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INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154
DOI: 10.3847/2041-8213/aba2cf Bibcode: 2020ApJ...898L..29M

Tiengo, A.; Sunyaev, R.; Götz, D. +23 more

We report on International Gamma-Ray Astrophysics Laboratory (INTEGRAL) observations of the soft γ-ray repeater SGR 1935+2154 performed between 2020 April 28 and May 3. Several short bursts with fluence of $\sim {10}^{-7}\mbox{--}{10}^{-6}$ erg cm-2 were detected by the Imager on-board INTEGRAL (IBIS) instrument in the 20-200 keV range.…

2020 The Astrophysical Journal
INTEGRAL 320
The Fourth Fermi-GBM Gamma-Ray Burst Catalog: A Decade of Data
DOI: 10.3847/1538-4357/ab7a18 Bibcode: 2020ApJ...893...46V

Meegan, C. A.; von Kienlin, A.; Kocevski, D. +18 more

We present the fourth in a series of catalogs of gamma-ray bursts (GRBs) observed with Fermi's Gamma-ray Burst Monitor (Fermi-GBM). It extends the six year catalog by four more years, now covering the 10 year time period from trigger enabling on 2008 July 12 to 2018 July 11. During this time period GBM triggered almost twice a day on transient eve…

2020 The Astrophysical Journal
INTEGRAL 255
A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy
DOI: 10.3847/2041-8213/ab8cc7 Bibcode: 2020ApJ...895L..23C

Lundqvist, P.; Reichart, D. E.; Kochanek, C. S. +35 more

We present X-ray and radio observations of the Fast Blue Optical Transient CRTS-CSS161010 J045834-081803 (CSS161010 hereafter) at t = 69-531 days. CSS161010 shows luminous X-ray (LX ∼ 5 × 1039 erg s-1) and radio (Lν ∼ 1029 erg s-1 Hz-1) emission. The radio emission peaked…

2020 The Astrophysical Journal
INTEGRAL 101
The Lowest-frequency Fast Radio Bursts: Sardinia Radio Telescope Detection of the Periodic FRB 180916 at 328 MHz
DOI: 10.3847/2041-8213/ab96c0 Bibcode: 2020ApJ...896L..40P

Palazzi, E.; Naletto, G.; Rea, N. +35 more

We report on the lowest-frequency detection to date of three bursts from the fast radio burst FRB 180916.J0158+65, observed at 328 MHz with the Sardinia Radio Telescope (SRT). The SRT observed the periodic repeater FRB 180916.J0158+65 for five days from 2020 February 20 to 24 during a time interval of active radio bursting, and detected the three …

2020 The Astrophysical Journal
INTEGRAL XMM-Newton 79
Gamma-Ray Urgent Archiver for Novel Opportunities (GUANO): Swift/BAT Event Data Dumps on Demand to Enable Sensitive Subthreshold GRB Searches
DOI: 10.3847/1538-4357/aba94f Bibcode: 2020ApJ...900...35T

Cenko, S. Bradley; Palmer, David M.; Barthelmy, Scott +3 more

We introduce a new capability of the Neil Gehrels Swift Observatory to provide event-level data from the Burst Alert Telescope (BAT) on demand in response to transients detected by other instruments. We show that the availability of these data can effectively increase the rate of detections and arcminute localizations of gamma-ray bursts (GRB) lik…

2020 The Astrophysical Journal
INTEGRAL 47
Gamma-Ray Emission of 60Fe and 26Al Radioactivity in Our Galaxy
DOI: 10.3847/1538-4357/ab6336 Bibcode: 2020ApJ...889..169W

Greiner, J.; Wang, W.; Siegert, T. +7 more

The isotopes 60Fe and 26Al originate from massive stars and their supernovae, reflecting ongoing nucleosynthesis in the Galaxy. We studied the gamma-ray emission from these isotopes at characteristic energies 1173, 1332, and 1809 keV with over 15 yr of SPI data, finding a line flux in 60Fe combined lines of $(0.31\…

2020 The Astrophysical Journal
INTEGRAL 42
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background
DOI: 10.3847/1538-4357/ab5aef Bibcode: 2020ApJ...889...17A

Kirkpatrick, Allison; Marchesi, Stefano; Urry, C. Megan +5 more

We constrain X-ray spectral shapes for the ensemble of active galactic nuclei (AGNs) based on the shape of the cosmic X-ray background (CXB). Specifically, we rule out regions of X-ray spectral parameter space that do not reproduce the CXB in the energy range 1-100 keV. The key X-ray spectral parameters are the photon index, Γ; the cutoff energy, …

2020 The Astrophysical Journal
INTEGRAL 19
The Extreme Red Excess in Blazar Ultraviolet Broad Emission Lines
DOI: 10.3847/1538-4357/abb950 Bibcode: 2020ApJ...903...44P

Berton, Marco; Punsly, Brian; Marziani, Paola +1 more

We present a study of quasars with very redward asymmetric (RA) ultraviolet (UV) broad emission lines (BELs). An excess of redshifted emission has been previously shown to occur in the BELs of radio-loud quasars and is most extreme in certain blazars. Paradoxically, blazars are objects that are characterized by a highly relativistic blueshifted ou…

2020 The Astrophysical Journal
INTEGRAL eHST 17
AGILE and Konus-Wind Observations of GRB 190114C: The Remarkable Prompt and Early Afterglow Phases
DOI: 10.3847/1538-4357/abc2d4 Bibcode: 2020ApJ...904..133U

Antonelli, L. A.; Costa, E.; Barbiellini, G. +36 more

GRB 190114C represents a breakthrough for the physics of gamma-ray bursts (GRBs), being the first GRB with delayed emission above 300 GeV, as reported by MAGIC. We present in this paper the sub-MeV/MeV data of the prompt and early afterglow emissions of GRB 190114C, as detected by AGILE and Konus-Wind, in the 20 keV-100 MeV energy range. The first…

2020 The Astrophysical Journal
INTEGRAL 15
2003-2019 Monitoring of the Crab Emission through INTEGRAL SPI, or Vice Versa
DOI: 10.3847/1538-4357/aba8a4 Bibcode: 2020ApJ...899..131J

Jourdain, E.; Roques, J. P.

The Crab Nebula is used by many instruments as a calibration source, in particular at high energy, where it is one of the brightest celestial objects. The spectrometer INTEGRAL SPI (20 keV-8 MeV), in operation since 2002 October, offers a large data set dedicated to this source, with regular campaigns planned twice per year. We have analyzed the a…

2020 The Astrophysical Journal
INTEGRAL 15