Hannah McCall

ORCID: 0000-0003-3537-3491
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About
Contact & Profiles
Research Areas
  • Astronomy and Astrophysical Research
  • Galaxies: Formation, Evolution, Phenomena
  • Astrophysics and Cosmic Phenomena
  • Gamma-ray bursts and supernovae
  • Astronomical Observations and Instrumentation
  • Stellar, planetary, and galactic studies
  • Astrophysical Phenomena and Observations
  • Radio Astronomy Observations and Technology
  • Historical Legal Studies and Society
  • Geophysics and Gravity Measurements
  • Pulsars and Gravitational Waves Research

University of Chicago
2024

University of Bonn
2024

Weatherford College
2023

The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying sky in December 2019, with aim of producing all-sky X-ray source lists and maps an unprecedented depth. Here we present catalogues both point-like extended sources using data acquired first six months survey operations (eRASS1; completed June 2020) over half whose proprietary rights lie German Consortium. We describe observation process, analysis pipelines, characteristics sources. With nearly 930...

10.1051/0004-6361/202347165 article EN cc-by Astronomy and Astrophysics 2024-01-31

Context. As the closest galaxy cluster, Virgo Cluster is an exemplary environment for study of large-scale filamentary structure and physical effects that are present in cluster outskirts but absent from more easily studied inner regions. Aims. Here, we analysis SRG/eROSITA data five all-sky surveys. Methods. eROSITA allows us to resolve entire its on scales between 1 kpc 3 Mpc, covering a total area sky about 25° by 25°. We utilized image manipulation techniques surface brightness profiles...

10.1051/0004-6361/202449391 article EN cc-by Astronomy and Astrophysics 2024-06-17

Context. The Virgo cluster is the nearest ( d = 16.5 Mpc) massive M ≥ 10 14 ⊙ ) galaxy and therefore a prime target for studying astrophysical processes in dense large-scale environments. In radio band, we can probe nonthermal components of interstellar medium, intracluster medium (ICM), active galactic nuclei (AGN). This allows an investigation impact environment on evolution galaxies contribution AGN to ICM heating. With ViCTORIA (VIrgo Cluster multi-Telescope Observations Radio...

10.1051/0004-6361/202346458 article EN cc-by Astronomy and Astrophysics 2023-06-21

As the closest galaxy cluster, Virgo Cluster is an exemplary environment for study of large-scale filamentary structure and physical effects that are present in cluster outskirts but absent from more easily studied inner regions. Here, we exploration SRG/eROSITA data five all-sky surveys. eROSITA allows us to resolve entire its on scales between 1 kpc 3 Mpc, covering a total area sky about 25 by degrees. We utilize image manipulation techniques surface brightness profiles search extended...

10.48550/arxiv.2401.17296 preprint EN arXiv (Cornell University) 2024-01-30

The Virgo cluster is the nearest massive galaxy and thus a prime target to study astrophysical processes in dense large-scale environments. In radio band, we can probe non-thermal components of inter-stellar medium (ISM), intracluster (ICM) active galactic nuclei (AGN). With ViCTORIA (Virgo Cluster multi-Telescope Observations Radio Interacting galaxies AGN) project, are carrying out multiple wide-field surveys at different frequencies. We aim investigate impact environment on evolution...

10.48550/arxiv.2306.04513 preprint EN other-oa arXiv (Cornell University) 2023-01-01
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