INAF IAS_F-Milano

PDF	NEUTRAL PION EMISSION FROM ACCELERATED PROTONS IN 11 nov. 2011 1 INAF-IASF Milano via E. Bassini 15

PDF	Gamma-loud Quasars: A View with BeppoSAX Bassini 15 20133

PDF	The Zoo of X-Ray Sources in the Galactic Center Region 9 janv. 2016 Astro?sica via Celoria 16

PDF	GOLIA: an INTEGRAL archive @INAF-IASF Milano INAF-IASF Milano. The archive comprises all the public data currently available (?8.5 years of data). The data are downloaded from the ISDC and a

PDF	Ultraviolet and Multiwavelength Variability of the Blazar 3C 279 I-20133 Milan Italy. 9 Istituto di Astro–sica Spaziale

PDF	Rapid X-Ray Variability of the BL Lacertae Object PKS 2155–304 I-20133 Milano Italy ; lucio=ifctr.mi.cnr.it. 4 Osservatorio Astronomico di Brera

PDF	Andrea De Luca – curriculum vitae et studiorum (2014 July) Current Current position: Staff researcher INAF/IASF Milano (since 15/06/2011) 12/01/2004: Ph.D. in Astrophysics and Astronomy

PDF	THE REMARKABLE ?-RAY ACTIVITY IN THE GRAVITATIONALLY 7 juil. 2011 14 INAF/IASF–Milano Via E. Bassini 15

PDF	PoS(extremesky2009)085 INAF/IASF- Bologna. Via Gobetti 101 40129 Bologna

PDF	Curriculum Vitae INAF/IASF–Milano INAF/Astronomical Observatory of Cagliari ... Permanent research position at INAF (Italian National Institute for Astrophysics) ...

PDF	NATIONAL INSTITUTE FOR ASTROPHYSICS - iasf-milanoinafit

PDF	As of November 19 2019 - INAF THE ART OF MEASURING GALAXY PHYSICAL PROPERTIES PROGRAM as of November 19 2019 MONDAY 18/11 09:00 - 09:30 REGISTRATION 09:30 - 09:45 WELCOME 09:45 - 10:15 Rachel Somerville (Flatiron Institute)

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NATIONAL INSTITUTE FOR ASTROPHYSICS - iasf-milanoinafit

I-20133 Milano Italia tel: +39 0223699-302 (segreteria) fax +39 022666017 www iasf-milano inaf it 3 • using the Python programming language The following qualifications will be considered a plus: • previous fellowships research grants or other research contracts relevant for the purposes of this call;

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Reduction of soft protons background in Simbol-X effects of

Author(s): A Tiengo SX-INAF-IASFMI-TN-0001 v 0 1 – March 30th 2007 INAF/IASF-MI Simbol-X Technical Note Figure 2:Energy loss (left panel) and corresponding final energy (right panel) for protons passing through the EPIC thick (solid line) and thin (dashed line) filter on board XMM-Newton

PDF	Astronomy https://doiorg/101051/0004-6361/201834022 7 INAF–IASF Milano Via Bassini 15 20133 Milano Italy 8 HH Wills Physics Laboratory Tyndall Avenue Bristol BS8 1TL UK 9 INAF-OAS Osservatorio di Astro?sica e Scienza dello Spazio di Bologna Via Gobetti 93/3 40129 Bologna Italy

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NATIONAL INSTITUTE FOR ASTROPHYSICS - iasf-milanoinafit

I-20133 Milano Italia tel: +39 0223699-302 (segreteria) fax +39 022666017 www iasf-milano inaf it 1 DD 44/2020 Subject: Selection procedure by qualifications and possible interview for the assignment of one post-doc fellowship entitled “STUDY OF STRONGLY MAGNETIZED NEUTRON STARS” NATIONAL INSTITUTE FOR ASTROPHYSICS

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Astronomy https://doiorg/101051/0004-6361/201832972

8 INAF IASF Milano via Bassini 15 20133 Milano Italy 9 Centre for Extragalactic Astronomy Department of Physics Durham University South Road Durham DH1 3LE UK 10 INAF – Astronomical Observatory of Padova 35122 Padova Italy 11 Inter-University Centre for Astronomy and Astrophysics Pune 411007 India

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DART - saxiasf-milanoinafit

INAF IASF Milano Pandora DART manual issue 0 2 DRAFT 12/11/2013 DART (Database Access and Retrieval Tool) An interface to astronomical databases Installation and Administration Manual This manual edited by L Chiappetti & P Franzetti on behalf of the Pandora team INAF - IASF Milano Version 0 2 DRAFT 12/11/2013 17:20 Document history : see table 3

PDF	Quick XXL database help - saxiasf-milanoinafit Quick XXL database help L Chiappetti - INAF IASF Milano - 05 october 2011 How to use this document Go in full screen mode (control-L in acrobat reader) and press return to

PDF	The Woodward effect and the dream of non-newtonian propulsion 5 The Woodward effect Measurable effects need high frequency in energy transfer -> em devices (capacitors at radio frequencies) “When the dielectric of an accelerated capacitor is submitted to a varying

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10 INAF - IASF - Milano Via Bassini 15 20133 Milano Italy 11 Main Astronomical Observatory Academy of Sciences of Ukraine 27 Akademika Zabolotnoho St 03680 Kyiv Ukraine 12 Dipartimento di Fisica e Astronomia Universitá di Bologna via Gobetti 93/2 40129 Bologna Italy

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PDF	1 DD 78/2019 Subject: Selection procedure by - INAF IASF-Milano 20 déc 2019 · www iasf-milano inaf it 1 DD 78/2019 Subject: Selection procedure by qualifications and possible interview for the assignment of one

PDF	NISP Spectroscopic simulations BGarilli (INAF, IASF-Milano) 9 juil 2011 · Consortium NISP Spectroscopic simulations B Garilli (INAF, IASF-Milano) Contributors P Franzetti, E Rossetti, N Roche Other contributors

PDF	Sandro Mereghetti INAF, IASF-‐Milano Sandro Mereghetti INAF, IASF-‐Milano N La Palombara, P Esposito, A Tiengo U Heber, S Geier, W R Hamann G L Israel, L Stella

PDF	Name Institute Country 1 Adami, Christophe LAM FR 2 - cosmos esa CH 59 Gastaldello, Fabio INAF-IASF Milano IT 60 Georgantopoulos, Ioannis National Observatory of Athens GR 61 Ghizzardi, Simona IASF-Milano/INAF IT

PDF	Euclid Space Mission: building the sky survey - Cambridge 8 INAF - IASF Milano, Via E Bassini 15, 20133 Milano, Italy 9 European Space Agency, ESAC, POB 78, 28691 Villanueva de la Canada, Madrid, Spain 10 INAF