- highest redshift galaxies
- AGNs
- galaxy populations
- dynamics inside a halo/galaxy
- galaxy formation
- ionisation history
- galaxy clusters
- DM, DE
- neutrinos
- power spectrum of density perturbations
- cosmic topology measurements, Gaussianity tests
- cosmic topology theory (or what might be the start of a theory)
- cosmic strings - possible detections
- fundamental physics
- statistics

- AstroPh:0301096 The Discovery of Two Lyman-α Emitters Beyond Redshift 6

- AstroPh:0211114 blazars in Xrays
- AstroPh:0211118 claim that radio loudness in AGNs does not depend on SuperMBH mass
- AstroPh:0301094 radio lobes may cause: magnetic fields and spread of metals in the IGM, and star formation - Gopal-Krishna, Wiita
- AstroPh:0301447 AGNs in clusters - plasma physics in clusters - Eilek

- AstroPh:0211080 - photometric redshifts of 6 million galaxies from the SloanDSS
- AstroPh:0210643 - the FundamentalPlane at z=1.27 - massive galaxies at high redshift, EROs
- AstroPh:0211068 - Phoenix Deep Survery - 2000 sources @1.4GHz to 60µJy in 4.56 sq.deg - estimated 0<z<1
- <a class="interwikiLink" href="https://arXiv.org/abs/astro-ph/0301457" title="'0301457' on astro-ph preprint archive">AstroPh:0301457 - UCDs - ultra-compact-dwarfs - the result of a dwarf elliptical being stripped of 99% of its

- AstroPh:0310661 - population evolution of K-band hyperluminous galaxies (HLIRGs) similar to most luminous radiogalaxies?
- AstroPh:0301427 - FIRBACK observations of 0.4<z<0.9 ultraluminous galaxies which contribute to the [CIB]
- AstroPh:0401032 - Some Current Issues in Galaxy Formation (June 2003)
**excellent short review**- Joe Silk - AstroPh:0401503 -
**characteristic scales**in galaxy formation: 10km/s, 30km/s, 100km/s, 300km/s - Dekel - AstroPh:0402276 - galaxy down-sizing from Subaru - some small galaxies form stars late - Kodama et al.

- AstroPh:0301149 - seem to be blue dwarf galaxies - Le Floc'h, Duc, Mirabel et al

- AstroPh:0210641 - Ω
_{m}and power spectrum from LSBs - McGaugh - AstroPh:0210658 - SuperMBH s have no significant effect on density profiles - Read, Gilmore
- AstroPh:0211074 - HST observations of BCGs and inferences for density profiles
- AstroPh:0307362 - in CDM models cannot destroy satellite galaxies sufficiently to match observations of UltraCompactDwarfs - S. Kazantzidis, B. Moore, L. Mayer
- AstroPh:0310660 - The origin and tidal evolution of cuspy triaxial haloes - Ben Moore, Stelios Kazantzidis, Juerg Diemand, Joachim Stadel
- AstroPh:0311155 - lack of small-scale power leads to artificially cuspy haloes? Discreteness effects in cosmological N-body simulations - Binney
- AstroPh:0401088 - missing satellite problem solved?

- AstroPh:0211105 - 2D spectroscopy of double-barred galaxies - relation to structure near nucleus - Moiseev

- AstroPh:0302343 - (100)
^{1/3}times better resolution in N-body simulations via Wavelets - Romeo et al - AstroPh:0210525 SPH simulations showing ellipticals forming which are
**not**the result of major mergers of spirals - Hernandez, Lee - AstroPh:0402248 - shock generated SFR vs density generated SFR in mergers - Barnes
- AstroPh:0402271 - stellar population synthesis - new models - Jimenez et al.

- AstroPh:0202318 - Gamma-Rays from Intergalactic Shocks
- AstroPh:0401003 - shoulder in QSO luminosity function due to maximum mass for SMBH mergers to match halo mergers - Mahmood, Devriendt, Silk
- AstroPh:0401087 - Quasar Feedback: the Missing Link in Structure Formation - Scannapieco, Peng Oh

- AstroPh:0211071 - Miralde-Escude
- AstroPh:0310593 - WMAP => reionisation at z=20 => need early star formation => either "extreme assumptions" or a component of isocurvature fluctuations - Naoshi Sugiyama, Saleem Zaroubi, Joseph Silk

