The 450 days X-ray monitoring of the changing-look AGN 1ES 1927+654
C. Ricci, M. Loewenstein, E. Kara, R. Remillard, B. Trakhtenbrot, I., Arcavi, K. C. Gendreau, Z. Arzoumanian, A. C. Fabian, R. Li, L. C. Ho, C. L., MacLeod, E. Cackett, D. Altamirano, P. Gandhi, P. Kosec, D. Pasham, J., Steiner, C.-H. Chan

TL;DR
This study presents a 450-day X-ray monitoring of the changing-look AGN 1ES 1927+654, revealing unprecedented variability, spectral evolution, and features indicating a new class of changing-look AGN.
Contribution
The paper provides the first extensive X-ray observational campaign of 1ES 1927+654, uncovering unique spectral and variability properties that suggest a new type of changing-look AGN.
Findings
Extreme variability in spectral shape and flux.
Blackbody temperature correlates with luminosity.
Presence of ionized outflows and broad emission features.
Abstract
1ES 1927+654 is a nearby active galactic nucleus (AGN) which underwent a changing-look event in early 2018, developing prominent broad Balmer lines which were absent in previous observations. We have followed up this object in the X-rays with an ongoing campaign that started in May 2018, and that includes 265 NICER (for a total of 678ks) and 14 Swift/XRT (26ks) observations, as well as three simultaneous XMM-Newton/NuSTAR (158/169 ks) exposures. In the X-rays, 1ES 1927+654 shows a behaviour unlike any previously known AGN. The source is extremely variable both in spectral shape and flux, and does not show any correlation between X-ray and UV flux on timescales of hours or weeks/months. After the outburst the power-law component almost completely disappeared, and the source showed an extremely soft continuum dominated by a blackbody component. The temperature of the blackbody increases…
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