'Extended sources' presentation slideshows

The XMM Large Scale Structure (XMM-LSS) Survey

The XMM Large Scale Structure (XMM-LSS) Survey. Andy Read University of Leicester (for the XMM-LSS Consortium). Marseille (LAM) Milano (AOB) Milano (IFCTR) Munich (MPA) Paris (IAP) Santiago (Uni. Cato.). A Europe /Chile Consortium. PI : Saclay, France. Birmingham Bristol

549 views • 43 slides

Milagro: A Wide Field of View Gamma-Ray Telescope

Milagro: A Wide Field of View Gamma-Ray Telescope. Julie McEnery. Outline. Why is this talk relevant to GLAST? Milagro detects air-shower particles at ground level Milagro is a wide field of view Gamma-ray telescope which operates in scanning mode

441 views • 34 slides

Group meeting

421 views • 31 slides

ANTARES Highlights

ANTARES Highlights. J.J. Hernandez-Rey IFIC (CSIC-UV). MANTS Meeting, 14-15 October 2013, Garching Germany. Highlighted topics. Point sources + 2 special extended sources + 2-pt correlation function Fermi Bubbles, Diffuse flux limits GRBs Flaring sources Dark Matter (Sun). 3.

353 views • 26 slides

Point source analysis: candidate source list, extended sources and energy

Point source analysis: candidate source list, extended sources and energy. Claudio Bogazzi AWG Videoconference 13/04/2011. Outline. Candidate source list: review, feedbacks and other experiments Extended sources: how to threat them Energy information: update. New candidate source list.

351 views • 25 slides

Point source analysis: candidate source list, extended sources and energy

Point source analysis: candidate source list, extended sources and energy. C. Bogazzi, J. P. Gomez AWG Videoconference 13/04/2011. Outline. Candidate source list: review, feedbacks and other experiments Extended sources: how to threat them Energy information: update.

377 views • 25 slides

290 views • 20 slides

Spatial gain calibration of MOS & pn: relevance to extended sources study

Spatial gain calibration of MOS & pn: relevance to extended sources study. Silvano Molendi (IASF-MI). Calibration. Spatial gain calibration for the EPIC MOS and pn is good to about 5, 10 eV respectively.

232 views • 17 slides

Pyramid wavefront sensor performance with laser guide stars

318 views • 16 slides

Source Detection I:Theory

Source Detection I:Theory. P. E. Freeman & V. Kashyap 3 rd X-ray Astronomy School 14 May 2003. The Challenge: Source Detection. What challenge??. (Granted, it does look easy here. This is a Hubble image of the globular cluster 47 Tuc, courtesy P. Edmonds.).

299 views • 16 slides

Source Detection I:Theory

Source Detection I:Theory. P. E. Freeman & V. Kashyap 3 rd X-ray Astronomy School 14 May 2003. The Challenge: Source Detection. What challenge??. (Granted, it does look easy here. This is a Hubble image of the globular cluster 47 Tuc, courtesy P. Edmonds.).

162 views • 16 slides

1st INTEGRAL Data Analysis Workshop ISDC , October 5-8, 2004 Imaging extended sources with JEM-X

1st INTEGRAL Data Analysis Workshop ISDC , October 5-8, 2004 Imaging extended sources with JEM-X. N. Lund C. Budtz-Jorgensen N.J. Westergaard J. Chevenez Danish Space Research Institute. Imaging of extended sources with a coded mask instrument.

232 views • 14 slides

2XMMp clusters in the SDSS

2XMMp clusters in the SDSS. Georg Lamer Axel Schwope Jan Kohnert. Extended sources in 2XMMp. Total extended sources: 6271 Selections: offax > 4 arcmin, all EPIC full frame abs (bII) > 20 o , ext_ml > 5 Remaining: 2136 In SDSS DR5 footprint: 867

208 views • 12 slides

Extragalactic AO Science

Extragalactic AO Science. James Larkin AOWG Strategic Planning Meeting September 19, 2004. W M =0.25, W L =0.75, H o =70 km/s/Mpc. 5 kpc. Good Optical/NIR Seeing. 2 kpc. 0.5 kpc. Keck Diffraction Limit @ 1.6 m m. Fundamental motivations.

158 views • 9 slides

Studying extended sources with JEM-X

Studying extended sources with JEM-X. N iels Lund Danish National Space Center. ASCA and JEM-X images of SN 1006. JEM-X 3-4 keV JEM-X 4-8 keV. ASCA 0.4-8 keV. JEM-X imaging of extended sources Coma cluster. 3 to 4 keV 4 to 8 keV.

206 views • 9 slides

Sounding Rocket ? LCAS Mission Candidates

Sounding Rocket ? LCAS Mission Candidates. Technological Advances: Off-plane gratings: being developed for use aboard IXO to achieve high spectral resolution in the soft x-ray bandpass GEM Detectors: a new, inexpensive, large format detector being studied for use aboard future space missions

159 views • 1 slides

The X-ray Universe 2005 26-30 September 2005, El Escorial, Madrid, Spain

The XMM-Newton Slew Survey. The XMM-Newton Slew Survey. ESAC. M.P. Esquej a , R.D. Saxton a , A.M. Read c , B. Altieri a , M.J. Freyberg b , D. Bermejo a , V. Lazaro a a European Space Agency (ESA), European Space Astronomy Centre (ESAC), Villafranca, Apartado 50727, 28080 Madrid, Spain

129 views • 1 slides