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181.
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SIMBOL-X: a formation flying mission for hard X-rays astrophysics. In: Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, pp. 59000P-1 - 59000P-10 (Eds. Citterio, O.; O'Dell, S. L.). Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, San Diego, CA, USA, August 03, 2005 - August 04, 2005. SPIE - The International Society for Optical Engineering, Bellingham (2005)
182.
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Cluster scaling and its redshift evolution from XMM-Newton. In: EPIC-XMM-Newton Consortium Meeting 5 Years of Science with XMM-Newton, pp. 111 - 113 (Eds. Briel, U. G.; Sembay, S.; Read, A.). EPIC XMM-Newton Consortium Meeting 2005, Schloß Ringberg, Tegernsee, Germany, April 11, 2005 - April 13, 2005. Max-Planck-Institut für extraterrestrische Physik, Garching b. München (2005)
183.
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Insight on the star-formation at high redshift from X-ray observations of clusters of galaxies. In: New Views on the Universe, pp. 133 - 136 (Eds. Celnikier, L.; Giraud-Héraud, Y.; Tran Thanh Van, J.). Vth Rencontres du Vietnam, Hanoi, Vietnam, August 05, 2004 - August 11, 2004. The Gioi Publishers, Vietnam (2005)
184.
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Cluster scaling and its redshift evolution from XMM-Newton. 35th COSPAR Scientific Assembly, Paris, France, July 18, 2004 - July 25, 2004. Clusters of Galaxies: New Insights from XMM-Newton, pp. 622 - 625 (2005)
185.
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New cluster candidates in the extended XMM lockman hole field. 35th COSPAR Scientific Assembly, Paris, France, July 18, 2004 - July 25, 2004. Clusters of Galaxies: New Insights from XMM-Newton, pp. 710 - 714 (2005)
186.
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Comparison of EPIC-pn ground-based and in-orbit calibration measurements. In: EPIC-XMM-Newton Consortium Meeting 5 Years of Science with XMM-Newton, pp. 159 - 167 (Eds. Briel, U. G.; Sembay, S.; Read, A.). EPIC XMM-Newton Consortium Meeting 2005, Schloß Ringberg, Tegernsee, Germany, April 11, 2005 - April 13, 2005. Max-Planck-Institut für extraterrestrische Physik, Garching b. München (2005)
187.
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The nearby ISM and the local bubble model. In: EPIC-XMM-Newton Consortium Meeting 5 Years of Science with XMM-Newton, pp. 21 - 22 (Eds. Briel, U. G.; Sembay, S.; Read, A.). EPIC XMM-Newton Consortium Meeting 2005, Schloß Ringberg, Tegernsee, Germany, April 11, 2005 - April 13, 2005. Max-Planck-Institut für extraterrestrische Physik, Garching b. München (2005)
188.
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Recent results on manufacturing of segmented X-ray mirrors with slumped glass. In: Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, pp. 59000W-1 - 59000W-8 (Eds. Citterio, O.; O'Dell, S. L.). Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, San Diego, CA, USA, August 03, 2005 - August 04, 2005. SPIE - The International Society for Optical Engineering, Bellingham (2005)
189.
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Results from a contamination experiment on the ISS. In: Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, pp. 59000N-1 - 59000N-12 (Eds. Citterio, O.; O'Dell, S. L.). Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, San Diego, CA, USA, August 03, 2005 - August 04, 2005. SPIE - The International Society for Optical Engineering, Bellingham (2005)
190.
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XMM-Newton observations of narrow-line Seyfert 1 galaxies. In: EPIC-XMM-Newton Consortium Meeting 5 Years of Science with XMM-Newton, pp. 85 - 86 (Eds. Briel, U. G.; Sembay, S.; Read, A.). EPIC XMM-Newton Consortium Meeting 2005, Schloß Ringberg, Tegernsee, Germany, April 11, 2005 - April 13, 2005. Max-Planck-Institut für extraterrestrische Physik, Garching b. München (2005)
191.
