papers

Publications (30)

astro-ph.CO2011

Ensemble X-ray variability of Active Galactic Nuclei from serendipitous source catalogues

F. Vagnetti, S. Turriziani, D. Trevese

The X-ray variability of the Active Galactic Nuclei (AGN) has been most often investigated with studies of individual, nearby, sources, and only a few ensemble analyses have been a…

astro-ph.IM2012

LOFT: the Large Observatory For X-ray Timing

M. Feroci, J. W. den Herder, E. Bozzo +245

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is curren…

astro-ph.HE2012

A simplified view of blazars: why BL Lacertae is actually a quasar in disguise

P. Padovani, P. Giommi, G. Polenta +3

We put forward a scenario where blazars are classified as flat-spectrum radio quasars, BL Lacs, low synchrotron, or high synchrotron peaked objects according to a varying combinati…

astro-ph.IM2024

EUSO-SPB1 Mission and Science

EUSO Collaboration, G. Abdellaoui, S. Abe +292

The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a N…

astro-ph.CO2010

Variability and the X-ray/UV ratio of Active Galactic Nuclei

F. Vagnetti, S. Turriziani, D. Trevese +1

The observed relation between the X-ray radiation from AGNs, originating in the corona, and the optical/UV radiation from the disk is usually described by the anticorrelation betwe…

astro-ph.IM2019

The EUSO@TurLab: Test of Mini-EUSO Engineering Model

H. Miyamoto, M. Battisti, A. Belov +47

The TurLab facility is a laboratory, equipped with a 5 m diameter and 1 m depth rotating tank, located in the Physics Department of the University of Turin. Originally, it was main…

astro-ph.HE2015

The innermost regions of relativistic jets and their magnetic fields in radio-loud Active Galactic Nuclei

I. Donnarumma, I. Agudo, L. Costamante +17

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT f…

astro-ph.IM2019

Space Debris detection and tracking with the techniques of cosmic ray physics

H. Miyamoto, M. Battisti, A. Belov +45

Space Debris (SD) consist of non-operational artificial objects orbiting around the Earth, which could possibly damage space vehicles, such as the International Space Station (ISS)…

astro-ph.HE2026

Science of High Resolution X-ray Imaging

H. L. Marshall, K. Weaver, M. Schattenburg +34

This report summarizes potential studies of the Hi-ReX Science Analysis Group for an Ultra-High Angular Resolution X-ray Observatory. Many potential science cases are presented, sp…

astro-ph.IM2014

The Large Observatory For x-ray Timing

M. Feroci, J. W. den Herder, E. Bozzo +341

The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final down-selection for a launch slot in 2022-2024. Thanks…

astro-ph.HE2015

Are many radio-selected BL Lacs radio quasars in disguise?

V. D'Elia, P. Padovani, P. Giommi +1

We show that a blazar classification in BL Lacs and Flat Spectrum Radio Quasars may not be adequate when it relies solely on the equivalent widths (EWs) of optical lines. In fact,…

astro-ph.CO2011

A simplified view of blazars: clearing the fog around long-standing selection effects

P. Giommi, P. Padovani, G. Polenta +3

We propose a scenario where blazars are classified as flat-spectrum radio quasars (FSRQs), BL Lacs, low synchrotron, or high synchrotron peaked objects according to a varying mix o…

astro-ph.IM2019

Mini-EUSO data acquisition and control software

F. Capel, A. Belov, G. Cambiè +6

We present the data acquisition and control software for the operation of the Mini-Extreme Universe Space Observatory (EUSO), a space-based fluorescence telescope for the observati…

astro-ph.HE2026

JEM-EUSO Collaboration contributions to the 37th International Cosmic Ray Conference

G. Abdellaoui, S. Abe, J. H. Adams +289

Compilation of papers presented by the JEM-EUSO Collaboration at the 37th International Cosmic Ray Conference (ICRC), held on July 12-23, 2021 (online) in Berlin, Germany.

physics.gen-ph2009

1st Roman Young Researchers Meeting Proceedings

E. Cannuccia, M. Migliaccio, D. Pietrobon +29

During the last few decades scientists have been able to test the bases of the physics paradigms, where the quantum mechanics has to match the cosmological scales. Between the extr…

astro-ph.HE2020

The Open Universe survey of Swift-XRT GRB fields: a complete sample of HBL blazars

P. Giommi, Y. L. Chang, S. Turriziani +22

We have analysed all the X-ray images centred on Gamma Ray Bursts generated by Swift over the last 15 years using automatic tools that do not require any expertise in X-ray astrono…

astro-ph2007

ROXA: a new multi-frequency selected large sample of blazars with SDSS and 2dF optical spectroscopy

