activity
20212026
most citedThe SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere

371 citations · 547 across the 32 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023

Broadband maps of eROSITA and their comparison with the ROSAT survey

Xueying Zheng, Gabriele Ponti, Michael Freyberg +13

By June of 2020, the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum Roentgen Gamma observatory had completed its first of the planned eigh…

astro-ph.HE2023

eROSITA studies of the Carina Nebula

Manami Sasaki, Jan Robrade, Martin G. H. Krause +4

During the first four all-sky surveys eRASS:4 carried out from December 2019 to 2021, the extended Roentgen Survey with an Imaging Telescope Array (eROSITA) on board Spektrum-Roent…

astro-ph.HE2023

S 308 and other X-ray emitting bubbles around Wolf-Rayet stars

Francesco Camilloni, Werner Becker, Manami Sasaki

S 308 is an X-ray emitting bubble that surrounds the Wolf-Rayet star WR6. The structure shines in the optical as well and is thus known as the Dolphin Nebula. Due to its large angu…

astro-ph.GA2023★ 29 cited

The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA

N. Locatelli, G. Ponti, X. Zheng +7

The first all-sky maps of the diffuse emission of high ionization lines observed in X-rays by SRG/eROSITA, provide an excellent probe for the study of the warm-hot phase (T~10^6 K)…

astro-ph.HE2023

Searching for X-Ray Counterparts of Degree Wide TeV Halos Around Middle-Aged Pulsars with SRG/eROSITA

A. Khokhriakova, W. Becker, G. Ponti +3

Context. Extended gamma-ray TeV emission (TeV halos) around middle-aged pulsars has been detected. A proposed model to explain these TeV halos is that electrons from a degree-wide…

astro-ph.GA2023★ 28 cited

SRG/eROSITA X-ray shadowing study of giant molecular clouds

Michael C. H. Yeung, Michael J. Freyberg, Gabriele Ponti +3

SRG/eROSITA is situated in a halo orbit around L2 where the highly variable solar wind charge exchange (SWCX) emission from Earth's magnetosheath is expected to be negligible. The…