- AstroPh:0210662, AstroPh:0210665 - cooling flows or not? XMM-Newton data
- AstroPh:0210667 simulations showing that finding SunyaevZeldovich effect is subtle - Schultz, Martin White
- AstroPh:0211422 SunyaevZeldovich review - Rephaeli Sep 2002
- AstroPh:0211430 point sources (positive temp fluctuations) versus negative (SunyaevZeldovich) - Rubino-Martin, Sunyaev
- AstroPh:0211408 - "quantised" galaxy positions/velocities from theory - Watts, Coles, Melott
- AstroPh:0301439 - cluster density profile: mass density versus number density to twice the virial radius - Biviano,

- AstroPh:0207353 - morphological redshift estimates of SunyaevZeldovich effect clusters
- AstroPh:0307539 - models (simulations) fail to match observed (z < 0.13) evolution in cluster eccentricities - Stephen Floor, Adrian Melott, Patrick Motl
- AstroPh:0405514 - cooling flows from SMBH heating? Yutaka Fujita (NAOJ), Thomas H. Reiprich (UVa)

- "First Year WMAP papers":http://de.arxiv.org/find/astro-ph/1/first%20year%20wilkinson/0/1/0/past/2/0 - summary paper is AstroPh:0302209
- HepPh:0210370 - review on DM and DE - Kamionkowski

- AstroPh:0211095 - use of CMB polarisation towards clusters to detect the WikiPedia:Integrated_sachs_wolfe Effect as a function of redshift, and hence some DE constraints
- AstroPh:0211100 - SNeIa seen in the near-infrared H band may be better standard candles
- AstroPh:0211084 - geometrical diagnostic for DE - Sahni et al.
- reverberation mapping - AstroPh:0211385 - using BELR of quasars as physical coordinate standard ruler, idea implemented since about 5 years ago in dedicated telescope by 吉井 (Yoshii)'s MagnumProject in Japan
- w=-1.06 (+0.20, -0.25) (68% confidence) - CMB - VerySmallArray - AstroPh:0205381 AstroPh:0212495 AstroPh:0212497 0212495 shows C
_{l}spectrum including 4th peak and possibly rise to 5th peak near l=1400, i.e. 0.1degree = 6 arcmin - GrQc:0203060 standard ruler - Is there an imprint of Planck scale physics on inflationary cosmology? - Shankaranarayanan ("Shanki")
- AstroPh:0210305 AstroPh:0210306 - Archeops results
- AstroPh:0302306 WMAP constraint on features in power spectrum - Bridle et al.
- AstroPh:0311622 N=194 SNe rule out flat Universe at 90% significance - Tirth + Paddy, AstroPh:0311622 similar results, include 14 HST SNe with 1 < z < 1.5
- AstroPh:0312424 X-ray clusters/SZ seem to favour
**w**Alcaniz_{Q}< -1 - AstroPh:0405282 DAMA/NaI 7 year results look good for having detected CDM - only problem is deciding which particle - Bernabei et al Gran Sasso
- AstroPh:0404205 Have Atmospheric Cerenkov Telescopes Observed Dark Matter? - Dan Hooper, Ignacio de la Calle Perez, Joseph Silk, Francesc Ferrer, Subir Sarkar
- INTEGRAL - non-heavy DM from central 1 kpc around Galactic Centre ? http://www.astro.uni.torun.pl/sympa/cosmo-torun/2004-05/msg00017.html

- AstroPh:0211067 - evidence for mirror matter from Eros??? - Foot, R. Mitra
- AstroPh:0403043 - claim that mirror matter H' or He' halo with some O' better fits DAMA/NaI energy spectrum than WIMPs - Foot
- HepPh:0402267 - Ω
_{b}to Ω_{m}from mirror matter implies ~1eV scale suggests relation to neutrino oscillations - Foot, Volkas

- GrQc:0406056 casimir energy from scalar field frozen in at Planck time gives Ω
_{Λ}today - Unnikrishnan

