The First Decade of Science with Chandra and XMM-Newton
arXiv:1003.1961 · doi:10.1038/nature08690
Abstract
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 less than 50 years after the first detection of an extra-solar X-ray source, represent an increase in sensitivity comparable in going from naked-eye observations to the most powerful optical telescopes over the past 400 years! In this review, we highlight some of the many discoveries made by Chandra and XMM-Newton that have transformed 21st century astronomy and briefly discuss prospects for future research.
8 pages, 10 figures, published in Nature
References in corpus (32)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- A direct empirical proof of the existence of dark matter
- Heating Hot Atmospheres with Active Galactic Nuclei
- Relativistic X-ray Lines from the Inner Accretion Disks Around Black Holes
- The role of black holes in galaxy formation and evolution
- The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- The Luminosity Function of X-ray Selected Active Galactic Nuclei: Evolution of Supermassive Black Holes at High Redshift
- X-Ray Spectroscopy of Stars
- A Neutron Star with a Carbon Atmosphere in the Cassiopeia A Supernova Remnant
- Discrete sources as the origin of the Galactic X-ray ridge emission
- X-ray Absorption and Reflection in Active Galactic Nuclei
- A Deep Chandra Observation of Kepler's Supernova Remnant: A Type Ia Event with Circumstellar Interaction
- X-rays from solar system objects
- Constraining supernova models using the hot gas in clusters of galaxies
- Million-Degree Plasma Pervading the Extended Orion Nebula
- Spectral Analysis of the Chandra Comet Survey
- Restrictions on parameters of sterile neutrino dark matter from observations of galaxy clusters
- High redshift quasars in the COSMOS survey: the space density of z>3 X-ray selected QSOs
- Beyond the myth of the supernova-remnant origin of cosmic rays
- XMM-Newton observations of the Lockman Hole: X-ray source catalogue and number counts
- A deep X-ray observation of M82 with XMM-Newton
- The X-ray soft excess in classical T Tauri stars
- The Absence of Adiabatic Contraction of the Radial Dark Matter Profile in the Galaxy Cluster A2589
- From discs to planetesimals I: evolution of gas and dust discs
- Latest results on Jovian disk X-rays from XMM-Newton
- The Polar Regions of Cassiopeia A: The Aftermath of a Gamma Ray Burst?
- Chandra LETG Observations of Supernova Remnant 1987A
- X-ray Evolution of SNR 1987A: The Radial Expansion
- The gaseous atmosphere of M87 seen with XMM-Newton
- The Solar Wind Charge-eXchange contribution to the Local Soft X-ray Background. Model to data comparison in the 0.1-1.0 keV band
- The Mass of the Black Hole in the X-ray Binary M33 X-7 and the Evolutionary Status of M33 X-7 and IC 10 X-1
Cited by in corpus (6)
- XMM-Newton (X-Ray Mulit-Mirror Mission) Observatory
- Deep Learning-Based Super-Resolution and De-Noising for XMM-Newton Images
- Classification of 4XMM-DR9 Sources by Machine Learning
- Search for continuous gravitational waves from HESS~J1427-608 with a hidden Markov model
- XMM-Newton
- Space Astronomy for the mid-21st Century: Robotically Maintained Space Telescopes