A dataset provided by the European Space Agency

Proposal ID 0870004
Obs ID 08700040001, 08700040002
Title Observing SN2011fe with INTEGRAL
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:0870004
DOI https://doi.org/10.57780/esa-pxr7uuu
Author Public
Abstract This observation targets SN2011fe which occurred on 23 August 2011 in the nearby galaxy M101 at 6.4 Mpc distance, aiming at high energy emission from 56Co decay gamma-ray lines and its associated Compton-scattered continuum. The prospected emission maximum from the 56Co lines should be ~early November. These ToO observations target the rise of such emission towards this maximum, which is expected to show characteristic differences for different progenitor and explosion models. Observations are in standard dither mode for broader usage of these public data, andcomplement another proprietary ToO on SN2011fe as was proposed for AO-8 and is scheduled in the first weeks after explosion and at expected gamma-ray maximum.
Publications
Temporal Coverage 2011-10-07T18:10:17Z / 2011-11-06T05:23:33Z
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 2025-03-25T09:54:36Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Public, 2025, 'Observing SN2011fe with INTEGRAL', 1.0, European Space Agency, https://doi.org/10.57780/esa-pxr7uuu