WFRF:(Brogna C)
Sökning: WFRF:(Brogna C) > The e-ASTROGAM gamm...
- 10 av 10
- Föregående post
- Nästa post
- Till träfflistan
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 04598naa a2200853 4500 | |
| 001 | oai:DiVA.org:kth-236378 | |
| 003 | SwePub | |
| 008 | 181105s2018 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2363782 URI |
| 024 | 7 | a https://doi.org/10.1117/12.23151512 DOI |
| 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 Tatischeff, V.4 aut |
| 245 | 1 0 | a The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s |
| 264 | 1 | b SPIE - International Society for Optical Engineering,c 2018 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20181105 | |
| 520 | a e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a γ-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the most powerful Galactic and extragalactic sources, elucidating the nature of their relativistic outflows and their effects on the surroundings. With a line sensitivity in the MeV energy range one to two orders of magnitude better than previous and current generation instruments, e-ASTROGAM will determine the origin of key isotopes fundamental for the understanding of supernova explosion and the chemical evolution of our Galaxy. The mission will be a major player of the multiwavelength, multimessenger time-domain astronomy of the 2030s, and provide unique data of significant interest to a broad astronomical community, complementary to powerful observatories such as LISA, LIGO, Virgo, KAGRA, the Einstein Telescope and the Cosmic Explorer, IceCube-Gen2 and KM3NeT, SKA, ALMA, JWST, E-ELT, LSST, Athena, and the Cherenkov Telescope Array. | |
| 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 Compton and pair creation telescope | |
| 653 | a Gamma-ray astronomy | |
| 653 | a gamma-ray polarization | |
| 653 | a high-energy astrophysical phenomena | |
| 653 | a space mission | |
| 653 | a time-domain astronomy | |
| 653 | a Cosmology | |
| 653 | a Observatories | |
| 653 | a Space telescopes | |
| 653 | a Supernovae | |
| 653 | a Astrophysical phenomena | |
| 653 | a Gamma ray polarization | |
| 653 | a Pair creation | |
| 653 | a Space missions | |
| 653 | a Time domain | |
| 653 | a Gamma rays | |
| 700 | 1 | a De Angelis, A.4 aut |
| 700 | 1 | a Tavani, M.4 aut |
| 700 | 1 | a Grenier, I.4 aut |
| 700 | 1 | a Oberlack, U.4 aut |
| 700 | 1 | a Hanlon, L.4 aut |
| 700 | 1 | a Walter, R.4 aut |
| 700 | 1 | a Argan, A.4 aut |
| 700 | 1 | a Von Ballmoos, P.4 aut |
| 700 | 1 | a Bulgarelli, A.4 aut |
| 700 | 1 | a Donnarumma, I.4 aut |
| 700 | 1 | a Hernanz, M.4 aut |
| 700 | 1 | a Kuvvetli, I.4 aut |
| 700 | 1 | a Mallamaci, M.4 aut |
| 700 | 1 | a Pearce, Mark,d 1970-u KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a Zdziarski, A.4 aut |
| 700 | 1 | a Aboudan, A.4 aut |
| 700 | 1 | a Ajello, M.4 aut |
| 700 | 1 | a Ambrosi, G.4 aut |
| 700 | 1 | a Bernard, D.4 aut |
| 700 | 1 | a Bernardini, E.4 aut |
| 700 | 1 | a Bonvicini, V.4 aut |
| 700 | 1 | a Brogna, A.4 aut |
| 700 | 1 | a Branchesi, M.4 aut |
| 700 | 1 | a Budtz-Jorgensen, C.4 aut |
| 700 | 1 | a Bykov, A.4 aut |
| 700 | 1 | a Campana, R.4 aut |
| 700 | 1 | a Cardillo, M.4 aut |
| 700 | 1 | a Marisaldi, Mario4 aut |
| 700 | 1 | a Zoglauer, A.4 aut |
| 710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
| 773 | 0 | t Proceedings of SPIE - The International Society for Optical Engineeringd : SPIE - International Society for Optical Engineeringz 9781510619517 |
| 856 | 4 | u http://spie.org/Publications/Proceedings/Volume/10699y conference |
| 856 | 4 | u https://backend.orbit.dtu.dk/ws/files/153623568/106992J.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-236378 |
| 856 | 4 8 | u https://doi.org/10.1117/12.2315151 |
Hitta via bibliotek
- Proceedings of SPIE - The International Society for Optical Engineering (Sök värdpublikationen i LIBRIS)
Till lärosätets databas
- 10 av 10
- Föregående post
- Nästa post
- Till träfflistan
Hitta mer i SwePub
- Av författaren/redakt...
- Tatischeff, V.
- De Angelis, A.
- Tavani, M.
- Grenier, I.
- Oberlack, U.
- Hanlon, L.
- visa fler...
- Walter, R.
- Argan, A.
- Von Ballmoos, P.
- Bulgarelli, A.
- Donnarumma, I.
- Hernanz, M.
- Kuvvetli, I.
- Mallamaci, M.
- Pearce, Mark, 19 ...
- Zdziarski, A.
- Aboudan, A.
- Ajello, M.
- Ambrosi, G.
- Bernard, D.
- Bernardini, E.
- Bonvicini, V.
- Brogna, A.
- Branchesi, M.
- Budtz-Jorgensen, ...
- Bykov, A.
- Campana, R.
- Cardillo, M.
- Marisaldi, Mario
- Zoglauer, A.
- visa färre...
- Om ämnet
-
- NATURVETENSKAP
- NATURVETENSKAP
- och Fysik
- och Astronomi astrof ...
- Artiklar i publikationen
- Proceedings of S ...
- Av lärosätet
- Kungliga Tekniska Högskolan
Sök utanför SwePub
- Sök vidare i:
- Google Book Search
- Google Scholar
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
- Copyright © LIBRIS - Nationella bibliotekssystem
- LIBRIS.kb.se
