GS
G. Schellenberger
astro-ph.GAastro-ph.COastro-ph.HEastro-ph.IMastro-ph.SR
On Valency
published · living versionsW_hr82v3qh·v1 · currentpublished
Radio view of the Peanut cluster: merger-induced stripping and a radio halo shortly after pericentric passage
with K. Rajpurohit, N. Lyskova, E. Churazov, W. Forman +23
1 version
Preprints & journals
63 papers in the corpus · 2014–2026Twenty-five years of XMM-Newton EPIC-MOS2 Unfocused Particle Background: Solar Cycle Modulation, Galactic Cosmic-Ray Correlation, and Implications for NewAthena2610.27121v1 · B. Vaia, F. Gastaldello, S. Molendi et al.2026 · 0 citationsarXiv
Direct imaging of sub-parsec binary SMBHs in the central galaxy of the NGC 5044 group2609.22433v1 · Francesco Ubertosi, Gerrit Schellenberger, Ewan O'Sullivan et al.2026 · 0 citationsarXiv
A radio continuum view of Stephan's Quintet: age, dynamics and origin of the shock2608.26461v1 · K. Rajpurohit, E. O'Sullivan, G. Schellenberger et al.2026 · 0 citationsarXiv
High-statistics simulations of NewAthena WFI background using Geant42607.26163v1 · Matthew K. Heine, Catherine E. Grant, Marshall W. Bautz et al.2026 · 0 citationsarXiv
The Treble Clef radio phoenix and its old nonthermal filaments2607.06659v2 · A. Botteon, M. Brienza, K. Rajpurohit et al.2026 · 0 citationsarXiv
Resolving the temporal evolution of M87 jet with -arcsec Chandra observations2606.13800v1 · Camille Poitras, Gerrit Schellenberger, Ralph Kraft et al.2026 · 0 citationsarXiv
AGN Fueling and Radio Jet Evolution in the Galaxy Group NGC 5044 revealed by VLBA HI Absorption and Proper-Motion Radio Observations2603.28864v1 · Francesco Ubertosi, Ewan O'Sullivan, Gerrit Schellenberger et al.2026 · 0 citationsarXiv
A MeerKAT view of the Neutral Atomic Gas in Stephan's Quintet2603.27097v1 · K. Rajpurohit, E. O'Sullivan, G. Schellenberger et al.2026 · 0 citationsarXiv
HST view of NGC 5044: Constraints on Filament Widths, Magnetic Support, Multiphase Structure, and Comparison with Cluster Environments2603.00249v2 · Prathamesh Tamhane, Ming Sun, William Waldron et al.2026 · 3 citationsarXiv
An X-ray-emitting protocluster at z ≈ 5.7 reveals rapid structure growth.41606151 · Bogdán, Ákos, Schellenberger, Gerrit, Li, Qiong et al.2026 · 1 citationNature. 2026;649(8099):1134-1138
Cross Calibration of Galaxy Cluster Temperatures Measured with NuSTAR, XMM-Newton, and Chandra2511.07693v1 · Fiona Lopez, Daniel R. Wik, Cicely Potter et al.2025 · 0 citationsApJ 990 23 (2025)
The Advanced X-ray Imaging Satellite (AXIS) Community Science Book2511.00253v2 · Michael Koss, Nafisa Aftab, Steven W. Allen et al.2025 · 3 citationsarXiv
Multiphase gas offsets in the atmospheres of central galaxies and their consequences for SMBH activation I. The hot and warm ionized gas phases2510.01323v1 · Francesco Ubertosi, Fabrizio Brighenti, Ewan O'Sullivan et al.2025 · 2 citationsarXiv
JVLA and VLBA study of the merging cool core CHIPS 1911+4455 at z~0.5: radio emission from an infant AGN and from a rapidly star-forming BCG2508.04778v1 · Francesco Ubertosi, Myriam Gitti, Pasquale Temi et al.2025 · 0 citationsarXiv
Extreme AGN feedback in the fossil galaxy group SDSSTG 44362506.13907v1 · D. Eckert, F. Gastaldello, L. Lovisari et al.2025 · 3 citationsA&A 701, A127 (2025)
