UK Infrared Deep Sky Survey. overview and status. Near-IR ... 5 surveys, 3 extragalactic. Significantly deeper than 2MASS. UKIDSS. Observing started May 2005 ...
High-Mass Star Formation UKIDSS & GLIMPSE Views. Melvin Hoare ... Robitaille et al. Model Fitter results to 2MASS, MSX, TIMMI2, IRAS. The CORNISH Survey ...
... hierarchical models do NOT match bulges: PLE better. Cimatti etal, VLT ... Infrared selection is the next big step. building on Denis, 2MASS, VISTA, UKIDSS. ...
G.De Zotti (INAF-OAPD), L.Danese (SISSA), L.Silva (INAF-OATS), G.L.Granato (INAF ... and Clusters) see also Farrah et al. (2006) THE UKIDSS DR1 Sample ...
... mag diagram for Galactic Centre and Nuclear Bulge fields by Andrew Gosling from ... The plot combines UKIDSS data (lower part) with 2MASS data (upper part) ...
Obtain spectra for 1 million galaxies and 100,000 quasars ... Highest known redshift quasar (z = 6.4) Large scale structure cosmological constraints ...
Wide-Field Astronomy Unit. University of Edinburgh (rgm@roe.ac.uk) 2 /24. Outline ... Astronomical data: original form ... Astronomical data: final form. Most ...
z=4 Model Quasar SDSS filter set. Crafoord Symposium, Sept 2005. 10 ... Will become ESO facility on completion of construction and commissioning in late ...
Next Generation Deep 2m Survey: Reconnoitering the Dark Ages Jeremy Mould, Swinburne University Recent Progress in theoretical and observational cosmology
Lecture 1 Aim: Become familiar with astronomy data Learn a bit of programming No set text Web resources Library My own books (maybe!) Programming environment:
Panoramic Survey of the Deep Universe Observing Galaxy Formation at High Redshift Toru Yamada National Astronomical Observatory of Japan Opt/IR Div., Subaru Telescope
WP 6200.1 - Partecipazione alla Definizione dei KP in GT WP 6200.2 Partecipazione alla Preparazione dei KP in GT WP 6200.3 Sviluppo di algoritmi di riduzione ...
'A Method for Determining the Physical Properties of the Coldest Known Brown Dwarfs' ... determination of the physical properties for these sources, including, ...
Deep Surveys: DXS(K=21; 35) , UDS (K=22.8; 0.77) Seeing 0.6' to 1.2' ... Able to build workflows i.e. pieces of code which run on the server and are reusable ...
Working data-grid. Pilot federations. Pilot visualisation ... 10 Key Science Drivers, using: Optical data in Edin & Camb. Near-IR data. X-Ray data. Radio data ...
SCUBA gals, starbursts, AGN) ... Old Stellar Populations at Early Epochs Ages and metallicities of stellar ... Old stellar populations: determine age ...
No compelling theory, must be observational driven. We can make ... Blake et al. 2006, Padmanabhan et al. 2006. Cosmological Constraints. Sullivan et al. (2003) ...
Brown dwarfs and star forming regions in the framework of the ... impact on different fields of Astrophysics, in particular on the area of star formation. ...
Database of potentially nearby PNe Improved integrated fluxes in Ha and [OIII] ... H. Bond / HST/ NASA AAO/UKST Survey Credit: ESA/ESO/NASA AAO/UKST Survey ?
The (second) widest ultracool binary: a challenge for very low-mass formation ... The widest system containing an L dwarf component. Primary: HD 221356 (F8.0V; ...
A critical review of global efforts in this area. Assess what ... weak lensing and acoustic baryonic oscillations (based on photo-z, i.e. requires IR as well) ...
http://www.ast.cam.ac.uk/vdfs/docs/photom.pdf. 10/13/09. Simon Hodgkin CASU. Overview. Conversion from WFCAM counts to Vega magnitudes at airmass unity in the MKO ...
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) ...
4 days for each of ~ 100 lucky' targets. 19 March 2006. Jonathan Zwart, Cavendish ... Wedding cake': 10 deep survey (1 year) 100 shallow survey (6 months) ...
Similar for most observatories. Defined ... Observing the warm cores of molecular clouds ... Radial velocity study of 14000 F and G stars over two decades years ...
Discover terrestrial-mass planets in the habitable zones of ... Astroseismology. Jet and shock physics. Masses and ages of star clusters in spiral galaxies ...
11 July 2005. Astrogrid Meeting. 1. CASU Data Centre. Jim Lewis. Cambridge ... INT Wide Field Survey and IPHAS. Raw data stored ... INT/WHT INGRID (1), INT ...
Spectra of quasars in Sloan Digital Sky Survey (SDSS) show presence of Gunn ... Surface brightness remains unchanged. But source appears M times larger on sky ...
Various codes currently available - Hyperz (Bolzonella et al. 2000) - Bpz (Benitez 1999) ... Storage MySpace in AstroGrid - Format. 18 August 2006. Paresh ...
Title: No Slide Title Author: andy lawrence Last modified by: James Created Date: 1/27/1997 3:20:31 PM Document presentation format: On-screen Show (4:3)
Gemini Keck. From Avi Loeb. reionization. Two Key Constraints: WMAP 3-yr: zreion=10 /-3 ... 0.6 (2-sigma) by fitting both DLA and IGM profiles. Damping wing? ...
all-sky survey to enable multiple science goals. applications from solar system to cosmology ... Static sky science. Enabled by stacking repeated scans to form ...
Chris Simpson. Liverpool John Moores University. and a cast of ... Ouchi et al. 2005, ApJ, 620, L1, Discovery of primeval LSS with forming clusters at z=6 ...
Mapping Galactic Spiral Arm Structure: The IPHAS Survey and Virtual Observatory Access ... IC 5070 the pelican nebula: Credit Nick Wright (UCL) 5o x 5o H -r' ...