'Ns ns' diaporamas de présentation

Review of observational study design and basic statistics for contingency tables

Review of observational study design and basic statistics for contingency tables. Coffee Chronicles BY MELISSA AUGUST, ANN MARIE BONARDI, VAL CASTRONOVO, MATTHEW

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Does the Pattern of Blood Pressure Effects During the Day Matter?

Does the Pattern of Blood Pressure Effects During the Day Matter?. Thomas Pickering MD, DPhil Behavioral Cardiovascular Health and Hypertension Program Division of General Medicine Columbia Presbyterian Medical Center New York. Issues. Diurnal rhythm of blood pressure

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Status of the LIGO Experiment

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Status of the LIGO Experiment

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Astrophysics of Gravitational-Wave Sources

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Cosmological Heavy Ion Collisions: Colliding Neutron Stars and Black Holes

HIM07-12@apctp. Cosmological Heavy Ion Collisions: Colliding Neutron Stars and Black Holes. Chang-Hwan Lee. Comparison. Contents. Gravitational Waves Short Hard Gamma-ray Bursts Current Observations & Prospect. Introduction. EM wave Theory: Maxwell (1873)

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Probing the Neutron Star Equation of State and Synergy with Advanced LIGO and Virgo

Probing the Neutron Star Equation of State and Synergy with Advanced LIGO and Virgo. Cole Miller University of Maryland. Outline. What we know about dense matter now Methods of constraining M and R from X-ray observations, and benefits of new observatories The promise of gravitational waves.

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DNS Operations

Phil Regnauld ccTLD workshop November 26-29 2007 Amman, Jordan. DNS Operations. Goals. Go beyond basic DNS administration, focus on service stability Identify common operational problems that plague authoritative nameserver administrators

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Italian-Korean@sejong

Italian-Korean@sejong. Double Neutron Star Binaries: Implications for LIGO. Chang-Hwan Lee @. Science 308 (2005) 939. Gravitation Wave from Binary Neutron Star. B1913+16 Hulse & Taylor (1975). Effect of Gravitational Wave Radiation 1993 Nobel Prize Hulse & Taylor.

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Rates from binaries: current status

Tomasz Bulik Warsaw University. Rates from binaries: current status. Plan. Rates based on observations Discoveries of new double pulsars Population synthesis: results and current issues Short Gamma-Ray Bursts Studies of exotic objects. Inspiral sources. Compact object binaries NS NS

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DECIGO : the Japanese Space Gravitational Wave Antenna

DECIGO : the Japanese Space Gravitational Wave Antenna. Illustration/ KAGAYA.

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LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology LIGO PAC Meeting Pasadena, 5 June 2003 LIGO-G030293-00-R. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate. Most Pessimistic

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LIGO: Towards a Gravitational-Wave Astronomy

LIGO: Towards a Gravitational-Wave Astronomy. Ray Frey, University of Oregon for the LIGO Scientific Collaboration LIGO-G0900437. Introduction Observational results; new directions Enhanced and Advanced LIGO, a worldwide network of GW observatories, and a new window on the cosmos.

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Merger phase simulations of binary-systems: status

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The Japanese Space Gravitational Wave Antenna - DECIGO

The Japanese Space Gravitational Wave Antenna - DECIGO. GWADW @ Elba, Italy May 30, 2006

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Internationalized Domain Names (IDN) and Reverse DNS

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Software Coordinator Report Alan Wiseman

Software Coordinator Report Alan Wiseman. LIGO-G020357-00-Z. Status of ASIS. Most of the original activities absorbed into UL Work Should it exist at all? If so, what issues should this committee address Better/More interaction with the source modeling research community

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