Using the XMM-Newton small window mode to investigate systematic uncertainties in the particle background of X-ray charge-coupled device detectors2503.04682v2 · Gerrit Schellenberger, Ralph Kraft, Paul Nulsen et al.2025 · 1 citationarXiv
Revisiting the Group-Dominant Elliptical NGC 5044 in the Radio Band: Continuum Emission and Detection of HI Absorption2501.02076v2 · Kamlesh Rajpurohit, Tirna Deb, Konstantinos Kolokythas et al.2025 · 3 citationsarXiv
SZ-X-ray Surface Brightness Fluctuations in the SPT-XMM clusters2412.05478v2 · Charles Romero, Massimo Gaspari, Gerrit Schellenberger et al.2024 · 4 citationsarXiv
Probing the high frequency variability of NGC 5044: the key to AGN feedback2409.06039v2 · Gerrit Schellenberger, Ewan O'Sullivan, Laurence David et al.2024 · 0 citationsarXiv
A Deep Dive into the NGC 741 Galaxy Group: Insights into a Spectacular Head-Tail Radio Galaxy from VLA, MeerKAT, uGMRT and LOFAR2408.15197v1 · K. Rajpurohit, E. O'Sullivan, G. Schellenberger et al.2024 · 5 citationsarXiv
Examining the local Universe isotropy with galaxy cluster velocity dispersion scaling relations2408.00726v1 · A. Pandya, K. Migkas, T. H. Reiprich et al.2024 · 7 citationsA&A, 691, A355 (2024)
Augmenting astronomical X-ray detectors with AI for enhanced sensitivity and reduced background2407.16764v1 · D. R. Wilkins, A. Poliszczuk, B. Schneider et al.2024 · 2 citationsProc. SPIE, 2024, 13093-65
Towards efficient machine-learning-based reduction of the cosmic-ray induced background in X-ray imaging detectors: increasing context awareness2407.16768v1 · Artem Poliszczuk, Dan Wilkins, Steven W. Allen et al.2024 · 2 citationsarXiv
Closing Pandora's Box -- The deepest X-ray observations of Abell 2744 and a multi-wavelength merger picture2407.03142v1 · Urmila Chadayammuri, 'Akos Bogd'an, Gerrit Schellenberger et al.2024 · 1 citationarXiv
Active Galaxy Science with the Line Emission Mapper: The Case for High-Resolution Soft X-ray Spectroscopy2406.18743v1 · Kimberly A. Weaver, Jenna M. Cann, Ryan W. Pfeifle et al.2024 · 1 citationarXiv
A hot core in the group-dominant elliptical galaxy NGC 7772405.13667v2 · Ewan O'Sullivan, Kamlesh Rajpurohit, Gerrit Schellenberger et al.2024 · 5 citationsarXiv
Advancing Precision Particle Background Estimation for Future X-ray Missions: Correlated Variability between AMS and Chandra/XMM-Newton2405.06602v1 · Arnab Sarkar, Catherine E. Grant, Eric D. Miller et al.2024 · 3 citationsarXiv
Surface Brightness Fluctuations in Two SPT clusters: a Pilot Study2404.04373v1 · Charles E. Romero, Massimo Gaspari, Gerrit Schellenberger et al.2024 · 7 citationsarXiv
The SRG/eROSITA All-Sky Survey: SRG/eROSITA cross-calibration with Chandra and XMM-Newton using galaxy cluster gas temperatures2401.17297v2 · K. Migkas, D. Kox, G. Schellenberger et al.2024 · 23 citationsA&A 688, A107 (2024)
ZWCL 1856.8 : A rare double radio relic system captured within NuSTAR and Chandra field of view2312.06020v1 · Aysegul Tumer, Daniel R. Wik, Gerrit Schellenberger et al.2023 · 2 citationsarXiv
Jet reorientation in central galaxies of clusters and groups: insights from VLBA and Chandra data2312.02283v1 · Francesco Ubertosi, Gerrit Schellenberger, Ewan O'Sullivan et al.2023 · 11 citationsarXiv
LEM All-Sky Survey: Soft X-ray Sky at Microcalorimeter Resolution2310.16038v1 · Ildar Khabibullin, Massimiliano Galeazzi, Akos Bogdan et al.2023 · 2 citationsarXiv
