CURRICULUM VITAE

Scott DodelsonFermi National Accelerator Laboratory

Box 500 MS-209Batavia, Illinois 60510

(630) 840-2426 ; (847) 982-0429

EMPLOYMENT

Fermi National Accelerator LaboratoryScientist III (2011-present)Interim Director, Center for Particle Astrophysics (2006-2008)Scientist II (2004-2011)Head Theoretical Astrophysics (2001-2006)Scientist I (1999-2004)Associate Scientist (1994-1999)Research Associate (1991-1994)

University of ChicagoProfessor, Part Time, Department of Astronomy and Astrophysics

(2004-present)Associate Professor, Part Time (1998-2004)Visiting Professor (1995-1998)

Northwestern UniversityVisiting Professor, Part Time, Department of Physics and Astronomy

(2004-5)

Harvard UniversityPost-doctoral Fellow, Department of Physics (1988-1991)

Columbia UniversityResearch Assistant, Physics (1985-1988)Research Assistant, Experimental Particle Physics (1983)

Weizmann Institute of ScienceResearch Assistant, Karyn Kupcinet International Science School (1982)

EDUCATION

Columbia UniversityPhD in Theoretical Physics, Advised by Gerald Feinberg (1988)Joint BA/BS in Applied Physics, Columbia College

and School of Engineering and Applied Science (1983)

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TEACHING AND MENTORING

2002-present: Supervised undergraduate theses: Sara Burtwell, “Correlation functionof SDSS galaxies,” (2002); Matt Billmire, “Lensing of the CMB by clus-ters of galaxies,” (2003); Brian Klein, “Weak Lensing by Clusters inHST Data” (2007).

1995-present: Taught in Department of Astronomy and Astrophysics at the Univer-sity of Chicago. Graduate seminars on the large scale structure of theuniverse, the cosmic microwave background, gravitational lensing, andQSO absorbtion systems. Core courses for first year graduate studentson Radiative Processes in Astrophysics, The Galaxy, and Cosmology.Undergraduate course on galaxies and the universe for physics majorsconcentrating in astronomy and PHYSCI 120 “The Universe and Howwe Know”. Taught astronomy course for sophomores at NorthwesternUniversity.

1995-present: Supervised graduate students: Kim Coble (PhD 1999), Ryan Scranton(2002), Eduardo Rozo (2006), Fabian Schmidt (2009), Melanie Simet(2012), Eric Baxter (2009-present), Alan Zablocky (2010-12), Tim Lin-den (2010-11), Sohyun Park (2011-12), Hsin-Yu Chen (2011-12), Young-soo Park (2012-present), Ross Cawthon (2012-present), Alessandro Man-zotti (2012-present).

1994-present: Supervised post-doctoral fellows. These include: Stephane Colombi (cur-rently faculty at IAP), Andrew Heckler (Ohio State), Yun Wang (Okla-homa), Istvan Szapudi (Hawaii), Antonio Riotto (Geneva), Will Kinney(Buffalo), Chris Metzler, Lam Hui (Columbia), Andrew Sornborger (UC,Davis), Ewan Stewart (KAIST), Zoltan Haiman (Columbia), PasqualeBlasi (Florence), Michael Blanton (NYU), Idit Zehavi (Case Western),Ravi Sheth (Penn), Andreas Berlind (Vanderbilt), John Beacom (OhioState), Nicole Bell (Melbourne), Patrick Greene (Texas), Kev Abaza-jian (Irvine), Gianfranco Bertone (GRAPPA Institute), Pengjie Zhang(Shanghai), Dan Hooper (FNAL), Kenji Kadota (Nagoya), Mark Jack-son (IAP, Paris), Chris Vale, Emiliano Sefusatti (ICTP), Pasquale Ser-pico (Savoie, CNRS), Hee-Jong Seo (Berkeley), Jeter Hall (LLNL),Jonghee Yoo (FNAL), Jason Steffen (Sierra), Jeff Kubo, Gajus Mik-naitis, Eun-Joo Ahn (FNAL), Alberto Vallinotto (LBL), and AndrewHearin (FNAL).

1987-1990: Volunteer: Brookline School System and Double Discovery Program inNew York City. Guided disadvantaged elementary student in indepen-dent research project. Tutored urban high school students in math andscience.

1982 - 1986: Preceptor of Columbia’s undergraduate physics labs.

GRANTS

• Framework for Analysis of Cosmological Surveys, DOE-HEP (2013-14)

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• Fermilab PI, Scientific Discovery through Advanced Computing,“Computation-Driven Discovery for the Dark Universe” (2012-14)

• Co-I, NSF Physics Frontier Center, “Pushing Cosmology to the Edge,”(2011-2016)

• PI, National Science Foundation Grant AST-0908072, “Precision Mea-sures of the Dark Sector,” (2009-2012)

• Co-I, DOE Discovering the Nature of Dark Energy Program, “TowardsPrecision Cosmology in the Non-linear Regime” (2008)

• Co-I, NASA Mission Concept Study Award NNX08AT71G S01 (2008-9)• PI, Brinson Post-dostoral Fellowship Program (2006, 2007)• PI, Fermilab-University of Chicago Strategic Collaborative Initiative,

“Computational Cosmology,” (2007)• PI, NASA Grant NAG5-10842, “Fundamental Physics from Space”

(2004-2006)• PI, National Science Foundation Grant 0118263, “Workshop on Cosmol-

ogy” (2001)• PI, National Science Foundation Grant PHY-0079251, “Probing Funda-

mental Physics with Cosmological Observations,” (2000-2003)• Co-I on Fermilab Astrophysics’ NASA ATP grants (1994-2003)

AWARDS

• Honorable Mention, Gravity Research Foundation (2011)• Strategic Laboratory Leadership Program, University of Chicago Busi-

ness School (2008)• Fellow, American Physical Society (2004)• Garden State Graduate Fellowship (1983)• Sigma Pi Sigma (Physics Honor Society) (1983)• Third, second prizes, Van Buren Math Prize Competition (1982,83)• Tau Beta Pi (National Engineering Honor Society) (1982)

PROFESSIONAL ACTIVITIES

• International Advisory Committee, 26th International Conference onNeutrino Physics and Astrophysics (Neutrino 2014)

• Chair, Candidacy Exam Committee, University of Chicago (2012-13)• Convener, Software Working Group, LSST Dark Energy Science Collab-

oration (2012-present)• Organizing Committee, XC3: External Correlations of the CMB and

Cosmology (2013)• Scientific Review, Swiss National Supercomputing Centre (2013)• Deputy Secretary-Treasurer, Division of Astrophysics, American Physical

Society (2013-14)• DOE HEP Dark Energy Science Plan Task Force (2012)• Hans Bethe Award Committee, American Physical Society (2012, 2013)• Co-Chair, Task Force on DES Scientific Computing (2012)

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• Convener, “Dark Energy and CMB” sub-group, Snowmass CommunityStudy (2012-13)

• Panelist, DOE Comparative Reviews (2012, 2013)• Reviewer, NASA Postdoctoral Program (2011)• Co-Lead, Inflation MA, Physics Frontier Center (2011-present)• Co-coordinator, Theory and Combined Probes Working Group, Dark

