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Suzaku and SWIFT-BAT observations of a newly discovered Compton-thick AGN
The X-ray variability history of Markarian 3
Swift discovery of the orbital period of the high mass X-ray binary IGR J015712−7259 in the Small Magellanic Cloud
The Palermo Swift-BAT hard X-ray catalogue
The populations of hard X-ray and γ-ray sources: a correlation study and new possible identifications
The Palermo Swift-BAT hard X-ray catalogue
The Swift-BAT survey reveals the orbital period of three high-mass X-ray binaries
The 54-day orbital period of AX J1820.5-1434 unveiled by Swift
Monitoring supergiant fast X-ray transients with Swift: results from the first year
The Swift gamma-ray burst GRB 050422
New flaring of an ultraluminous X-ray source in NGC 1365
The Swift-BAT hard X-ray sky monitoring unveils the orbital periodof the HMXB IGR J16493-4348
GRB 050505: a high-redshift burst discovered by Swift
Variability and spectral energy distributions of low-luminosity active galactic nuclei: a simultaneous X-ray/UV look with Swift
Detection of an orbital period in the supergiant high-mass X-ray binary IGR J16465-4507 with Swift-BAT
Multiple flaring activity in the supergiant fast X-ray transient IGR J08408−4503 observed with Swift
Swift/XRT monitoring of the supergiant fast X-ray transient IGR J18483−0311 for an entire orbital period
The Palermo Swift-BAT hard X-ray catalogue
First detection of the Crab Nebula at TeV energies with a Cherenkov telescope in a dual-mirror Schwarzschild-Couder configuration: the ASTRI-Horn telescope
Swift-XRT six-year monitoring of the ultraluminous X-ray source M33 X-8
A search for Galactic transients disguised as gamma-ray bursts
The blazar content in the Swift-BAT hard X-ray sky
The broad-band X-ray spectrum of the Seyfert 1 galaxy, MCG+8-11-11
Evidence for a resonant cyclotron line in IGR J16493−4348 from the Swift-BAT hard X-ray survey
Swift follow-up observations of unclassified ASCA sources
Timing accuracy of the Swift X-Ray Telescope in WT mode
NuSTAR reveals that the heavily obscured nucleus of NGC 2785 was the contaminant of IRAS 09104+4109 in the BeppoSAX/PDS hard X-rays
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