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Istituto Di Radioastronomia Inaf
ISTITUTO DI RADIOASTRONOMIA INAF STATUS REPORT October 2007 http://www.ira.inaf.it/ Chapter 1. STRUCTURE AND ORGANIZATION The Istituto di Radioastronomia (IRA) is presently the only INAF structure with divisions distributed over the national territory. Such an organization came about because IRA was originally a part of the National Council of Research (CNR), which imposed the first of its own reforms in 2001. The transition from CNR to INAF began in 2004 and was completed on January 1st , 2005. The Institute has its headquarters in Bologna in the CNR campus area, and two divisions in Firenze and Noto. The Medicina station belongs to the Bologna headquarters. A fourth division is foreseen in Cagliari at the Sardinia Radiotelescope site. The IRA operates 3 radio telescopes: the Northern Cross Radio Telescope (Medicina), and two 32-m dishes (Medicina and Noto), which are used primarily for Very Long Baseline Interferometry (VLBI) observations. The IRA leads the construction of the Sardinia Radio Telescope (SRT), a 64-m dish of new design. This is one of the INAF large projects nowadays. The aims of the Institute comprise: - the pursuit of excellence in many research areas ranging from observational radio astronomy, both galactic and extragalactic, to cosmology, to geodesy and Earth studies; - the design and management of the Italian radio astronomical facilities; - the design and fabrication of instrumentation operating in bands from radio to infrared and visible. Main activities of the various sites include: Bologna: The headquarters are responsible for the institute management and act as interface with the INAF central headquarters in Roma. Much of the astronomical research is done in Bologna, with major areas in cosmology, extragalactic astrophysics, star formation and geodesy. -
Radio Astronomy Across Europe
Radio astronomy across Europe Wilfred Frieswijk* & ERATec Network Activity [email protected] * ASTRON Netherlands Institute for Radio Astronomy Abstract Europe has a long and outstanding history in radio astronomy. It currently hosts numerous of world-class facilities spread around the globe, some of which well-known, others being less familiar. The map below gives an overview of associated radio observatories accessible for the general astronomical community. Trans-national access (TNA) Capabilities The objectives of the Transnational Access portion of RadioNet3 are ERATec The receivers available on the various • to draw together all of the European radio facilities under one umbrella; The main activity of the RadioNet3 telescopes operate in the radio regime, • to enable the European user community to have easy and transparent European Radio Astronomy Technical covering frequencies from ~10 MHz access to the entire range of facilities; Forum is to organise and support to 1 THz. With dish-sizes ranging • to offer the European user community an integrated, professional and meetings and workshops that help to from ~10 to 100 meters and baselines consistent level of user support. identify synergies and develop up to >1000 kilometers, spatial complementary capabilities at the website: http://www.radionet-eu.org/transnational-access resolutions can be achieved down to observatories, to determine how the sub-arc-second scales, thus matching pooling of resources might lead to those obtained at infrared- and optical Open time common solutions -
EPSC2018-1115-2, 2018 European Planetary Science Congress 2018 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2018
