activity
19992026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 39.4k across the 206 of their papers we have counts for

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astro-ph2006

Soft X and Gamma ray emission from TeV sources observed with Swift and INTEGRAL

A. De Rosa, P. Ubertini, A. Bazzano +4

The soft X-ray and soft gamma observations of the new discovered TeV sources by HESS and MAGIC are crucial to discriminate between various emitting scenarios and to fully understan…

astro-ph2005★ 16 cited

Is the INTEGRAL/IBIS source IGR J17204-3554 a gamma-ray emitting galaxy hidden behind the molecular cloud NGC 6334 ?

L. Bassani, A. De Rosa, A. Bazzano +9

We report on the identification of a soft gamma-ray source, IGR J17204-3554, detected with the IBIS imager on board the INTEGRAL satellite. The source has a 20-100 keV flux of ~3x1…

astro-ph2005★ 54 cited

INTEGRAL IGR J18135-1751=HESS J1813-178: A new cosmic high energy accelerator from keV to TeV

P. Ubertini, L. Bassani, A. Malizia +10

We report the discovery of a soft gamma ray source, namely IGR J18135-1751, detected with the IBIS imager on board the INTEGRAL satellite. The source is persistent and has a 20-100…

astro-ph2002★ 357 cited

A long hard look at MCG-6-30-15 with XMM-Newton

A. C. Fabian, S. Vaughan, K. Nandra +6

We present first results from a 325 ks observation of the Seyfert 1 galaxy MCG-6-30-15 with XMM-Newton and BeppoSAX. The strong, broad, skewed iron line is clearly detected and is…

astro-ph2002★ 21 cited

The complex iron line in NGC 7469 observed by BeppoSAX

A. De Rosa, A. C. Fabian, L. Piro

In this letter we present analysis of BeppoSAX data from a long look at the Seyfert 1 galaxy NGC 7469. The presence of a soft excess below 0.8 keV is confirmed by our analysis and…

astro-ph2002★ 37 cited

The BeppoSAX broad-band spectrum and variability of the Seyfert 1 NGC 3783

A. De Rosa, L. Piro, F. Fiore +5

BeppoSAX observed the Seyfert 1 galaxy NGC 3783 for ~ 5 days from 1998 June 6 to 1998 June 10. The average flux during the observation was F(2-10 keV) ~ 6 X 10^{-11} erg cm^-2 s^-1…