2df PowerPoint PPT Presentations

Title: SUMSS Author: Elaine Sadler Last modified by: astrop10 Created Date: 11/17/1999 10:06:56 AM Document presentation format: Overhead Other titles

Shaun Cole. ICC, University of Durham. Main Contributors: ... Completeness and magnitude limit masks from Cole et al 2005 using methods of Norberg et al 2002 ...

Halo mass-to-light ratios. Group luminosity ... The halo model ... Halo M/L to local group level measure efficiency peak ...

Tom Shanks, Phil Outram, Jose Cruz da Angela, Bill Frith and Nic Ross. University of Durham ... 2QZ SDSS-2dF QSO Redshift Surveys. 2QZ P(k) vs SDSS DR2 LRG P(k) ...

To have spectral stability better than 1/20 pixel over 4 hours. ... Mini-shuffle: charge shuffle by few pixels to give blended ON/OFF pairs, good to ...

Hierarchical Galaxy Clustering in the 2dFGRS. Peder Norberg (ETHZ) in ... statistical homogeneity and isotropy of the cosmic density field: not true on ...

... find a group of galaxies. A new 2dF GRS group ... for groups and clusters of galaxies ... Spatial distribution of galaxy systems : one of the main ...

In Standard Model, assumed that neutrinos have no mass. This is by choice and is not required a priori ' ... From CMB anisotropy [astro-ph/0210306] Dark Matter ...

Statistical analysis of the X-ray emission properties of type-1 AGN in the ... M. Page Mullard Space Science Laboratory-UCL (UK) ...

Luminosity Function from 2dF Quasar Survey. Luminosity Function from 2dF Quasar Survey. Luminosity Function from 2dF Quasar Survey ...

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Title: The 2dF Galaxy Redshift Survey Author: Ofer Lahav Last modified by: Ofer Created Date: 4/8/2002 11:55:24 AM Document presentation format: On-screen Show

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Limits on Neutrino masses. Bimodality in the 2dFGRS. Colour (B-R) Peacock 2003. Blue ... Weighing Neutrinos with 2dFGRS. Free streaming effect: Wn/Wm 0.13 ...

Supercluster-void network 2dF data ... Right: The same field but phases randomized. There are no filaments, clusters & superclusters ...

... 2dF UVX QSO clustering Gravitational Growth rate at z~1.6 via QSOs QSO Lensing vs galaxy ugrizYJHK ... halo mass relation Checking profile vs radius ...

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' ...

Wiener Reconstruction of the Galaxy Redshift Surveys. Pirin ... Density Field of 2dFGRS in Declination Strips ... (For details see Zaroubi et al 1995, ...

Past and more recent SN constraints. Today's landscape ... SCP 2003 (Knop et al.) CMB 2dF : w = -1.05 0.15-0.20 (stat) /- 0.09 (syst) R. Pain ...

ELT Instrument Technologies. AAO-proposed development packages. Fibres. Tunable filters ... Robots. 2dF on AAT. OzPoz on VLT. FMOS-Echidna on Subaru. MOMFOS on GSMT ...

Matthew Page, Francisco Carrera, Mirko Krumpe, Jacobo Herrero, Amalia Corral ... XMM-Newton SSC ... Optical spectra from 2dF system on AAT in 27 pointings ...

large consortium projects (MACHO, 2dF, SLOAN, VISTA...) next steps ... computing fabric management. differentiated service network technology ...

... multiplex gain of an order of magnitude over the current 2dF instrument plus ... These are 2.5 magnitudes fainter than the current 2dFGRS limit and they would be ...

Korea Institute for Advanced Study (KIAS) A Proposal for LAMOST & AS2. Dark matter halos surrounding galaxies, ... [Prada et al. 03; Brainerd 04] - [SDSS & 2dF] ...

Why (else) is J0537-6910 interesting to us? Ben Owen. Penn State. 2006 March 22 ... So many glitches so big that spindown age -f/(2df/dt) decreases at 1yr/yr! ...

