Resource Letter: TACMB-1: The theory of anisotropies in the ... - iucaa

230. ‘‘Dark Energy and the CMB,’’ S. Dodelson and L. Knox, Phys. Rev.
Lett. 84, 3523–3527 2000, astro-ph/9909454. I
231. ‘‘Characterizing the Peak in the CMB Angular Power Spectrum,’’ L.
Knox and L. Page, Phys. Rev. Lett. 85, 1366–1369 2000, astro-ph/
0002162. I
232. ‘‘Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations,’’
A. H. Jaffe et al., astro-ph/0007333. A
233. ‘‘Boomerang returns unexpectedly,’’ M. White, D. Scott, and E.
Piepaoli, ApJ to appear 2000, astro-ph/0004385. A
234. ‘‘First Estimations of Cosmological Parameters from BOOM-
ERANG,’’ A. E. Lange et al., astro-ph/0005004S. A
235. ‘‘New CMB constraints on the cosmic matter budget: Trouble for nucleosynthesis’’
M. Tegmark and M. Zaldarriaga, Phys. Rev. Lett. 85,
2240 2000, astro-ph/0004393. A
236. ‘‘Cosmic microwave background constrains on the epoch of reionization,’’
L. M. Griffiths, D. Barbosa, and A. R. Liddle, Mon. Not. R.
Astron. Soc. 308, 854 1999, astro-ph/9812125. A
237. ‘‘Ringing in the new cosmology,’’ W. Hu, Nature London 404
6781, 939–940 2000. E
238. ‘‘Cosmological Constraints from Current Cosmic Microwave Background
and Type IA Supernova Data; A Brute Force, Eight-Parameter
Analysis,’’ M. Tegmark, ApJL 514, L69–72 1999, astro-ph/9809201.
A
239. ‘‘Comparing and Combining Cosmic Microwave Background Data
Sets,’’ M. Tegmark, ApJ 519, 513 1999, astro-ph/9809001. A
240. ‘‘CMB Observables and Their Cosmological Implications,’’ W. Hu, M.
Fukugita, M. Zaldarriaga, and M. Tegmark, astro-ph/006436. A
Web resources
Most of these range from elementary to advanced material
within each set of pages.
241. D. Scott’s pages on the CMB http://www.astro.ubc.ca/people/scott/
cmb/html
242. Hu, W., web pages: http://background.uchicago.edu/whu/
243. Tegmark, CMB movies at http://www.hep.upenn.edu/max/cmb/
moview.html
244. http://astron.berkeley.edu/mwhite
245. E. Gawiser’s reading list at http://mamacass.ucsd.edu/people/gawiser/
cmb_group.html
246. J. Cohn’s CMB web links: http://astron.berkeley.edu/jcohn/chaut/
cmb_refs.html
247. BOOMERANG experiment CMB introduction, http://
www.physics.ucsb.edu/boomerang/press_images/cmbfacts/
cmbfacts.shtml
248. CMBFAST, a code to calculate CMB fluctuations, at http://
www.sns.ias.edu/matiasz/CMBFAST/cmbfast.html and http://
physics.nyu.edu/matiasz/CMBFAST/cmbfast.html
249. Code for Anisotropies in the Microwave Background at http://
www.mrao.cam.ac.uk/aml1005/cmb/
250. RECFAST, a code to calculation how recombination occurred, http://
cfa-www.harvard.edu/sasselov/rec/
251. Related web sites
•http://background.uchicago.edu/whu/metaanim.html
•http://astron.berkeley.edu/mwhite/movies.html
252. Pages with lists of cmb experiments:
•http://background.uchicago.edu/whu/cmbex.html
•http://astron.berkeley.edu/mwhite/cmbexptlist.html
•http://www.hep.upenn.edu/max/cmb/experiments.html
253. General cosmology sites
•N. Wright’s cosmology tutorial http://www.astro.ucla.edu/wright/
cosmolog.htm
•MAP satellite introduction to cosmology http://map.gsfc.nasa.gov/
html/web_site.html
•J. Cohn and M. White’s What is Theoretical Cosmology http://
astron.berkeley.edu/jcohn/tcosmo.html
Foregrounds
This is a huge field, see papers below for further and
earlier references.
254. Microwave Foregrounds, edited by A. de Oliveira-Costa and M. Tegmark
ASP, San Francisco, 1999. A
255. ‘‘Removing Real-World Foregrounds from Cosmic Microwave Background
Maps,’’ M. Tegmark, ApJ 502, 1–61998, astro-ph/9712038.
