Towards the Epeak rest -E iso correlation in GRBs in the BATSE Catalog: A progress report

Bibcode
2005NCimC..28..319P
DOI
10.1393/ncc/i2005-10050-4
Pizzichini, G.; Ferrero, P.; Genghini, M.; Gianotti, F.; Topinka, M.
Bibliographical reference

Il Nuovo Cimento C, vol. 28, Issue 3, p.319

Advertised on:
5
2005
Number of authors
5
IAC number of authors
0
Citations
4
Refereed citations
3
Description
The present paper is a progress report on our work towards estimating the energy emission involved in the many Gamma-Ray Bursts for which no redshift has been actually measured. Once such an estimate is obtained, we can try to extend the E peak rest-Eiso relation found by Amati et al.(Astron. Astrophys., 390 (2002) 81) to those events. Following Atteia (Astron. Astrophys., 407 (2003) L1) we obtain a pseudo-redshift () estimate which then allows us to estimate E peak rest and Eiso for each burst.
Type
Refereed

It may interest you

  • Refereed
    Euclid preparation. XL. Impact of magnification on spectroscopic galaxy clustering
    In this paper we investigate the impact of lensing magnification on the analysis of Euclid's spectroscopic survey using the multipoles of the two-point correlation function for galaxy clustering. We determine the impact of lensing magnification on cosmological constraints as well as the expected shift in the best-fit parameters if magnification is
    Euclid Collaboration et al.

    Advertised on:

    5
    2024
    Bibcode
    2024A&A...685A.167E
    Citations
    0
  • Refereed
    Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy
    Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation is still small, limiting our ability to understand the diversity of the atmospheric composition and
    Kuzuhara, Masayuki et al.

    Advertised on:

    6
    2024
    Bibcode
    2024ApJ...967L..21K
    Citations
    0
  • Refereed
    TOI-4438 b: a transiting mini-Neptune amenable to atmospheric characterization
    We report the confirmation and mass determination of a mini-Neptune transiting the M3.5 V star TOI-4438 (G 182-34) every 7.44 days. A transit signal was detected with NASA's TESS space mission in the sectors 40, 52, and 53. In order to validate the planet TOI-4438 b and to determine the system properties, we combined TESS data with high-precision
    Goffo, E. et al.

    Advertised on:

    5
    2024
    Bibcode
    2024A&A...685A.147G
    Citations
    0