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Kavli IPMU Interdisciplinary Colloquium An Introduction to Observational Cosmology I Naoki Yoshida Department of Physics University of Tokyo 2 1 Elements of modern cosmology…

cos_kdh.ppt1 observations : H0 = 72 ± 8 km s−1 Mpc−1 t0 ≥14 ± 2 Gyr old globular clusters H0 t0 ≥1.0 ± 0.15 H0 t0 = 2 3 for ΩM

cos_kdh.ppt1 observations : H0 = 72 ± 8 km s−1 Mpc−1 t0 ≥14 ± 2 Gyr old globular clusters H0 t0 ≥1.0 ± 0.15 H0 t0 = 2 3 for ΩM

ASIC needs for “observational cosmology” Gary S Varner University of Hawai’i HEPIC 2013 LBNL May 30th 2013 2 What’s in out • Very broad topic minimize overlap with…

July 1, 2013 The marriage between programming and logic has been a fertile one. In particular, since the definition of the simply typed λ-calculus, a number of type

Observational Properties of Stellar Continua Balmer Jump, Continuum Slope Filters and Colors Balmer Line Wings Correcting for Interstellar Reddening Cool, faint Hot, bright…

Astrochemistry - Lecture 7, Observational astrochemistryJorma Harju Department of Physics Friday, March 1, 2013, 12:15-13:45, Lecture room D117 Course web page Historical

21cm cosmology T. Chang, UP, J. Peterson, P. McDonald PRL 100, 091303 (2008) UP, L. Staveley-Smith, J. Peterson, T. Chang, MNRAS, 394, 6 (2009) 21cm: HI hyperfine transition…

* before explosion 31 March 2010 Accelerated expansion : Type Ia SNe, 1998 * MORE REDSHIFT (more expansion since explosion) FAINTER  (further back in time) ~ apparent…

Observational Properties of the Soft Gamma RepeatersKevin Hurley UC Berkeley A FEW SGR FACTS • SGRs are sources of short (~100 ms), repeating bursts of soft γ-

Introduction Experiments, observational studies, and models Introduction Experiments, Observational Studies, and Models Patrick Breheny January 13 Patrick Breheny BST 760:…

OBSERVATIONAL ASTRONOMY – I Vitaly Neustroev Lecture 3 The high-energy spectrum  Extreme ultraviolet EUV: 100 – 1000 Å 12-120 eV  Soft X-rays: 10 – 100 Å 120…

Galaxies and Cosmology 5 points, vt-2007 Teacher: Göran Östlin Lecture 12 Lecture 12 contents Cosmological problems Observational Cosmology: - Galaxy formation and evolution:…

Cosmology with WFMOS Jan 14, 09 @NAOJ Masahiro Takada (IPMU) Precision Cosmology ΛCDM structure formation scenario mh2=0.12770.008 etc ~96% of the Universe is dark,…

Cosmology with WFMOS Jan 14, 09 @NAOJ Masahiro Takada (IPMU) Precision Cosmology ΛCDM structure formation scenario mh2=0.12770.008 etc ~96% of the Universe is dark,…

Particle Physics and Cosmology cosmological neutrino abundance relic particles examples: neutrinos baryons cold dark matter ( WIMPS ) neutrinos neutrino background radiation…

Neutrinos in Cosmology (I) Sergio Pastor (IFIC Valencia) Universidad de Buenos Aires Febrero 2009 ν Neutrinos in Cosmology 1st lecture Introduction: neutrinos and the History…

MASSIVE NEUTRINOS AND COSMOLOGY Sergio Pastor (IFIC) ν CuTAPP 2005, Ringberg Castle Outline Current bounds and future sensitivities Effect of neutrino mass on cosmological…

Cluster Cosmology at LPPC Illuminating Dark Energy with BCS and PISCO F. William High 2nd Year Grad Student Harvard Univ Dept of Physics Monday, 21 August 2006 F. William…

Scalar Field CosmologyCosmological models with a canonical scalar field Superpotential method in cosmology Scalar Field Cosmology Cosmological models with a canonical scalar