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Cosmological Evolution of FR II Radio Galaxies

Cosmological Evolution of FR II Radio Galaxies

Cosmological Evolution of FR II Radio Galaxies. Paramita Barai PhD Prospectus Talk Physics & Astronomy Georgia State University 19 th Oct, 2004. Contents. Introduction, Motivation, Goals & Procedures Radio Observation Samples Models of Radio Source Evolution

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736 views • 59 slides
Eric Linder 7 June 2012

Eric Linder 7 June 2012

Chasing Down Cosmic Acceleration. Eric Linder 7 June 2012. UC Berkeley & Berkeley Lab . . GR. ?. ?. Us. New Stuff. Us. Old New Stuff. Describing Our Universe. STScI. 95% of the universe is unknown!. STScI. Mapping Our History.

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438 views • 33 slides
X-ray Production

X-ray Production

X-ray Production. kVp KINETIC ENERGY OF ELECTRONS. CATHODE --------. MADE OF TUNGSTEN + 1%-3% THORIUM. TUNGSTEN. Z # 74 MELTING POINT- 3,410 DEG. CELSIUS . THORIUM. Z # 90. THERMIONIC EMISSION. CATHODE HEATED UP TO AT LEAST 2,200 DEG. CELSIUS. ANODE +++++. TUNGSTEN

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625 views • 30 slides
Eric Linder University of California, Berkeley Lawrence Berkeley National Lab

Eric Linder University of California, Berkeley Lawrence Berkeley National Lab

Course on Dark Energy Cosmology at the Beach 2009. Eric Linder University of California, Berkeley Lawrence Berkeley National Lab. JDEM constraints. Outline. Lecture 1: Dark Energy in Space The panoply of observations Lecture 2: Dark Energy in Theory The garden of models

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283 views • 28 slides
Transient Sources

Transient Sources

Transient Sources. S. R. Kulkarni California Institute of Technology Pasadena. Why is the radio band important?. Almost all non-thermal phenomena produce decimeter emission There are few (three) centimeter wave interferometers VLA has (completely) dominated GRB science

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379 views • 27 slides
Normal Curve Area Problems involving only z (not x yet)

Normal Curve Area Problems involving only z (not x yet)

Normal Curve Area Problems involving only z (not x yet). To accompany Hawkes lesson 6.2 A few slides are from Hawkes Plus much original content by D.R.S. HAWKES LEARNING SYSTEMS math courseware specialists. Continuous Random Variables 6.2 Reading a Normal Curve Table.

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453 views • 23 slides
The PFIT Project WW05'14

The PFIT Project WW05'14

The PFIT Project WW05'14. Intel Corporation Nick Klein Phuong Ho Padmashree Patil Ben Schwarz Gary Davis Jan 30, 2014. The PFIT Project. Agenda Motivation/Opportunity Proposed Solution/Approximate Cost Development/Timeline. Motivation/Opportunity.

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267 views • 13 slides
The Present and Future of GRB Cosmography

The Present and Future of GRB Cosmography

The Present and Future of GRB Cosmography. Andrew S. Friedman (Harvard-CfA) & Joshua S. Bloom (Harvard-CfA / UC Berkeley). www.cosmicbooms.net. Outline. Motivations: What is GRB Cosmography? Brief History Current Work Future Prospects. Motivations.

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375 views • 12 slides
Wide Field Astronomy from Space

Wide Field Astronomy from Space

Wide Field Astronomy from Space. Steven Beckwith Space Telescope Science Institute January 9, 2002. F n (F n + DW B n ) 1/2. A Dn h n. ). (. 1/2. t 1/2. S/N = . Limits:. Space advantages: Low B n Small DW over FOV PSF stability Photometric stability Full sky coverage

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223 views • 12 slides
VDDA syndrome on two AMS modules

VDDA syndrome on two AMS modules

VDDA syndrome on two AMS modules. This analysis refers to two chips (5 e B) respectively of modules (20210210140103 and 20210210122103) and their mating sensors. If the chip is operated, tha faults appear close to row 32 of columns 10&11 (chip5) and of row 32 of columns 1&2 (chipB).

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179 views • 9 slides
Welcome to the ECEN 325 LAB!

Welcome to the ECEN 325 LAB!

Welcome to the ECEN 325 LAB!. TA: Younghoon Song (john) Office Hours: T & R 10-11am Office : WBRC 114. Important!. To run PSPICE simulations in the ECE Department computers you have to temporarily save your files (Eg. schematics) in the computer desktop.

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330 views • 8 slides

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