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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

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