S. Turriziani, E. Cavazzuti, P. Giommi

Context. Although Blazars are a small fraction of the overall AGN population they are expected to be the dominant population of extragalactic sources in the hard X-ray and gamma-ra…

astro-ph.HE2021

X-ray spectra, light-curves and SEDs of blazars frequently observed by Swift

P. Giommi, M. Perri, M. Capalbi +19

Blazars research is one of the hot topics of contemporary extra-galactic astrophysics. That is because these sources are the most abundant type of extra-galactic gamma-ray sources…

astro-ph.IM2021

Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities

P. Rosati, S. Basa, A. W. Blain +37

The proposed THESEUS mission will vastly expand the capabilities to monitor the high-energy sky, and will exploit large samples of gamma-ray bursts to probe the early Universe back…

astro-ph.HE2013

A new insight into the innermost jet regions: probing extreme jet variability with LOFT

I. Donnarumma, A. Tramacere, S. Turriziani +4

Blazars are highly variable sources over timescales that can be as low as minutes. This is the case of the High Energy Peaked BL Lac (HBL) objects showing strong variability in X-r…

astro-ph.IM2020

Mini-EUSO mission to study Earth UV emissions on board the ISS

S. Bacholle, P. Barrillon, M. Battisti +57

Mini-EUSO is a telescope observing the Earth in the ultraviolet band from the International Space Station. It is a part of the JEM-EUSO program, paving the way to future larger mis…

astro-ph.HE2019

Mini-EUSO engineering model: tests in open-sky condition

F. Bisconti, D. Barghini, M. Battisti +45

Mini-EUSO is a UV telescope that will look downwards to the Earth's atmosphere onboard the International Space Station. With the design of the ultra-high energy cosmic ray fluoresc…

astro-ph.HE2019

Open Universe for Blazars: a new generation of astronomical products based on 14 years of Swift-XRT data

P. Giommi, C. H. Brandt, U. Barres de Almeida +14

Open Universe for blazars is a set of high-transparency data products for blazar science, and the tools designed to generate them. Blazar astrophysics is becoming increasingly data…

astro-ph.IM2018

First observations of speed of light tracks by a fluorescence detector looking down on the atmosphere

G. Abdellaoui, S. Abe, J. H. Adams +311

EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^…

astro-ph.IM2021

Time Domain Astronomy with the THESEUS Satellite

S. Mereghetti, S. Balman, M. Caballero-Garcia +74

THESEUS is a medium size space mission of the European Space Agency, currently under evaluation for a possible launch in 2032. Its main objectives are to investigate the early Univ…

astro-ph.HE2019

Contributions to the 36th International Cosmic Ray Conference (ICRC 2019) of the JEM-EUSO Collaboration

G. Abdellaoui, S. Abe, J. H. Adams +309

Compilation of papers presented by the JEM-EUSO Collaboration at the 36th International Cosmic Ray Conference (ICRC), held July 24 through August 1, 2019 in Madison, Wisconsin.

astro-ph.HE2026

PeV neutrons as origin of separated SS433 TeV signals

D. Fargion, P. G. De Sanctis Lucentini, S. Turriziani +2

The SS433, a well-known binary system with an internal black hole, have shown since half a century, an inner (a few year light distances) twin precessing jets spirals. These beams…

astro-ph.IM2019

Mini-EUSO experiment to study UV emission of terrestrial and astrophysical origin onboard of the International Space Station

M. Casolino, M. Battisti, A. Belov +42

Mini-EUSO will observe the Earth in the UV range (300 - 400 nm) offering the opportunity to study a variety of atmospheric events such as Transient Luminous Events (TLEs), meteors…

astro-ph2007

ROXA J081009.9+384757.0: a erg/s blazar with hard X-ray synchrotron peak or a new type of radio loud AGN?

P. Giommi, E. Massaro, P. Padovani +10

We report the discovery of ROXA J081009.9+384757.0 = SDSS J081009.9+384757.0, a z=3.95 blazar with a highly unusual Spectral Energy Distribution (SED). This object was first notice…

astro-ph.CO2013

A multi-epoch spectroscopic study of the BAL quasar APM 08279+5255: I. C IV absorption variability

D. Trevese, F. G. Saturni, F. Vagnetti +3

Broad Absorption Lines indicate gas outflows with velocities from thousands km/s to about 0.2 the speed of light, which may be present in all quasars and may play a major role in t…