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The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study
DOI: 10.1093/mnras/stac1295 Bibcode: 2022MNRAS.514.1557P

Ness, J. -U.; Munari, U.; Orio, M. +12 more

On 2021 August 8, the recurrent nova RS Ophiuchi (RS Oph) erupted again, after an interval of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on August 9.9 (0.37 d after the optical peak), and continued until the source passed behind the Sun at the start of November, 86 d later. Observations then restarted on day …

2022 Monthly Notices of the Royal Astronomical Society
Exosat Gaia 33
Model-independent redshift estimation of BL Lac objects through very-high-energy observations
DOI: 10.1093/mnras/stab3173 Bibcode: 2022MNRAS.511..994M

Bhatt, Nilay; Malik, Zahoor; Sahayanathan, Sunder +3 more

The very-high-energy (VHE) gamma-ray spectral indices of blazars show a strong correlation with the source redshift. The absence of any such correlation in low-energy gamma-rays and X-rays indicates the presence of extragalactic background light (EBL)-induced absorption of VHE gamma-rays. By employing a linear regression analysis, this observation…

2022 Monthly Notices of the Royal Astronomical Society
Exosat 9