'High background' diaporamas de présentation

Sudden jumps in the absolute energy scale and their origin

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Sudden jumps in the absolute energy scale and their origin

443 views • 40 slides

Final Results of the DEAR Experiment and Future Plans at the SIDDHARTA Experiment

636 views • 39 slides

Status and Prospect of sKEKB

524 views • 38 slides

350 views • 25 slides

Challenges in the Measurement of Neutron Star Radii

Challenges in the Measurement of Neutron Star Radii. Cole Miller University of Maryland. Collaborators: Romain Artigue , Didier Barret , Sudip Bhattacharyya, Stratos Boutloukos , Novarah Kazmi , Fred Lamb, Ka Ho Lo. Outline. NS masses are known up to 2 M sun . What about radii?.

383 views • 24 slides

Status of the XMM- Newton Slew Survey

Status of the XMM- Newton Slew Survey. P. Esquej, R. Saxton, B. Altieri, A. Read, M. Freyberg, D. Bermejo, V. Lazaro. Outline. Overview & initial impression about the XMM-Newton slew observations Data processing & source searching strategy: current status

222 views • 21 slides

Protecting the quality of HIV testing in the new HIV testing environment

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The XMM-Newton Slew Survey

The XMM-Newton Slew Survey. Richard Saxton 1 , M. Pilar Esquej 1 , Andy Read 2 , Michael Freyberg 3 , Bruno Altieri 1 , Diego Bermejo 4 , Veronica Lazaro 4, Pedro Rodriguez 1 1 ESAC 2 University of Leicester, U.K. 3 MPE, Garching, Germany 4 University of Madrid, Spain. Overview.

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PMP HD_ILCE Informal Meeting at DfT London 30 th March 2009

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PMP HD_ILCE Informal Meeting at DfT London 30 th March 2009

165 views • 16 slides

Status of the XMM- Newton Slew Survey

Status of the XMM- Newton Slew Survey. P. Esquej, R. Saxton, B. Altieri, A. Read, M. Freyberg, D. Bermejo, V. Lazaro. Outline. Overview Processing challenges Attitude reconstruction and positional accuracy Spurious sources Extended sources Conclusions. Overview.

254 views • 15 slides

Status of the XMM- Newton Slew Survey

Status of the XMM- Newton Slew Survey. P. Esquej, R. Saxton, B. Altieri, A. Read, M. Freyberg, D. Bermejo, V. Lazaro. Outline. Overview Processing challenges Attitude reconstruction and positional accuracy Spurious sources Extended sources Conclusions. Overview.

294 views • 15 slides

MCP MicroPitting and Performance Issues

203 views • 12 slides

How Well Can We Measure Neutron Star Radii?

How Well Can We Measure Neutron Star Radii?. Cole Miller University of Maryland. Collaborators: Romain Artigue , Didier Barret , Sudip Bhattacharyya, Stratos Boutloukos , Novarah Kazmi , Fred Lamb, Ka Ho Lo. Measuring stellar radii. Ordinary star, like the Sun

222 views • 9 slides

PHENIX Status @ 7.7 GeV

PHENIX Status @ 7.7 GeV. Stefan Bathe, Time Meeting, May 11 , 2010. Accumulated luminosity. BBCLL1(>1 tubes). 2 nd attempt at 6 m beta* also caused high background rate. As of Sunday morning, luminosity twice higher than before due to higher intensity.

169 views • 7 slides

Have a look at IHC Troubleshooting Tips

Tips or guide requires to following to target the main cause of a barrier with your protocol and test out outcomes. visit https://immunostaining.info

28 views • 2 slides

A. Zoglauer*, R. Andritschke, and G. Kanbach,

79 views • 1 slides