Milky way. The 2dF Galaxy Redshift Survey: spectra and redshifts. Mon. Not. R. Astron. ... Milky way. 0. 500. 1000. First scan of fMRI data -5. 0. 5. T statistic ...

Methods to investigate dark energy and dark matter: galaxy ... Galaxy and quasar survey. 400,000 galaxies with redshifts. Galaxy surveys: SDSS and 2dF ...

n-2004, Paris Massive Neutrinos and Cosmology * Brief history of Hot Dark Matter * Limits on the total Neutrino mass from redshift surveys: Mn

Lecture #10 Studenmund (2006): Chapter 10 Objectives What is heteroscedasticity? What are the consequences? How is heteroscedasticity be identified?

Supercluster. SCL 126. Maret Einasto, Erik Tago, Jaak Jaaniste, Jaan Einasto, Ivan Suhhonenko and ... R.A. 13h Dec. 3o, Distance: 240 Mpc. 7 Abell clusters, 4 ...

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Title: Paired Data and Inferences on Popn Variances Subject: STA 6166 Author: Portier, Kenneth Last modified by: atrindad Created Date: 1/4/1999 1:49:36 PM

Title: SUMSS Author: Elaine Sadler Last modified by: Elaine Sadler Created Date: 11/17/1999 10:06:56 AM Document presentation format: Overhead Other titles

2MASS Galaxy Catalog T. Jarrett 6dFGS Workshop (Jul 03) All Sky released 500 million sources (PSC) 1.65 million sources (XSC) 98% galaxies (XSC) 10

Observational Cosmology

Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006 ... Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006. The zoo plot in ( 2, 1) plane ...

Large Scale Structure in 2MRS

Neutrino Physics and Cosmology. 3rd lecture. Bounds on m? from CMB, ... on m? from cosmology ... (measurement) of neutrino masses from Cosmology. DATA ...

This IS the model that we use! 4. GM. ynk. ynj. yn2. yn1. n. yik. yij. yi2. yi1. i. y2k. y2j. y22 ... y2k. y2j. y22. y21. 2. y1k. y1j. y12. y11. 1. k. j. 2. 1 ...

Title: --- , , Author: SEC Last modified by: admin Created Date: 12/5/2006 12:56:29 AM

Computational Challenges in the Simulation of Water & Ice: the Motivation for an Improved Description of Water-Water Interactions ROH = 0.9572

CFRP REINFORCEMENTS AND RETROFITTINGS OF RC STRUCTURES

Neutrino Masses from LSS Neutrino Masses from the CMB (III) The Dark Energy Survey Ofer Lahav University College London

What are the key scientific questions? ... Spectroscopy from HYDRA & WYFFOS. Reddening. The time domain.? Largely unexplored regime. ...

VST: 2.6m f/5.5, 1.4 deg F field, active primary mirror ... disassembly. salerno. livorno. To Paranal. Aug 3: On Paranal ! Summary. 1500 sq.deg. ...

By studying these, astronomers hope to develop a better ... Maintaining a target frame-rate (Funkhouser and S quin, 1993) Fixed level of interactivity ...

is called the neutrino free-streaming. scale and roughly corresponds to the ... On scales much larger than the free streaming scale, on the other hand, ...

`Piggyback' redshift surveys of radio galaxies at z 0.3 ... Needs new large-area (50-100 deg2) sub-mJy radio survey. ... the local radio-source population is ...

Constraining evolution in the Halo Model using galaxy redshift surveys (astro-ph ... Halo Model N-body simulation provides a practical way of building ...

Genetics and Genetic Prediction in Plant Breeding

After the decoupling, acoustic patterns of photon and baryon density fields were ... There's no significant disturbances that erase acoustic patterns ...

Neutrino masses from double beta decay Kai Zuber University of Sussex

baryon and CDM. experience. gravitational. clustering ... Baryon acoustic oscillations (SDSS) Bounds on parameters from other data: SNIa (Om), HST (h) ...