Energy Survey (2011-present)• Local Organizing Committee, SUSY 2011• Reviewer, Consolider Program, Spanish Ministry of Science and Innova-

tion (2011)• External Reviewer, Research Grants Council, Hong Kong (2011)• Reviewer, DOE Early Career Research Program (2011)• Summer Public Lectures and Dialogs Committee, Aspen Center for

Physics (2011)• Co-convenor, Meeting of the Division of Particles and Fields, APS

(2011)• Chicagoland Task Force on Computational Cosmology, co-Chair (2011)• Reviewer for Discovery Grants submitted to National Sciences and Engi-

neering Research Council of Canada (NSERC)• Reviewer for Swiss National Science Foundation (2010)• Admissions Committee, Aspen Center for Physics (4 years)• Scientific Organizing Committee, Fermilab Symposium on the Cosmic

Frontier (2011)• International Coordinator, Kavli Institute for Theoretical Physics China

4-week Cosmology Program• International Advisory Committee, TAUP 2011• Reviewer, Consolider Cosmology Program (2010)• DOE Visiting Committee, Caltech (2010)• Summer Program Committee, Aspen Center for Physics (2010)• Chair, NASA Astrophysics Theory Program Review Panel “Cosmic Mi-

crowave Background” (2009)• Chair, NSF Review Panel “Large Scale Structure” (2009)• Co-Chair, Scientific Committee, Theoretical Advanced Studies Institute

(TASI) (2009)• Chair, Summer Program Committee, Aspen Center for Physics (2009)• Strategic Planning Committee, Kavli Institute for Cosmological Physics

(2008-9)• Chair, Organizing Committee, CMBPol Theory Workshop (2008)• Editor, Physics Letters B (2008-present)• Advisor, Annual Review of Nuclear and Particle Science (2007)• External Referee: Israel Science Foundation, Natural Sciences and Engi-

neering Research Council of Canada (2007)• Chair, NASA Astronomy and Physics Research and Analysis panel

(2007)

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• Panel Member for DOE Innovative and Novel Computational Impact onTheory and Experiment (INCITE) Program (2006)

• Member, Astronomy and Astrophysics Advisory Committee (2006-09)• Member, Aspen Center for Physics (2006-present)• Program Committee, Annual Meeting Division of Particle of Fields

(2006)• Managing Editor, International Journal of Modern Physics D (2004-08)• Divisional Editor, Physical Review D (2004-06)• Organizer, “Fundamental Physics from Clusters of Galaxies” (2004)• Editor, Journal of Astroparticle Physics (2003-present)• Member, Local Advisory Committee, Center for Cosmological Physics,

Chicago (2001-5)• Head, External Advisory Committee, Theoretical Astrophysics Center,

Denmark (2002)• Co-organizer, Workshop on Neutrinos and Cosmology, Fermilab and

Cosmo-02 (2002)• Co-Organizer “Chicago Chattaqua on Cosmology,” for thirty college

teachers (1999,2001)• Co-Organizer “Pritzker Symposium and Workshop on Inflation,” (1999)

“Inner Space/Outer Space II,” and “Santa Fe Workshop on Cosmology”(1999).

• Organized “Sloan Digital Sky Survey Collaboration Meeting” and “Miss-ing Energy in the Universe” Workshop (1998)

• Panel member for National Science Foundation research proposals• Panel member for NASA Astrophysics Theory Program research propos-

als• Reviewer for Department of Energy research proposals• Referee for Physical Review D, Physical Review Letters, AstrophysicalJournal, Astrophysical Journal Letters, Annals of Physics, Physics Let-ters, New Astronomy, Nature, JCAP

• Preceptor overseeing undergraduate labs, Columbia University (1985)

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Books

Modern Cosmology (Academic Press, Amsterdam, 2003).

CMB Polarization Workshop: Theory and Foregrounds: CMBPol Mission ConceptStudy, Editor (American Institute of Physics, 2009).

Physics of the Large and the Small: Tasi 2009, Proceedings of the 2009 TheoreticalAdvanced Study Institute in Elementary Particle Physics, co-Editor (World Scientific2011).

Scientific Publications

[1] S. Dodelson and M. D. Schneider, “Simulation Covariance Error,” arXiv:1304.2593.

[2] Z. Hou, et al., “Constraints on Cosmology from the Cosmic Microwave BackgroundPower Spectrum of the 2500-square degree SPT-SZ Survey,” arXiv:1212.6267.

[3] A. R. Zentner, E. Semboloni, S. Dodelson, T. Eifler, E. Krause and A. P. Hearin,“Accounting for Baryons in Cosmological Constraints from Cosmic Shear,” to bepublished in Phys. Rev. D arXiv:1212.1177.

[4] A. Abate et al., “Large Synoptic Survey Telescope: Dark Energy Science Collabora-tion,” arXiv:1211.0310.

[5] S. Park and S. Dodelson, “ Structure formation in a nonlocally modified gravitymodel,” Phys. Rev. D 87, 024003 (2013).

[6] P. Adshead, E .Baxter, S. Dodelson, and A. Lidz, “Non-Gaussianity and ExcursionSet Theory: Halo Bias,” Phys. Rev. D 86 063526 (2012).

[7] L. Boubekeur, S. Dodelson, and O. Vives, “Cold Positrons from Decaying DarkMatter,’ Phys. Rev. D 86, 103520 (2012).

[8] L. Widrow, S. Gardner, B. Yanny, S. Dodelson, and H.-Y. Chen, “Galactoseismology:Discovery of Vertical Waves in the Galactic Disk,” Astrophys. J. 750 L41 (2012).

[9] S. Dodelson, “The Real Problem with MOND,” International Journal of ModernPhysics D 20, 2749 (2011).

[10] H. Lin, S. Dodelson, et al., “The SDSS Coadd: Cosmic Shear Measurement,” Astro-phys. J. 761, 15 (2012).

[11] M. Simet, J. Kubo, S. Dodelson, et al., “The SDSS Coadd: Cross-Correlation WeakLensing and Tomography of Galaxy Clusters,” Astrophys. J. 748 128 (2012).

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[12] R. Reis, M. Soares-Santos, J. Annis, S. Dodelson, et al., “The SDSS Coadd: A GalaxyPhotometric Redshift Catalog,” Astrophys. J. 747, 59 (2012).

[13] J. Annis, et al., “The SDSS Coadd: 275 deg2 of Deep SDSS Imaging on Stripe 82,”Submitted toAstrophys. J. arXiv:1111.6619 [astro-ph.CO].

[14] H.-J. Seo, M. Sato, M. Takada, and S. Dodelson, “Dark Energy from the log-transformed convergence field,” Astrophys. J. 748 57 (2012).

[15] P. Draper, S. Dodelson, J. Hao, and E. Rozo, “The Sunyaev-Zeldovich Signal of themaxBCG SDSS Galaxy Clusters in WMAP,” Phys. Rev. D 85 023005 (2012).

[16] E. J. Baxter and S. Dodelson, “A Robust Approach to Constraining Dark Matterfrom Gamma-Ray Data,” Phys.Rev.D 83, 123516 (2011).

[17] K. Abazajian, E. Calabrese, A. Cooray, F. De Bernardis, S. Dodelson et al., “Cosmo-logical and Astrophysical Neutrino Mass Measurements,” Astroparticle Physics 35,177 (2011).