EPSC Abstracts Vol. 12, EPSC2018-1115-2, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 Ultra-short Period Rocky Super-Earths Luca Malavolta (1,2) , Andrew W. Mayo (3,4) , Tom Louden (5) , Vinesh M. Rajpaul (6) , Aldo S. Bonomo (7) , Lars A. Buchhave (4) , Laura Kreidberg (3,8) , Martti H. Kristiansen (9,10), Mercedes Lopez-Morales (3) , Annelies Mortier (11) , Andrew Vanderburg (3,12) , Adrien Coffinet (13), David Ehrenreich (13) , Christophe Lovis (13), Francois Bouchy (13), David Charbonneau (3) , David R. Ciardi (14), Andrew Collier Cameron (11) , Rosario Cosentino (15), Ian J. M. Crossfield (16,17), Mario Damasso (7) , Courtney D. Dressing (18) , Xavier Dumusque(13) , Mark E. Everett (19) , Pedro Figueira (20), Aldo F. M. Fiorenzano (15), Erica J. Gonzales (16,28), Raphaëlle D. Haywood (3,27) , Avet Harutyunyan (15), Lea Hirsch (18) , Steve B. Howell (21) , John Asher Johnson (3) , David W. Latham (3) , Eric Lopez (22), Michel Mayor (13), Giusi Micela (23), Emilio Molinari (15,24) , Valerio Nascimbeni (1,2) , Francesco Pepe (13), David F. Phillips (3) , Giampaolo Piotto (1,2) , Ken Rice (25), Dimitar Sasselov (3) , Damien Ségransan (13) , Alessandro Sozzetti (7) , Stéphane Udry (13), and Chris Watson (26) (1) Dipartimento di Fisica e Astronomia “Galileo Galilei,” Università di Padova, Italy ([email protected]) (2) INAF— Osservatorio Astronomico di Padova, Italy (3) Harvard-Smithsonian Center for Astrophysics, USA (4) Centre for Star and Planet Formation, Denmark (5) Department -
Geographical Distribution of the Italian Astronomical Observatories
Figure 25.1: Geographical distribution of the Italian Astronomical Observatories 226 25. Italian Astronomical Observatories and their Historical Instruments Collections Ileana Chinnici (Palermo, Italy) 25.1 A Brief Historical Introduction made by famous instruments-makers of that time, such as Ramsden, Short, Sisson, etc. while the typical equip- Italy has a high number of astronomical observatories ment of an Italian observatory in the middle of the 19th in comparison with its territorial extension. This is due century consisted of astronomical instruments made by to historical reasons, as Italy results from a political Reichenbach, Fraunhofer, Repsold, Merz and others. process of unification and annexation of several small The ancient observatories, built upon towers or states into which the country was divided – a process palaces in the middle of the cities, have mostly preserved (the Risorgimento) which was carried out mainly around their original building and their historical architecture; th the half of 19 century. a special mention is to be deserved to the Naples Obser- The first “institutional” Observatories in Italy were vatory, located on the hill of the Capodimonte: it was th established in the 18 century, as in the majority of the first architectural complex in Italy specially planned the other European nations. At that time, Italy was and built to be an astronomical observatory; it dates composed by seven states and since 1711 to 1819 each back to 1819, thus preceding the Pulkovo Observatory, of these states established one or two Observatories in established in 1839, which will serve later as architec- its territory. tural model for many observatories all over the world. -
EPSC2018-234, 2018 European Planetary Science Congress 2018 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2018
EPSC Abstracts Vol. 12, EPSC2018-234, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 GAPS: Results from 5 years of observations R. Claudi(1), S. Benatti (1), C. Boccato (1), E. Covino (2), S. Desidera (1), R. Gratton (1), A.F. Lanza (3), A. Maggio (4), G.Micela (4), E. Molinari (5), I. Pagano (3), G. Piotto (6), E. Poretti (7,8), R. Smareglia (9), A. Sozzetti (10), and the GAPS Team (1) INAF - Astronomical Observatory of Padova ([email protected]), (2) INAF - Astronomical Observatory of Capodimonte, (3) INAF - Astrophysical Observatory of Catania, (4) INAF - Astronomical Observatory of Palermo, (5) INAF - Astronomical Observatory of Cagliari, (6) University of Padova, Dep. of Physics and Astronomy, (7) INAF - TNG, Fundación Galileo Galilei, (8) INAF Astronomical Observatory of Brera, Italy, (9) INAF - Astronomical Observatory of Trieste; (10) INAF - Astronomical Observatory of Torino The "Global Architecture of Planetary Systems" the APACHE (Astronomical Observatory of the Au- (GAPS) Project is the result of a collaboration among tonomous Region of the Aosta Valley, [2]) and EXO- part of the Italian exoplanetary community that ex- RAP1 (Serra la Nave Observatory) surveys, from the ploited the great capabilities of the HARPS–N instru- INAF–Astrophysical Observatory of Asiago and by a ment. It gathers more than 60 astronomers from sev- number of amateur astronomers. Thanks to the wide eral institutes of the Italian National Institute for As- expertise of the GAPS members (high-resolution spec- trophysics (INAF) and Italian Universities (Padova, troscopy, stellar activity and pulsations, crowded stel- Torino and Milano). -
