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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 03997naa a2200853 4500 | |
| 001 | oai:DiVA.org:kth-81265 | |
| 003 | SwePub | |
| 008 | 120210s2005 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-812652 URI |
| 040 | a (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a kon2 swepub-publicationtype |
| 100 | 1 | a Andersson, V.4 aut |
| 245 | 1 0 | a Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO) |
| 264 | 1 | c 2005 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20120328 | |
| 520 | a We are developing a new balloon-borne instrument (PoGO), to measure polarization of soft gamma rays (30-200 keV) using asymmetry in azimuth angle distribution of Compton scattering. PoGO is designed to detect 10 % polarization in 100mCrab sources in a 6-8 hour observation and bring a new dimension to studies on gamma ray emission/transportation mechanism in pulsars, AGNs, black hole binaries, and neutron star surface. The concept is an adaptation to polarization measurements of well-type phoswich counter consisting of a fast plastic scintillator (the detection part), a slow plastic scintillator (the active collimator) and a BGO scintillator (the bottom anti-counter). PoGO consists of close-packed array of 217 hexagonal well-type phoswich counters and has a narrow field-of-view (~ 5 deg2) to reduce possible source confusion. A prototype instrument has been tested in the polarized soft gamma-ray beams at Advanced Photon Source (ANL) and at Photon Factory (KEK). On the results, the polarization dependence of EGS4 has been validated and that of Geant4 has been corrected. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a Computer simulation | |
| 653 | a Electromagnetic wave polarization | |
| 653 | a Imaging techniques | |
| 653 | a Monte Carlo methods | |
| 653 | a Optimization | |
| 653 | a Orbits | |
| 653 | a Photons | |
| 653 | a Radiation detectors | |
| 653 | a Solar system | |
| 653 | a Synchrotron radiation | |
| 700 | 1 | a Chen, P.4 aut |
| 700 | 1 | a Kamae, T.4 aut |
| 700 | 1 | a Madejski, G.4 aut |
| 700 | 1 | a Mizuno, T.4 aut |
| 700 | 1 | a Ng, J. S. T.4 aut |
| 700 | 1 | a Suhonen, M.4 aut |
| 700 | 1 | a Tajima, H.4 aut |
| 700 | 1 | a Thurston, T.4 aut |
| 700 | 1 | a Bogaert, G.4 aut |
| 700 | 1 | a Fukazawa, Y.4 aut |
| 700 | 1 | a Saito, Y.4 aut |
| 700 | 1 | a Takahashi, T.4 aut |
| 700 | 1 | a Barbier, L.4 aut |
| 700 | 1 | a Bloser, P.4 aut |
| 700 | 1 | a Cline, T.4 aut |
| 700 | 1 | a Harding, A.4 aut |
| 700 | 1 | a Hunter, S.4 aut |
| 700 | 1 | a Krizmanic, J.4 aut |
| 700 | 1 | a Mitchell, J.4 aut |
| 700 | 1 | a Streitmatter, R.4 aut |
| 700 | 1 | a Fernholz, R.4 aut |
| 700 | 1 | a Groth, E.4 aut |
| 700 | 1 | a Marlow, D.4 aut |
| 700 | 1 | a Carlson, Peru KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1ua4u32 |
| 700 | 1 | a Klamra, Wlodzimierzu KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1je1ghu |
| 700 | 1 | a Pearce, Marku KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a Bjornsson, C. -I4 aut |
| 700 | 1 | a Fransson, C.4 aut |
| 700 | 1 | a Larsson, S.4 aut |
| 700 | 1 | a Ryde, Felix,d 1970-u Stockholm University4 aut0 (Swepub:kth)u1tlyg6w |
| 700 | 1 | a Arimoto, M.4 aut |
| 700 | 1 | a Ikagawa, T.4 aut |
| 700 | 1 | a Kanai, Y.4 aut |
| 700 | 1 | a Kataoka, J.4 aut |
| 700 | 1 | a Kawai, N.4 aut |
| 700 | 1 | a Yatsu, Y.4 aut |
| 700 | 1 | a Gunji, S.4 aut |
| 700 | 1 | a Sakurai, H.4 aut |
| 700 | 1 | a Yamashita, Y.4 aut |
| 710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
| 773 | 0 | t Proceedings of the 22nd Texas Symposium on Relativistic Astrophysics at Stanfordg , s. 736-743q <736-743 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-81265 |
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