A dataset provided by the European Space Agency

Proposal ID 0320044
Obs ID 03200440001
Title INTEGRAL identifies the Hard X-ray excess in Blazars fields
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:0320044
DOI https://doi.org/10.57780/esa-iy298ia
Author Wolter
Abstract Thanks to the BeppoSAX satellite unprecedentedly wide energy band, extending up to 200 keV with the PDS instrument, our knowledge of the spectra of blazars has improved substantially. However, the results were limited by the PDS lack of imaging capabilities.In a number of blazars, the PDS detected strong excesses in the 20-100 keV band, with respect to the extrapolation from softer X-ray energies (0.5-10 keV). This implies either a new spectral component or a contaminating source that falls into the field of view of the PDS. We expect that the contaminant sources are mostly known objects that have a yet undiscovered bright emission in the hard X-ray band.With its spatial resolution in the 20-100 keV band, INTEGRAL has the unique capability of disentangling the problem. If the excess is due to the blazar, we will provide new input to our knowledge of the physics of this class of sources. If, instead, there is a serendipitous contaminating source, we will be able to probe the still poorly studied 20-100 keV region and make significant progress in the understanding of the hard X-ray background.
Publications
Temporal Coverage 2006-05-24T11:56:14Z / 2006-06-01T16:21:20Z
Version 1.0
Mission Description The INTEGRAL (International Gamma-Ray Astrophysics Laboratory) mission, launched by the European Space Agency (ESA) on October 17, 2002, was designed to study high-energy phenomena in the universe. INTEGRAL was operating until february 2025 and it was equipped with three high-energy instruments: the Imager on Board the INTEGRAL Satellite (IBIS), the Spectrometer on INTEGRAL (SPI), and the JEM-X (Joint European Monitor for X-rays). Its Optical Monitoring Camera (OMC) provided optical V-band magnitude measurements, complementing the high-energy observations.
Creator Contact https://www.cosmos.esa.int/web/integral/helpdesk
Date Published 2025-03-25T09:54:32Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Wolter, 2025, 'INTEGRAL identifies the Hard X-ray excess in Blazars' fields', 1.0, European Space Agency, https://doi.org/10.57780/esa-iy298ia