scientific advancement has been fueled by progressively larger
Supervisors: Ph.D., Dr.scient. Hans C. Fogedby and Prof. Per Bak Institute of Physics & Astronomy, University of Århus, DK-8000 Århus C, Denmark.
Curriculum vitae Personal Name: Kim Christensen. Sex: Male. Date of birth: 1st December, 1962. Place of birth: Søndre Sogn, Viborg, Denmark. Nationality: Danish. Affiliation: Imperial College London, Blackett
Please note that only the German version of the Curriculum is legally binding. All other linguistic versions are provided for information only
Please note that only the German version of the Curriculum is legally binding. All other linguistic versions are provided for information only Curriculum for the Erasmus Mundus Joint Master Program in
Understanding the Accelerating Universe using the MSE. Gong-Bo Zhao NAOC
Understanding the Accelerating Universe using the MSE Gong-Bo Zhao NAOC Nobel Prize 2011 a > 0 The expansion of the Universe can accelerate if In GR, to add new repulsive matter, which contributes 70%
Science Drivers for Big Data Joseph Lazio SKA Program Development Office & Jet Propulsion Laboratory, California Institute of Technology
Science Drivers for Big Data Joseph Lazio SKA Program Development Office & Jet Propulsion Laboratory, California Institute of Technology 2010 California Institute of Technology. Government sponsorship
UR Undergraduate Physics and Astronomy Program Learning Objectives and Assessment Plan
UR hysics and Astronomy rogram Learning Objectives and Assessment lan UR Undergraduate hysics and Astronomy rogram Learning Objectives and Assessment lan A. BS hysics undergraduate program learning objectives
arxiv:1207.3646v1 [cs.ce] 16 Jul 2012
![arxiv:1207.3646v1 [cs.ce] 16 Jul 2012](/thumbs/27/12206435.jpg "arxiv:1207.3646v1 [cs.ce] 16 Jul 2012")
jcis@epacis.org OGCOSMO: An auxiliary tool for the study of the Universe within hierarchical scenario of structure formation arxiv:1207.3646v1 [cs.ce] 16 Jul 2012 Eduardo S. Pereira 1, Oswaldo D. Miranda
Programme Specification Mphys (Hons) Physics with Astronomy
Programme Specification Mphys (Hons) Physics with Astronomy 1 Awarding Institution 2 Teaching Institution 3 Programme Accredited by 4 Final Award 5 Programme title 6 UCAS Code 7 QAA Subject Benchmark 8
A Preliminary Summary of The VLA Sky Survey
A Preliminary Summary of The VLA Sky Survey Eric J. Murphy and Stefi Baum (On behalf of the entire Science Survey Group) 1 Executive Summary After months of critical deliberation, the Survey Science Group
Programme name Mathematical Science with Computer Science Mathematical Science with Computer Science with Placement
PROGRAMME SPECIFICATION KEY FACTS Programme name Mathematical Science with Computer Science Mathematical Science with Computer Science with Placement Award BSc (Hons) School School of Mathematics, Computer
The Applied and Computational Mathematics (ACM) Program at The Johns Hopkins University (JHU) is
The Applied and Computational Mathematics Program at The Johns Hopkins University James C. Spall The Applied and Computational Mathematics Program emphasizes mathematical and computational techniques of
arxiv:astro-ph/9511100v1 21 Nov 1995
An Upper Mass Bound of a Two-Component Protogalaxy Keiko Miyahata and Satoru Ikeuchi Department of Earth and Space Science, Faculty of Science, Osaka University, Machikaneyama-cho, Toyonaka, Osaka 560
