The Alcock-Paczynski Probe of Cosmology Lyman- forest, LSS, And Cosmic Consistency Albert Stebbins Fermilab Dark Energy Workshop Center for Cosmological Physics
... to other components provide angle to camera and path calculator avoid bumping into objects Design Construction of tower RS232 - I2C interface Master: ...
Disentangling dynamic and geometric distortions Federico Marulli Dipartimento di Astronomia, Universit di Bologna Marulli, Bianchi, Branchini, Guzzo, Moscardini and ...
Stability of compact stars (white dwarfs and neutron stars) . G.S.Bisnovatyi-Kogan Space Research Institute RAN, Moscow Joint Institute of Nuclear Researches, Dubna
We calculated an Anisotropic Correlation Function, ?(s,s//), from SDSS LRG ... survey such as WFMOS (Wide-Field Multi-Object Spectrograph) gets available. ...
m = number of Fourier modes measured in the survey. n = mean ... BAO ring is shifted inwards and broadened. Broadening peak smoothes oscillations. x(r) P(k) ...
Kick velocity Why do neutron stars move so rapidly? Stars vs. Neutron Stars Pulsar velocity distribution SN explosions should not be symmetric! SN and kick explosion ...
After the decoupling, acoustic patterns of photon and baryon density fields were ... There's no significant disturbances that erase acoustic patterns ...
... Royal Astronomy in 1791, with the title 'On Nebulous Stars, Properly So Called ' ... to the conclusion that planetary nebulae were nebulous material around a star. ...
Lecture 5. Population synthesis of NSs Sergei Popov (SAI MSU) Population synthesis in astrophysics Why PS is necessary? Tasks Two variants Examples Magnetorotational ...
The endpoint of massive stars in binaries: singlets, doublets? ... Baryon poor outflows. GRB. 3e50erg. Black hole output. Rotational energy of black hole ...
The 2dF-SDSS LRG And QSO (2SLAQ) Survey. Clustering techniques ... `Bump' in the 2 Point Correlation Function at ~100 h-1 Mpc. Due to ``baryon acoustic oscillations' ...
Review of High Energy Astrophysics Research in Mainland China Zhang, Shuang Nan Tsinghua Center for Astrophysics (THCA) and Physics Department Tsinghua University ...
AM CVn Workshop -- Nijmegen 4.7.2005. Non stationary features in light curves of ... ?: orbit O: disc precession (apsidal advance) N:Nodal regression or f2: pulsation? ...
Gamma ray bursts from binary black holes Agnieszka Janiuk Center for Theoretical Physics, Polish Academy of Sciences, Warsaw Collaboration: Szymon Charzy ski (Warsaw ...
Cluster velocity velocity correlation functions as probes of dark energy ... With a smaller beam a cluster stands out better against the confusing background ...
The Elusive Nature of (early) R-stars Inma Dom nguez Tangata: L. Piersanti O. Straniero (INAF-OACT) C. Abia O. Zamora (UGR) R. Cabez n D. Garc a-Senz (UPC)
(Rosswog 07; Faber 06; Lee 09) a. r - Process Heating (not included in present simulations! ... NS Matter A ~ 100 Nuclei Free Neutrons (Lattimer 77; Meyer 89) ...
Short history of the paradigm: internal vs external shocks. Afterglows: external shocks ... Assume Isotropy. Energy and Power. GRB are powerful. AGN: L 1048 erg/s ...
AGB Star Yields for Everyone John Lattanzio1 and Amanda Karakas2 1: Centre for Stellar and Planetary Astrophysics, Monash University,Australia 2: Origins Institute ...
1. The Magnetothermal Instability and its Application to ... Magneto-Rotational. Magneto-Thermal. Keplerian Profile. Conserved Quantity: Angular Momentum ...
7 known planets: HD 209458, TrES-1, OGLE-TR-10, 56, 111, 113, and 132 ... TrES-1. Model test results. Fit Parameters. Equations. 4 unknowns: M1, R1, M2, and R2 ...
Generic picture of an accreting system (pm,swift) A collapse of a rotating envelope ... Timing is good as SWIFT is to be launched soon. It used to be used ...
The light curve of the reverse shock alone (without the contribution of the forward shock) ... bright is the optical flash? E isotropic equivalent energy ...
Locating and. Observing. Optical. Counterparts to. Unmodeled. Pulses in Gravitational ... we have a goal of ~1 hour from IFO event to first EM observation ...
The thin accretion disk models describes a cooling-dominated flow in which the ... model provides the picture of how gases flow near the vicinity of a black hole ...
Radio beam geometry and velocity kick distribution Arzoumanian, Chernoff & Cordes (2002) ... to 978 radio pulsars (Galactic plane) to 120 supernovae in the Gould Belt ...
The quasar 0957 561: the first multiply-imaged source discovered ... Quasar Timings ... Timing of multiply lensed quasars used to favour H0~50kms-1Mpc. Finding ...
What is the Dark Energy? David Spergel Princeton University One of the most challenging problems in Physics Several cosmological observations demonstrated that the ...
stars that go bump in the night. Credit: Matthew Bate (IoA, Cambridge) ... Ms spectroscopic mass Mc-Ls & g. Mp pulsation mass & g. Md direct mass R, , , g ...
Time variation w' is a critical clue to fundamental physics. Deep surveys of galaxies and SN to z 1. Large ... Corasaniti & Copeland 2002. w(a) = w0 wa(1-a) ...
24, June 2002. white dwarf mergers. The progeny of binary white dwarf mergers; ... Progeny of WD WD mergers ? Extreme Helium stars. RCrB stars. subdwarf B stars ...
Comparison with observations: spectra, light curves and spectral evolution ... The energy range for COMTEL was 1-30 Mev; EGRET energy range was 20 Mev to 30 Gev. ...
... and are also thermalized to a high temperature. The clever part is next: consider what would happen if, as a result of its thermal motion, ... (D~3 Gpc) L ~ fD2 ...
(1) Models, (2) Descriptions, and (3) Flows ... Global models of thin accretion disk developed ... picture of how gases flow near the vicinity of a black hole ...
General motivation for extragalactic studies. More objects. Cleaner star formation history ... Emission resolved & luminosity functions measured (Sarazin, Irwin ...
Prospects for GRB Science with GLAST Jonathan Granot University of Hertfordshire (Royal Society Wolfson Research Merit Award Holder) Collaborators: J. Cohen-Tanugi, E ...
Binary Accretion or WD-WD Merger 'Failed' Type Ia SN ... 25% of Swift Bursts (2 classes?) Similarity To GRB Ongoing Engine Activity EEE/EGRB ~ 1-30 ! ...
Cosmology with Galaxy Correlations from Photometric Redshift Surveys ... DES, JEDI, LSST, SNAP... Almost every proposed dark energy survey plans to measure BAO. ...