Add to ORKGThe Circinus Galaxy has been observed, for the first time above 10 keV, by BeppoSAX. An excess emission above the extrapolation of the best fit 0.1-10keV spectrum is apparent in the PDS data. The most likely explanation is that we are observing the nucleus through a column density of similar to 4 x 10(24) cm(-2), i.e. large enough to completely block the radiation below 10 keV but small enough to permit partial transmission above this energy
The Circinus galaxy is one of the closest obscured active galactic nuclei (AGNs), making it an ideal...
We report on a 300 ks BeppoSAX(0.12-200 keV) observation of Circinus X-1 (CirX-1) at phases between ...
We report on a dramatic flux (50 % increase in the LECS and MECS band) and spectral variation betwee...
The Circinus Galaxy has been observed, for the first time above 10 keV, by BeppoSAX. An excess emiss...
We report Suzaku observations of the active, Compton-thick Circinus galaxy. Observations were obtain...
We report Suzaku observations of the active, Compton-thick Circinus galaxy. Observations were obtain...
We report on a 300 ks BeppoSAX (0.12-200 keV) observation of Circinus X-1 (Cir X-1) at phases betwee...
We report on a 300 ks BeppoSAX (0.12 - 200 keV) observation of Circinus X-1 (Cir X-1) at phases betw...
We report on a 300 ks BeppoSAX (0.12-200 keV) observation of Circinus X-1 (Cir X-1) at phases betwee...
We report on a dramatic flux (similar to 50% increase in the LECS and MECS band) and spectral variat...
We report on the results of a new BeppoSAX (0.12-200 keV) observation of the peculiar X-ray binary s...
We report on the first detection above similar to 10 keV of the archetypal Compton-thick Seyfert 2 g...
The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. Fr...
The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. Fr...
We discuss an accurate measurement of the CXB in the 15-50 keV range performed with the Phoswich Det...
The Circinus galaxy is one of the closest obscured active galactic nuclei (AGNs), making it an ideal...
We report on a 300 ks BeppoSAX(0.12-200 keV) observation of Circinus X-1 (CirX-1) at phases between ...
We report on a dramatic flux (50 % increase in the LECS and MECS band) and spectral variation betwee...
The Circinus Galaxy has been observed, for the first time above 10 keV, by BeppoSAX. An excess emiss...
We report Suzaku observations of the active, Compton-thick Circinus galaxy. Observations were obtain...
We report Suzaku observations of the active, Compton-thick Circinus galaxy. Observations were obtain...
We report on a 300 ks BeppoSAX (0.12-200 keV) observation of Circinus X-1 (Cir X-1) at phases betwee...
We report on a 300 ks BeppoSAX (0.12 - 200 keV) observation of Circinus X-1 (Cir X-1) at phases betw...
We report on a 300 ks BeppoSAX (0.12-200 keV) observation of Circinus X-1 (Cir X-1) at phases betwee...
We report on a dramatic flux (similar to 50% increase in the LECS and MECS band) and spectral variat...
We report on the results of a new BeppoSAX (0.12-200 keV) observation of the peculiar X-ray binary s...
We report on the first detection above similar to 10 keV of the archetypal Compton-thick Seyfert 2 g...
The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. Fr...
The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. Fr...
We discuss an accurate measurement of the CXB in the 15-50 keV range performed with the Phoswich Det...
The Circinus galaxy is one of the closest obscured active galactic nuclei (AGNs), making it an ideal...
We report on a 300 ks BeppoSAX(0.12-200 keV) observation of Circinus X-1 (CirX-1) at phases between ...
We report on a dramatic flux (50 % increase in the LECS and MECS band) and spectral variation betwee...