[18] A. Vallinotto, S. Dodelson, and P. Zhang, “Magnification as a Tool in Weak Lensing,”Phys. Rev. D 84 103004 (2011).

[19] H.-J. Seo, M. Sato, S. Dodelson, B. Jain, and M. Takada, “Re-capturing cosmic in-formation,” Astrophys. J. Lett. 729, L11 (2011).

[20] E. Baxter, S. Dodelson, S. M. Koushiappas, and L. E. Strigari, “Constraining DarkMatter in Galactic Substructure,” Phys. Rev. D 82, 123511 (2010).

[21] C. Shapiro, S. Dodelson, B. Hoyle, L. Samushia, and B. Flaugher, ,“Will MultipleProbes of Dark Energy find Modified Gravity?,” Phys. Rev. D D82, 043520 (2010).

[22] L.Krauss, S. Dodelson, and S. Meyer, “Primordial Gravitational Waves and Cosmol-ogy,” Science 328 989 (2010).

[23] S. Dodelson, “Cross-Correlating Probes of Primordial Gravitational Waves,” Phys.Rev. D 82, 023522 (2010).

[24] H.-J. Seo, S. Dodelson, J. Marriner, D. Mcginnis, A. Stebbins, C. Stoughton, and A.Vallinotto, “A ground-based 21cm Baryon acoustic oscillation survey,” Astrophys. J.721, 164 (2010).

[25] S. Dodelson and M. Vesterinen, “Cosmic Neutrino Last Scattering Surface,” Phys.Rev. Lett. 103 171301 (2009).

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[26] F. Schmidt, E. Rozo, S. Dodelson, L. Hui, and E. Sheldon, “Lensing Bias in CosmicShear,” Astrophys. J. 702 593 (2009).

[27] F. Schmidt, E. Rozo, S. Dodelson, L. Hui, and E. Sheldon, “Size Bias in GalaxySurveys,” Phys. Rev. Lett. 103 051301 (2009).

[28] S. Dodelson, A. Belikov, D. Hooper, and P. Serpico, “Identifying Dark Matter Anni-hilation Products In The Diffuse Gamma Ray Background,” Phys. Rev. D 80 083504(2009).

[29] J. Aguirre et al., “Observing the Evolution of the Universe,” arXiv:0903.0902.

[30] S. Dodelson et al., “The Origin of the Universe as Revealed Through the Polarizationof the Cosmic Microwave Background,” arXiv:0902.3796.

[31] J. Peterson et al., “21 cm Intensity Mapping,” arXiv:0902.3091.

[32] S. Dodelson, “Backgrounds and Projected Limits from Dark Matter Direct DetectionExpermients,” Phys. Rev. D 79 043508 (2009).

[33] D. Baumann, et al., “CMBPol Mission Concept Study: Probing Inflation with CMBPolarization,” arXiv:0811.3919.

[34] D. Baumann, A. Cooray, S. Dodelson et al., “CMBPol Mission Concept Study: AMission to Map our Origins,” arXiv:0811.3911.

[35] P. Zhang, R. Bean, M. Liguori, and S. Dodelson, “Weighing the spatial and temporalfluctuations of the dark universe,” Submitted to Phys. Rev. Lett. arXiv:0809.2836.

[36] S. Dodelson, F. Schmidt, and A. Vallinotto, “Universal Weak Lensing Distortion ofCosmological Correlation Functions,” Phys. Rev. D 78 043508 (2008).

[37] F. Schmidt, A. Vallinotto, E. Sefusatti, and S. Dodelson, “Weak Lensing Effects onthe Galaxy Three-Point Correlation Function,” Phys. Rev. D 78 043513 (2008).

[38] S. Dodelson, D. Hooper, and P. Serpico, “Extracting the Gamma Ray Signal fromDark Matter Annihilation in the Galactic Center Region,” Phys. Rev. D, 77, 063512(2008).

[39] S. Dodelson and C. Vale, “Gravitational lensing, the cosmic microwave background,and cluster masses,” J. Phys. A 40, 6621 (2007).

[40] C. Shapiro and S. Dodelson, “Combining Weak Lensing Tomography with Halo Clus-tering to Probe Dark Energy,” Phys. Rev. D, 76, 083515 (2007).

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[41] F. Schmidt, M. Liguori, and S. Dodelson, “Galaxy-CMB Cross-Correlation as a Probeof Alternative Models of Gravity,” Phys. Rev. D, 76, 083518 (2007).

[42] P. Zhang, M. Liguori, R. Bean, and S. Dodelson, “ Probing Gravity at CosmologicalScales by Measurements which Test the Relationship between Gravitational Lensingand Matter Overdensity,” Phys. Rev. Lett., 99, 141302 (2007).

[43] A. Vallinotto, S. Dodelson, C. Schmid, and J.-P. Uzan, “Weak Lensing of BaryonAcoustic Oscillations,” Phys. Rev. D 75, 103509 (2007).

[44] D. Hooper and S. Dodelson, “What can Gamma Ray Bursts teach us about DarkEnergy?” J. Astroparticle Phys., 27, 113 (2007).

[45] A. Melchiorri, P. Serra, S. Dodelson, and A. Slozar, “New constraints on neutrinomasses from cosmology,” New Astronomy Review, 50, 1020-4 (2006).

[46] S. Dodelson and M. Liguori, “Can Cosmic Structure Form without Dark Matter?”Phys. Rev. Lett. 97, 231301 (2006).

[47] S. Dodelson, A. Melchiorri, and A. Slozar, “Is Cosmology compatible with SterileNeutrinos?” Phys. Rev. Lett. 97, 04301 (2006).

[48] S. Dodelson and A. Vallinotto, “Learning from the Scatter in Type Ia Supernovae,”Phys. Rev. D 74, 063515 (2006).

[49] T. Abbott et al., “The Dark Energy Survey,” astro-ph/0510346.

[50] S. Dodelson, C. Shapiro, and M. J. White, “Reduced Shear Power Spectrum,” Phys.Rev. D 73, 023009 (2006).

[51] J. Albert et al., “Probing Dark Energy via Weak Gravitational Lensing with theSupernova Acceleration Probe,” astro-ph/0507460.

[52] J. Albert et al., “Supernova Acceleration Probe: Studying Dark Energy with Type IaSupernovae,” astro-ph/0507459.

[53] J. Albert et al., “Seeing the Nature of the Accelerating Physics: It’s a SNAP,” astro-

ph/0507458.

[54] K. Kadota, S. Dodelson, W. Hu, E. D. Stewart, “Precision of inflaton potential recon-struction from CMB using the general slow-roll approximation,” Phys. Rev. D 72,023510 (2005).

[55] S. Dodelson, E.W. Kolb, S. Matarrese, A. Riotto, P. Zhang, “Second order geodesiccorrections to cosmic shear,” Phys. Rev. D 72, 103004 (2005).

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[56] S. Dodelson and P. Zhang, “The Weak Lensing Bispectrum,” Phys. Rev. D 72, 083001(2005).

[57] S. Barwick et al., “APS Neutrino Study: Report of the Neutrino Astrophysics andCosmology Working Group,” astro-ph/0412544.

