… In total, we have 41 spectra covering epochs from 34 to 281 days … 10 49 erg. Thus the total
energy radiated by SN 2023aew from explosion until our last detection is (6.56 ± 0.18) × 10 49 …

… Staying in quiescence for 49 yr, 4U 1730–22 became active and had two outbursts in 2021
and 2022; 10 thermonuclear X-ray bursts were detected with Insight-HXMT. Among them, the …

Cosmological models and their parameters are widely debated, especially about whether
the current discrepancy between the values of the Hubble constant, H 0, obtained by Type Ia …

Recurrent novae are repeating thermonuclear explosions in the outer layers of white dwarfs,
due to the accretion of fresh material from a binary companion. The shock generated when …

… –Lemaître constant H 0 between 2012 and 2022, which includes 109 model-independent …
Therefore, we employ the statistical analysis approach proposed by López-Corredoira (2022…

… Petrosian, Singal & Mutchnick (2022) have pointed out the presence of the circularity problem
in … (2022) and their innovative approach in the QSO realm, which we apply in this study. …

… The data for the charged CRs [5–34] have been extracted from the Cosmic Ray Database
(CRDB) [35]. Below 104 GeV, the all-particle spectrum is the sum of spline fits of the most …

HESS J1356-645 is considered to be a pulsar wind nebula (PWN) associated with the pulsar
PSR J1357-6429. We reanalyze the GeV gamma-ray emission in the direction of HESS …

The blazar 4C 31.03 recently underwent a major γ-ray outburst at the beginning of 2023 after
a prolonged quiescent phase. Fermi-LAT reported a daily average flux of 5 × 10 − 6 phs cm …

… (2022) and our wide jet parameter, the absorption frequency ν a is larger than 10 GHz, and
the flux depends on E iso , K and n 0 ( F ν ∝ E iso , K 5 / 6 n 0 1 / 2 ). The flux with large E iso …