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GOFAR

Galactic Outflows and Feedback in the Astro-H eR

Total Cost €

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EC-Contrib. €

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Partnership

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 GOFAR project word cloud

Explore the words cloud of the GOFAR project. It provides you a very rough idea of what is the project "GOFAR" about.

sensitivity    opportunity    he    cubed    train    velocity    location    observatory    intergalactic    detect    galaxy    confirm    feedback    skills    light    soon    ionized    astro    power    umd    horse    spectroscopic    coming    atoms    owing    gsfc    group    facility    spectroscopy    data    ions    plasmas    ray    filaments    spectral    decade    sought    energy    world    wind    technion    outflows    candidate    igm    absorption    scales    astronomy    winds    govern    universe    resolving    claimed    attempt    outflow    adjacent    training    missing    laboratory    center    university    instrumentation    space    nuclei    previously    speed    enriching    match    sxs    implied    rate    resolution    diagnostics    medium    position    soft    active    mass    galactic    agn    hottest    collisionally    gofar    fastest    goddard    components    kinetic    hardware    nasa    host    launch    astrophysical    forefront    centre    photo    unprecedented    dominate    first    leads    flight    influence    japanese    fraction    combination    shell    kev    maryland    astrophysics    spectrometer    1c   

Project "GOFAR" data sheet

The following table provides information about the project.

Coordinator
TECHNION - ISRAEL INSTITUTE OF TECHNOLOGY 

Organization address
address: SENATE BUILDING TECHNION CITY
city: HAIFA
postcode: 32000
website: www.technion.ac.il

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Israel [IL]
 Project website http://www.technion.ac.il/en/2017/04/black-hole-winds-the-magnetic-hydrodynamic-model/
 Total cost 198˙836 €
 EC max contribution 198˙836 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2014
 Funding Scheme MSCA-IF-GF
 Starting year 2015
 Duration (year-month-day) from 2015-08-01   to  2017-10-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    TECHNION - ISRAEL INSTITUTE OF TECHNOLOGY IL (HAIFA) coordinator 198˙836.00
2    University of Maryland US (College Park) partner 0.00

Map

 Project objective

Training: The GOFAR proposal is to train the Technion candidate to work on the Soft X-ray Spectrometer (SXS) built by NASA’s Goddard Space Flight Center (GSFC), for launch soon on the Japanese space observatory Astro-H that will be the working horse of X-Ray Astronomy in the next decade. The X-ray Astrophysics Laboratory at GSFC, the world centre for astrophysical X-ray spectroscopy and instrumentation will set up a data analysis facility at the adjacent University of Maryland (UMD), who will host GOFAR. Owing to its unprecedented combination of spectral resolution and sensitivity between 6 – 7 keV, the SXS will detect and measure, better than ever before, the hottest and most ionized X-ray astrophysical plasmas. GOFAR will thus position the candidate and his Technion group at the forefront of X-ray astrophysical research in the coming decade, but will also improve his project-management skills for the university hardware projects that he leads.

Research: We propose to develop new spectroscopic diagnostics to match the spectral resolving power and sensitivity of the SXS for K- and L- shell ions in both photo- and collisionally- ionized plasmas, focusing on active galactic nuclei (AGN) outflows. We will measure the most ionized components of the winds, implied previously to dominate the outflow mass and energy. We propose to measure the location, mass outflow rate, and kinetic power of the wind, which govern its influence on the host galaxy. This will be the first opportunity to confirm and measure in detail the fastest components of AGN winds that were claimed to reach a fraction of the speed of light (~ 0.1c). Since the kinetic power in the wind scales as the outflow velocity cubed, these components are the most promising AGN energy feedback, and for enriching the intergalactic medium (IGM). We will attempt to identify absorption from filaments of the IGM, which represent the long sought-after missing atoms of the Universe.