- HepPh:0210389 - neutrino model implies "DM candidate" - right-handed neutrino - Krauss, Nasri, Trodden
- HepPh:0211254 - axions as CDM - hints from galactic rotation curves and a feature in an IRAS map for axions
- AstroPh:0212345 -
**nanolensing**of GRBs by planetary mass objects - Mark Walker, Geraint Lewis - AstroPh:0401140 - DM = neutralinos which annihilate and explain cooling flow problem in gal clusters - Totani
- AstroPh:0212414 - DE & DM as two limits of the same thing (Chaplygin fluid) - Gonzalez-Diaz
- AstroPh:0307350 - DM = value of scalar field, DE = energy density of the same field - distance-z relations - Mark B. Hoffman
- AstroPh:0406194 - DM as scalar field (spin-0 fundamental interaction) - explains early formation of big ellipticals - Matos, Urena-Lopez

- AstroPh:0305364 - Weyssenhoff fluid in FLRW model, brane models - Marek Szydłowski, Adam Krawiec
- AstroPh:0306438 -
*R*, with^{n}**n<0**in Hilbert-Einstein action provides DE and early inflation - Carroll, Duvvuri, Trodden, Turner - AstroPh:0307311 - Closed Universes, de Sitter Space and Inflation => DE + low quadrupole/octupole + high k effects - Lasenby, Doran
- HepTh:0307128 - Phantom cosmologies - Mariusz P. Dabrowski, Tomasz Stachowiak, Marek Szydlowski
- AstroPh:0308515 - Quintessence From The Decay of a Superheavy Dark Matter - Houri Ziaeepour
- AstroPh:0310609 - phenomenological hypothesis: Ω
_{Λ}α Ω_{m}? - Majernik - AstroPh:0311247 - Partial rip scenario - a cosmology with a growing cosmological term - Hrvoje Stefancic
- AstroPh:0405200 - time and the radial components of the energy momentum tensor for a Schwarzschild metric are equal - applying the same property to cosmology gives a cosmo constant - Yukio Tomozawa
- HepTh:0406060 - Vacuum Fluctuations of Energy Density can lead to the observed Cosmological Constant - Thanu Padmanabhan
- GrQc:0407070 - Searching for a solution to the cosmological constant problem - a toy model - Wojciech P. Tarkowski (St Paul Research Lab, Warszawa)
- AstroPh:0409073 - Dynamics of the Universe with global rotation - Wlodzimierz Godlowski, Marek Szydlowski (Krakow)

- AstroPh:0302357 - a
**decelerating**universe is consistent with SNeIa and CMB (including WMAP) data - Vishwakarma - AstroPh:0301087 - Does DE become negative in the future for supergravity and many other M-theory models? - Kallosh, Linde

- AstroPh:0211106 - detecting neutrinos via observational cosmology??? - Hannestad
- HepPh:0302131 - WMAPping out Neutrino Masses

- AstroPh:0211090 - calibration of σ
_{8}from better simulations applied to observations - Viana et al. - AstroPh:0301641 - inverse approach for an N-body simulation - reconstructing the initial density perturbations from

- AstroPh:0302138 - CMBEASY: an Object Oriented Code for the Cosmic Microwave Background - Doran - http://www.cmbeasy.org
- AstroPh:0302306 - see above - Bridle, Lewis, Weller, Efstathiou
- AstroPh:0306206 - high blazar contribution to l=500 (20-50%) up to l=800 (50-100%) of WMAP, Boomerang
- AstroPh:0312174 - P(k) from WMAP has infrared cutoff and is lumpy - Shafieloo, Souradeep

- AstroPh:0307515 - unbiased hybrid estimator that combines a maximum likelihood estimator at low multipoles and pseudo-C
_{l}estimates at high multipoles - G. Efstathiou - AstroPh:0310382 - trans-planckian oscillations - Martin, Ringeval

