English PDF version - INFN Sezione di Ferrara
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Surname First name Farinelli Ruben<br />
Curriculum vitae et stu<strong>di</strong>orum<br />
Personal informations<br />
Address via Gramicia 32, I44100, <strong>Ferrara</strong>, Italy<br />
Telephone 0039053297436 Mobile: 00393483397737<br />
Email farinelli@fe.infn.it<br />
Citizenship Italian<br />
Date of birth August, 1, 1975<br />
Mother tongue Italian<br />
Name and address of employer INAFIASFC, via U. La Malfa 153, I90146, Palermo, Italy<br />
Physics Department, <strong>Ferrara</strong> University<br />
via Saragat 1, I44100, <strong>Ferrara</strong>, Italy<br />
Other languages <strong>English</strong>: Excellent level<br />
French: Average level<br />
2011<br />
Position held<br />
Postdoc experience<br />
Non tenuretrack research position on SFXTs at INAFIASFC, Palermo, Italy<br />
20032010 Non tenuretrack research position in High Energy Astrophysics<br />
at the Physics Department of <strong>Ferrara</strong> University, Italy<br />
Main field of research Xray Binaries<br />
Gamma Ray Bursts
Main activities and<br />
responsibilities<br />
Membership<br />
Peerreview activities<br />
Data reduction and analysis of observations performed with<br />
Xray satellites (RXTE, BeppoSAX, INTEGRAL, Swift)<br />
Magnetohydrodynamical simulations of the boundary layer of accretion<br />
<strong>di</strong>sks in Xray binary systems hosting a neutron star or a black hole<br />
using FLASH (joint project with team at UNAM, Mexico)<br />
Ra<strong>di</strong>ative transfer problems in Xray binaries and Gamma Ray Bursts:<br />
theory, numerical solutions and Montecarlo simulations<br />
Development of numerical models for the XSPEC package<br />
CompTB already available at website<br />
http://heasarc.nasa.gov/docs/xanadu/xspec/newmodels.html<br />
Other models<br />
GRBCOMP for prompt emission of Gamma Ray Bursts<br />
(Titarchuk et al. 2011, ApJ submitted, Frontera et al. 2011, in prep.)<br />
COMPMAG for cylindrical accretion onto polar cap of magnetized NS<br />
(Farinelli et al. 2011, in prep.)<br />
Member of the scientific team of the DUAL mission, proposed in response<br />
to the ESA second Cosmic Vision call<br />
Referee of Astronomy & Astrophysics , PASJ and Revista Mexicana de<br />
Astronomia y Astrofisica<br />
Date December 20, 1999<br />
Education and training<br />
Title awarded Graduation in Astronomy at the Bologna University<br />
Title of the thesis Osservazioni con HST del nucleo dell'ammasso globulare NGC 2808<br />
Evaluation 110/110 Cum Laude<br />
Advisor Prof. Pierluigi Battistini<br />
Coadvisors Prof. Flavio Fusi Pecci<br />
Dott. Michele Bellazzini<br />
Date January 29, 2003<br />
Title awarded PhD in Physics at the <strong>Ferrara</strong> University<br />
Title of the thesis Spectral study of Low Mass XRay Binaries with BeppoSAX<br />
Evaluation Very good<br />
Advisor Prof. Filippo Frontera<br />
External committee member Prof. Luigi Stella
Official University Courses<br />
Academic year 2004/05, 2005/06, 2006/07, 2007/08<br />
Faculty Engineering, <strong>Ferrara</strong> University<br />
Position help Contract Professor<br />
Title of the course Numerical applications of Classical Mechanics<br />
Academic year 2005/06<br />
Faculty Pharmacy, <strong>Ferrara</strong> University<br />
Position held Contract Professor<br />
Title of the courses Preliminary Mathematics<br />
Preliminary Physics<br />
Academic year 2007/08<br />
Faculty Physics, <strong>Ferrara</strong> University<br />
Position held Contract Professor<br />
Title of the course High Energy Astrophysics<br />
Students advisor activities at the Physics Department<br />
of the <strong>Ferrara</strong> University<br />
2007/08<br />
2004/05<br />
2002/03<br />
Comptonization in ultrastrong magnetic fields: a theoretical and<br />
numerical approach<br />
Identificazione con INTEGRAL <strong>di</strong> sorgenti seren<strong>di</strong>pity viste con lo<br />