[58] Kevork Abazajian, Eric R. Switzer, Scott Dodelson, Katrin Heitmann, Salman Habib,“The nonlinear cosmological matter power spectrum with massive neutrinos. 1. Thehalo model,” Phys. Rev. D 71, 043507 (2005).

[59] G. Aldering et al., “Supernova Acceleration Probe: A Satellite Experiment to Studythe Nature of Dark Energy,” astro-ph/0405232

[60] J. F. Beacom, N. F. Bell, and S. Dodelson, “Neutrinoless Universe,” Phys. Rev. Lett.93, 121302 (2004).

[61] S. Dodelson, “CMB-Cluster Lensing,” Phys. Rev. D 70, 023009 (2004).

[62] E. Rozo, S. Dodelson, and J. A. Frieman, “Halo Model Analysis of Cluster Statistics,”Phys. Rev. D 70, 083008 (2004).

[63] M. Tegmark, M. R.Blanton, M. A. Strauss, K. Abazajian, S. Dodelson, et al., “Cos-mological Parameters from SDSS and WMAP,” Phys. Rev. D 69, 103501 (2004).

[64] M. Ahmed, S. Dodelson, P. B. Greene, and R. Sorkin, “Everpresent Lambda,” Phys.Rev. D 69, 103523 (2004).

[65] S. Dodelson, “Coherent Phase Argument for Inflation,” in Particle Physics and Cos-mology (AIP Conf. Proc. 689:184 (2003).

[66] S. Dodelson, “Cluster Masses accounting for structure along the line of sight,” to bepublished in Phys. Rev. D, astro-ph/0309277 (2003).

[67] K. Abazajian et al., “The First Data Release of the Sloan Digital Sky Survey,” Astron.J. 126, 2081 (2003).

[68] S. Dodelson and G. D. Starkman, “Galaxy-CMB Lensing,” astro-ph/0305467 (2003).

[69] S. Dodelson and L. Hui, “A Horizon Ratio Bound for Inflationary Fluctuations,” Phys.Rev. Lett. 91, 131301 (2003).

[70] S. Dodelson, E. Rozo, and A. Stebbins, “Primordial Gravity Waves and Weak Lens-ing,” Phys. Rev. Lett. 91, 021301 (2003).

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[71] K. Abazajian and S. Dodelson, “Neutrino Mass and Dark Energy from Weak Lensing,”Phys. Rev. Lett. 91, 041301 (2003).

[72] J. R. Chisholm, S. Dodelson, and E. W. Kolb, “Stellar-Mass Black Holes in the SolarNeighborhood,” Astrophys. J 596, 437 (2003).

[73] SDSS Collaboration, I. Szapudi, J. A. Frieman, R. Scoccimarro, A. S. Szalay,A. J. Connolly, S. Dodelson, et al., “Higher Order Moments of the Angular Distribu-tion of Galaxies from Early SDSS Data,” Astrophys. J. 570, 75-85 (2002).

[74] W. Hu and S. Dodelson, “Cosmic Microwave Background Anisotropies,” Ann. Rev.Astron. Astrophys. 40, 171 (2002).

[75] S. Dodelson and E. Stewart, “Scale Dependent Spectral Index in Slow Roll Inflation,”Phys. Rev. D65, 101301 (2002).

[76] SDSS Collaboration, S. Dodelson, et al., “The 3D Power Spectrum from AngularClustering of Galaxies in Early SDSS Data,” Astrophys. J. 572, 140-156 (2002).

[77] SDSS Collaboration, M. Tegmark, S. Dodelson, et al., “The Angular Power Spectrumof Galaxies from Early SDSS Data,” Astrophys. J. 571, 191-205 (2002).

[78] SDSS Collaboration, A. Connolly, R. Scranton, D. Johnston, S. Dodelson, et al., “TheAngular Correlation Function of Galaxies from Early SDSS Data,”Astrophys. J. 579,42-48 (2002).

[79] SDSS Collaboration, R. Scranton, D. Johnston, S. Dodelson, et al., “Analysis of Sys-tematic Effects and Statistical Uncertainties in Angular Clustering of Galaxies fromEarly SDSS Data,” Astrophys. J. 579, 48-75 (2002).

[80] SDSS Collaboration, A. S. Szalay, B. Jain, T. Matsubara, R. Scranton, M. S. Vogeley,A. Connolly, S. Dodelson, et al., “KL Estimation of the Power Spectrum Parame-ters from the Angular Distribution of Galaxies in Early SDSS Data,” submitted toAstrophys. J. astro-ph/0107419 (2001).

[81] K. Coble, S. Dodelson et al., “Cosmic Microwave Background Anisotropy Measure-ment from Python V,” Astrophys. J. 584, 585 (2001).

[82] R. Scranton and S. Dodelson, “Non-Linear Effects on the Angular Correlation Func-tion,” submitted to MNRAS astro-ph/0002360 (2000).

[83] S. Dodelson, M. Kaplinghat, and E. Stewart, “Tracking, Oscillating Energy,” Phys.Rev. Lett. 85, 5276 (2000).

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[84] S. Dodelson, “Cosmic Microwave Background: Past, Future, and Present,” Int. J.Mod. Phys. A15S1, 765 (2000).

[85] P. M. Ricker, S. Dodelson, and D. Q. Lamb, “COSMOS: A Hybrid N-Body/Hydro-dynamics Code for Cosmological Problems,” Astrophys. J. 536, 122 (2000).

[86] S. Dodelson and L. Knox, “Dark Energy and the CMB,” Phys. Rev. Lett. 84, 3523(2000).

[87] S. Dodelson and E. Gaztanaga, “Inverting the Angular Correlation Function,” Mon.Not. Roy. Ast. Soc. 312, 774 (2000).

[88] G. W. Wilson et al., “New CMB Power Spectrum Constraints from MSAMI,” Astro-phys. J. 532, 57 (2000).

[89] M. Kaplinghat, R. E. Lopez, S. Dodelson, and R. J. Scherrer,“Improved Treatmentof Cosmic Microwave Background Fluctuations Induced by a Late-decaying MassiveNeutrino,” Phys. Rev. D 60, 123508 (1999).

[90] K. Coble, et al., “Anisotropy in the Cosmic Microwave Background at Degree AngularScales: Python V Results,” Astrophys. J. 519 L5-L8 (1999).

[91] R. E. Lopez, S. Dodelson, A. Heckler, and M. S. Turner, “Precision Detection of theCosmic Neutrino Background,” Phys. Rev. Lett. 82 3952-55 (1999).

[92] R. E. Lopez, S. Dodelson, R. J. Scherrer, M. S. Turner, “Probing Unstable MassiveNeutrinos with Current Cosmic Microwave Background Observations,” Phys. Rev.Lett. 81 3075-78 (1998).

[93] L. Knox, R. Scoccimarro, and S. Dodelson, “The Impact of Inhomogeneous Reioniza-tion on Cosmic Microwave Background Anisotropy,” Phys. Rev. Lett. 81 2004-2007(1998).

[94] S. Dodelson, L. Hui, and A. Jaffe, “Likelihood Analysis of Galaxy Surveys,” submittedto ApJ astro-ph/9712074 (1997).

[95] S. Dodelson and C. Wiegert, “Bending of Light by Vector Perturbations,” submittedto Phys. Rev. D astro-ph/9710080 (1997).

