…, G Pelletier, S Pita, G Pühlhofer, M Punch… - Astronomy & …, 2011 - aanda.org Combined HESS gamma-ray spectrum of RX J1713.7−3946 generated from data of 2003, 2004, and 2005 (Data set III, Table 1). Data are corrected for the variation in optical efficiency. Error bars are ± 1σ statistical errors. These data might be described by a power ... Cited by 1 - Related articles - All 3 versions
[PDF] from arxiv.org…, PO Petrucci, S Pita, G Pühlhofer, M Punch… - Physical Review Letters, 2011 - APS A. Abramowski,1 F. Acero,2 F. Aharonian,3,4,5 AG Akhperjanian,5,6 G. Anton,7 A. Barnacka,8,9 U. Barres de Almeida,10 AR Bazer-Bachi,11 Y. Becherini,12,13 J. Becker,14 B. Behera,15 K. Bernlöhr,3,16 A. Bochow,3 C. Boisson,17 J. Bolmont,18 P. Bordas,19 V. ... Cited by 1 - Related articles - All 6 versions
[PDF] from arxiv.org…, JP Lenain, M de Naurois, M Punch… - Arxiv preprint arXiv: …, 2011 - arxiv.org Very-high energy (VHE) emission has been detected from PKS 0447-439 with the HESS Cherenkov telescope array. This blazar is one of the brightest hard-spectrum extragalactic ob- jects in the Fermi bright source list. Its detection with HESS triggered Target of Opportunity ... Related articles - All 4 versions
…, S Pita, G Puehlhofer, M Punch… - Astronomy & …, 2011 - aanda.org The γ-ray pulsar PSR B1706−44 and the adjacent supernova remnant (SNR) candidate G 343.1−2.3 were observed by HESS during a dedicated observation campaign in 2007. As a result of this observation campaign, a new source of very-high-energy (VHE; E > 100 GeV) γ-ray ... Related articles - All 5 versions