activity
19962017
most citedThe Fermi Gamma-Ray Burst Monitor

1.6k citations · 2.4k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.CO2017★ 16 cited

Cosmology with XMM galaxy clusters: the X-CLASS/GROND catalogue and photometric redshifts

J. Ridl, N. Clerc, T. Sadibekova +11

The XMM Cluster Archive Super Survey (X-CLASS) is a serendipitously-detected X-ray-selected sample of 845 galaxy clusters based on 2774 XMM archival observations and covering appro…

astro-ph.SR2010★ 27 cited

The absence of sub-minute periodicity in classical T Tauri stars

H. M. Günther, N. Lewandowska, M. P. G. Hundertmark +6

Classical T Tauri stars (CTTS) are young, late-type objects, that still accrete matter from a circumstellar disk. Analytical treatments and numerical simulations predict instabilit…

astro-ph.HE2009★ 10 cited

Centaurus A at Hard X-rays and Soft Gamma-rays

H. Steinle

Centaurus A, at a distance of less than 4 Mpc, is the nearest radio-loud AGN. Its emission is detected from radio to very-high energy gamma-rays. Despite the fact that Cen A is one…

astro-ph.IM2009★ 1.6k cited

The Fermi Gamma-Ray Burst Monitor

Charles Meegan, Giselher Lichti, P. N. Bhat +18

The Gamma-Ray Burst Monitor (GBM) will significantly augment the science return from the Fermi Observatory in the study of Gamma-Ray Bursts (GRBs). The primary objective of GBM is…

astro-ph2008★ 105 cited

Ground-based calibration and characterization of the Fermi Gamma-Ray Burst Monitor Detectors

Elisabetta Bissaldi, Andreas von Kienlin, Giselher G. Lichti +18

One of the scientific objectives of NASA's Fermi Gamma-ray Space Telescope is the study of Gamma-Ray Bursts (GRBs). The Fermi Gamma-Ray Burst Monitor (GBM) was designed to detect a…

astro-ph2007★ 1 cited

Calibration of the GLAST Burst Monitor detectors

Andreas von Kienlin, Elisabetta Bissaldi, Giselher G. Lichti +15

The GLAST Burst Monitor (GBM) will augment the capabilities of GLAST for the detection of cosmic gamma-ray bursts by extending the energy range (20 MeV to > 300 GeV) of the Large A…