strumento PSD a bordo <strong>di</strong> BeppoSAX<br />
La natura delle binarie X <strong>di</strong> piccola massa ad alta luminosita':<br />
il caso <strong>di</strong> GX 3+1 osservata con INTEGRAL
<strong>Ferrara</strong>, May 2010<br />
Nizza, September 2010<br />
Operating system Linux<br />
Operating system Windows<br />
Lecturer activity to PhD Students<br />
Invited lecture for ICRANet/IRAP PhD<br />
Invited lecture for Erasmus Mundus IRAPPhD<br />
Informatics skills and competences<br />
Highlevel knowledge of the features of Linux, inclu<strong>di</strong>ng hard<strong>di</strong>sk<br />
partitioning, system configuration and upgrades, networking, source<br />
and binary S/W installation, scripting<br />
Highlevel knowledge and managing of the astronomical FITS file format<br />
Highlevel programming with C and Perl languages also using support<br />
from the CFITSIO and Gnu Scientific Library<br />
Astronomical software: FTOOLS, XSPEC, XIMAGE, XRONOS<br />
Graphical tools: IDL, QDP, GIMP, GNUPLOT<br />
Basic knowledge of HTML and Bash<br />
Frequent use of Powerpoint and Word<br />
Joint national and international approved scientific proposals<br />
for funds and satellite observations<br />
2009, PRINMIUR<br />
Gamma Ray Bursts: dai progenitori alla Fisica del processo dell'emissione "prompt"<br />
P.I. Filippo Frontera<br />
2007, PRININAF<br />
Bulk Motion Comptonisation models in Xray binaries: from phenomenology to physics<br />
P.I. Massimo Cocchi
1. INTEGRAL Proposal ID #0830091 (A08) , 2010 (CoPI), Data rights for To0<br />
The evolution of Comptonization in XTE J1701462: from A to Z<br />
2. Chandra Proposal ID # 11400197 (AO11), 2009 (CoPI)<br />
Investigating New Integral Sources with Chandra Observing time: 2 x 20 ksec (ToO)<br />
3. INTEGRAL Proposal ID # (AO7), 2009 (CoPI)<br />
The evolution of Comptonization in XTE J1701462:from A to Z Key Programme Observation<br />
4. Chandra Proposal ID # 11400197 (AO11), 2009 (CoPI)<br />
Investigating New Integral Sources with Chandra Observing time: 2 x 20 ksec (ToO)<br />
5. INTEGRAL Proposal ID # (AO7), 2009 (CoPI)<br />
The evolution of Comptonization in XTE J1701462:from A to Z Key Programme Observation Role: CoPI<br />
6. Chandra Proposal ID # 10400008 (AO10), 2008 (CoPI)<br />
Investigating New Integral Sources with Chandra Observing time: 20 ksec (ToO)<br />
7. INTEGRAL Proposal ID # 0630021 (AO6), 2008 (CoPI)<br />
Hard Xray emission from persistent NS LMXBs in the Galactic Centre Key Programme Observation<br />
8. INTEGRAL Proposal ID # 0633011 (AO6), 2008 (CoPI)<br />
Hard Xray emission from persistent NS LMXBs in the Galactic Disk Key Programme Observation<br />
9. INTEGRAL Proposal ID #0632000 (AO6), 2008 (CoPI) Hard Xray emission from Cyg X2<br />
Key Programme Observation<br />
10. INTEGRAL Proposal ID #0530003 (AO5), 2007 (CoPI)<br />
Hard Xray emission from persistent NS LMXBs Key Programme Observation<br />
11. INTEGRAL Proposal ID #0532004 (AO5), 2007 (CoPI) Hard Xray emission from Cyg X2<br />
Key Programme Observation<br />
12. INTEGRAL Proposal ID #053101 (AO5 Key Programme 2), 2007 (PI)<br />
Searching with INTEGRAL for possible counterparts of unresolved Xray sources observed with<br />
the PDS onboard BeppoSAX North Ecliptic Pole Key Program<br />
13. Chandra Proposal ID #09400414 (AO9), 2007 (CoPI)<br />
Investigating New Integral sorgenti with Chandra Observing time: 20 ksec (ToO)<br />
14. INTEGRAL Proposal ID #0430021 (AO4), 2006 (CoPI)<br />
Hard Xray emission from persistent NS LMXBs Key Programme Observation<br />
15. RXTE Proposal ID #90022, 2004 (CoPI)<br />
Persistent bright LMXBs in the Galactic plane Observing time: 252 ksec<br />
16. RXTE Proposal ID #90022, 2003 (CoPI)<br />
Persistent bright LMXBs in the Galactic plane Observing time: 72 ksec
Oral contributions to international meetings<br />
Meeting place and date Title of the presentation<br />
12th ItalianKorean Symposium on<br />
Relativistic Astrophysics<br />
