... groups of galaxies and their evolution ... Claimed galaxy at z = 10. ... Clusters of Galaxies: Largest Objects in the Universe. courtesy V. Springel MPA ...
XEUS: Future european X-ray observatory to investigate the Early Evolution ... PXD4-Clocked Cleargate. 128x64 pixels. PXD5-Common Cleargate. 128x64 pixels ...
... be spectrally confused in the 6-15' PSFs of XMM, Con-X and XEUS ... Obtain deep X-ray spectra (XMM, Con-X, XEUS) to: confirm spectroscopic identifications ...
... usually in binary. systems with O-B spectral class massive stars. ... Required new generation of X-ray telescopes and observatories: NeXT, Spectrum-XG, XEUS ...
3D Dark Matter maps. Needs X-Ray Selection Criteria. EWOVII = 1 mA = NOVII ... Constellation-X (or XEUS, or dedicated X-Ray WHIM missions) will allow the ...
... [ee]e^e_e`eaebecedeeefegeheiejekelemeneoepeqereseteuevewexeyeze{e|e}e~ee e e e ... DllDddLllTttTllttTddlldttdd8JHv G[XT|tDlbLtjLldTtl|t dY y Tld ...
Kinetic Inductance Detectors SRON Stephen Yates, Jochem Baselmans, Andrey Baryshev, Jan Joost Lankwarden, Henk Hoevers. TNO G. Gerini, A. Neto, D. Bekers.
Max-Planck-Institut f r ... The XMM-Newton/Chandra Era The XMM-Newton ... PowerPoint-Pr sentation Simulation of line profiles for ionized discs PowerPoint ...
Diagnostics used: Bolometry. Zeff from bremsstrahlung. Carbon dynamics ... Compare A B, gap scan at 700 kA. NSTX. XP-950, Monday Physics Meeting (Paul/Gerhardt) ...
Room temperature bolometer. Imaging micro-bolometer array. Works in room temperature ... of sub-mm bolometers. Remote, planetary & atmospheric sensing ...
FIRST EUROPEAN MISSION TO THE MOON. Launch scheduled for 24 March, 2003 ... Potential follow on to ESA's cornerstone X-ray spectroscopy mission (XMM-Newton) ...
The DEPFET Active Pixel Sensor as Vertex Detector for the ILC DEPFET collaboration: Bonn, Mannheim, MPI, Aachen, Prague Vertex Detector at ILC DEPFET Principle
A: XMM-Newton spectrum of NGC 6240. ... Mrk 110 as observed with XMM-Newton. From left to right, ... even for the brightest O VII detection based on XMM-Newton. ...
What are the conditions for life and planetary formation? How does the Solar System work? ... Pulsar velocities: anisotropic neutrino emission from a supernova ...
Cassini-Huygens (ESA, NASA) 1997 - Saturn and the moon Titan mission ... Huygens Probe to Titan, 14.1.2005 - FMI - Oulu U. - in situ meas. - Titan model ...
Hard to discriminate between Ia models, but see extremes Hydra A / M87 ... Similar results in Hydra A. 4. Enrichment by winds. XMM-Newton RGS results ...
Observing galaxy cluster simulations with an X-ray telescope. Elena Rasia ... SIMULATIONS: GADGET/GADGET2 Tree SPH (Springel et al .'01; Springel 05) ...
3. Survey of X-ray Pulsars ... An unprecedently deep X-ray pulsar survey will likely compensate observational ... Sky for Unknown Pulsars or Bursting events ...
Andrew Taylor. Jim Sadlier. Richard Wade. Colin Whitehouse. John Wood ... Facilities (ISIS, SRS, ING, JAC, CLF) Technology (RAL, DL, ATC) Science Programme ...
High Resolution X-Ray/UV Spectroscopy of the Intergalactic Medium: Hunting and Modeling the Missing Baryons in the WHIM Fabrizio Nicastro (Harvard-Smithsonian Center ...
A reflection component from the disc potentially could explain both the positive ... years, many examples of disc reflection from BH binaries have been detected ...
The baseline design of the Imaging X-ray ex.: tech. break-through in oder to achieve 1 eV ... and integrate cryogenic imaging X-ray detectors and read-out ...
Studio Astrofisica delle Alte Energie-Missioni-Roma January ... PHAROS. INAF-OAMP. 13.515,68. 13.515,68. HXMT. INAF-IASF-BO. 23.054,83. 23.054,83. 1.443.390,67 ...
The observed baryons are only 10-40% of the expected valued from big-bang nucleosynthesis. ... baryon candidate. X-ray will be a window to the missing baryon. ...
Cranfield Space Research Centre staff teach and research in a wide range of ... Control of Collocated Geostationary Satellites (S.Hardacre, PhD, 1996) ...
Interpretation: AGN obscured at their birth (Fabian 1998, Hopkins 06) Number of C-thick AGN: largely unknown but see talks by Fabian & Comastri. 2-3:1. 4:1 ...
Contrairement la grande majorit des astres qui rayonnent dans une troite ... G n ration actuelle : CCD. D veloppements futurs : r seau de micro calorim tres. ...
Brief History of X-ray Astronomy. Instrumentation and the X-ray missions ... Background Isotropy. Difference between X-ray and optical surveys. The HDF (optical) ...