The Hydrostatic Mass of A478: Discrepant Results From Chandra, NuSTAR, and XMM-Newton2309.11743v1 · Cicely Potter, Aysegul Tumer (2, Qian H. S. Wang et al.2023 · 4 citationsarXiv
Abell 746: A highly disturbed cluster undergoing multiple mergers2309.01716v2 · K. Rajpurohit, L. Lovisari, A. Botteon et al.2023 · 16 citationsarXiv
A detached double X-ray tail in the merging galaxy cluster Z8338 with a large double tail2308.00328v1 · Chong Ge, Ming Sun, Paul E. J. Nulsen et al.2023 · 4 citationsarXiv
Properties of the Line-of-Sight Velocity Field in the Hot and X-ray Emitting Circumgalactic Medium of Nearby Simulated Disk Galaxies2307.01269v2 · J. A. ZuHone, G. Schellenberger, A. Ogorzalek et al.2023 · 11 citationsarXiv
X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback2307.01277v2 · Nhut Truong, Annalisa Pillepich, Dylan Nelson et al.2023 · 29 citationsarXiv
Circumgalactic Medium on the Largest Scales: Detecting X-ray Absorption Lines with Large-Area Microcalorimeters2306.05449v1 · Akos Bogdan, Ildar Khabibullin, Orsolya Kovacs et al.2023 · 10 citationsarXiv
Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies2306.05453v1 · Dylan Nelson, Chris Byrohl, Anna Ogorzalek et al.2023 · 19 citationsarXiv
Inferences from surface brightness fluctuations of Zwicky 3146 via the Sunyaev-Zeldovich effect and X-ray observations2305.05790v1 · Charles E. Romero, Massimo Gaspari, Gerrit Schellenberger et al.2023 · 17 citationsarXiv
Feedback in the merging galaxy group NGC63382303.08833v1 · Gerrit Schellenberger, Ewan O'Sullivan, Simona Giacintucci et al.2023 · 8 citationsarXiv
Waking the monster: the onset of AGN feedback in galaxy clusters hosting young central radio galaxies2303.04821v2 · Francesco Ubertosi, Myriam Gitti, Fabrizio Brighenti et al.2023 · 11 citationsA&A 673, A52 (2023)
Reducing the background in X-ray imaging detectors via machine learning2208.07906v1 · D. R. Wilkins, S. W. Allen, E. D. Miller et al.2022 · 4 citationsProc. SPIE, 2022, 12181, 155
Intracluster magnetic filaments and an encounter with a radio jet2206.14319v1 · Lawrence Rudnick, Marcus Bruggen, Gianfranco Brunetti et al.2022 · 48 citationsarXiv
The contribution of non-central radio galaxies to AGN feedback in rich galaxy clusters2204.06102v1 · Ruchika Seth, Ewan O'Sullivan, Biny Sebastian et al.2022 · 5 citationsarXiv
The unusually weak and exceptionally steep radio relic in Abell 21082111.09225v1 · Gerrit Schellenberger, Simona Giacintucci, Lorenzo Lovisari et al.2021 · 20 citationsarXiv
Molecular gas along the old radio jets of the cluster-central type 2 quasar IRAS 09104+41092109.13756v2 · Ewan O'Sullivan, Francoise Combes, Arif Babul et al.2021 · 13 citationsarXiv
The thermalisation of massive galaxy clusters2109.06199v1 · Mauro Sereno, Lorenzo Lovisari, Weiguang Cui et al.2021 · 18 citationsarXiv
Cosmological implications of the anisotropy of ten galaxy cluster scaling relations2103.13904v1 · K. Migkas, F. Pacaud, G. Schellenberger et al.2021 · 122 citationsA&A 649, A151 (2021)
The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview2010.11972v2 · M. Arnaud, S. Ettori, G.W. Pratt et al.2020 · 98 citationsA&A 650, A104 (2021)
Career total: 103 works. 63 are in this corpus.Showing the 50 most recent.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.