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BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog
DOI: 10.3847/1538-4365/aa96ad Bibcode: 2017ApJS..233...17R

Treister, E.; Bauer, F. E.; Paltani, S. +18 more

Hard X-ray (≥10 keV) observations of active galactic nuclei (AGNs) can shed light on some of the most obscured episodes of accretion onto supermassive black holes. The 70-month Swift/BAT all-sky survey, which probes the 14-195 keV energy range, has currently detected 838 AGNs. We report here on the broadband X-ray (0.3-150 keV) characteristics of …

2017 The Astrophysical Journal Supplement Series
AKARI Suzaku XMM-Newton 425
IACHEC Cross-calibration of Chandra, NuSTAR, Swift, Suzaku, XMM-Newton with 3C 273 and PKS 2155-304
DOI: 10.3847/1538-3881/153/1/2 Bibcode: 2017AJ....153....2M

Miller, Eric D.; Guainazzi, Matteo; Madsen, Kristin K. +5 more

On behalf of the International Astronomical Consortium for High Energy Calibration, we present results from the cross-calibration campaigns in 2012 on 3C 273 and in 2013 on PKS 2155-304 between the then active X-ray observatories Chandra, NuSTAR, Suzaku, Swift, and XMM-Newton. We compare measured fluxes between instrument pairs in two energy bands…

2017 The Astronomical Journal
Suzaku XMM-Newton 117
The XMM cluster outskirts project (X‑ COP )
DOI: 10.1002/asna.201713345 Bibcode: 2017AN....338..293E

Pointecouteau, E.; Paltani, S.; Molendi, S. +3 more

Galaxy clusters are thought to grow hierarchically through the continuous merging and accretion of smaller structures across cosmic time. In the local Universe, these phenomena are still active in the outer regions of massive clusters ($R>R_{500}$), where the matter distribution is expected to become clumpy and asymmetric because of the presenc…

2017 Astronomische Nachrichten
Planck Suzaku XMM-Newton 95
Witnessing the growth of the nearest galaxy cluster: thermodynamics of the Virgo Cluster outskirts
DOI: 10.1093/mnras/stx919 Bibcode: 2017MNRAS.469.1476S

Simionescu, A.; Allen, S. W.; Werner, N. +2 more

We present results from Suzaku Key Project observations of the Virgo Cluster, the nearest galaxy cluster to us, mapping its X-ray properties along four long 'arms' extending beyond the virial radius. The entropy profiles along all four azimuths increase with radius, then level out beyond ∼0.5r200, while the average pressure at large rad…

2017 Monthly Notices of the Royal Astronomical Society
Planck Suzaku 79
A uniform metallicity in the outskirts of massive, nearby galaxy clusters
DOI: 10.1093/mnras/stx1542 Bibcode: 2017MNRAS.470.4583U

Simionescu, A.; Allen, S. W.; Werner, N. +2 more

Suzaku measurements of a homogeneous metal distribution of Z ∼ 0.3 Solar in the outskirts of the nearby Perseus cluster suggest that chemical elements were deposited and mixed into the intergalactic medium before clusters formed, likely over 10 billion years ago. A key prediction of this early enrichment scenario is that the intracluster medium in…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 77
The high-Eddington NLS1 Ark 564 has the coolest corona
DOI: 10.1093/mnras/stx792 Bibcode: 2017MNRAS.468.3489K

Fabian, A. C.; Reynolds, C. S.; Lohfink, A. +4 more

Ark 564 is an archetypal narrow-line Seyfert 1 that has been well observed in soft X-rays from 0.3-10 keV, revealing a steep spectrum, strong soft excess, iron K emission line and dramatic variability on the order of hours. Because of its very steep spectrum, observations of the source above 10 keV have been sparse. We report here on the first NuS…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 74
Deep LOFAR observations of the merging galaxy cluster CIZA J2242.8+5301
DOI: 10.1093/mnras/stx1645 Bibcode: 2017MNRAS.471.1107H

Brunetti, G.; White, G. J.; Shimwell, T. W. +20 more

Previous studies have shown that CIZA J2242.8+5301 (the 'Sausage' cluster, z = 0.192) is a massive merging galaxy cluster that hosts a radio halo and multiple relics. In this paper, we present deep, high-fidelity, low-frequency images made with the LOw-Frequency Array (LOFAR) between 115.5 and 179 MHz. These images, with a noise of 140 µJy b…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 66
Analysis of NuSTAR and Suzaku observations of Cyg X-1 in the hard state: evidence for a truncated disc geometry
DOI: 10.1093/mnras/stx2283 Bibcode: 2017MNRAS.472.4220B

Parker, Michael; Zdziarski, Andrzej A.; Basak, Rupal +1 more

The geometry of the accretion flow in black hole X-ray binaries in the hard state, in particular the position of the disc inner edge, has been a subject of intense debate in recent years. We address this issue by performing a spectral study of simultaneous observations of Cyg X-1 in the hard state by NuSTAR and Suzaku. The same data were analysed …

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 65
Magnetar Broadband X-Ray Spectra Correlated with Magnetic Fields: Suzaku Archive of SGRs and AXPs Combined with NuSTAR, Swift, and RXTE
DOI: 10.3847/1538-4365/aa6f0a Bibcode: 2017ApJS..231....8E

Enoto, Teruaki; Makishima, Kazuo; Kitaguchi, Takao +7 more

The 1-70 keV persistent spectra of 15 magnetars, observed with Suzaku from 2006 to 2013, were studied as a complete sample. Combined with early NuSTAR observations of four hard X-ray emitters, nine objects showed a hard power-law emission dominating at ≳ 10 keV with the 15-60 keV flux of ∼1-11× {10}-11 erg s-1 cm-2

2017 The Astrophysical Journal Supplement Series
INTEGRAL Suzaku 59
Suzaku observations of the merging galaxy cluster Abell 2255: The northeast radio relic
DOI: 10.1051/0004-6361/201628400 Bibcode: 2017A&A...600A.100A

Zhang, Y. -Y.; Kaastra, J. S.; Fukazawa, Y. +12 more

We present the results of deep 140 ks Suzaku X-ray observations of the north-east (NE) radio relic of the merging galaxy cluster Abell 2255. The temperature structure of Abell 2255 is measured out to 0.9 times the virial radius (1.9 Mpc) in the NE direction for the first time. The Suzaku temperature map of the central region suggests a complex tem…

2017 Astronomy and Astrophysics
Suzaku XMM-Newton 58