| Publications |
- XMM-Newton first-light observations of the Hickson galaxy group 16 |Turner, M. J. L., Reeves, J. N., et al. | A&A | 365-110 | 2001 | 2001A&A...365L.110T | http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.110T
- The detection of diffuse emission in HCG 16 with XMM-Newton |Belsole, E., Sauvageot, J.-L., et al. | A&A | 398-1 | 2003 | 2003A&A...398....1B | http://ui.adsabs.harvard.edu/#abs/2003A&A...398....1B
- An X-ray view of 82 LINERs with Chandra and XMM-Newton data |Gonzalez-Martin, O., Masegosa, J., et al. | A&A | 506-1107 | 2009 | 2009A&A...506.1107G | http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1107G
- The close environments of accreting massive black holes are shaped by radiative feedback |Ricci, Claudio, Trakhtenbrot, Benny, et al. | Natur | 549-488 | 2017 | 2017Natur.549..488R | http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R
- BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation |Trakhtenbrot, Benny, Ricci, Claudio, et al. | MNRAS | 470-800 | 2017 | 2017MNRAS.470..800T | http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T
- BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog |Ricci, C., Trakhtenbrot, B., et al. | ApJS | 233-17 | 2017 | 2017ApJS..233...17R | http://ui.adsabs.harvard.edu/#abs/2017ApJS..233...17R
- Hard X-Ray View of HCG 16 (Arp 318) |Oda, Saeko, Ueda, Yoshihiro, et al. | ApJ | 855-79 | 2018 | 2018ApJ...855...79O | http://ui.adsabs.harvard.edu/#abs/2018ApJ...855...79O
- The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs |Powell, M. C., Cappelluti, N., et al. | ApJ | 858-110 | 2018 | 2018ApJ...858..110P | http://ui.adsabs.harvard.edu/#abs/2018ApJ...858..110P
- Hot corona properties of Swift/BAT-detected AGNs |Wang, Chan, Yu, Li-Ming, et al. | MNRAS | 487-2463 | 2019 | 2019MNRAS.487.2463W | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.2463W
- The properties of the AGN torus as revealed from a set of unbiased NuSTAR observations |Zhao, X., Marchesi, S., et al. | A&A | 650-57 | 2021 | 2021A&A...650A..57Z | http://ui.adsabs.harvard.edu/#abs/2021A&A...650A..57Z
- Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT |Yamada, Satoshi, Ueda, Yoshihiro, et al. | ApJS | 257-61 | 2021 | 2021ApJS..257...61Y | http://ui.adsabs.harvard.edu/#abs/2021ApJS..257...61Y
- Hydrogen column density variability in a sample of local Compton-thin AGN |Torres-Alb\\u00e0, N., Marchesi, S., et al. | A&A | 678-154 | 2023 | 2023A&A...678A.154T | http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.154T
- A Simple Method for Predicting N H Variability in Active Galactic Nuclei |Cox, Isaiah S., Torres-Alb\\u00e0, N\\u00faria, et al. | ApJ | 958-155 | 2023 | 2023ApJ...958..155C | http://ui.adsabs.harvard.edu/#abs/2023ApJ...958..155C
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| Mission Description |
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