A Review of Front-End Receivers for the INAF Radio Telescopes
2nd URSI AT-RASC, Gran Canaria, 28 May – 1 June 2018 A Review of Front-End Receivers for the INAF Radio Telescopes P. Bolli(1), M. Beltrán(1), M. Burgay(2), C. Contavalle(3), P. Marongiu(2), A. Orfei(3), T. Pisanu(2), C. Stanghellini(3), S.J. Tingay(4), G. Zacchiroli(3), and A. Zanichelli(3) (1) INAF – Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy (2) INAF – Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047 Selargius (CA), Italy (3) INAF – Istituto di Radioastronomia, via Piero Gobetti 101, 40129 Bologna, Italy (4) Curtin University – Curtin Institute of Radio Astronomy, 1 Turner Ave, Technology Park, Bentley 6102, Western Australia Abstract facilities was charged to conduct this review. The group provides the authorship for this paper. This paper describes a rigorous process started within the Italian National Institute for Astrophysics (INAF) to The working group interacted with many Italian and review existing and future radio astronomical front-end foreign astronomers and technologists. The two most receivers for the INAF radio telescopes. The main goal of significant examples of this approach have been: i) the the review was to increase the level of coordination in survey of the characteristics of some of the major receiver development, improving at the same time the International radio telescopes to benchmark the scientific impact from the national facilities. The working performance of Italian telescopes against recognized top- group in charge of the review collected information on the class worldwide radio astronomy facilities; ii) the call for front-ends in operation and under development at the INAF ideas addressed to the whole Italian astronomical radio telescopes and new ideas for future receivers from the community to survey scientific interest in the development Italian astronomical community. -
1 the Founding of Arcetri Observatory in Florence
THE FOUNDING OF ARCETRI OBSERVATORY IN FLORENCE Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: The first idea of establishing a public astronomical observatory in Florence, Capital of the Grand Duchy of Tuscany, dates to the mid of the 18th century. Initially, the use of a low building on a high ground was proposed, and the hill of Arcetri suggested as a proper location. At the end of the century, the Florence Observatory - or Specola - was built instead on a tower at the same level as the city’s centre. As soon as astronomers started to use this observatory, they recognized all its flaws and struggled to search for a better location. Giovanni Battista Donati, director of the Specola of Florence from the eve of the Italian Unification in 1859, finally succeeded in creating a new observatory: first, he obtained funds from the Parliament of the Kingdom of Italy to build an equatorial mount for the Amici 28-cm refractor, which could not be installed conveniently in the tower of the Specola; then, he went through the process of selecting a proper site, seeking funds and finally building Arcetri Observatory. Although Donati was a pioneer of spectroscopy and astrophysics, his intent was to establish a modern observatory for classical astronomy, as the Italian peninsula did not have a national observatory like those located in many foreign capitals – Florence was the capital of the Kingdom of Italy from 1865 to 1871. To promote the project, Donati made use of writings by one of the most authoritative European astronomers, Otto Wilhelm Struve. -
The National Institute for Astrophysics (Inaf)