[96] B. Allen, R. R. Caldwell, S. Dodelson, L. Knox, E. P. S. Shellard, and A. Stebbins,“CMB Anisotropy Induced by Cosmic Strings on Angular Scales > 15 Arcminutes,”Phys. Rev. Lett. 79, 2624-27 (1997).

[97] S. Dodelson, W. Kinney, and E. W. Kolb, “Cosmic microwave background measure-ments can discriminate among inflation models,” Phys. Rev. D 56, 3207-15 (1997).

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[98] S. Dodelson, “Anisotropies in the Cosmic Microwave Background: Theory,” astro-ph/9702134 to be published in the Proceedings of the 18th Texas Symposium onRelativistic Astrophysics, ed. J. A. Frieman, A. Olinto, and D. N. Schramm (1997).

[99] K. Coble, S. Dodelson, and J.A. Frieman, “Dynamical Lambda Models of StructureFormation,” Phys. Rev. D 55, 1851-9 (1997).

[100] S. Dodelson, “Determining Cosmic Microwave Background Anisotropies in the Pres-ence of Foregrounds,” Astrophys. J. 482, 577-587 (1997).

[101] S. Dodelson, E. Gates, and M.S. Turner, “Cold Dark Matter Models,” Science 274,69-75 (1996).

[102] S. Dodelson and A.S. Stebbins, “Comment on a paper by Fang, Huang, and Wu,”FERMILAB-PUB-96-068-A (1996).

[103] S. Dodelson, E. Gates, and A.S. Stebbins, “Cold + Hot Dark Matter and the CosmicMicrowave Background,” Astrophys. J. 467, 10-18 (1996).

[104] S. Colombi, S. Dodelson, and L.M. Widrow, “Large Scale Structure Tests of WarmDark Matter,” Astrophys. J. 458, 1-17 (1996).

[105] S. Dodelson and J. M. Jubas, “Reionization and its Imprint on the Cosmic MicrowaveBackground,” Astrophys. J. 439, 503 (1995).

[106] S. Dodelson and A. Kosowsky, “Analysis of small and medium scale Cosmic MicrowaveBackground Experiments,” Physical Review Letters 75, 604 (1995).

[107] S. Dodelson, A. Kosowsky, and S. T. Myers, “Noise Correlations in Cosmic MicrowaveBackground Experiments,” Astrophys. J. 440, L37 (1995).

[108] S. Dodelson and A. Kosowsky, “Inflation Confronts the CMB: An Analysis Includingthe Effects of Foreground”, in CMB Anisotropies Two Years After COBE: Obser-vation, Theory and the Future, edited by L. M. Krauss (World Scientific, Singapore1994), 112-116.

[109] S. Dodelson, G. Gyuk, and M.S. Turner,“Is A Massive Tau Neutrino Just what ColdDark Matter Needs?” Phys. Rev. Lett. 72, 3754-7 (1994).

[110] S. Dodelson, L. Knox, and E. Kolb, “Testing Inflation with the Cosmic MicrowaveBackground,” Phys. Rev. Lett. 72, 3444-7 (1994).

[111] S. Dodelson, G. Gyuk, and M.S. Turner, “Primordial Nucleosynthesis with a decayingtau neutrino,” Phys. Rev. D 49, 5068-81 (1994).

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[112] S. Dodelson and J. M. Jubas, “Cosmological Signatures of Decaying Dark Matter,”Mon. Not. Roy. Acad. Soc. 266, 886-890 (1994).

[113] S. Dodelson and A. Stebbins, “Analysis of Small Scale MBR Anisotropy in the Pres-ence of Foreground Contamination,” Astrophys. J. 433, 440-454 (1994).

[114] S. Dodelson and L. M. Widrow, “Sterile Neutrinos as Dark Matter,” Phys. Rev. Lett.72, 17-20 (1994).

[115] S. Dodelson and J. M. Jubas, “Microwave Anisotropies in the Light of COBE,” Phys.Rev. Lett. 70, 2224-2227 (1993).

[116] B. Fields, S. Dodelson, and M. S. Turner, “Effect of Neutrino Heating on PrimordialNucleosynthesis,” Phys. Rev. D 47, 4309-4314 (1993).

[117] S. Dodelson and B. Gradwohl, “How Effective is the Effective Potential?”, Nucl. Phys.B 400, 435-459 (1993).

[118] S. Dodelson and M. S. Turner, “Nonequilibrium Neutrino Statistical Mechanics in theExpanding Universe,” Phys Rev. D 46, 3372-3387 (1992).

[119] S. Dodelson, B. R. Greene, and L. M. Widrow, “Baryogenesis, Dark Matter, and theWidth of the Z,” Nucl. Phys. B 372, 467-493 (1992).

[120] S. Dodelson and J. Jubas, “Reionization and Decaying Dark Matter,” Phys. Rev. D45, 1076-1090 (1992).

[121] S. Dodelson, B. R. Greene, and L. M. Widrow, “Inverse Phase Transitions: DoesBaryogensis lead to Dark Matter?”, in Particle Physics from Underground to Heaven,edited by G. Domokos and S. Kovesi-Domokos (World Scientific, Singapore 1992),391-401.

[122] S. Dodelson, J. A. Frieman, and M. S. Turner, “Constraints to the Decays of DiracNeutrinos from SN 1987A”, Phys. Rev. Lett. 68, 2572-2575 (1992).

[123] K. M. Benson, J. Bernstein, and S. Dodelson, “Phase Structure and the EffectivePotential at Fixed Charge,” Phys. Rev. D 44, 2480-2497 (1991).

[124] S. Dodelson and G. Feinberg, “Neutrino – Two Photon Vertex,” Phys. Rev. D 43,913-920 (1991).

[125] J. Bernstein and S. Dodelson, “Relativistic Bose Gas,” Phys. Rev. Lett. 66, 683-686(1991).

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[126] S. Dodelson and L. M. Widrow, “Baryogenesis without Baryon Number Violation,”Mod. Phys. Lett. A 5, 1623-1628 (1990).

[127] S. Dodelson and L. M. Widrow, “Baryogenesis in a Baryon-symmetric Universe,”Phys. Rev. D 42, 326-342 (1990).

[128] S. Dodelson and L. M. Widrow, “Baryon-symmetric Baryogenesis,” Phys. Rev. Lett.64, 340-343 (1990).

[129] J. Bernstein and S. Dodelson, “Aspects of the Zel’dovich-Sunyaev Mechanism,” Phys.Rev. D 41, 354-373 (1990).

[130] J. Bernstein and S. Dodelson, “Comment on Reheated Universe by Unstable Neutri-nos,” Phys. Rev. Lett. 62, 1804 (1989).

[131] S. Dodelson, “Cosmological Implications of Unstable Technibaryons,” Phys. Rev. D40, 3252-3262 (1989).

[132] S. Dodelson, “Post-inflationary Era and Baryogenesis,” Phys. Rev. D 37, 2059-2070(1988).

[133] S. Dodelson, “Relativistic Treatment of Ortho-Para H2 Transitions,” J. Phys. B 19,2871-2879 (1986).

Popularizations

[1] “Why modified gravity,” Scilogs, (2013).

