-
Article
What Can We Learn about Compton-Thin AGN Tori from Their X-ray Spectra? *
We have developed a Monte Carlo code for simulation of X-ray spectra of active galactic nuclei (AGN) based on a model of a clumpy obscuring torus. Using this code, we investigate the diagnostic power of X-ray ...
-
Article
Detection of large-scale X-ray bubbles in the Milky Way halo
The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation. There is observational evidence of energy injection into the halo...
-
Article
On-ground calibration of the ART-XC/SRG mirror system and detector unit at IKI. Part III
We have performed tests of the SRG project’s ART-XC telescope’s flight spare units of the mirror system (MS) and the URD focal plane X-ray detector. During the tests, the MS was illuminated by a quasi-parallel...
-
Article
On-ground calibration of the ART-XC/SRG mirror system and detector unit at IKI. Part II
We have performed calibration tests of a spare CdTe detector unit of the ART-XC/SRG telescope at the Space Research Institute’s 60-m-long X-ray test facility. During the tests, we illuminated the detector with...
-
Article
On-ground calibration of the ART-XC/SRG mirror system and detector unit at IKI. Part I
From October 2016 to September 2017, we performed tests of the ART-XC /SRG spare mirror system and detector unit at the 60-m-long IKI X-ray test facility. We describe some technical features of this test facil...
-
Article
Calibration of the ART-XC mirror modules at MSFC
The Astronomical Röntgen Telescope X-ray Concentrator (ART-XC) is a hard X-ray telescope with energy response up to 30 keV, to be launched on board the Spectrum Röntgen Gamma (SRG) spacecraft in 2018. ART-XC c...
-
Article
Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J
The detection of 56Co γ-ray emission from the supernova 2014J proves that type Ia supernovae result from a thermonuclear explosion of a carbon–oxygen white dwarf or of a pair of merging white dwarfs.
-
Article
Discrete sources as the origin of the Galactic X-ray ridge emission
An apparently diffuse Galactic ridge of X-ray emission, which appears from Earth to be virtually coincident with the Milky Way disk, has puzzled X-ray astronomers since it was first observed about 25 years ago...
-
Chapter and Conference Paper
Statistics of Local Hard X-Ray Selected AGN: Contribution of Obscured Accretion Onto Supermassive Black Holes
-
Chapter and Conference Paper
Supermassive Black Holes in Elliptical Galaxies: Switching from Very Bright to Very Dim
Relativistic outflows (mainly observed in the radio) are a characteristic feature of both Galactic stellar mass black holes and supermassive black holes (SMBHs). Simultaneous radio and X-ray observations of Ga...
-
Chapter
Annihilation of positrons in the Galaxy
Observations of electron-positron annihilation radiation from the Galactic Center region with the SPI instrument aboard INTEGRAL are summarized. The measured width of the 511 keV line and inferred fraction of ...
-
Article
Annihilation of positrons in the Galaxy
Observations of electron-positron annihilation radiation from the Galactic Center region with the SPI instrument aboard INTEGRAL are summarized. The measured width of the 511 keV line and inferred fraction of ...
-
Chapter
Hard X-Ray and Gamma Ray Spectroscopy
-
Article
Review of GRANAT observations of gamma-ray bursts
The GRANAT observatory was launched into a high apogee orbit on 1 December, 1989. Three instruments onboard GRANAT - PHEBUS, WATCH and SIGMA are able to detect gamma-ray bursts in a very broad energy range fro...