THE NATIONAL INSTITUTE FOR ASTROPHYSICS (INAF) A.Costa INAF oact National Institute for Astrophysics (INAF) The roles of the INAF are: • Defining and coordinating the national research policies in astronomy and astrophysics; • Representing the Italian astronomical community in all the related international boards; • Funding and performing world-class research programs in Astrophysics and Space Sciences. National Institute for Astrophysics (INAF) 1. Galaxies and Cosmology 2. Stars, Stellar Populations and Interstellar medium 3. Sun and Solar system 4. Relativistics and Particle Astrophysics 5. Advanced Technologies and Instrumentation HQ in Rome 16 Institutes and Observatories 2 National facilities (TNG, Canarias), LBT (AZ, USA) about 1400 people INAF: Radioastronomy in Italy Longtime tradition in Radioastronomy 3 Radio Facilities INAF: Radioastronomy in Italy Longtime tradition in Radioastronomy 3 Radio Facilities Medicina 32m Northern Cross INAF: Radioastronomy in Italy Longtime tradition in Radioastronomy 3 Radio Facilities Medicina 32m Northern Cross Noto 32m INAF: Radioastronomy in Italy Longtime tradition in Radioastronomy 3 Radio Facilities Medicina 32m Northern Cross Noto 32m SRT 64m Osservatorio Astrofisico di Catania One of the 16 INAF Structures HQs in Catania, inside University of Catania Campus Synergy with UNICT Staff: 62 (researchs/technicians/amministratives) 30 non-staff (Students, PdD students, post-doc……)…..) INAF: Cloud Related Projects EOSCPilot VisIVO Science Demonstrator Main Achievements • Integration of visual analytics -
Paola Santini
PAOLA SANTINI PERSONAL INFORMATION Date of birth: 30th Dec 1981 Email: [email protected] Office address: INAF - Osservatorio Astronomico di Roma Via di Frascati 33 00078 Monte Porzio Catone (Roma, Italy) Office phone: +39 06 94286469 Date of CV: April 2019 CURRENT POSITION Staff researcher at INAF - Astronomical Observatory of Rome (INAF-OAR). PREVIOUS POSITIONS 2014 - 2018 Fixed-term researcher, INAF - Astronomical Observatory of Rome. 2009 - 2014 Postdoctoral research fellowship, INAF - Astronomical Observatory of Rome. 2010 - 2011 Visiting scientist (6 months), Max Planck Institut f¨urExtraterrestrische Physik, Garching (Germany). 2006 - 2009 Research fellowship, INAF - Astronomical Observatory of Rome. Career breaks 2015 { Maternity leave (5 months). 2017 - 2018 { Maternity leave (5 months). EDUCATION 2012 Post-graduate Master degree in Space Science and Technology, University of Roma \Tor Vergata". Final mark: 110/110 cum laude. Dissertation: \Space debris: an observational point of view". Supervisor: Prof.ssa Alessandra Celletti. Internship report: \Feasibility study: space-based observations of the space envi- ronment" Thales Alenia Space. 2009 PhD in Astronomy, University of Rome \La Sapienza". Dissertation: "The cos- mic history of star formation and mass assembly: a mid-IR view of high redshift galaxies". Supervisors: Dr. Adriano Fontana and Prof. Paolo de Bernardis. 2006 - 2008 Participation to 4 national and international PhD schools. 2005 Degree in Physics, University of Rome \La Sapienza", final mark 110/110 cum laude. Dissertation: \Controllo degli effetti strumentali sui dati di polarizzazione dell'esperimento BOOMERanG" (\Control of instrumental effects on polarization data of BOOMERanG experiment"). Supervisor: Prof. Paolo de Bernardis. 2003 Erasmus project, Cambridge University, UK. Attended two astrophysical classes: Gravitational Astrophysics and Cosmology (Prof. -
The Strategic Vision for Astronomy in Italy 2014-2023
INAF (Italian National Institute for Astrophysics) The Strategic Vision for Astronomy in Italy 2014-2023 Cover figure: The Prawn Nebula from the VST (ESO courtesy) From the Scientific Council of INAF: Enzo Brocato, Stefano Covino, Silvia Masi, Francesca Matteucci, Stefano Orsini, Bianca Poggianti, Pietro Schipani Contents 1 Preface 4 2 Scientific challenges in the 21th century: science questions for the next decade 6 2.1 Our parent star: the Sun . 6 2.2 The planetary systems of the Sun and other stars . 7 2.3 The building blocks of the Universe: the stars . 11 2.4 History of the formation and evolution of the Milky Way and nearby galaxies . 12 2.5 Formation and evolution of galaxies and cosmic structures . 14 2.6 Geometry of the Universe . 16 2.7 High energy Astrophysics . 17 2.8 New Physics and multi-messenger Astronomy . 18 3 Research in technology 21 3.1 Cutting edge technology . 21 3.2 Interdisciplinary technology . 