Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: CGRO/BATSE Data Support the New Paradigm for GRB Prompt Emission and the
  New L$_{i}^{nTh}$-E$_{peak,i}^{nTh,rest}$ relation   The paradigm for GRB prompt emission is changing. Since early in the CGRO
era, the empirical Band function has been considered a good description of the
keV-MeV spectra although its shape is very often inconsistent with the
predictions of the pure synchrotron emission scenarios. We have recently
established a new observational model analyzing data of the NASA Fermi
Gamma-ray Space Telescope. In this model, GRB prompt emission is a combination
of three main emission components: (i) a thermal-like component that we
interpreted so far as the jet photosphere emission, (ii) a non-thermal
component that we interpreted so far as synchrotron radiation, and (iii) an
additional non-thermal (cutoff) power-law most likely of inverse Compton
origin. In this article we reanalyze some of the bright GRBs observed with
CGRO/BATSE with the new model, namely GRBs 941017, 970111 and 990123. We
conclude that BATSE data are fully consistent with the recent results obtained
with Fermi: some bright BATSE GRBs exhibit three separate components during the
prompt phase with similar spectral parameters as these reported from Fermi
data. In addition, the analysis of the BATSE GRBs with the new model results in
a relation between the time-resolved energy flux of the non-thermal component
and its corresponding $\nu$F$_\nu$ peak energy (i.e.,
F$_{i}^{nTh}$-E$_{peak,i}^{nTh}$) that has a similar index as the one initially
derived from Fermi data. For GRBs with known redshift (z) this results in a
possible universal relation between the luminosity of the non-thermal component
and its corresponding $\nu$F$_\nu$ peak energy in the rest frame (i.e.,
L$_{i}^{nTh}$-E$_{peak,i}^{NT,rest}$). We estimated z for GRBs 941017 and
970111 using GRB 990123--with z=1.61--as a reference. The estimated z for GRB
941017 is typical for long GRBs and the estimated z for GRB 970111 is right in
the range of the expected values for this burst.

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The categories of this paper are: eess
28
The categories of this paper are: alg-geom
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The categories of this paper are: dg-ga
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The categories of this paper are: adap-org
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The categories of this paper are: econ
0
The categories of this paper are: hep-ph
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The categories of this paper are: comp-gas
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The categories of this paper are: hep-ex
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The categories of this paper are: hep-lat
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The categories of this paper are: patt-sol
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The categories of this paper are: q-alg
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The categories of this paper are: quant-ph
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The categories of this paper are: mtrl-th
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The categories of this paper are: hep-th
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The categories of this paper are: nucl-ex
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The categories of this paper are: cs