Archival Science with the ESAC Science Archives and Virtual Observatory
Archival Science with the ESAC Science Archives and Virtual Observatory Deborah Baines Science Archives and VO Team Scientist European Space Agency (ESA) European Space Astronomy Centre (ESAC) Science
Faber-Jackson relation: Fundamental Plane: Faber-Jackson Relation
Faber-Jackson relation: Faber-Jackson Relation In 1976, Faber & Jackson found that: Roughly, L! " 4 More luminous galaxies have deeper potentials Can show that this follows from the Virial Theorem Why
Computational Astrophysics and Cosmology. Professor Ben Moore, University of Zurich, Switzerland
Program Title Computational Astrophysics and Cosmology Program Acronym ASTROSIM Principal Applicant Professor Ben Moore, University of Zurich, Switzerland Abstract This program aims to bring together European
THESIS PROJECT PROPOSAL FORM
INSTITUTO DE ASTROFÍSICA DE CANARIAS GRADUATE STUDIES DIVISION THESIS PROJECT PROPOSAL FORM NAME OF THE PROPONENT: Jorge Sánchez Almeida Casiana Muñoz Tuñón Alfonso López Aguerri AFFILIATION: (Please indicate
Dr. Timothy D. Morton
Dr. Timothy D. Morton Curriculum Vitae 4 Ivy Lane, Peyton Hall Princeton, NJ, USA 08544 +1 (609) 258 3801 +1 (609) 258 8226 tdm@astro.princeton.edu Education and Work Experience 2007 2013 California Institute
Undergraduate Physics Degree Programs (2015-16)
Undergraduate Physics Degree Programs (2015-16) Physics is concerned with the most basic principles that underlie all phenomena in the universe. Physicists ask, How does the world work? They search for
Dark Energy Survey White Paper for the Dark Energy Task Force Submitted June 15, 2005
Dark Energy Survey White Paper for the Dark Energy Task Force Submitted June 15, 2005 Overview: We plan to carry out a deep optical-near infrared survey of 5000 sq. deg of the South Galactic Cap to ~24
Cosmic Structure Formation and Dynamics: Cosmological N-body Simulations of Galaxy Formation and Magnetohydrodynamic Simulations of Solar Atmosphere
Chapter 3 Epoch Making Simulation Cosmic Structure Formation and Dynamics: Cosmological N-body Simulations of Galaxy Formation and Magnetohydrodynamic Simulations of Solar Atmosphere Project Representative
Institut für Kern- und Teilchenphysik Neutrinos & Cosmology
Neutrinos & Cosmology 1 Cosmology: WHY??? From laboratory experiment limits can be set ONLY in neutrino mass difference No information if neutrino masses are degenerated From kinematic experiment limits
Department of Political Science Phone: (805) 893-5902 University of California, Santa Barbara Fax: (805) 893-3309
NEIL NARANG Department of Political Science Phone: (805) 893-5902 University of California, Santa Barbara Fax: (805) 893-3309 Ellison Hall, Office 3710 Email: narangn@polsci.ucsb.edu Santa Barbara, CA
Exploring the Universe Through the Hubble Space Telescope
Exploring the Universe Through the Hubble Space Telescope WEEK FIVE: THE HUBBLE DEEP FIELD + LIMITATIONS OF HUBBLE, COLLABORATIONS, AND THE FUTURE OF ASTRONOMY Date: October 14, 2013 Instructor: Robert
THEORETICAL PHYSICS @TCD
THEORETICAL PHYSICS @TCD 1 2 4 3 5 6 TR035 Theoretical Physics String Theory 1 Subatomic Collision at CERN 2 Magnetic Molecules Showing Opposite Spin States 3 Crystal Lattice 4 Foam Structure 5 Cosmic
Cosmic Dust in an Expanding Universe?
