Palermo

发表

Palermo, 2008 .

XMM-Newton First-Light Observations of the Hickson Galaxy Group 16

M. Barbera, UK, M. J. L. Turner, 2000, astro-ph/0010612.

Jackson, Prestridge, Palermo, 2007 .

Design of embedded mixed-criticality CONTRol systems under consideration of EXtra-functional properties -Specification of the run-time management infrastructure

Massimo, Giuseppe, William, 2014 .

Multiwavelength study of the very long GRB 020410

M. Feroci, L. Amati, UK, 2004 .

The structure of blue supergiant winds and the accretion in supergiant high-mass X-ray binaries

S. Mereghetti, A. Paizis, Milano, 2009, 0906.3185.

THE CLOSE T TAURI BINARY SYSTEM V4046 Sgr: ROTATIONALLY MODULATED X-RAY EMISSION FROM ACCRETION SHOCKS

Ny, Cambridge, Observatoire de Geneve, 2012, 1204.0964.

LAMP: the long-term accretion monitoring programme of T Tauri stars in Chamaeleon I

Dublin Institute for Advanced Studies, Garching, Palermo, 2012, 1209.0462.

The optical to γ-ray emission of the Crab pulsar: a multicomponent model

Roma, Palermo, Italy., 2006, astro-ph/0607410.

BeppoSAX follow-up search for the X-ray afterglow of GRB970111

A.J.Castro-Tirado, Roma, ESA, 1998 .

HARD X-RAY RADIATION IN THE COMA CLUSTER SPECTRUM

S. Molendi, Milano, G. Matt, 1999 .

XMM-Newton observations of the field of γ-ray burst 980425

Frascati, Hunstville, Palermo, 2003, astro-ph/0304521.

The X-ray spectrum and variability of the Seyfert 2 galaxy NGC 7172

Roma, Palermo, M. Guainazzi, 1998, astro-ph/9803151.

XMM-Newton and INTEGRAL view of the hard state of EXO 1745-248 during its 2015 outburst

Napoli, Amsterdam, Barcelona, 2017, 1703.07389.

An X-ray study of the dipping low mass X-ray binary XB 1323-619

Astronomy, Noordwijk, Palermo, 1999, astro-ph/9909208.

Spectral classification and HR diagram of pre-main sequence stars in NGC 6530 ,,

Palermo, S. Sciortino, G. Micela, 2012, 1209.0898.

The X-ray variability history of Markarian 3

Palermo, V. Parola, INAF-IASF, 2012, 1209.0706.

High energy properties of X-ray sources observed with BeppoSAX

Palermo, E. Palazzi, E. Pian, 1998, astro-ph/9802078.

X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391

Palermo, Italy., G. Micela, 2004, astro-ph/0410099.

INTEGRAL observations of the variability of OAO 1657 415

Bamberg, Esac, Palermo, 2008, 0805.1811.

Multi-wavelength observing of a forming solar-like star

Garching, Grenoble, Palermo, 2009, 0906.4880.

BeppoSAX observation of PSR B1937+21

Bonn, Garching, Manchester, 2003, astro-ph/0310299.

On the Characterization of GJ 504: A Magnetically Active Planet-host Star Observed by the Transiting Exoplanet Survey Satellite (TESS)

Mitaka, Tokyo, Cea, 2022, Astrophysical Journal.

Morphology and Density Structure of Post-CME Current Sheets

Cambridge, Belgium, Zagreb, 2009, 0902.3705.

XMM-Newton observations of the field of γ-ray burst 980425

Frascati, Hunstville, Palermo, 2003, astro-ph/0304521.

Athena charged particle diverter simulations: effects of micro-roughness on proton scattering using Geant4

Brno, Astrophysics, Ceitec, 2022, Astronomical Telescopes + Instrumentation.

BeppoSAX follow-up search for the X-ray afterglow of GRB970111

A.J.Castro-Tirado, Roma, P.Giommi, 1998, astro-ph/9803015.

Multiwavelength study of the very long GRB 020410

Palermo, Utrecht, Madrid, 2004, astro-ph/0403584.

Spectral Variability and Iron Line Emission in the ASCA Observations of the Seyfert 1 Galaxy NGC 4051

Riken, Palermo, Italy., 1996, astro-ph/9610180.

Identification of carbon dioxide in an exoplanet atmosphere

Tucson, Ny, Lunar, 2022, Nature.

The Milagro anticenter hot spots: cosmic rays from the Geminga supernova?

Firenze, Palermo, M. Salvati, 2008, 0802.2181.

Detection of magnetic field in the B2 star $\rho$ Oph A with ESO FORS2

Cambridge, Austria, Palermo, 2017, 1712.00728.

Coronal properties of active G-type stars in different evolutionary phases

Palermo, Italy., A. Maggio, 2005, astro-ph/0501631.

X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391

Palermo, Italy., G. Micela, 2004, astro-ph/0410099.

Spectral Variability and Iron Line Emission in the ASCA Observations of the Seyfert 1 Galaxy NGC 4051

Riken, Palermo, Italy., 1996, astro-ph/9610180.

An X-ray study of the dipping low mass X-ray binary XB 1323-619

Astronomy, Noordwijk, Palermo, 1999, astro-ph/9909208.

The near-IR counterpart of IGR J17480-2446 in Terzan 5

Barcelona, Palermo, Spain., 2012, 1210.8261.

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

Padova, Milano, Palermo, 2022, 2202.11158.

Variability and spectral energy distributions of low-luminosity active galactic nuclei: a simultaneous X-ray/UV look with Swift

Israel, Pisa, Palermo, 2009, 0909.1906.

Detection of barium in the atmospheres of the ultra-hot gas giants WASP-76b and WASP-121b

Observatoire de Geneve, Porto, Portugal, 2022, Astronomy & Astrophysics.

Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope Array

Tokyo, Engineering, India., 2023, The Astrophysical Journal.

The Comptonized X-ray source X1724-308 in the globular cluster Terzan 2

Noordwijk, Palermo, D. Fiume, 1998, astro-ph/9809014.

HARPS-N Solar RVs Are Dominated by Large, Bright Magnetic Regions

F. Bouchy, Edinburgh, C. A. Watson, 2019, The Astrophysical Journal.

Estimating Magnetic Filling Factors from Simultaneous Spectroscopy and Photometry: Disentangling Spots, Plage, and Network

Exeter, Observatoire de Geneve, Padova, 2021, The Astrophysical Journal.

Evidence of nonthermal particles in coronal loops heated impulsively by nanoflares

Greenbelt, Palermo, Montana State University, 2014, Science.

The all-sky PLATO input catalogue

Heidelberg, Laboratoire d'Astrophysique de Marseille, Observatoire de Geneve, 2021, Astronomy & Astrophysics.

Performances of a new generation tracking detector: the MEG II cylindrical drift chamber

Tokyo, Pisa, Roma, 2023, The European Physical Journal C.

The Structure of Stellar Coronae in Active Binary Systems

Palermo, A. Dupree, J. Sanz-Forcada, 2002, astro-ph/0210652.