A dataset provided by the European Space Agency

Proposal ID 0120133
Obs ID 01201330001
Title Cosmic-Ray Acceleration in SN1006: Synchrotron Radiation and Nonthermal Bremsstrahlung in Hard X-Rays
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:0120133
DOI https://doi.org/10.57780/esa-2uskzc3
Author Reynolds
Abstract We propose a 900 ksec observation of the remnant of the supernova of 1006 AD, the Rosetta Stoneobject for the study of electron acceleration to very high energies. The combination of IBIS and Jem-Xspatial and spectral coverage should allow testing of the hyposthesis that the emission above 3 keVis dominantly synchrotron, and should either detect, or put limits on, a contribution from nonthermalbremsstrahlung. The angular diameter of SN 1006, 30, is large enough that IBIS will have sufficientspatial resolution to perform a simple discrimination on the highest-energy detectable hard X-rays:synchrotron emission should come from two opposing limbs, while bremsstrahlung should have amore uniform ring morphology. Jem-X will resolve SN 1006 with about 10 beams across its diameter,ample to search for a bremsstrahlung contribution and comparable to ASCA resolution at thermalX-ray energies. The energy range of 5 to 50 keV shows the lowest-energy suprathermal cosmic-rayelectrons, through bremsstrahlung, and the highest-energy electrons, through synchrotron radiation.Quantitative inferences from detections or limits can include the efficiency of shock acceleration ofelectrons, the maximum energies to which electrons can be accelerated, and indirect constraintson the mean remnant magnetic field strength. INTEGRAL can make a major contribution to theunderstanding of nonthermal emission from this important object, and through it, to the understandingof acceleration of particles at shocks anywhere in astrophysics.
Publications
Temporal Coverage 2003-01-11T17:59:30Z / 2004-01-31T19:47:26Z
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 2026-03-05T13:05:51Z
Keywords INTEGRAL gamma-ray data, ESA INTEGRAL mission dataset, gamma-ray astronomy observations, high-energy astrophysics data, IBIS imaging data, SPI spectrometer data, JEM-X X-ray monitoring data, OMC optical monitoring data, coded mask telescope observations, gamma-ray spectroscopy dataset, MeV astrophysics data, keV–MeV photon observations, gamma-ray burst observations dataset, black hole gamma-ray data, neutron star high-energy observations, positron annihilation 511 keV line data, Galactic Center gamma-ray emission dataset, supernova nucleosynthesis gamma-ray lines, active galactic nuclei high-energy data, transient astrophysical source monitoring, calibrated photon event lists, gamma-ray light curves, high-energy spectra data, sky maps gamma-ray, time-series astrophysical observations, long-term gamma-ray monitoring dataset
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Reynolds, 2026, 'Cosmic-Ray Acceleration in SN1006: Synchrotron Radiation and Nonthermal Bremsstrahlung in Hard X-Rays', 1.0, European Space Agency, https://doi.org/10.57780/esa-2uskzc3