Zobrazeno 1 - 10
of 57
pro vyhledávání: '"Heinrich W. Braeuninger"'
Autor:
Giancarlo Parodi, Peter Friedrich, Oberto Citterio, Bernd Aschenbach, Mauro Ghigo, Günther Hasinger, G. Pareschi, Heinrich W. Braeuninger, Francesco Mazzoleni
Publikováno v:
Advances in Space Research. 34:2637-2645
One of the main guidelines for future X-ray astronomy projects like, e.g., XEUS (ESA) and Generation-X (NASA) is to utilize grazing-incidence focusing optics with extremely large telescopes (several tens of m2 at 1 keV), with a dramatic increase in c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::19f82910303b3fd3da6bf73b28c2eeb7
https://doi.org/10.1016/j.asr.2003.03.064
https://doi.org/10.1016/j.asr.2003.03.064
Autor:
Heinrich W. Braeuninger, S. Cebrián, R. Hartmann, A. Rodriquez, J. Franz, Lothar Strueder, R. Kotthaus, Peter Friedrich, D. Kang, Gerhard Lutz, Markus Kuster
The CAST experiment at CERN (European Organization of Nuclear Research) searches for axions from the sun. The axion is a pseudoscalar particle that was motivated by theory thirty years ago, with the intention to solve the strong CP problem. Together
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e542857757f7a02c0659c05b638fb6d2
http://cds.cern.ch/record/876385
http://cds.cern.ch/record/876385
Autor:
Gianpiero Tagliaferri, John A. Nousek, Alan A. Wells, Wolfgang Burkert, M. Capalbi, Sergio Campana, Heinrich W. Braeuninger, Oberto Citterio, A. Moretti, Joanne E. Hill, A. F. Abbey, K. Mukerjee, Paolo Giommi, A. P. Beardmore, David N. Burrows, J. P. Osborne, Lorella Angelini, A. Short, C. Pagani, F. Tamburelli, Guido Chincarini, G. Cusumano, Gisela Hartner, J. A. Kennea
The Swift Gamma-Ray Explorer is designed to make prompt multiwavelength observations of Gamma-Ray Bursts (GRBs) and GRB afterglows. The X-ray Telescope (XRT) enables Swift to determine GRB positions with a few arcseconds accuracy within 100 seconds o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77404dbeb6e0d93120ff5991d9e6accc
Autor:
Norbert Meidinger, Lothar Strueder, Guenther Kettenring, Joachim E. Truemper, Siegfried Mueller, Stefan Bonerz, Robert Hartmann, Heike Soltau, Ulrich G. Briel, H. Hippmann, Gisela Hartner, Eckhard Kendziorra, Peter Predehl, Günther Hasinger, Heinrich W. Braeuninger, Elmar Pfeffermann, W. Kink, Peter Friedrich
Publikováno v:
SPIE Proceedings.
The main scientific objective of the ROSITA mission is to extend the X-ray all-sky survey of ROSAT to higher energies to gain an unbiased sample of all types of celestial X-ray sources in the medium energy band. During this mission the whole sky will
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6ac2cb3248545ccda82b76aec69a66e1
https://doi.org/10.1117/12.461167
https://doi.org/10.1117/12.461167
Autor:
Martin A. Stuebig, Heinrich W. Braeuninger, Jakob Englhauser, Bernd Aschenbach, Norbert Meidinger, Lothar Strueder, Ralf Srama, Robert Hartmann, Joachim E. Truemper, Gisela Hartner, Gerhard Drolshagen
Publikováno v:
SPIE Proceedings.