[2] “Dark Matter ... and why we need your help,” Physics for Kids, Aspen, CO (2012).

[3] “Science Year,” Astronomy, World Book Encyclopedia (2012).

[4] “Astrophysics,” Great Minds Program, Illinois Math and Science Academy (2012).

[5] “Science Year,” Astronomy, World Book Encyclopedia (2011).

[6] “Dark Matter vs. Modified Gravity,” KICP Short Course for Planetariums, Chicago(2010).

[7] “Dark Matter ... and why we need your help,” Physics for Kids, Aspen, CO (2010).

[8] “Science Year,” Astronomy, World Book Encyclopedia (2010).

[9] “Astro Confidential,” Astronomy Magazine (March, 2010).

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[10] “Ask an Astronmer,” Astronomy Magazine (June, August 2007).

[11] “Redshift 101”, Astronomy Magazine (May, 2007).

[12] “MiniBoone Results”, New Scientist Podcast, (2007).

[13] “Recent Cosmological Discoveries: Questions and Answers”, Princeton UniversityAlumni Reunion (2006).

[14] Symposium on The Origin of the Universe, Augustana College (2004).

[15] Five articles in World Book Encyclopedia (2004).

[16] “Dark Energy,” Society of Physics Students, Northwestern University (2004).

[17] “Dark Energy,” Ask-A-Scientist, Fermilab (2004).

[18] “Let there be Light,” First Congregational Church (2001).

[19] Co-Organizer, “Chicago Chattaqua on Cosmology,” for thirty college teachers (2001).

[20] “Vacuum Energy in the Universe,” Dow Corning Technical Exchange Society (2000).

[21] “Big Bang, Kansas, and Creationsim: A Scientist’s Perspective,” Saginaw Valley StateUniversity (2000).

[22] Co-Organizer, “A Symposium on the Nature of Science,” for School teachers (800 ex-pected) on evolution and cosmology, http://www-ed.fnal.gov/symposium , March,2000.

[23] Co-Organizer, “Chicago Chattaqua on Cosmology,” for thirty college teachers, June1999.

[24] Extension 702: The Milt Rosenberg Show , Radio talk show about cosmology andstring theory (February 1999).

[25] “The Missing Energy in the Universe,” Lecture to Naperville Astronomical Association(1998).

[26] “The Big Bang,” Letter to the Editor, Commentary, May (1998).

[27] “Pillars of Cosmology,” Six display panels introducing cosmology to the public. Pre-pared for Fermilab’s Open House, attended by 15,000 people (1997).

[28] “Scientific Thinking,” Regular column in Youthline-USA, weekly newspaper for chil-dren (1997).

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[29] “The Physics of Baseball,” Talk to Friends of Fermilab (1997)

[30] “Anti-Matter in the Universe,” in Ask the Experts, Scientific American Web Site(1997).

[31] Movie: “Cosmic Radiation Through the Ages,” with A. Stebbins (1996).

[32] Review of 3K: The Cosmic Microwave Background Radiation (R. B. Partridge) forScience, 274 (1996).

[33] “The Great Attractor,” in Macmillan Encyclopedia of Physics, (Macmillan, New York,1996).

[34] “Dark Matter,” in Macmillan Encyclopedia of Physics, (Macmillan, New York, 1996).

[35] “The Great Wall,” in Macmillan Encyclopedia of Physics, (Macmillan, New York,1996).

Invited Lectures

[1] “Resolving the Unresolved in Fermi,” Stanford Cosmology Seminar (2013).

[2] “View from the Cosmic Frontier,” Intensity Frontier Workshop, Argonne NationalLaboratory (2013).

[3] “Cosmology after Planck,” Joint Stony Brook/Brookhaven Cosmology Seminar(2013).

[4] “Science Analysis Framework Update,” DES Council Operations Review (2013).

[5] “Inflation: Status and Prospects,” Cosmology Seminar, Penn (2013).

[6] “Dark Energy and the CMB,” SLAC Cosmic Frontier Workshop (2013).

[7] “Neutrinos in the Cosmos,” SLAC Cosmic Frontier Workshop (2013).

[8] “Current and future constraints on neutrinos in the cosmos,” Neutrino Workshop,Aspen Center for Physics (2013).

[9] “Inflation,” Physics of the Universe Summit, California (2013).

[10] “DES Software Framework,” LSST DESC meeting, SLAC (2013).

[11] “Dark Energy and Beyond,” LSST DESC meeting, SLAC (2013).

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[12] “DES Computing,” NERSC Planning Workshop, Washington D.C. (2012).

[13] “Inflation,” Gravity and Cosmology Seminar, University of North Carolina (2012).

[14] “Modified Gravity vs. the Dark Sector,” Colloquium, University of Florida (2012).

[15] “Inflation,” High Energy Physics Seminar, University of Florida (2012).

[16] “CMB Science in the Post-WMAP Era,” Cosmo 2012, Beijing, China (2012).

[17] “The Dark Sector vs. Modified Gravity,” Kavli Prize Week, Oslo, Norway (2012).

[18] “Introduction to Cosmology: Three Lectures,” ICTP Summer School, Trieste, Italy(2012).

[19] “The Current State of Dark Energy,” LSST Dark Energy Science Collaboration Meet-ing, Philadelphia, PA (2012).

[20] “The Cosmic Frontier,” Eleventh Conference on the Intersections of Particle and Nu-clear Physics, Tampa, FL (2012).

[21] “Cosmological Constraints on Neutrinos,” Short-Baseline Focus Group, Fermilab(2012).

[22] “Modified Gravity vs. the Dark Sector,” Colloquium, University of California, SanDiego (2012).

[23] “Gravitational Lensing,” University of California, San Diego (2012).

[24] “Gravitational Lensing,” Simon Fraser University (2012).

[25] “Modified Gravity vs. the Dark Sector,” Colloquium, University of British Columbia(2012).

[26] “Gravitational Lensing,” Challenges IV, Brazil (2011).

[27] “Cosmic Microwave Background,” Challenges IV, Brazil (2011).

[28] “Inflation,” SUSY-2011, Chicago (2011).

[29] “Modified Gravity vs. the Dark Sector,” Colloquium, IUCAA Pune, India (2011).

[30] “Gravity on Large Scales,” Lepton Photon, Mumbai, India (2011).

[31] “Cosmology,” Workshop on Novel Telescopes for 21 cm Cosmology, Penticton, BC(2011).

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[32] “Dark Energy and Modified Gravity,” CCAPP Symposium, Ohio State (2011).

[33] “The Dark Sector vs. Modified Gravity,” Colloquium, Institute for Physics and Math-ematics of the Universe, Japan (2011).

[34] “Gravitational Lensing: Shedding Light on Dark Energy and Inflation,” Seminar,University of Tokyo, Japan (2011).

[35] “The Dark Sector vs. Modified Gravity,” Colloquium, University of Michigan (2011).

[36] “The Dark Sector vs. Modified Gravity,” Colloquium, University of Illinois at Urbana(2011).

[37] “The Dark Sector vs. Modified Gravity,” Colloquium, Penn State University (2010).

[38] “Dark Matter in the Era of the LHC,” Invited Talk, Il Prometeo Workshop III, Va-lencia, Spain (2010).