I
256. ‘‘A method for subtracting foregrounds from multifrequency CMB sky
maps,’’ M. Tegmark and G. Efstathiou, Mon. Not. R. Astron. Soc. 281,
1297–1314 1996, astro-ph/9507009. A
257. ‘‘Foregrounds and Forecasts for the Cosmic Microwave Background,’’
M. Tegmark, D. J. Eisenstein, W. Hu, and A. de Oliveira-Costa, ApJ
530, 133–165 2000, astro-ph/9905257. A
258. ‘‘Forecasting foreground impact on cosmic microwave background
measurements,’’ L. Knox, Mon. Not. R. Astron. Soc. 307, 9771999,
astro-ph/9811358. A
259. ‘‘Extragalactic foregrounds of the Cosmic Microwave Background:
Prospects for the MAP Mission,’’ A. Refregier, D. N. Spergel, and T.
Herbig, ApJ 531, 312000, astro-ph/9806348. A
Observations
260. C. L. Bennett et al., ‘‘4-Year COBE DMR Cosmic Microwave Background
Observations: Maps and Basic Results, ApJL 464, L11996,
astro-ph/9601067. A
261. ‘‘A flat Universe from high-resolution maps of the cosmic microwave
background radiation,’’ P. de Bernardis et al., NAT 404, 955–959
2000, astro-ph/0004404. A
262. ‘‘First Estimations of Cosmological Parameters from BOOM-
ERANG,’’ A. E. Lange et al., astro-ph/0005004. A
263. ‘‘MAXIMA-1: A Measurement of the Cosmic Microwave Background
Anisotropy on Angular Scales of 10 Arcminutes to 5 Degrees,’’ S.
Hanany et al., astro-ph/0005123. A
264. ‘‘Future Cosmic Microwave Background Experiments,’’ M. Halpern
and D. Scott, to appear in Microwave Foregrounds, edited by A. de
Oliveira-Costa and M. Tegmark ASP, San Francisco, 1999, astro-ph/
9904188. I
Observational issues
265. ‘‘‘Sample variance’ in small-scale cosmic microwave background anisotropy
experiments,’’ D. Scott, M. Srednicki, and M. White, ApJ 421,
L5–7 1994, astro-ph/9305030. A
266. ‘‘CMB Anisotropies, Large-Scale Structure and the Future,’’ D. Scott,
to appear in Proceedings of the ASP Symposium: Clusters, Lensing
and the Future, edited by Virginia Trimble, astro-ph/9509035 1995.
I
267. ‘‘Cosmic Microwave Background experiments targeting the cosmic
strings Doppler peak signal,’’ J. Magueijo and M. Hobson, astro-ph/
9602023. A
268. ‘‘Window functions of cosmic microwave background experiments,’’
M. White and M. Srednicki, ApJ 443, 61995, astro-ph/9402037. A
269. ‘‘Cosmic Microwave Background Anisotropy Window Functions Revisited,’’
L. Knox, Phys. Rev. D 60, 103516 1999, astro-ph/9902046.
A
Below are a few of the many articles discussing analysis
issues for the upcoming data. This field is rapidly developing
and no compilation can hope to be complete.
270. ‘‘Analysis Issues for Large CMB Data Sets,’’ K. M. Gorski, E. Hivon,
and B. D. Wandelt, to appear in Proceedings of the MPAÕESO Conference
on Evolution of Large-Scale Structure: From Recombination
to Garching, edited by A. J. Banday, R. K. Sheth, and L. Da
Costa Print Partners Ipskamp, The Netherlands, 1999, astro-ph/
9812350. A
271. ‘‘Karhunen-Loeve Eigenvalue Problems in Cosmology: How Should
We Tackle Large Data Sets’’ M. Tegmark, A. N. Taylor, and A. F.
Heavens, ApJ 480, 22–35 1997, astro-ph/9603021. A
272. ‘‘How to Make Maps from Cosmic Microwave Background Data
Without Losing Information,’’ M. Tegmark, ApJL 480, L87–90
1997, astro-ph/9611130. A
273. ‘‘Estimating the power spectrum of the cosmic microwave background,’’
J. R. Bond, A. H. Jaffe, and L. Knox, Phys. Rev. D 57, 2117
1998, astro-ph/9708203. A
274. ‘‘Radical Compression of Cosmic Microwave Background Data,’’ J. R.
117 Am. J. Phys., Vol. 70, No. 2, February 2002
Martin White and J. D. Cohn 117