A dataset provided by the European Space Agency

Proposal ID 0320013
Obs ID 03200130001, 03200130003
Title Galactic positron annihilation radiation: discriminating bulge, halo, and disk components by mid-latitude observations
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:0320013
DOI https://doi.org/10.57780/esa-rs6ujk8
Author Weidenspointner
Abstract Recently, we published the first all-sky map at 511 keV (Knoedlseder et al., 2004), which clearly showed that the positron annihilation radiation from our galaxy is concentrated around the galactic center. The observed emission could not be unambiguously decomposed into bulge, halo, and disk components. We propose to resolve the ambiguity concerning a halo component by observing at intermediate latitudes (b=+/-25deg) North and South of the galactic center for 2*10^6 s each. Any 511 keV line emission from these regions is dominated by the halo component. The proposed observations are therefore ideally suited to establish the existence of, or to setstringent limits on, a galactic halo component. The existence or non-existence of a halo component has far-reaching implications for the annihilation rate and the origin of positrons in our galaxy in general, and in the bulge and disk in particular. Possible halo positron sources are members of the old stellar population (such asType~Ia supernovae, novae, or low-mass X-ray binaries) or light dark matter.
Publications
Temporal Coverage 2006-02-21T00:59:01Z / 2006-08-25T19:54:41Z
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, Weidenspointner, 2025, 'Galactic positron annihilation radiation: discriminating bulge, halo, and disk components by mid-latitude observations', 1.0, European Space Agency, https://doi.org/10.57780/esa-rs6ujk8