The pn-CCD is the focal plane detector of one of the three X-ray telescopes aboard the XMM-Newton observatory. During revolution #156 more than 30 individual bright pixels lightened up out of approximately 150,000 pixels of the 6 cm × 6 cm large det
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::04a75de554d06983a9cb73201c98fa3d
https://doi.org/10.1117/12.461154
https://doi.org/10.1117/12.461154
Autor:
N. Krause, Peter Holl, Robert Hartmann, Gerhard Lutz, Jakob Englhauser, Elmar Pfeffermann, R. Eckhardt, Heike Soltau, Norbert Meidinger, Rainer Richter, Heinrich W. Braeuninger, Lothar Strueder, Stefan Bonerz, Joachim E. Truemper, Günther Hasinger
Publikováno v:
SPIE Proceedings.
The pn-CCD was developed as focal plane detector for the XMM-Newton mission and operates successfully for more than 30 months in orbit without performance degradation. In order to match the new requirements of the future ROSITA mission which will per
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::904731e0e2cd2e3833b9290a034f7583
https://doi.org/10.1117/12.461156
https://doi.org/10.1117/12.461156
Autor:
Gerhard Schaller, N. Krause, Stefan Bonerz, D. Carathanassis, Heinrich W. Braeuninger, Lothar Strueder, Norbert Meidinger, Heike Soltau, Rainer Richter, R. Eckhardt, M. Schnecke-Radau, Joachim E. Truemper, Günther Hasinger, Gerhard Lutz, Peter Holl, Robert Hartmann
Publikováno v:
SPIE Proceedings.
The pn-CCD camera on EPIC-XMM is the most advanced imaging X-ray spectrometer, as it combines high quantum efficiency, high speed readout and high energy resolution. The camera operates for almost two years as calibrated prior to launch. Future missi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::33ecc99188a63f92148672ce67e7e143
https://doi.org/10.1117/12.454232
https://doi.org/10.1117/12.454232
Autor:
Giovanni Pareschi, Giancarlo Parodi, Wolfgang Burkert, Mauro Ghigo, Oberto Citterio, Francesco Mazzoleni, Heinrich W. Braeuninger, Gisela Hartner
Publikováno v:
SPIE Proceedings.
In this paper we will review the activities devoted to the development of soft (0.1-10 keV) and hard (10-100 keV) X-ray optics for future astronomical missions that were carried out at the Brera Astronomical Observatory (OAB, Italy) during the last y
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0d1b8d6ba49ff1b6316e20609834259e
https://doi.org/10.1117/12.454370
https://doi.org/10.1117/12.454370
Autor:
Anthony J. Peacock, Marco W. Beijersbergen, Richard Willingale, Marcos Bavdaz, Bernd Aschenbach, Heinrich W. Braeuninger
Publikováno v:
SPIE Proceedings.
The X-ray optics for the X-ray Evolving Universe Spectroscopy Mission (XEUS) have to satisfy the demanding requirements of this ambitious mission. XEUS is under study at the European Space Agency in the frame of the Horizon 2000+ program, utilizing t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a979caf17a731f19c414c9de69a00f2
https://doi.org/10.1117/12.407545
https://doi.org/10.1117/12.407545
Autor:
Lothar Strueder, R. Eckhardt, Gerhard Lutz, Markus Kuster, N. Krause, W. Kink, Christoph von Zanthier, Joachim E. Truemper, A. Viehl, Norbert Meidinger, Heike Soltau, Claus Reppin, S. Krisch, Gisela Hartner, Rainer Richter, Frank Haberl, Diana Stoetter, H. Hippmann, Bernd Aschenbach, S. Kemmer, Heinrich W. Braeuninger, Ulrich G. Briel, D. Hauff, Peter Holl, Robert Hartmann, P. Solc, Elmar Pfeffermann, Josef Kemmer, Konrad Dennerl, Eckhard Kendziorra
Publikováno v:
SPIE Proceedings.
XMM-Newton, the most powerful X-ray telescope ever built was launched from the european space port Kourou on december 10 last year. Three large X-ray Wolter type mirror systems are focusing the incoming X-rays from 100 eV up to 15,000 eV onto the foc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::216f805d27e30e4075d53f842a63a724
https://doi.org/10.1117/12.391614
https://doi.org/10.1117/12.391614