A dataset provided by the European Space Agency

Proposal ID 0420021
Obs ID 04200210001
Title Galactic positron annihilation radiation: proving the existence of halo emission 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:0420021
DOI https://doi.org/10.57780/esa-9trc66r
Author Weidenspointner
Abstract We propose to continue and complete our program for observing the sky at intermediate Galactic latitudes above and below the Galactic bulge with the goal of establishing the large-scale spatial distribution of positron annihilation radiation, and in particular of proving the existence of a halo component. The detection of an annihilation halo would constitute a significant break-through for positron astrophysics, with far-reaching implications for origin, diffusion, and annihilation of positrons in our Galaxy.We have published the first sky maps in the 511 keV line (Knoedlseder et al. 2005) and in the positronium continuum (Weidenspointner et al. 2006), which clearly showed that the positron annihilation radiation from our Galaxy is brightest around the Galactic center. The observed emission could not be unambiguously decomposed into bulge, halo, and disk components. But recent analyses suggest more and more strongly the existence of a very extended halo component. We propose to address this issue by observing at intermediate latitudes south of the Galactic center (l=0 deg, b=-25 deg) for 2 Ms, complementing a similar Cycle 3 observation north of the Galactic center (l=0 deg, b=+25 deg). Any 511 keV line emission from these regions - for which there is increasing evidence - is dominated by the halo component. The proposed observations are therefore ideally suited to establish the existence of, or to set stringent limits on, a Galactic halo component. Possible in situ halo positron sources include members of the old stellar population (such as Type Ia supernovae, novae, or low-mass X-ray binaries) or light dark matter.
Publications
Temporal Coverage 2006-10-12T07:03:49Z / 2006-11-11T14:29:18Z
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 2025-03-25T09:54:34Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Weidenspointner, 2025, 'Galactic positron annihilation radiation: proving the existence of halo emission by mid-latitude observations', 1.0, European Space Agency, https://doi.org/10.57780/esa-9trc66r