M. Catone

发表

CHANDRA VIEW OF THE WARM-HOT INTERGALACTIC MEDIUM TOWARD 1ES 1553+113: ABSORPTION-LINE DETECTIONS AND IDENTIFICATIONS. I.

Tucson, Ny, Cambridge, 2012, 1210.7177.

Radio recombination lines from obscured quasars with the SKA

Cambridge, Pisa, Electronics, 2015, 1511.03267.

New Hard-TeV Extreme Blazars Detected with the MAGIC Telescopes

India., Armenia, Munchen, 2019, The Astrophysical Journal Supplement Series.

AX J1910.7+0917: the slowest X-ray pulsar

Moscow, Milano, -INAF, 2017, 1705.01791.

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

Napoli, Amsterdam, Barcelona, 2017, 1703.07389.

X-ray detection of warm ionized matter in the Galactic halo

Cambridge, Columbus, Roma, 2015, 1512.03611.

Stellar Populations in the Galactic Center

H Germany, D. O. Astronomy, Italy., 2013, 1304.6211.

On the RR Lyrae Stars in Globulars. V. The Complete Near-infrared (JHKs) Census of ω Centauri RR Lyrae Variables

European Southern Observatory, Chicago, Chile, 2018, 1802.03578.

Four years of Fermi LAT flare advocate activity

Padova, Roma, Frascati, 2011, 1111.6803.

PAHs urban concentrations maps using support vector machines

M. Catone, Via Fontana Candida, 2017 .

Submitted to The Astrophysical Journal on 29/1/2005 A XMM-Newton View of the Soft Gamma-ray Repeater SGR 1806–20: Long Term Variability in the pre-Super Giant Flare Epoch

UK., M. Feroci, L. Stella, 2005 .

Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves. II. Period–Fourier–Metallicity Relations for First Overtone RR Lyrae

Hilo, Napoli, Spain, 2022, The Astrophysical Journal.

Detailed chemical composition of Galactic Cepheids. A determination of the Galactic abundance gradie

Santiago, Gepi, Garching, 2007, astro-ph/0701499.

SWIFT observations of TeV BL Lacertae objects

Astrophysics, Maryland., Greenbelt, 2006, astro-ph/0611276.

The distance to NGC 5904 (M 5) via the subdwarf main sequence fitting method

Santiago, Roma, Spain., 2004, astro-ph/0403277.

Surface density of dark matter haloes on galactic and cluster scales

Roma, Sp, V. Cardone, 2012, 1212.6797.

ON THE DISTANCE OF THE GLOBULAR CLUSTER M4 (NGC 6121) USING RR LYRAE STARS. I. OPTICAL AND NEAR-INFRARED PERIOD–LUMINOSITY AND PERIOD–WESENHEIT RELATIONS

Carnegie Observatories, Canada, Napoli, 2014, 1411.6826.

Simultaneous XMM-Newton and HST-COS observation of 1H 0419–577 - II. Broadband spectral modeling of a variable Seyfert galaxy

University College London, Dorking, Surrey, 2014, 1401.5614.

Metals in the IGM approaching the re-ionization epoch: results from X-shooter at the VLT

Cambridge, Firenze, A. Cimatti, 2013, 1306.4604.

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

Barcelona, Palermo, Spain., 2012, 1210.8261.

ON THE DISTANCE OF THE MAGELLANIC CLOUDS USING CEPHEID NIR AND OPTICAL–NIR PERIOD–WESENHEIT RELATIONS

European Southern Observatory, Napoli, Munchen, 2012, 1212.4376.

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

Padova, Milano, Palermo, 2022, 2202.11158.

XMM-Newton observation of the deep minimum state of PG 2112+059 - A spectrum dominated by reflection from the accretion disk?

Esac, Noordwijk, Madrid, 2007, 0709.2412.

Spatial and temporal changes in Aniene river basin (Latium,Italy) using landscape metrics and moving window technique

M. Catone, A. Moro, G. Galante, 2009 .

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.

Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations

Astrophysics, Porto, Portugal, 2020, Astronomy & Astrophysics.

On the Use of Field RR Lyrae as Galactic Probes. V. Optical and Radial Velocity Curve Templates

Tokyo, Tx, Austin, 2021, The Astrophysical Journal.

On the Use of Field RR Lyrae as Galactic Probes. II. A New ΔS Calibration to Estimate Their Metallicity

Tokyo, Tx, Austin, 2020, The Astrophysical Journal.

Low-redshift quasars in the SDSS Stripe 82 – II. Associated companion galaxies and signature of star formation

Astronomy, Padova, Milano, 2020, Monthly Notices of the Royal Astronomical Society.

Separation between RR Lyrae and type II Cepheids and their importance for a distance determination: the case of omega Cen

Tokyo, Seattle, Liverpool John Moores University, 2020, Astronomy & Astrophysics.

A long hard look at the minimum state of PG 2112+059 with XMM-Newton

Villafranca del Castillo, Santander, Instituto de Fisica de Cantabria, 2009, 0912.4456.

TELEMEDICINE SYSTEMS: METHODS FOR SAFETY AND QUALITY OF SERVICE ANALYSIS OF SYSTEMS CONNECTED VIA A COMMUNICATION NETWORK

G. L. Amicucci, M. Minichino, E. Ciancamerla, 2008 .

N-body model of magnetic flux tubes reconnecting in the solar atmosphere

Roma, F. Berrilli, G. Consolini, 2016, 1601.07105.

Confirming the Detection of two WHIM Systems along the Line of Sight to 1ES 1553+113

Cambridge, Italy., Ma, 2018, 1811.03498.

Accretion-ejection connection in the young brown dwarf candidate ISO-ChaI 217 ?

Eberhard Karls, L. E. Fermi, M. Catone, 2014 .

Classical Cepheids, what else?

Tokyo, Amsterdam, Roma, 2012, Proceedings of the International Astronomical Union.

Cepheids as distance indicators and stellar tracers

Roma, V. Braga, I. Roma, 2024, The Astronomy and Astrophysics Review.