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20082025
most citedThe First Fermi LAT Gamma-Ray Burst Catalog

297 citations · 2.8k across the 63 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.SR2021★ 18 cited

Recurrent strong outbursts of an EXor-like young eruptive star Gaia20eae

Fernando Cruz-Sáenz de Miera, Ágnes Kóspál, Péter Ábrahám +21

We present follow-up photometric and spectroscopic observations, and subsequent analysis of Gaia20eae. This source triggered photometric alerts during 2020 after showing a 3…

astro-ph.HE2021

The Disk-Corona Model and Mass Estimates of the Ultraluminous X-ray Source Holmberg IX X-1

Ramandeep Gill, Eda Sonbas, Kalvir S. Dhuga +1

The origin of the variable X-ray emission in the keV energy range of ultraluminous X-ray sources (ULXs) remains unclear, making it difficult to constrain the mass of th…

astro-ph.HE2021★ 2 cited

A Temporal Scale to Track the Spectral Transitions in Low-Mass X-ray Binaries

E. Sonbas, K. Mohamed, K. S. Dhuga +1

The results of a temporal analysis of observations for a sample of nine low-mass X-ray binaries (LMXBs) are presented. Of these sources, five host a neutron star (NS) primary (4U16…

astro-ph.EP2021★ 12 cited

Probing Transit Timing Variations of Three Hot-Jupiters: HATP-36b, HATP-56b, and WASP-52b

E. Sonbas, N. Karaman, A. Özdönmez +5

We report the results of new transit observations for the three hot Jupiter-like planets HATP-36b, HATP-56b and WASP-52b respectively. Transit timing variations (TTVs) are presente…

astro-ph.EP2021★ 16 cited

Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

A. Marciniak, J. Ďurech, V. Alí-Lagoa +73

Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly…

astro-ph.GA2021★ 12 cited

The Transient Ultra-luminous X-ray Source, ULX-4, in M51

S. Allak, A. Akyuz, İ. Akkaya Oralhan +6

We present the results of a temporal and spectral analysis of the transient source ULX-4 in the galaxy M51. The data used were drawn from Chandra, XMM-Newton and Swift-XRT archives…