activity
20072015
most citedAn adaptive-binning method for generating constant-uncertainty/constant-significance light curves with Fermi-LAT data

95 citations · 216 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2015★ 10 cited

Fermi-LAT Detection of a Hard Spectrum Flare from the Gravitationally Lensed Blazar B0218+357

S. Buson, C. C. Cheung, S. Larsson +1

The Fermi-LAT has observed new gamma-ray flares from the blazar B0218+357 during July 2014. While no significant change in the gamma-ray spectrum has been previously observed throu…

astro-ph.HE2012★ 95 cited

An adaptive-binning method for generating constant-uncertainty/constant-significance light curves with Fermi-LAT data

B. Lott, L. Escande, S. Larsson +1

We present a method enabling the creation of constant-uncertainty/constant-significance light curves with the data of the Fermi-Large Area Telescope (LAT). The adaptive-binning met…

astro-ph.SR2012

Spin period evolution of the X-ray pulsar GX 1+4

A. González-Galán, E. Kuulkers, P. Kretschmar +4

We report on the long-term evolution of the spin period of the symbiotic X-ray pulsar GX 1+4 and a possible interpretation within a model of quasi-spherical accretion. New period m…

astro-ph.HE2011★ 54 cited

Spin period evolution of GX 1+4

A. González-Galán, E. Kuulkers, P. Kretschmar +4

We aim both to complement the existing data on the spin history of the peculiar accreting X-ray pulsar GX 1+4 with more past and current data from BeppoSAX, INTEGRAL, and Fermi and…

astro-ph.HE2011

The MAGIC view of PG 1553+113

E. Prandini, F. Tavecchio, S. Buson +1

We present the results of five years (2005-2009) of MAGIC observations of the BL Lac object PG 1553+113 at very high energies (VHEs). Adding the new data set (2007-2009) to previou…

astro-ph.HE2011★ 1 cited

Pulse period evolution of GX 1+4

A. González-Galán, E. Kuulkers, P. Kretschmar +4

We report on the long-term evolution of the spin period of the symbiotic X-ray pulsar GX 1+4 and a possible interpretation within a model of quasi-spherical accretion. New period m…