- AstroPh:0302209 - WMAP - Spergel et al. "finite universe model"
- AstroPh:0302496 - WMAP - Tegmark et al. - AstroPh:0307282 - against topology interpretation
- AstroPh:0303643 - WMAP non-random phases - Chiang et al.
- AstroPh:0305248 - non-Gaussianity tests - Raeth, P. Schuecker
- AstroPh:0405519 - WMAP 1yr bispectrum against Gaussianity (frequentist test), inconsistency with other tests - Kate Land, Joao Magueijo
- AstroPh:0310273 - Detection of non-Gaussianity in the WMAP 1-year data using spherical wavelets - P. Vielva, E. Martinez-Gonzalez, R. B. Barreiro, J. L. Sanz, L. Cayon
- AstroPh:0402602 - Wavelets and WMAP non-Gaussianity - Pia Mukherjee, Yun Wang
- AstroPh:0409397 - Foreground contributions (correlated with cosmic ray distributions) to the Cosmic Microwave Background - Tadeusz Wibig, Arnold W. Wolfendale
- AstroPh:0304290 - opposite quasar pairs - Weatherley et al.
- AstroPh:0305020, AstroPh:0304558, AstroPh:0303636 - WMAP low quadrupole => not topology, but double inflation, or other early universe physics?
- AstroPh:0307507 - Asymmetries in the CMB anisotropy field (WMAP) - Eriksen, Hansen, Banday, Gorski, Lilje
- AstroPh:0303127 - low WMAP quadrupole from positive curvature? AstroPh:0306431 - significance of low WMAP quadrupole - AstroPh:0310207 - max likelihood analysis gives higher WMAP quadrupole - G. Efstathiou
- AstroPh:0310186 - standard analysis of WMAP misleading since some assumptions wrong - Antony Lewis
- AstroPh:0310233 - circles test with WMAP
**against**many torus-like models up to 16.8 h^{-1}Gpc in size - Cornish, Spergel, Starkman, Komatsu - AstroPh:0310253 - Poincare dodecahedral model
**likely**from WMAP data - Luminet, Weeks, Riazuelo, Lehoucq, Uzan - AstroPh:0402608 - Poincare 11deg circles? - TCfA group
- AstroPh:0310511 - multipole vector analysis of WMAP data in
**favour**of non-Gaussianity and cross-correlations of fluctuations on scales $2\; <\; l\; <\; 8$ - AstroPh:0310542, AstroPh:0310601 - low multipoles in WMAP ILC (internal linear combination) map are non-poissonian and contain foreground residues - P.D. Naselsky, A.G. Doroshkevich, O.V. Verkhodanov
- HepTh:0311059 Influence of Super-Horizon Scales on Cosmological Observables Generated during Inflation - Matarrese, Musso, Riotto
- AstroPh:0403353 low multipoles from Oort cloud (outer solar system)? - Dominik J. Schwarz (CERN), Glenn D. Starkman (CERN, Case Western Reserve University), Dragan Huterer (CWRU), Craig J. Copi
- AstroPh:0405544 low multipoles natural (no fudging) from stochastic inflation - M. Liguori, S. Matarrese (Univ. of Padova and INFN), M. Musso (Univ. of Pavia and INFN), A. Riotto
- AstroPh:0403597 hyperbolic models with long "horns" do not create flat spots; Picard model (hyperbolic) matches WMAP data - Aurich et al.

- GrQc:0310002 Peaks in the Hartle-Hawking Wave Function from Sums over Topologies (some 3-manifolds are much more likely than others) - Anderson, Carlip, Ratcliffe, Surya, Tschantz

- AstroPh:0410073 - Kibble discusses new interest in cosmic strings, and the two following observational hints. The first one seems quite serious, at first glance:
- AstroPh:0302547 gravitational lens - Sazhin et al
- AstroPh:0406516 gravitational lens - Sazhin et al
- AstroPh:0406434 grav lens - Schild et al.

- AstroPh:0310764 - observational constraints (OH, HCO
^{+}, HI) on evolution of fundamental constants #α, the proton g-factor g_{p}and y=m_{e}/m_{p}- Jayaram Chengalur, Nissim Kanekar - AstroPh:0211402 - observational constraints on quantisation of time (Planck time, around t=10
^{-43}s) - GrQc:0301070 - observational constraints on theology via gravitational lensing by CTCs (wormholes)
- AstroPh:0302131 - Meta-Theory of Everything - Max Tegmark - this is fun stuff, but not careful like GFR Ellis et al's analysis AstroPh:0305292
- GrQc:0307112, GrQc:0211082 - a singularity-free inflationary universe
**the Emergent Universe**- George F.R. Ellis, Jeff Murugan, Christos G. Tsagas, Roy Maartens - AstroPh:0305292 - Multiverses and physical cosmology - G.F.R. Ellis, U. Kirchner, W.R. Stoeger -
**very clear discussion**

- http://de.arxiv.org/abs/physics/0408039 - On Bayesian Treatment of Systematic Uncertainties in Confidence Interval Calculation - Fredrik Tegenfeldt (ISU & CERN), Jan Conrad (CERN) - http://tegen.home.cern.ch/tegen/statistics.html

Topic revision: r1 - 21 Oct 2004, BoudRoukema

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