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Related papers: Highlights from XMM-Newton

200 papers

NASA's Chandra X-ray Observatory and ESA's XMM-Newton made their first observations one decade ago. The unprecedented and complementary capabilities of these observatories to detect, image, and measure the energy of cosmic X-rays, achieved…

High Energy Astrophysical Phenomena · Physics 2015-07-15 Maria Santos-Lleo , Norbert Schartel , Harvey Tananbaum , Wallace Tucker , Martin C. Weisskopf

The X-ray observatories XMM-Newton and Chandra provided a wealth of exciting new results. Chandra delivered X-ray images of outstanding detail, reaching subarcsecond spatial resolution for the first time in X-ray astronomy. XMM-Newton…

Astrophysics · Physics 2007-05-23 Stefanie Komossa

Within 40 years of the detection of the first extrasolar X-ray source in 1962,NASA's Chandra X-ray Observatory has achieved an increase in sensitivity of 10 orders of magnitude, comparable to the gain in going from naked-eye observations to…

High Energy Astrophysical Phenomena · Physics 2014-06-02 H Tananbaum , M C Weisskopf , W Tucker , B Wilkes , P Edmonds

Significant advances in science always take place when the state of the art in instrumentation improves dramatically. NASA's Chandra X-Ray Observatory represents such an advance. Launched in July of 1999, Chandra is an observatory designed…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 Martin C. Weisskopf

The X-ray Multi-Mirror Mission XMM-Newton is ESA's largest observatory so far; it is dedicated to explore the Universe in the 0.2 - 15 keV X-ray band of the electromagnetic spectrum. Because of its large collecting area very faint sources…

Astrophysics · Physics 2007-05-23 W. Becker , B. Aschenbach

The Chandra X-Ray Observatory (CXO), the x-ray component of NASA's Great Observatories, was launched on 1999, July 23 by the Space Shuttle Columbia. After satellite systems activation, the first x-rays focussed by the telescope were…

Astrophysics · Physics 2008-11-26 M. C. Weisskopf , B. Brinkman , C. Canizares , G. Garmire , S. Murray , L. P. Van Speybroeck

Over the past 13 years, the Chandra X-ray Observatory's ability to provide high resolution X-ray images and spectra have established it as one of the most versatile and powerful tools for astrophysical research in the 21st century. Chandra…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 Martin C. Weisskopf

XMM-Newton, a European Space Agency observatory, has been observing the X-ray, ultra-violet and optical sky for 23 years. During this time, astronomy has evolved from mainly studying single sources to populations and from a single…

In December 2024, the European Space Agency's (ESA) XMM-Newton X-ray Observatory celebrated the 25th anniversary of its launch. The annual number of peer-reviewed articles utilising XMM-Newton data has exhibited a consistent upward…

Instrumentation and Methods for Astrophysics · Physics 2025-11-06 Norbert Schartel , Maria Santos-Lleo

We review X-ray studies of the highest redshift (z > 4) quasars, focusing on recent advances enabled largely by the capabilities of Chandra and XMM-Newton. Included are discussions of basic X-ray population studies, X-ray spectroscopy,…

Astrophysics · Physics 2007-05-23 W. N. Brandt , C. Vignali , X. Fan , S. Kaspi , D. P. Schneider

XMM-Newton has deeply changed our picture of X-ray emission of hot, massive stars. High-resolution X-ray spectroscopy as well as monitoring of these objects helped us gain a deeper insight into the physics of single massive stars with or…

Solar and Stellar Astrophysics · Physics 2017-05-10 Gregor Rauw

ESA's large X-ray space observatory XMM-Newton is in its fifth year of operations. We give a general overview of the status of calibration of the five X-ray instruments and the Optical Monitor. A main point of interest in the last year…

The universe provides numerous extremely interesting astrophysical sources of synchrotron X radiation. The Chandra X-ray Observatory and other X-ray missions provide powerful probes of these and other cosmic X-ray sources. Chandra is the…

Astrophysics · Physics 2007-05-23 Martin C. Weisskopf

XMM-Newton is the direct precursor of the future ESA ATHENA mission. A study of its particle-induced background provides therefore significant insight for the ATHENA mission design. We make use of about 12 years of data, products from the…

The Chandra X-ray Observatory is a mainstay of modern observational astrophysics. With the highest angular resolution of any X-ray facility, its imaging and spectral capabilities in the 0.5-10 keV band have led to both unique and…

High Energy Astrophysical Phenomena · Physics 2025-10-31 Patrick Slane , Ákos Bogdán , David Pooley

Since the launch of Chandra and XMM-Newton, high-resolution X-ray spectra of cosmic sources of all kinds have become available. These spectra have resulted in major scientific breakthroughs. However, due to the techniques used, in general…

High Energy Astrophysical Phenomena · Physics 2017-05-10 J. S. Kaastra

The XMM-OM instrument extends the spectral coverage of the XMM-Newton observatory into the ultraviolet and optical range. It provides imaging and time-resolved data on targets simultaneously with observations in the EPIC and RGS. It also…

Thanks to the large collecting area (3 x ~1500 cm$^2$ at 1.5 keV) and wide field of view (30' across in full field mode) of the X-ray cameras on board the European Space Agency X-ray observatory XMM-Newton, each individual pointing can…

This brief review of recent X-ray observations of young supernova remnants highlights results obtained by the Chandra and XMM Newton Observatories since their launch last year. Their impressive capabilities are illustrated by results for…

Astrophysics · Physics 2009-11-06 Una Hwang

XMM-Newton was launched into space on a highly eccentric 48 hour orbit on December 10th 1999. XMM-Newton is now in its fifth year of operation and has been an outstanding success, observing the Cosmos with imaging, spectroscopy and timing…

Astrophysics · Physics 2009-11-10 S. Sembay , A. Abbey , B. Altieri , R. Ambrosi , D. Baskill , P. Ferrando , K. Mukerjee , A. Read , M. J. L. Turner
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