ICRANETPescara<br />
July 48, 2011<br />
IASFBologna<br />
September 8, 2010<br />
CNOC<br />
Congresso Nazionale Oggetti Compatti<br />
Santa Margherita <strong>di</strong> Pula (CA), Italy<br />
September 2225, 2009<br />
The 12 th Marcel Grossman Meeting<br />
Paris, France<br />
July 1212, 2009<br />
The Xray Universe 2008<br />
Granada, Spain<br />
May 2730, 2008<br />
5 th CNOC<br />
(Congresso Nazionale Oggetti Compatti)<br />
San Vito Lo Capo (TP), Italy<br />
September 1114, 2007<br />
4 th ItalianSino Workshop<br />
International Center for Relativistic<br />
Astrophysics<br />
Pescara, Italy<br />
July 2029, 2007<br />
INTEGRAL Consortium Meeting<br />
INTEGRAL Science Data Center<br />
Geneva, Switzerland<br />
April 1718, 2007<br />
Invited talk<br />
Upscattering spectral formation model for the prompt emission of<br />
Gamma Ray Bursts<br />
Invited talk<br />
On the Xray and gammaray emergent spectrum of super<br />
Ed<strong>di</strong>ngton explosion of very massive stars. Application to spectral<br />
appearances of gammaray bursts<br />
Comptonization in ultrastrong magnetic fields. Numerical<br />
solution of the ra<strong>di</strong>ative transfer equation and application to the<br />
neutron star case<br />
Transition layer in accretion <strong>di</strong>sk around compact objects as origin<br />
of production of hard Xray emission<br />
A new Comptonization model for lowmagnetized accreting<br />
neutron stars in LMXBs<br />
Transition layers around compact objects (black holes and neutron<br />
stars): Evolution of their hydrodynamical structure and size as a<br />
function of the mass accretion rate<br />
Transition layers around compact objects (black holes and neutron<br />
stars): Evolution of their hydrodynamical structure and size as a<br />
function of the mass accretion rate<br />
A new Comptonization model for XSPEC: first results on a sample<br />
of LMXBs
11 th Marcel Grossman meeting on<br />
General Relativity<br />
Berlino, Germany<br />
July 2329, 2006<br />
6 th INTEGRAL Workshop<br />
"The obscured Universe"<br />
Moscow, Russia<br />
July 28, 2006<br />
The multicolored landscape of compact<br />
objects and their explosive origin<br />
Cefalu', Italy<br />
June 1124, 2006<br />
Internal INTEGRAL Science Workshop<br />
ESTEC, The Netherlands<br />
January 1821, 2005<br />
4 th CNOC<br />
(Congresso Nazionale Oggetti Compatti)<br />
Padova, Italy<br />
December 24, 2004<br />
5 th INTEGRAL Workshop<br />
"The INTEGRAL Universe"<br />
Monaco <strong>di</strong> Baviera, Germany<br />
February 1620, 2004<br />
Evolution of Xray spectra of Neutron Star LMXBs: two<br />
blackbodylike components as a signature of NS, accretion <strong>di</strong>sk<br />
and transient hard Xray tails as a Comptonization signature<br />
Average hard Xray emission from neutron star LMXBs: a view<br />
with INTEGRAL<br />
The Xray spectrum of the bursting atoll source 4U 172834<br />
observed with INTEGRAL<br />
Two years of INTEGRAL Core Program observations of the bright<br />
bursting LMXBs GX 3+1: <strong>di</strong>scovery of a variable nonthermal<br />
comptonization component<br />
Long timeaveraged highenergy spectral properties of a sample of<br />
LMXBs observed with INTEGRAL<br />
INTEGRAL observations of four Neutron Star Low mass Xray<br />
Binaries: GX 3+1, GX 3540, GX 349+ and the Rapid Burster
Liceo Classico “Celio”<br />
Rovigo 2005<br />
Liceo Scientifico<br />
“P. Paleocapa” Rovigo<br />
May 5, 2006<br />
Accademia dei Concor<strong>di</strong><br />
Rovigo, December 10 2007<br />
Scientific <strong>di</strong>vulgation<br />
Lectures of General Astronomy<br />
Public conference entitled<br />
Sapere Scientifico e Formazione dello studente europeo<br />
Invited talk<br />
La ricerca scientifica, oggi, nelle esperienze degli ex alunni<br />
del Paleocapa<br />
Celebrations for 20years of the Rovigo Astrophyl Group<br />
Invited talk<br />
L'Universo alle alte energie: storia dell'Astrofisica dei raggi X