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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
HILIGT, upper limit servers I-Overview
DOI: 10.1016/j.ascom.2021.100531 Bibcode: 2022A&C....3800531S

Gabriel, C.; Kretschmar, P.; Kuulkers, E. +10 more

The advent of all-sky facilities, such as the Neil Gehrels Swift observatory, the All Sky Automated Search for Supernovae (ASAS-SN), eROSITA and Gaia has led to a new appreciation of the importance of transient sources in solving outstanding astrophysical questions. Identification and catalogue cross-matching of transients has been eased over the …

2022 Astronomy and Computing
Exosat INTEGRAL XMM-Newton 27
Localized thermonuclear bursts from accreting magnetic white dwarfs
DOI: 10.1038/s41586-022-04495-6 Bibcode: 2022Natur.604..447S

Knigge, C.; de Martino, D.; Done, C. +16 more

Nova explosions are caused by global thermonuclear runaways triggered in the surface layers of accreting white dwarfs1-3. It has been predicted4-6 that localized thermonuclear bursts on white dwarfs can also take place, similar to type-I X-ray bursts observed in accreting neutron stars. Unexplained rapid bursts from the binar…

2022 Nature
Exosat Gaia 22
HILIGT, Upper Limit Servers II - Implementing the data servers
DOI: 10.1016/j.ascom.2021.100529 Bibcode: 2022A&C....3800529K

Freyberg, M. J.; Wilms, J.; Savchenko, V. +7 more

The High-Energy Lightcurve Generator (HILIGT) is a new web-based tool which allows the user to generate long-term lightcurves of X-ray sources. It provides historical data and calculates upper limits from image data in real-time. HILIGT utilizes data from twelve satellites, both modern missions such as XMM-Newton and Swift, and earlier facilities …

2022 Astronomy and Computing
Exosat INTEGRAL XMM-Newton 19
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