22 3.3 Technology transfer . 22 4 Infrastructures 24 4.1 Ground-based large projects . 24 4.2 Space missions . 27 5 Human resources 29 6 Education and outreach 31 6.1 Education . 31 6.2 Outreach . 31 7 Italian contributions to Astronomy: the present and the future 33 8 Concluding remarks 38 3 Chapter 1 Preface Astronomy is the oldest science in the world. It started with the astronomical observations in China and Babylon thousands of years ago and continued through the centuries with Aristarcos and Tolomeus in Greece and Copernicus and Galileo in Europe. It was in Italy with Galileo Galilei in 1609 that the science we call Astronomy started. -
SN 2005Cs in M51 II. Complete Evolution in the Optical And
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 29 October 2018 (MN LATEX style file v2.2) SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared A. Pastorello1 ⋆, S. Valenti1, L. Zampieri2, H. Navasardyan2, S. Taubenberger3, S. J. Smartt1, A. A. Arkharov4,O.Barnbantner¨ 5, H. Barwig5, S. Benetti2, P. Birtwhistle6, M. T. Botticella1, E. Cappellaro2 , M. Del Principe7, F. Di Mille8, G. Di Rico7, M. Dolci7, N. Elias-Rosa9, N. V. Efimova4,10, M. Fiedler11, A. Harutyunyan2,12, P. A. Hoflich¨ 13, W. Kloehr14, V. M. Larionov4,10,15, V. Lorenzi12, J. R. Maund16,17, N. Napoleone18, M. Ragni7, M. Richmond19, C. Ries5, S. Spiro18,20,1, S. Temporin21, M. Turatto22 and J. C. Wheeler17 1 Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, United Kingdom 2 INAF Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy 3 Max-Planck-Institut f¨ur Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei M¨unchen, Germany 4 Central Astronomical Observatory of Pulkovo, 196140 St. Petersburg, Russia 5 Universit¨ats-Sternwarte M¨unchen, Scheinerstr. 1, 81679 M¨unchen, Germany 6 Great Shefford Observatory, Phlox Cottage, Wantage Road, Great Shefford RG17 7DA, UK 7 INAF Osservatorio Astronomico di Collurania, via M. Maggini, 64100 Teramo, Italy 8 Dipartmento of Astronomia, Universit´adi Padova, Vicolo dell’Osservatorio 2, 35122 Padova, Italy 9 Spitzer Science Center, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USA 10 Astronomical Institute of St. Petersburg University, St. Petersburg, Petrodvorets, Universitetsky pr. -
Istituto Nazionale Di Astrofisica National Institute for Astrophysics
I.N.A.F. ISTITUTO NAZIONALE DI ASTROFISICA NATIONAL INSTITUTE FOR ASTROPHYSICS INAF POST-DOCTORAL FELLOWSHIPS PROGRAMME 2010 JOB DESCRIPTION The National Institute for Astrophysics (INAF) is the italian agency for astrophysical research. It runs 19 research Observatories/Institutes in the country and the Telescopio Nazionale Galileo (TNG) in the Canary Islands. INAF contributes, among other projects, to the Large Binocular Telescope (LBT) in Arizona and the Very Long Baseline Interferometry (VLBI) network. In the last few years, INAF has been rated as the most productive Italian research institution in the field of Physics, and according to a recent ISI Thompson evaluation it ranks 5th in the world as regards refereed publications in astrophysics. INAF comprises about 550 research staff, 450 technical and administrative support staff, 300 postdoctoral and graduate students. INAF main active areas of interest are the study of the Universe in all its aspects, from the Solar System to Cosmology, and the development of advanced instrumentation and technology for both ground-based and satellites observations. Since many of these technologies are potentially useful in our lives as well, INAF is also deeply engaged in creating and strengthening opportunities for technological transfer. Thanks to Italian participation in the European Southern Observatory (ESO), INAF researchers have access to the most advanced optical instrumentation. In the radio domain, INAF participates with two antennas (in Medicina and Noto) in the worldwide Very Large Base Interferometry (VLBI) to which it will be soon added the 64 meters Sardinia Radio Telescope (SRT) antenna now under construction. In the near future, INAF is going to play an important role in huge international programmes as the Square Kilometer Array (SKA) and the European Extremely Large Telescope (E-ELT).