DSpace Repository

Browsing by Author "Bartalucci, I."

Browsing by Author "Bartalucci, I."

Sort by: Order: Results:

  • Chandra ACIS-I particle background: an analytical model 
    Bartalucci, I.; Mazzotta, P.; Bourdin, H.; Vikhlinin, Alexey A. (2014)
    <br/> Aims: Imaging and spectroscopy of X-ray extended sources require a proper characterisation of a spatially unresolved background signal. This background includes sky and instrumental components, each of which are ...
  • The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state 
    Bartalucci, I.; Arnaud, M.; Pratt, G. W.; Démoclès, J.; Lovisari, Lorenzo (2019)
    We study the dynamical state and the integrated total mass profiles of 75 massive (M<SUB>500</SUB> &gt; 5 × 10<SUP>14</SUP> M<SUB>?</SUB>) Sunyaev-Zeldovich(SZ)-selected clusters at 0.08 ) Sunyaev-Zeldovich(SZ)-selected ...
  • Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra 
    Bartalucci, I.; Arnaud, M.; Pratt, G. W.; Vikhlinin, A.; Pointecouteau, E.; Forman, W. R.; Jones, C.; Mazzotta, P.; Andrade-Santos, F. (2017)
    We examined the reconstruction of galaxy cluster radial density profiles obtained from Chandra and XMM-Newton X-ray observations, using high quality data for a sample of twelve objects covering a range of morphologies and ...
  • Resolving galaxy cluster gas properties at z 1 with XMM-Newton and Chandra 
    Bartalucci, I.; Arnaud, M.; Pratt, G. W.; Démoclès, J.; van der Burg, R. F. J.; Mazzotta, P. (2017)
    Massive, high-redshift, galaxy clusters are useful laboratories to test cosmological models and to probe structure formation and evolution, but observations are challenging due to cosmological dimming and angular distance ...

Search DSpace

Browse

My Account