Planck energy - E - ev Cosmic Dust in an Expanding Universe? QED Radiations, Discovery Bay, Hong Kong, China nanoqed@gmail.com Copyright 2016 Horizon Research Publishing All rights reserved. Abstract Dust
Rashad Moarref 1/5. Rashad Moarref. Postdoctoral Scholar in Aerospace Graduate Aerospace Laboratories Phone: (626) 395 4459
Rashad Moarref 1/5 Rashad Moarref Postdoctoral Scholar in Aerospace Graduate Aerospace Laboratories Phone: (626) 395 4459 California Institute of Technology E-mail: rashad@caltech.edu 1200 E California
High Energy Physics (HEP) Program Status Update to the AAAC Meeting. June 1, 2015
OFFICE OF SCIENCE High Energy Physics (HEP) Program Status Update to the AAAC Meeting June 1, 2015 Kathy Turner Program Manager, Cosmic Frontier Office of High Energy Physics Office of Science, U.S. Department
arxiv:1302.1640v2 [astro-ph.co] 11 Apr 2013
![arxiv:1302.1640v2 [astro-ph.co] 11 Apr 2013](/thumbs/29/13917488.jpg "arxiv:1302.1640v2 [astro-ph.co] 11 Apr 2013")
Draft version April, 03 Preprint typeset using L A TEX style emulateapj v. 5// MASS-DEPENDENT BARYON ACOUSTIC OSCILLATION SIGNAL AND HALO BIAS Qiao Wang and Hu Zhan Key Laboratory of Optical Astronomy,
arxiv:astro-ph/0312025v1 1 Dec 2003
Chinese Journal of Astronomy and Astrophysics manuscript no. (L A TEX: sigma8.tex; printed on August 25, 2013; 4:09) arxiv:astro-ph/0312025v1 1 Dec 2003 The amplitude of mass fluctuations and mass density
Origins of the Cosmos Summer 2016. Pre-course assessment
Origins of the Cosmos Summer 2016 Pre-course assessment In order to grant two graduate credits for the workshop, we do require you to spend some hours before arriving at Penn State. We encourage all of
Virtual Observatories A New Era for Astronomy. Reinaldo R. de Carvalho DAS-INPE/MCT 2010
Virtual Observatories Virtual Observatories 1%%&'&$#-&6!&9:#,*3),!#,6!6#$C!&,&$D2 *:#%&+-3;& D&);&-$2!!"! "!" &,&$D2 %),-&,-!"#$%&'&#()*! $#%&!(!!! $ '!%&$ $! (% %)'6!6#$C!;#--&$G $! '!!! $#63#-3),G $!
Exceptionally massive and bright, the earliest stars changed the course of cosmic history
THE FIRST STARS IN THE UNIVERSE Exceptionally massive and bright, the earliest stars changed the course of cosmic history BY RICHARD B. LARSON AND VOLKER BROMM ILLUSTRATIONS BY DON DIXON We live in a universe
11th Paris Cosmology Colloquium OBSERVATOIRE DE PARIS 16, 17, 18 AUGUST 2007
11th Paris Cosmology Colloquium DARK MATTER, DARK ENERGY, CMB AND LSS : UNDERSTANDING THE PHYSICS OF THE UNIVERSE OBSERVATOIRE DE PARIS 16, 17, 18 AUGUST 2007 ALL SESSIONS take place at "SALLE DU CONSEIL
6 A High Merger Fraction in the Rich Cluster MS 1054 03 at z =0:83: Direct Evidence for Hierarchical Formation of Massive Galaxies y
6 A High Merger Fraction in the Rich Cluster MS 1054 03 at z =0:83: Direct Evidence for Hierarchical Formation of Massive Galaxies y ABSTRACT We present a morphological study of the galaxy population of
NATALKA PATSIURKO. Current Position: Lecturer, Concordia University, Department of Sociology and Anthropology
NATALKA PATSIURKO Current Position: Lecturer, Concordia University, Department of Sociology and Anthropology Address: Concordia University, Dept. of Sociology and Anthropology 1455 de Maisonneuve West
World of Particles Big Bang Thomas Gajdosik. Big Bang (model)
Big Bang (model) What can be seen / measured? basically only light (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)
Curriculum Vitae. Rohini Kumar
Curriculum Vitae Rohini Kumar Contact Information University Address: Mathematics, 1150 Faculty/Administration Building 656 W. Kirby Detroit, MI 48202 Phone: 313.577.2479 email: rkumar@math.wayne.edu Personal
HANDBOOK FOR THE APPLIED AND COMPUTATIONAL MATHEMATICS OPTION. Department of Mathematics Virginia Polytechnic Institute & State University
HANDBOOK FOR THE APPLIED AND COMPUTATIONAL MATHEMATICS OPTION Department of Mathematics Virginia Polytechnic Institute & State University Revised June 2013 2 THE APPLIED AND COMPUTATIONAL MATHEMATICS OPTION
MEIRA LEVINSON. 54 Arborway, Jamaica Plain, MA 02130 (617) 983-5909 meiral@mindspring.com
MEIRA LEVINSON 54 Arborway, Jamaica Plain, MA 02130 (617) 983-5909 meiral@mindspring.com Education Nuffield College, University of Oxford, Oxford, England D.Phil., Politics, March 1997 Thesis title: Autonomy,
2010 Master of Science Computer Science Department, University of Massachusetts Amherst
Scott Niekum Postdoctoral Research Fellow The Robotics Institute, Carnegie Mellon University Contact Information Smith Hall, Room 228 Carnegie Mellon University 5000 Forbes Avenue Pittsburgh, PA 15213
Trusted. Independent. Global.