 Publications

year authors and title journal last update
List of publications.
2017 M. Mehdipour, J. S. Kaastra, G. A. Kriss, N. Arav, E. Behar, S. Bianchi, G. Branduardi-Raymont, M. Cappi, E. Costantini, J. Ebrero, L. Di Gesu, S. Kaspi, J. Mao, B. De Marco, G. Matt, S. Paltani, U. Peretz, B. M. Peterson, P.-O. Petrucci, C. Pinto, G. Ponti, F. Ursini, C. P. de Vries, D. J. Walton
Chasing obscuration in type-I AGN: discovery of an eclipsing clumpy wind at the outer broad-line region of NGC 3783
published pages: A28, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731175
Astronomy & Astrophysics 607 2019-07-23
2016 E. S. Kammoun, G. Risaliti, D. Stern, H. D. Jun, M. Graham, A. Celotti, E. Behar, M. Elvis, F. A. Harrison, G. Matt, D. J. Walton
Coronal properties of the luminous radio-quiet quasar QSO B2202–209
published pages: 1665-1671, ISSN: 0035-8711, DOI: 10.1093/mnras/stw2897
Monthly Notices of the Royal Astronomical Society 465/2 2019-07-23
2017 Ehud Behar, Uria Peretz, Gerard A. Kriss, Jelle Kaastra, Nahum Arav, Stefano Bianchi, Graziella Branduardi-Raymont, Massimo Cappi, Elisa Costantini, Barbara De Marco, Laura Di Gesu, Jacobo Ebrero, Shai Kaspi, Missagh Mehdipour, Stéphane Paltani, Pierre-Olivier Petrucci, Gabriele Ponti, Francesco Ursini
Multi-wavelength campaign on NGC 7469
published pages: A17, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201629943
Astronomy & Astrophysics 601 2019-07-23
2015 M. Whewell, G. Branduardi-Raymont, J. S. Kaastra, M. Mehdipour, K. C. Steenbrugge, S. Bianchi, E. Behar, J. Ebrero, M. Cappi, E. Costantini, B. De Marco, L. Di Gesu, G. A. Kriss, S. Paltani, B. M. Peterson, P.-O. Petrucci, C. Pinto, G. Ponti
Anatomy of the AGN in NGC 5548
published pages: A79, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201526742
Astronomy & Astrophysics 581 2019-07-23
2016 K. Fukumura, F. Tombesi, D. Kazanas, C. Shrader, E. Behar, I. Contopoulos
Fast ionized X-ray absorbers in AGNs
published pages: 454-458, ISSN: 0004-6337, DOI: 10.1002/asna.201612329
Astronomische Nachrichten 337/4-5 2019-07-23
2018 D.-H. Kwon, W. Lee, S. Preval, C.P. Ballance, E. Behar, J. Colgan, C.J. Fontes, T. Nakano, B. Li, X. Ding, C.Z. Dong, Y.B. Fu, N.R. Badnell, M. O’Mullane, H.-K. Chung, B.J. Braams
Iso-nuclear tungsten dielectronic recombination rates for use in magnetically-confined fusion plasmas
published pages: 250-262, ISSN: 0092-640X, DOI: 10.1016/j.adt.2017.04.002
Atomic Data and Nuclear Data Tables 119 2019-07-23
2016 J. N. Reeves, V. Braito, E. Nardini, E. Behar, P. T. O’Brien, F. Tombesi, T. J. Turner, M. T. Costa
DISCOVERY OF BROAD SOFT X-RAY ABSORPTION LINES FROM THE QUASAR WIND IN PDS 456
published pages: 20, ISSN: 1538-4357, DOI: 10.3847/0004-637X/824/1/20
The Astrophysical Journal 824/1 2019-07-23
2015 Ranieri D. Baldi, Ehud Behar, Ari Laor, Assaf Horesh
Milimetre-band variability of the radio-quiet nucleus of NGC 7469
published pages: 4277-4281, ISSN: 0035-8711, DOI: 10.1093/mnras/stv2284
Monthly Notices of the Royal Astronomical Society 454/4 2019-07-23
2016 Ranieri D. Baldi, Alessandro Capetti, Andrew Robinson, Ari Laor, Ehud Behar
Radio-loud Narrow Line Seyfert 1 under a different perspective: a revised black hole mass estimate from optical spectropolarimetry
published pages: L69-L73, ISSN: 1745-3933, DOI: 10.1093/mnrasl/slw019
Monthly Notices of the Royal Astronomical Society: Letters 458/1 2019-07-23
2016 M. Cappi, B. De Marco, G. Ponti, F. Ursini, P.-O. Petrucci, S. Bianchi, J. S. Kaastra, G. A. Kriss, M. Mehdipour, M. Whewell, N. Arav, E. Behar, R. Boissay, G. Branduardi-Raymont, E. Costantini, J. Ebrero, L. Di Gesu, F. A. Harrison, S. Kaspi, G. Matt, S. Paltani, B. M. Peterson, K. C. Steenbrugge, D. J. Walton
Anatomy of the AGN in NGC 5548
published pages: A27, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201628464
Astronomy & Astrophysics 592 2019-07-23
2016 Lee Yacobi, Dafne Guetta, Ehud Behar
IMPLICATION OF THE NON-DETECTION OF GZK NEUTRINOS
published pages: 89, ISSN: 1538-4357, DOI: 10.3847/0004-637X/823/2/89
The Astrophysical Journal 823/2 2019-07-23
2016 U. Peretz, M. Orio, E Behar, A. Bianchini, J. Gallagher, T. Rauch, B. Tofflemire, P. Zemko
CHEMICAL AND PHYSICAL PARAMETERS FROM X-RAY HIGH-RESOLUTION SPECTRA OF THE GALACTIC NOVA V959 MON
published pages: 2, ISSN: 1538-4357, DOI: 10.3847/0004-637X/829/1/2
The Astrophysical Journal 829/1 2019-07-23
2016 R. W. Goosmann, T. Holczer, M. Mouchet, A.-M. Dumont, E. Behar, O. Godet, A. C. Gonçalves, S. Kaspi
The thermal instability of the warm absorber in NGC 3783
published pages: A76, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201425199
Astronomy & Astrophysics 589 2019-07-23

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