Search Results - "Farinelli, Ruben"

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  1. 1

    A numerical jet model for the prompt emission of gamma-ray bursts by Farinelli, Ruben, Basak, Rupal, Amati, Lorenzo, Guidorzi, Cristiano, Frontera, Filippo

    “…ABSTRACT Gamma-ray bursts (GRBs) are known to be highly collimated events, and are mostly detectable when they are seen on-axis or very nearly on-axis…”
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    Journal Article
  2. 2

    A New Comptonization Model for Weakly Magnetized, Accreting Neutron Stars in Low-Mass X-Ray Binaries by Farinelli, Ruben, Titarchuk, Lev, Paizis, Ada, Frontera, Filippo

    Published in The Astrophysical journal (10-06-2008)
    “…We have developed a new model for the X-ray spectral fitting package XSPEC that takes into account the effects of both thermal and dynamical (i.e., bulk)…”
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    Journal Article
  3. 3

    The IXPE View of Neutron Star Low-Mass X-ray Binaries by Ursini, Francesco, Gnarini, Andrea, Capitanio, Fiamma, Bobrikova, Anna, Cocchi, Massimo, Di Marco, Alessandro, Fabiani, Sergio, Farinelli, Ruben, La Monaca, Fabio, Rankin, John, Saade, Mary Lynne, Poutanen, Juri

    Published in Galaxies (01-08-2024)
    “…Low-mass X-ray binaries hosting weakly magnetized neutron stars (NS-LMXBs) are among the brightest sources in the X-ray sky. Since 2021, the Imaging X-ray…”
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    Journal Article
  4. 4

    AN UPSCATTERING SPECTRAL FORMATION MODEL FOR THE PROMPT EMISSION OF GAMMA-RAY BURSTS by TITARCHUK, Lev, FARINELUI, Ruben, FRONTERA, Filippo, AMATI, Lorenzo

    Published in The Astrophysical journal (20-06-2012)
    “…We propose a model for the spectral formation of gamma-ray burst (GRB) prompt emission, where the phenomenological Band function is usually applied to describe…”
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    Journal Article
  5. 5

    The Hard X-Ray Tails in Neutron Star Low-Mass X-Ray Binaries: BeppoSAX Observations and Possible Theoretical Explanation of the Case of GX 17+2 by Farinelli, Ruben, Titarchuk, Lev, Frontera, Filippo

    Published in The Astrophysical journal (20-06-2007)
    “…We report results of a new spectral analysis of two BeppoSAX observations of the Z source GX 17+ 2. In one of the observations, the source exhibited a…”
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    Journal Article
  6. 6
  7. 7

    First spectropolarimetric observation of the neutron star low-mass X-ray binary GX 3+1 by Gnarini, Andrea, Farinelli, Ruben, Ursini, Francesco, Bianchi, Stefano, Capitanio, Fiamma, Matt, Giorgio, Ng, Mason, Tarana, Antonella, Bobrikova, Anna, Cocchi, Massimo, Fabiani, Sergio, Kaaret, Philip, Poutanen, Juri, Ravi, Swati

    Published 15-11-2024
    “…We report the first simultaneous X-ray spectropolarimetric observation of the bright atoll neutron star low-mass X-ray binary GX 3+1, performed by the Imaging…”
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    Journal Article
  8. 8

    The IXPE View of Neutron Star Low-Mass X-ray Binaries by Ursini, Francesco, Gnarini, Andrea, Capitanio, Fiamma, Bobrikova, Anna, Cocchi, Massimo, Di Marco, Alessandro, Fabiani, Sergio, Farinelli, Ruben, La Monaca, Fabio, Rankin, John, Saade, Mary Lynne, Poutanen, Juri

    Published 11-09-2024
    “…Low-mass X-ray binaries hosting weakly magnetized neutron stars (NS-LMXBs) are among the brightest sources in the X-ray sky. Since 2021, the Imaging X-ray…”
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    Journal Article
  9. 9

    A numerical jet model for the prompt emission of gamma-ray bursts by Farinelli, Ruben, Basak, Rupal, Amati, Lorenzo, Guidorzi, Cristiano, Frontera, Filippo

    Published 08-01-2021
    “…Gamma-ray bursts (GRBs) are known to be highly collimated events, and are mostly detectable when they are seen on-axis or very nearly on-axis. However, GRBs…”
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    Journal Article
  10. 10

    Polarization properties of weakly magnetized Neutron Stars in Low Mass X-ray Binaries by Gnarini, Andrea, Ursini, Francesco, Matt, Giorgio, Bianchi, Stefano, Capitanio, Fiamma, Cocchi, Massimo, Farinelli, Ruben, Zhang, Wenda

    Published 01-06-2022
    “…X-ray polarimetry missions like IXPE will be able to measure for the first time the polarization properties of accreting, weakly magnetized neutron stars in…”
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    Journal Article
  11. 11

    Scientific simulations and optimization of the XGIS instrument on board THESEUS by Mereghetti, Sandro, Ghirlanda, Giancarlo, Salvaterra, Ruben, Campana, Riccardo, Labanti, Claudio, Connell, Paul H, Farinelli, Ruben, Frontera, Filippo, Fuschino, Fabio, Gasent-Blesa, Jose L, Guidorzi, Cristiano, Lissoni, Michele, Rigoselli, Michela, Stephen, John B, Amati, Lorenzo

    Published 17-02-2021
    “…The XGIS (X and Gamma Imaging Spectrometer) is one of the three instruments onboard the THESEUS mission (ESA M5, currently in Phase-A). Thanks to its wide…”
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    Journal Article
  12. 12

    The Mass-Radius relation for Neutron Stars in $f(R)$ gravity by Capozziello, Salvatore, De Laurentis, Mariafelicia, Farinelli, Ruben, Odintsov, Sergei D

    Published 10-09-2015
    “…Phys. Rev. D 93, 023501 (2016) We discuss the Mass -Radius diagram for static neutron star models obtained by the numerical solution of modified…”
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    Journal Article
  13. 13

    An upscattering spectral formation model for the prompt emission of Gamma-Ray Bursts by Titarchuk, Lev, Farinelli, Ruben, Frontera, Filippo, Amati, Lorenzo

    Published 15-04-2012
    “…We propose a model for the spectral formation of Gamma Ray Burst (GRB) prompt emission, where the phenomenological Band's function is usually applied to…”
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    Journal Article
  14. 14

    Comptonization signatures in the prompt emission of Gamma Ray Bursts by Frontera, Filippo, Amati, Lorenzo, Farinelli, Ruben, Dichiara, Simone, Guidorzi, Cristiano, Landi, Raffaella, Titarchuk, Lev

    Published 02-01-2014
    “…We report results of a systematic study of the broad--band (2--2000 keV) time--resolved prompt emission spectra of a sample of Gamma-Ray Bursts (GRBs) detected…”
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    Journal Article
  15. 15

    Two-phase X-ray burst from GX 3+1 observed by INTEGRAL by Chenevez, Jerome, Falanga, Maurizio, Brandt, Soeren, Farinelli, Ruben, Frontera, Filippo, Goldwurm, Andrea, Zand, Jean in 't, Kuulkers, Erik, Lund, Niels

    Published 22-12-2005
    “…INTEGRAL detected on August 31, 2004, an unusual thermonuclear X-ray burst from the low-mass X-ray binary GX 3+1. Its duration was 30 min, which is between the…”
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    Journal Article
  16. 16