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Project contact: Mark Pearce.

Brief overview

Left: An overview of the PoGOLite gondola. The polarimeter is the cylindrical object in the centre and is shown in more detail in the right-hand figure (approximately 1 metre long). A one million cubic metre stratospheric balloon connects to the top of the gondola and will lift PoGOLite to an operational altitude of 40 km.


The light-weight Polarized Gamma-ray Observer (PoGOLite) experiment is designed to measure the polarization of soft gamma rays in the 25 keV- 80 keV energy range. Polarized gamma rays are expected from a wide variety of sources including rotation-powered pulsars, accreting black holes and neutron stars, and jet-dominated active galaxies. Polarization has never been measured at soft gamma-ray energies where non-thermal processes are likely to produce high degrees of polarization. The polarization is derived from the azimuthal distribution of Compton scattering angles in the sensitive volume of the instrument. The scattering angle will be measured by detecting coincident Compton scattering and photo-absorption sites in an array of 217 phoswich detectors. Polarization measurement requires high purity coincident signal detection. PoGOLite applies a well-type Phoswich Detector technology for this purpose. The technology has proven to be very effective in reducing source-confusion and cosmic-ray-induced backgrounds. The PoGOLite experiment is being developed by groups in Japan, Sweden, USA and France. Collaboration homepage.


PoGOLite 'pathfinder' mission: a reduced volume instrument (61 detector units) is scheduled to fly from Esrange, northern Sweden in August 2010.

Thanks to an initiative by PoGOLite team member Magnus Axelsson, PoGOLite was featured on stamps issued by the Swedish post office in January 2009 to mark the International Year of Astronomy!
PoGOLite stamps
The stamps also appeared on the front cover of the 2008 annual report for the School of Engineering Sciences at KTH and in articles in 'Populär Astronomi' and 'Forskning och Framsteg'.

Who's who

From Sweden, the Particle and Astroparticle Physics group within the Physics Department at The Royal Institute of Technology (KTH) and the Astronomy Department at Stockholm University participate. The PoGOLite team consists of:

Seniors: Wlodek Klamra (KTH), Stefan Larsson (KTH/SU), Göran Olofsson (SU), Mark Pearce (KTH), Felix Ryde (KTH).
Postdocs: Magnus Axelsson (SU), Miranda Jackson (KTH).
PhD students: Mózsi Kiss (KTH), Cecilia Marini Bettolo (KTH).
Engineering support: Stefan Rydström (KTH), H-G. Florén (SU), Pau Mallol (KTH)

We collaborate with Nikolay Ivchenko from the KTH Alfvén Lab on studies of X-ray auroral backgrounds.We regularly host Master's students, and their theses are listed below.

Selected publications / talks

Postgraduate Theses

Master's Theses

Funding

Our participation in PoGOLite was made possible through a substantial grant in 2005 from The Knut and Alice Wallenberg Foundation. We receive programmatic support from The Swedish National Space Board, who also fund the pathfinder flight in 2010. The Swedish Research Council (Committee for research infrastructure) funds our work on the attitude control and gondola systems. Several PoGOLite team members receive support ('friköp') from The Swedish Research Council or The Swedish National Space Board. The Göran Gustafsson Foundation is funding work on the star tracker systems.