A dataset provided by the European Space Agency

Name: TESTING FOR RELATIVISTIC REFLECTION IN NGC 1052
Published: 2018-03-29T22:00:00Z

Proposal ID	079098
Title	TESTING FOR RELATIVISTIC REFLECTION IN NGC 1052
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790980101
DOI	https://doi.org/10.5270/esa-qcd35aj
Principal Investigator, PI	Dr Elizabeth Rivers
Abstract	We propose a 60 ks NuSTAR observation of NGC 1052 with simultaneous XMM-Newtoncoverage in order to accurately model the reflection features in this source.NGC 1052 is a LINER with a low Eddington rate that has shown hints of a broad FeKa line but no Compton reflection hump in the past. A short NuSTAR observationof the source, indicated that there may indeed be Compton reflection in thissource and a harder continuum than previously thought. Unfortunately, lack ofstatistics and low resolution in the Fe K bandpass of the current data negatethe possibility of a robust measurement. A longer broadband observation willallow us to robustly measure the reflection signatures and simultaneous XMMcoverage will allow us to carefully and consistently test for relativistic reflection.
Publications	The inner view of NGC 1052 using multiple X-ray observations \|Osorio-Clavijo, N., Gonz\\u00e1lez-Mart\\u00edn, O., et al. \| MNRAS \| 491-29 \| 2020 \| 2020MNRAS.491...29O \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491...29O Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Fundamental X-ray corona parameters of Swift/BAT AGN \|Hinkle, Jason T., Mushotzky, Richard, \| MNRAS \| 506-4960 \| 2021 \| 2021MNRAS.506.4960H \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.4960H Properties of the Obscuring Torus in NGC 1052 from Multiepoch Broadband X-Ray Spectroscopy \|Balokovi\\u0107, M., Cabral, S. E., et al. \| ApJ \| 916-90 \| 2021 \| 2021ApJ...916...90B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916...90B Spectral variability in NGC 1042 ULX1 \|Ghosh, Tanuman, Rana, Vikram, \| MNRAS \| 517-4247 \| 2022 \| 2022MNRAS.517.4247G \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.4247G Constraining the X-ray reflection in low accretion-rate active galactic nuclei using XMM-Newton, NuSTAR, and Swift \|Diaz, Y., Hern\\u00e0ndez-Garc\\u00eda, L., et al. \| A&A \| 669-114 \| 2023 \| 2023A&A...669A.114D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.114D Coronal properties of low-accreting AGNs using Swift, XMM-Newton, and NuSTAR observations \|Jana, Arghajit, Chatterjee, Arka, et al. \| MNRAS \| 524-4670 \| 2023 \| 2023MNRAS.524.4670J \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.4670J The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-01-17T02:05:31Z/2017-01-17T21:40:31Z
Version	17.56_20190403_1200
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2018-03-29T22:00:00Z
Keywords	"NuSTAR", "xmm newton coverage", "low eddington rate", "compton reflection", "XMM", "data negate", "robust measurement", "harder continuum", "short nustar", "NGC 1052", "relativistic reflection", "XMM-Newton", "ngc 1052", "xmm coverage", "low resolution", "compton reflection hump", "reflection signatures"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elizabeth Rivers, 2018, 'TESTING FOR RELATIVISTIC REFLECTION IN NGC 1052', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qcd35aj