Seb Oliver's Distant Universe WWW page (F3147)  

"The Distant Universe"
F3147, Spring 2003

About these Pages

The links on this pages will be updated as the course progresses. If you would like to get copies of the notes in advance of the lectures then you may be better off going to Last Year's Page

Course Documents

LinksPrint formats
Course Document PDF Format
Course Outline PDF Format
Reading Lists Reading List
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Lecture Notes

Lecture Original HTML Print Format Animations last change
1 slides per page 6 slides per page
1Introduction MS PowerPoint HTML 1-P PDF 6-P PDF Hubble Deep Field Zoom
Structure formation (a)
Structure formation (b)
Structure formation (c)
7th January
2Homeogeneity & Isotropy MS PowerPoint HTML 1-P PDF 6-P PDF No animations 23rd January
3Nearly-Newtonian Cosmology
Geometry
MS PowerPoint HTML 1-P PDF 6-P PDF No animations 23rd January
4 Equation of State
Fate of the Universe
MS PowerPoint HTML 1-P PDF 6-P PDF No animations 23rd January
5 The Early Universe MS PowerPoint HTML 1-P PDF 6-P PDF Expanding Universe
23rd January
6 Observational Parameters & Distance Measures MS PowerPoint HTML 1-P PDF 6-P PDF No animations 23rd January
7 Classic Cosmological Tests MS PowerPoint HTML 1-P PDF 6-P PDF No animations 23rd January
8 (see 7) Classic Tests MS PowerPoint HTML 1-P PDF 6-P PDF No animations
9 K-corrections MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
10 Luminosity Functions MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
11 V/Vmax Morphological Evolution MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
12 Number Counts
Passive Evolution
MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
13 Global history of star-formation MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
14 Distant Absorbers MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
15 Distant Absorbers 2 MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
16 Gunn-Peterson Effect
Lyman alpha emitting galaxies
Photometric Redshifts
MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
17 Dusty Galaxies MS PowerPoint HTML 1-P PDF 6-P PDF 4th March
18 Background Light. MS PowerPoint HTML 1-P PDF 6-P PDF Hauser and Dek Review Paper 15th April
19 Structure Formation .. MS PowerPoint HTML 1-P PDF 6-P PDF 15th April
20 Gravitational Lensing .. MS PowerPoint HTML 1-P PDF 6-P PDF Gravitational Lensing Notes 15 th April

Problem Sheets

Set Title Reading Questions Solutions
Sheet 1 Standard Hot Big Bang High-redshift Supernovae experiments Perlmutter et al., B.A.A.S., volume 29, page 1351 (1997)
Gurvits, L. I., Kellermann, K. I. \& Frey, S. 1999, A\&A, 342, 378
PDF Format PDF
Sheet 2 Distances Distance Measures in Cosmology, Hogg Astro-ph/9905116 PDF Format XLS Spread sheet XLS Spread sheet (PDF) q5 (PDF) q5 (PDF)
Sheet 3 Luminosity Functions & Evolution ``High-redshift star fromation in the Hubble Deep Field revealed by a submillimetre-wavelength survey'' Hughes et al. 1998 Nature 394, 16. ADS link PDF file PDF Format HTML Page 1 Page 2 Page 3 Page 4 Page 5 Page 6
Sheet 4 The earliest galaxies Short paper (11 pages, single column) on Lyman-break galaxies Steidel C.C. et al. PDF Format Q1-3 Q4
JPG(a) JPG(b) JPG(c)
Sheet 5 Various PDF Format PDF
JPG(Q1 1) JPG(Q1 2) JPG(Q2 1) JPG(Q2 2) JPG(Q2 3) JPG(Q3 1) JPG(Q3 2)

Asignment

The Morphological Evolution of Galaxies

Formula Sheets

Annotated Formulae Sheet PDF Format
Physical Constants sheet Exam Version

Links

This section provides some WWW sites you may find interesting and will grow with time

The Exam

The exam is on Wednesday 28th May 2003 at 14:00 and will be one and a half hours in which you should attempt two out of three questions

Questions could take a number of different forms

  1. "Written"
  2. e.g. short notes, notes or short essays. The mark allocation should give you an indication of how much material is expected on questions such as these. Notes could be written as a sequence of points, essays would be a more carefully constructed argument. Topics for these could come from anywhere in the lectured material.
  3. "Book-work"
  4. by this I mean questions which recreate an argument or show understanding of information given in the lectures, for example deriving a formulae. You would also be expected to show some physical understanding of arguments, e.g. to explain how a formulae might be used in practice.
  5. "Calculations"
  6. You would be expected to be able to perform calculations using the material from the lectures. Such calculations are likely to be very similar to problems encountered in the work sheets

Combinations of some of those ingredients may be used in a single question.

Past Papers

The paper from 1999-2000 course "The Early Univese" had a very similar syllabus.

If you haven't already found them then you can get copies of past exam papers from The Past Exam Papers Project page.

Acknowledgments

Many thanks to Malin Sjodahl who did my "Early Universe" course in 2000 and gave me a copy of her notes, which are often clearer than my own! Thanks also due to John Peacock for supplying me with a Tex version of his formulae sheets.

Contact addresses and numbers

S.Oliver Sussex.ac.uk
last updated 9th January 2003
original January 2001
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