Trusted. Independent. Global. 1 Born in Salzfurtkapelle Joined QS in 2007 QSIU s Research Manager Took on responsibility for data & knowledge management of the QS WUR Travel to various parts of the world
Yevgeny Goncharov WORK EXPERIENCE
Yevgeny Goncharov Quantitative Risk Management 181 West Madison Street 41 st Floor Chicago, Illinois 60602 Phone: (312) 782-7716 yevgeny.goncharov@qrm.com WORK EXPERIENCE Academic Background 1998 2003
University of Illinois at Chicago Office: SEO 521 Department of Mathematics, Statistics, (312) 413-2605 and Computer Science
Andrew Suk Contact Information Research Interests Employment University of Illinois at Chicago Office: SEO 521 Department of Mathematics, Statistics, (312) 413-2605 and Computer Science suk@math.uic.edu
Programme name Mathematical Science with Computer Science Mathematical Science with Computer Science with Placement
PROGRAMME SPECIFICATION KEY FACTS Programme name Mathematical Science with Computer Science Mathematical Science with Computer Science with Placement Award MMath School School of Mathematics, Computer
Curriculum Vitae Daisuke Nagai
Contact Information Positions: Curriculum Vitae Daisuke Nagai Associate Professor of Physics & Astronomy, Yale University Academic Co-Director, Yale Center for Research Computing Campus Address: 56 Hillhouse
Relating Accretion Rate and Jet Power in Elliptical Galaxies
Relating Accretion Rate and Jet Power in Elliptical Galaxies Robert Dunn Institute of Astronomy, Cambridge Steve Allen (KIPAC), Andy Fabian (IoA), Greg Taylor (UNM) & Chris Reynolds (Maryland) MNRAS, in
GRAN SASSO SCIENCE INSTITUTE PhD PROGRAMS CALL FOR APPLICATIONS 2016
GRAN SASSO SCIENCE INSTITUTE PhD PROGRAMS CALL FOR APPLICATIONS 2016 The Gran Sasso Science Institute (GSSI), based in L Aquila, Italy, offers post-graduate training to obtain Philosophiae Doctor (Ph.D)
The Planck Legacy Archive: current status, contents and future development. Xavier Dupac ESA-ESAC Villanueva de la Cañada, Spain
The Planck Legacy Archive: current status, contents and future development Xavier Dupac ESA-ESAC Villanueva de la Cañada, Spain Outline Introduction Schedule Scientific contents of the PLA Additional contents
REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe
REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe The End of Physics Albert A. Michelson, at the dedication of Ryerson Physics Lab, U. of Chicago, 1894 The Miracle Year - 1905 Relativity Quantum
Astronomical Data Analysis Software & Systems XVI
Astronomical Data Analysis Software & Systems XVI 15-18 October 2006 Tucson, Arizona, USA Events ADASS XVI Today Calendar Conference Schedule Meeting Program Recent News Birds of a Feather Banquet Conference
Master of Science in Mathematics
Master of Science in Mathematics Outline of the program 2015 2017 National Research University Higher School of Economics, Moscow Moscow is one of the major research centers of the world and is a leading
Curriculum Vitae et Studiorum. Giovanni Losurdo
Curriculum Vitae et Studiorum Giovanni Losurdo Email: losurdo@fi.infn.it losurdo@ego-gw.it Tel: +390554572260 - +39050752317 Homepage: http://hep.fi.infn.it/gruppo2/losurdo Place and date of birth: Bari
Mathematics Department Phone: (972)742-3479 Princeton University Fine Hall. Email: jonfick@princeton.edu Washington Road Princeton, NJ 08544-1000
Mathematics Department Phone: (972)742-3479 Princeton University Fine Hall Email: jonfick@princeton.edu Washington Road Princeton, NJ 08544-1000 Education PhD in Mathematics, Rice University, Advisor:
Galaxy clusters with the Square Kilometer Array
Spanish SKA White Book, 2015 Ascaso et al. 37 Galaxy clusters with the Square Kilometer Array B. Ascaso 1, Y. Ascasibar 2, J.M. Diego 3, and S. Planelles 4,5 1 GEPI, Observatoire de Paris, CNRS, Université