The Konus-Wind catalog of gamma-ray bursts with known redshifts. II. Waiting mode bursts simultaneously detected by Swift/BAT. (arXiv:2012.14849v2 [astro-ph.HE] UPDATED)

The Konus-Wind catalog of gamma-ray bursts with known redshifts. II. Waiting mode bursts simultaneously detected by Swift/BAT. (arXiv:2012.14849v2 [astro-ph.HE] UPDATED)
<a href="http://arxiv.org/find/astro-ph/1/au:+Tsvetkova_A/0/1/0/all/0/1">A. Tsvetkova</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Frederiks_D/0/1/0/all/0/1">D. Frederiks</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Svinkin_D/0/1/0/all/0/1">D. Svinkin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aptekar_R/0/1/0/all/0/1">R. Aptekar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cline_T/0/1/0/all/0/1">T. L. Cline</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Golenetskii_S/0/1/0/all/0/1">S. Golenetskii</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hurley_K/0/1/0/all/0/1">K. Hurley</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lysenko_A/0/1/0/all/0/1">A. Lysenko</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ridnaia_A/0/1/0/all/0/1">A. Ridnaia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ulanov_M/0/1/0/all/0/1">M. Ulanov</a>

In the Second part of The Konus-Wind Catalog of Gamma-Ray Bursts with Known
Redshifts (first part: Tsvetkova et al. 2017; T17), we present the results of a
systematic study of gamma-ray bursts (GRBs) with reliable redshift estimates
detected simultaneously by the Konus-Wind (KW) experiment (in the waiting mode)
and by the Swift/BAT (BAT) telescope during the period from 2005 January to the
end of 2018. By taking advantage of the high sensitivity of BAT and the wide
spectral band of KW we were able to constrain the peak spectral energies, the
broadband energy fluences, and the peak fluxes for the joint KW-BAT sample of
167 weak, relatively soft GRBs (including four short bursts). Based on the GRB
redshifts, which span the range $0.04 leq z leq 9.4$, we estimate the
rest-frame, isotropic-equivalent energy, and peak luminosity. For 14 GRBs with
reasonably constrained jet breaks, we provide the collimation-corrected values
of the energetics. This work extends the sample of KW GRBs with known redshifts
to 338 GRBs, the largest set of cosmological GRBs studied to date over a broad
energy band. With the full KW sample, accounting for the instrumental bias, we
explore GRB rest-frame properties, including hardness-intensity correlations,
GRB luminosity evolution, luminosity and isotropic-energy functions, and the
evolution of the GRB formation rate, which we find to be in general agreement
with those reported in T17 and other previous studies.

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