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A compact setup of fast pnCCDs for exotic atom measurements. In: Physics with ultra slow antiproton beams, pp. 341 - 346 (Eds. Yamazaki, Y.; Wada, M.). Physics with ultra slow antiproton beams, Wako, Japan, March 14, 2005 - March 16, 2005. American Institute of Physics, Melville, N.Y., USA (2005)
192.
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Requirements for a future astronomical data analysis environment. In: Astronomical Data Analysis Software and Systems XIV, pp. 124 - 128 (Eds. Shopbell, P.L.; Britton, M.C.; Ebert, R.). Astronomical Data Analysis Software and Systems XIV, Pasadena, CA, USA, October 24, 2004 - October 27, 2004. Astronomical Society of the Pacific, San Francisco, CA, USA (2005)
193.
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Searching faint and extended sources in the X-ray universe. In: Bayesian Inference and Maximum Entropy Methods in Science and Engineering, pp. 162 - 169 (Eds. Knuth, K.H.; Abbas, A.E.; Morris, R.D.; Castle, J.P.). 25th International Workshop on Bayesian Inference and Maximum Entropy Methods in Science and Engineering (MaxEnt 05), San Jose,CA, August 07, 2005 - August 12, 2005. American Institute of Physics, Melville, N.Y., USA (2005)
194.
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Simulations of X-rays from solar wind charge exchange at Mars: parameter dependence. 35th COSPAR Scientific Assembly, Paris, France, July 18, 2004 - July 25, 2004. Planetary Atmospheres, Ionospheres, and Magnetospheres, pp. 2057 - 2065 (2005)
195.
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The magnificient seven: nearby isolated neutron stars with strong magnetic fields. In: EPIC-XMM-Newton Consortium Meeting 5 Years of Science with XMM-Newton, pp. 39 - 44 (Eds. Briel, U. G.; Sembay, S.; Read, A.). EPIC XMM-Newton Consortium Meeting 2005, Schloß Ringberg, Tegernsee, Germany, April 11, 2005 - April 13, 2005. Max-Planck-Institut für extraterrestrische Physik, Garching b. München (2005)
196.
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Results of a fast pnCCD detector system. In: Astronomical Adaptive Optics Systems and Applications II, pp. 59030N-1 - 59030N-9 (Eds. Tyson, R.K.; Lloyd-Hart, M.). Astronomical Adaptive Optics Systems and Applications II, San Diego, CA, USA, August 03, 2005 - August 04, 2005. Society of Photo-Optical Instrumentation Engineers, Bellingham, Wash., USA (2005)
197.
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Evolution of X-ray selected AGN. In: Multiwavelength mapping of galaxy formation and evolution, pp. 68 - 75 (Ed. Renzini Bender R., A.). ESO Workshop on multiwavelength mapping of galaxy formation and evolution, Venice, Italy, October 13, 2003 - October 16, 2003. Springer, Berlin [et al.] (2005)
198.
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When supermassive black holes were growing: clues form deep X-ray surveys. In: Growing black holes: accretion in a cosmological context, pp. 418 - 431 (Eds. Merloni, A.; Nayakshin, S.; Sunyaev, R. A.). Growing Black Holes: Accretion in a Cosmological Context, Garching, Germany, June 21, 2004 - June 25, 2004. Springer, Berlin (2005)
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28 (3), p. ? - ? (2005)
The GLAST burst monitor instrument response simulation system. 4th Workshop on Gamma-Ray Bursts in the Afterglow Era, Rome, Italy, October 18, 2004 - October 22, 2004. Nuovo Cimento della Societa Italiana di Fisica C - Geophysics and Space Physics 200.
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Gamma-ray absorptions in the SED of QSO. In: High Energy Gamma-Ray Astronomy, pp. 573 - 577 (Eds. Aharonian, F. A.; Völk, H. J.; Horns, D.). 2nd International Symposium on High Energy Gamma-Ray Astronomy, Heidelberg, Germany, July 26, 2004 - July 30, 2004. American Institute of Physics, Melville, NY (2005)