[39] “Combined Probes Working Group Summary Talk,” DES Collaboration Meeting(2010).

[40] “Challenges for Modified Gravity,” Workshop on Modified Gravity and the Dark Sec-tor, Strasbourg, France (2010).

[41] “Cosmology,” Three Lectures at Summer School, Pan American Studies Institute(PASI) (2010).

[42] “The Dark Sector vs. Modified Gravity,” Colloquium, Yale University (2010).

[43] “Lensing and Neutrino Masses,” INT Workshop on Neutrino Masses, University ofWashington (2010).

[44] “Dark Matter and the Constitutional Convention,” Inaugural Workshop on ParticleAstrophysics, University of Pennsylvania (2009).

[45] “Combining Probes with an eye on Modified Gravity,” DES Collaboration Meeting(2009).

[46] “Inflation and Gravitational Waves,” Seminar, University of Wisconsin, Milwaukee(2009).

[47] “Quarks to the Cosmos and Einstein,” Colloquium, Brown University (2009).

[48] “Gravitational Waves on the Horizon,” Invited Talk, Primordial Gravitational Waves,Cambridge (2009).

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[49] “Quantum Theory, Symmetries, and Cosmology,” Plenary Talk, Quantum Theoryand Symmetries 6, Lexington, KY (2009).

[50] “Astroparticle Physics, Two Lectures,” CTEQ Summer School, Madison, WI(2009).

[51] “TeVeS: Modifed Gravity Inside Out,” Aspen Center for Physics (2009).

[52] “CMBPol,” High Energy Seminar, Argonne National Laboratory(2009).

[53] “Issues in Gravitational Lensing,” Seminar, University of Pennsylvania(2009).

[54] “Fundamental Physics from Space,” Colloquium, Rochester University (2009).

[55] “Issues in Gravitational Lensing,” Seminar, Perimeter Institute (2009).

[56] “Primordial Gravitational Waves,” Special Session, Annual Meeting, American Asso-ciation for the Advancement of Science (2009).

[57] “Cosmic Microwave Background,” Aspen Winter Workshop (2009).

[58] “Evidence for Inflation,” Special Session, Annual Meeting, American AstronomicalSociety (2009).

[59] “Fundamental Physics from Space,” Colloquium, University of North Carolina (2008).

[60] “Dark Matter vs. Modified Gravity,” Seminar, University of North Carolina (2008).

[61] “Cosmology, Four Lectures,” Maria Laach Summer School (2008).

[62] “Fundamental Physics From Space,” Summer Lecture Series, Fermilab (2008).

[63] “Observational Cosmology, Three Lectures,” Theoretical Advanced Studies Institute,Boulder, Colorado (2008).

[64] “Present and Future of Observational Cosmology,” Users Meeting, Fermilab (2008).

[65] “Summary Talk,” Particle Physics and Cosmology 2008 Albuquerque, NM (2008).

[66] “Dark Matter vs. Modified Gravity,” Seminar, University of Minnesota (2008).

[67] “Dark Matter vs. Modified Gravity,” Seminar, Simon Fraser University (2008).

[68] “Fundamental Physics from Space,” Colloquium, Simon Fraser University (2008).

[69] “Dark Matter vs. Modified Gravity,” Colloquium, Syracuse University (2007).

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[70] “Computational Cosmology,” Physics Advisory Committee, Fermilab (2007).

[71] “Fundamental Physics from Space,” Colloquium, Illinois Institute of Technology(2007).

[72] “Dark Matter vs. Modified Gravity,” Workshop on Modern Cosmology, PerimeterInstitute (2007).

[73] “Cosmology for Particle Physicists, 3 Lectures,” SLAC Summer Institute (2007).

[74] “Fundamental Physics from Space,” Summer Lecture, Fermilab (2007).

[75] “Neutrinos in Cosmology,” Wine & Cheese Seminar, Fermilab (2007).

[76] “Beyond-the-Standard-Model Cosmology,” Colloquium, University of Pittsburgh(2006).

[77] “Cosmology,” Plenary Talk, Joint Meeting of Pacific Region Particle Physics Com-munities, Hawaii (2006).

[78] “SDSS Publication Policy,” Special Session, Joint Meeting of Pacific Region ParticlePhysics Communities, Hawaii (2006).

[79] “Two Lectures on Cosmology,” Pan-American Advanced Studies Institute, PuertoVallarta, Mexico (2006).

[80] “Modified Gravity vs. Dark Matter,” Colloquium, CCAPP Ohio State University(2006).

[81] “Fundamental Physics from Space,” Colloquium, Northern Illinois University (2006).

[82] “Modified Gravity vs. Dark Matter,” Fermliab (2006).

[83] “Fundamental Physics from Space,” Colloquium, Northern Illinois University (2006).

[84] “Gravitational Lensing,” Plenary Talk, IRGAC, Barcelona, Spain (2006).

[85] “Precision Cosmology and Neutrinos,” Plenary Talk, Neutrino 2006, Santa Fe (2006).

[86] “Five Lectures on Cosmology,” Theoretical Advanced Studies Institute, Boulder, Col-orado (2006).

[87] “Three Lectures on the Clumpy Universe,” Academic Lectures II, Fermilab (2006).

[88] “Three Lectures on the Smooth Universe,” Academic Lectures I, Fermilab (2006).

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[89] “CMB-Cluster Lensing,” Fundamental Physics With Cosmic Microwave BackgroundRadiation, UC Irvine (2006).

[90] “Fundamental Physics from Space,” University of Kentucky (2006).

[91] “Cosmic Deflections,” University of Kentucky (2006).

[92] “Cosmic Deflections,” Harvard University (2006).

[93] “Gravitational Lensing,” University of Illinois (2005).

[94] “Five Lectures on Cosmology,” INPE Advanced Course, Sao Jose dos Campos, Brazil(2005).

[95] “CMB Primary Anisotropies,” Frontiers in Contemporary Physics, Vanderbilt Uni-versity (2005).

[96] “CMB Secondary Anisotropies,” Frontiers in Contemporary Physics, Vanderbilt Uni-versity (2005).

[97] “Gravitational Lensing,” Colloquium, Columbia University (2005).

[98] “Dark Energy in the Universe,” High Energy Seminar, Argonne National Lab (2005).

[99] “Second Order Corrections to Cosmic Shear,” SNAP Science Meeting (2005).

[100] “Learning from Lensing: Power Spectrum and Bispectrum,” Workshop, Ohio StateUniversity (2005).

[101] “ Dark Energy,” Colloquium, Vanderbilt University (2004).

[102] “Cosmology constraints on Neutrinos,” Argonne Theory Institute on Higgs SUSY andExtra Dimensions (2004).

[103] “Dark Energy, Clusters, and Lensing,” Northwestern University (2004).

[104] “Dark Energy, Clusters, and Lensing,” University of North Carolina (2004).

[105] “Dark Energy, Clusters, and Lensing,” Mitchell Symposium on Observational Cos-mology (2004).

[106] “Weak Lensing,” Seminar, University of Wisconsin, Madison (2003).

[107] “Dark Energy in the Universe,” Colloquium, University of British Columbia (2003).

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[108] “SDSS and the CMB,” Kingston Workshop on the CMB (2003).

[109] “Massive Neutrinos and the Cosmos,” Colloquium, University of Kansas (2003).

