'Kpc' presentation slideshows

Carbapenams

Carbapenams, Newer antibiotics,

2.14k views • 89 slides

Carbapenamases Facts and Diagnosis

Carbapenamases Facts and Diagnosis

1.6k views • 68 slides

Evidence for Feedback in the IGM at High Redshift

Evidence for Feedback in the IGM at High Redshift. Barlow (CIT), Becker (CIT), Boksenberg(IoA), Sargent (CIT), Simcoe (MIT), Rauch (OCIW). (based on QSO absorption line data from Keck HIRES, ESI and LRIS). How does the undisturbed IGM look ?.

721 views • 60 slides

Carbapenamases in Antibiotic Resstance

Carbapenamases in Antibiotic Reistance

3.82k views • 53 slides

Kuwait Petroleum Corporation (KPC)

828 views • 53 slides

TeV ???????

513 views • 36 slides

Local Group of Galaxies in the EGRET era and perspectives for GLAST Igor V. Moskalenko Stanford

Gamma-ray Large Area Space Telescope. Local Group of Galaxies in the EGRET era and perspectives for GLAST Igor V. Moskalenko Stanford. Local Group of Galaxies. Milky Way and M31 are the dominant galaxies in the group Many others are irregular or dwarf spheroidal

483 views • 35 slides

Radio Sources and the Evolution of the ICM

Radio Sources and the Evolution of the ICM. David De Young US National Optical Astronomy Obs. Thomas W. Jones University of Minnesota Cosmic Magnetism Bologna - August 2005. Radio Sources and the Evolution of the ICM. Two Major Topics:

432 views • 35 slides

Supported by UNICEF, UNESCO, The World Bank, SERP, MHRD, MWCD, CARE India State Research Partners

Quality Variations in Early Childhood Education. Supported by UNICEF, UNESCO, The World Bank, SERP, MHRD, MWCD, CARE India State Research Partners NIPCCD Guwahati & Andhra Mahila Sabha Hyderabad. Overview of presentation. Background of the study.

480 views • 34 slides

Science by LCGT

Science by LCGT. Hideyuki Tagoshi (Osaka University). 2011/02/04 LCGT f2f meeting. Contents. Compact binary Coalescence (CBC) NS-NS Merger rate, event rate Parameter estimation accuracy Gravitational Collapse Pulsar Stochastic background. Detection of GW.

322 views • 32 slides

Hot Gaseous Halos of Disk Galaxies

409 views • 31 slides

What is getting in and/or out of nearby disk galaxies?

413 views • 29 slides

V. Bobylev and A. Bajkova Pulkovo Observatory, St. Petersburg, Russia

V. Bobylev and A. Bajkova Pulkovo Observatory, St. Petersburg, Russia. GALAXY STUDY USING RADIO OBSERVATIONS OF MASERS. 18-22 October 2010. INTRODUCTION. Khoperskov, Tyurina, Astron. Rep., 47, 443 (2003). INTRODUCTION. VGPS-HI VLA Galactic Plane Survey (Stil et al. 2006)

398 views • 25 slides

Dark Matter Particle Physics View

Dark Matter Particle Physics View. Outline DM candidates Direct DM Search Indirect DM Search Possible Manifestations DM Profile of the Milky Way. Dmitri Kazakov JINR/ITEP. Problem # 3. What is Dark Matter ?. ?. ?. ?. DARK. TRANSPARENT. INVISIBLE. What is it made of ?.

367 views • 22 slides

Astrometry of Water Masers in Post-AGB Stars

Astrometry of Water Masers in Post-AGB Stars. Hiroshi Imai Graduate School of Science and Engineering, Kagoshima University. Contents. Astrometry with VLBA , and VERA (EVN for OH masers) Results of astrometry IRAS 19134+2131 K3-35 IRAS 19312+1950 IRAS 18286-0959 IRAS 22480+6002

415 views • 18 slides

Parsec-scale Constraints on the ISM From the Millisecond Pulsars in Terzan5

Jason Hessels (McGill) Ingrid Stairs (UBC) David Kaplan (MIT). Fernando Camilo (Columbia) Paulo Freire (Arecibo Obs) Victoria Kaspi (McGill). Parsec-scale Constraints on the ISM From the Millisecond Pulsars in Terzan5. Scott Ransom (NRAO Charlottesville).

259 views • 14 slides

Binary Quasars in the Sloan Digital Sky Survey

Binary Quasars in the Sloan Digital Sky Survey. Joseph F. Hennawi Berkeley. Hubble Symposium April 7, 2005. Suspects. Naohisa Inada (Tokyo). Gordon Richards (Princeton). Masamune Oguri (Princeton). Michael Strauss (Princeton). Conclusions.

244 views • 13 slides

The Size of Absorption Line Systems

198 views • 12 slides

Morphological Analysis of LAEs

Morphological Analysis of LAEs. Group Discussion Chair: Nicholas Bond. Possible Uses of this Discussion. Ascertain status of our current knowledge of LAE morphologies Guide the future direction of LAE morphology determination Critique methods already in use

260 views • 10 slides

108 views • 1 slides