BAT AGN spectroscopic survey. V. X-ray properties of the Swift/BAT 70-month AGN catalog

C Ricci, B Trakhtenbrot, MJ Koss, Y Ueda… - The Astrophysical …, 2017 - iopscience.iop.org
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 …

The close environments of accreting massive black holes are shaped by radiative feedback

C Ricci, B Trakhtenbrot, MJ Koss, Y Ueda… - Nature, 2017 - nature.com
The majority of the accreting supermassive black holes in the Universe are obscured by
large columns of gas and dust,,. The location and evolution of this obscuring material have …

The third swift burst alert telescope gamma-ray burst catalog

A Lien, T Sakamoto, SD Barthelmy… - The Astrophysical …, 2016 - iopscience.iop.org
ABSTRACT To date, the Burst Alert Telescope (BAT) onboard Swift has detected∼ 1000
gamma-ray bursts (GRBs), of which∼ 360 GRBs have redshift measurements, ranging from …

WATCHDOG: a comprehensive all-sky database of galactic black hole X-ray binaries

BE Tetarenko, GR Sivakoff, CO Heinke… - The Astrophysical …, 2016 - iopscience.iop.org
With the advent of more sensitive all-sky instruments, the transient universe is being probed
in greater depth than ever before. Taking advantage of available resources, we have …

Leptohadronic blazar models applied to the 2014–2015 flare of TXS 0506+ 056

X Rodrigues, S Gao, A Fedynitch… - The Astrophysical …, 2019 - iopscience.iop.org
We investigate whether the emission of neutrinos observed in 2014–2015 from the direction
of the blazar TXS 0506+ 056 can be accommodated with leptohadronic multiwavelength …

NICER and Fermi GBM observations of the first galactic ultraluminous X-ray pulsar Swift J0243. 6+ 6124

CA Wilson-Hodge, C Malacaria, PA Jenke… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract Swift J0243. 6+ 6124 is a newly discovered Galactic Be/X-ray binary, revealed in
late 2017 September in a giant outburst with a peak luminosity of 2× 10 39 (d/7 kpc) 2 erg s …

A state change in the missing link binary pulsar system PSR J1023+ 0038

BW Stappers, AM Archibald, JWT Hessels… - The Astrophysical …, 2014 - iopscience.iop.org
We present radio and γ-ray observations, which, along with concurrent X-ray observations,
reveal that the binary millisecond pulsar (MSP)/low-mass X-ray binary transition system PSR …

MAXI J1820+070 with NuSTAR I. An increase in variability frequency but a stable reflection spectrum: coronal properties and implications for the inner disc in black …

DJK Buisson, AC Fabian, D Barret… - Monthly Notices of …, 2019 - academic.oup.com
ABSTRACT MAXI J1820+ 070 (optical counterpart ASASSN-18ey) is a black hole candidate
discovered through its recent very bright outburst. The low extinction column and long …

Multi-epoch modeling of TXS 0506+ 056 and implications for long-term high-energy neutrino emission

M Petropoulou, K Murase, M Santander… - The Astrophysical …, 2020 - iopscience.iop.org
The IceCube report of as~ 3.5 excess of 13± 5 neutrino events in the direction of the
blazar TXS 0506+ 056 in 2014–2015 and the 2017 detection of a high-energy neutrino …

The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study

KL Page, AP Beardmore, JP Osborne… - Monthly Notices of …, 2022 - academic.oup.com
On 2021 August 8, the recurrent nova RS Ophiuchi (RS Oph) erupted again, after an interval
of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on …