[110] “ Cosmological Puzzles,” Tropical Workshop on Particle Physics & Cosmology, Cairns(2003).

[111] “Cosmic Harmony,” Tropical Workshop on Particle Physics & Cosmology, Cairns(2003).

[112] “Sloan Digital Sky Survey,” Colloquium, University of Wisconsin, Madison (2003).

[113] “Dark Energy in the Universe,” Experimental Seminar, SLAC (2003).

[114] “Running, CMB, and the Lyman alpha forest,” Workshop on CMB, Minnesota (2003).

[115] “What can we learn about Neutrinos from Large Scale Structure,” KITP Symposiumon Neutrinos, Santa Barbara (2003).

[116] “First Impressions of the WMAP Results,” Enrico Fermi Mini-Symposium (2003).

[117] “Dark Energy in the Universe,” Illinois Institute of Technology (2002).

[118] “Dark Energy in the Universe,” Physics Colloquium, Brandeis University (2002).

[119] “Dark Energy in the Universe,” Joint Theoretical/Experimental Seminar, Fermilab(2002).

[120] “CMB Lensing by Galaxies,” Workshop on CDM Structure, Chicago (2002).

[121] “CMB Anisotropies: Primary and Secondary,” Invited Review Talk, Santa Fe Cos-mology Workshop (2002).

[122] “Cosmology Past the Crossroads,” Colloquium, Aspen Center for Physics (2002).

[123] “Solving the Why Now Problem,” Invited talk, APS Divisions of Particles and Fields,Annual Meeting (2002).

[124] “Results from the Sloan Digital Sky Survey,” Plenary talk at Pheno02, Wisconsin(2002).

[125] “Dark Energy in the Universe,” Illinois Institute of Technology (2001).

[126] “Can the Inflationary paradigm ever be more than a plausible myth?” Plenary talkat Frontier of the Universe Blois, France (2001).

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[127] “Cosmology and Particle Physics,” High Energy Physics Advisory Panel (HEPAP)(2001).

[128] “Angular Clustering in the SDSS,” Workshop on CDM Halos, Fermilab (2001).

[129] “CMB: Past, Future, and Present,” Purdue University (2000).

[130] “CMB: Past, Future, and Present,” Brookhaven National Laboratory (2000).

[131] “Large Scale Structure from Early SDSS Data,” Enrico Fermi Institute (2000).

[132] “CMB: Past, Future, and Present,” Ohio State University (2000).

[133] “CMB: Past, Future, and Present,” Plenary Talk at PASCOS 99, Lake Tahoe, CA(1999).

[134] “CMB: Future and Present,” Plenary Talk at COSMOS 99, Trieste, Italy (1999).

[135] “Cosmic Microwave Background,” Plenary Talk at Lepton-Photon 99, Stanford Uni-versity (1999).

[136] “The Inverse Problem,” Sante Fe Workshop on Large Scale Structure, (1999).

[137] “The History of the History of the Universe,” Physics Colloquium, NorthwesternUniversity (1999).

[138] “MSAM Results” and “Implications for Open Inflation,” Pritzker Workshop on Infla-tion (1999).

[139] “Latest Results from the CMB,” Astrophysics Colloquium, Northwestern University(1999).

[140] “Lensed QSOs with the Sloan Digital Sky Survey,” Missing Energy Workshop, Fer-milab (1998).

[141] “What will we learn from the CMB?” Colloquium, Wayne State University (1998).

[142] “CMB and Parameters,” Coral Gables Conference on High Energy Physics and Cos-mology (1998).

[143] “Numerical Issues in Cosmology,” Computational Methods Seminar, University ofChicago (1997).

[144] “What will we learn from the CMB?” Plenary talk at Birth of the Universe Conference,Rome, Italy (1997).

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[145] “Large Scale Structure and the Csomic Microwave Background,” Bartol ResearchInstitute (1997).

[146] “The End of Cosmic Confusion,” Colloqium, University of Chicago (1997).

[147] “The End of Cosmic Confusion,” Coral Gables Conference on High Energy Physicsand Cosmology (1997).

[148] “Cosmic Microwave Background: Theory,” Plenary talk at 18th Texas Symposium onRelativistic Astrophysics, Chicago, IL (1996)

[149] “The End of Cosmic Confusion,” Columbia University (1996)

[150] “The End of Cosmic Confusion,” Notre Dame University (1996)

[151] “The End of Cosmic Confusion,” Case Western Reserve University (1996)

[152] “Determining CMB Anisotropy in the presence of foregrounds,” Moriond Conferenceon CMB (1996).

[153] “The Doppler Peaks and the CMB,” University of Chicago (1996).

[154] “Learning from the Cosmic Microwave Background,” Enrico Fermi Institute (1995).

[155] “Foreground Separation in Anisotropy Experiments,” Conference on Cosmic Back-ground Radiations, Santa Barbara (1995).

[156] “The Hubble Constant,” Fermilab (1994).

[157] “Warm Dark Matter,” Particle and Nuclear Astrophysics in the Next Millenium,Snowmass Summer Study (1994); University of Pennsylvania (1994).

[158] “Testing Inflation with the Cosmic Microwave Background,” Goddard Institute forSpace Science (1993); Ohio State University (1993); Case Western Reserve University(1994); Workshop on the Cosmic Microwave Background, Case Western Reserve Uni-versity (1994); Particle and Nuclear Astrophysics in the Next Millenium, SnowmassSummer Study (1994); Marcel Grossman Meeting on General Relativity, Stanford(1994); Annual Meeting of Division of Particles and Fields, New Mexico (1994).

[159] “Cosmic Microwave Background: From Inflation to Dust,” Canadian Institute of The-oretical Astrophysics (1993); Queens University (1993).

[160] “CDM confronts the CMB: an analysis including the effects of foreground,” CosmicMicrowave Background Workshop, Capri, Italy (1993).

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[161] “Anisotropies in the Cosmic Microwave Background,” Great Lakes Cosmology Work-shop, University of Michigan (1993).

[162] “Sterile Neutrinos as Dark Matter,” Princeton University (1993).

[163] “Microwave Anisotropies in Light of COBE,” Annual meeting of Division of Particlesand Fields, Batavia, IL (1992).

[164] “Decaying Dark Matter,” Purdue University (1992).

[165] “Tunneling Rates: Is the Effective Potential a good approximation?” Workshop onCosmological Phase Transitions, University of California at Santa Barbara (1992).

[166] “Towards a Quantitative Understanding of the Electroweak Phase Tranistion,” BartolResearch Institute (1992).

[167] “Is Symmetry Restored at High Temperature?” Cornell (1991); University of Wis-consin (1992).

[168] “Constraints on Neutrino Decays from SN 1987A,” Many Aspects of Neutrino Physicsconference, Fermilab (1991); Workshop on 17 keV Question, University of Californiaat Berkeley (1991).

[169] “Relativistic Bose-Einstein Condensation,” MIT (1991); Boston University (1991).

[170] “Baryon-symmetric Baryogenesis,” Fermilab (1989); joint CFA-Tufts early universeseminar (1989); Brown University (1990).

[171] “Distortions of the Microwave Background,” University of Georgia (1989); Universityof Massachusetts, Amherst (1989).

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