GO
Go Ogiya
astro-ph.GAastro-ph.COastro-ph.HEastro-ph.IMcs.PFgr-qcphysics.comp-ph
On Valency
published · living versionsW_t74a3zq6·v1 · currentpublished
Searching for clues of past binary supermassive black hole mergers in nuclear star clusters
with Alessandra Mastrobuono-Battisti, Oliver Hahn, Mathias Schultheis
1 version
Preprints & journals
33 papers in the corpus · 2011–2026Dynamical evolution of dark matter subhaloes in the Milky Way: role of the Galactic disc2606.18708v2 · Junnan Shen, Go Ogiya, Jens Stucker2026 · 0 citationsarXiv
Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies2603.24020v2 · Zhihao Yin, Go Ogiya, Frank C. van den Bosch2026 · 1 citationMon Not R Astron Soc (2026)
Recovering the infall mass for Milky Way satellite galaxy Sextans2603.08940v1 · Tingting Tian, Jiang Chang, Go Ogiya et al.2026 · 0 citationsarXiv
New insights on low-mass dark matter subhalo tidal tracks via numerical simulations2506.01152v2 · Alejandra Aguirre-Santaella, Miguel A. S'anchez-Conde, Go Ogiya2025 · 3 citationsMon Not R Astron Soc (2025)
Prograde and retrograde stars in nuclear cluster mergers. Evolution of the supermassive black hole binary and the host galactic nucleus2411.05063v1 · Alessandra Mastrobuono-Battisti, Pau Amaro Seoane, Marius Josep Fullana i Alfonso et al.2024 · 0 citationsarXiv
Environmental effects on Low Surface Brightness Galaxies in the IllustrisTNG simulation2407.15529v1 · Luis Enrique P'erez-Montano, Bernardo Cervantes Sodi, Vicente Rodriguez-Gomez et al.2024 · 13 citationsarXiv
Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations2312.02275v3 · Diptajyoti Mukherjee, A. Miguel Holgado, Go Ogiya et al.2023 · 15 citationsarXiv
Formation of dense filaments induced by runaway supermassive black holes2309.09031v3 · Go Ogiya, Daisuke Nagai2023 · 7 citationsarXiv
Searching for clues of past binary supermassive black hole mergers in nuclear star clusters2303.12826v1 · Alessandra Mastrobuono-Battisti, Go Ogiya, Oliver Hahn et al.2023 · 7 citationsarXivon Valency
The effect of stellar encounters on the dark matter annihilation signal from prompt cusps2301.04670v2 · Jens Stucker, Go Ogiya, Simon D.M. White et al.2023 · 16 citationsarXiv
Testing the galaxy collision induced formation scenario for the trail of dark matter deficient galaxies with the susceptibility of globular clusters to the tidal force2211.05993v1 · Go Ogiya, Frank C. van den Bosch, Andreas Burkert et al.2022 · 8 citationsarXiv
Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations2207.08652v1 · Alejandra Aguirre-Santaella, Miguel A. S'anchez-Conde, Go Ogiya et al.2022 · 18 citationsarXiv
Tidal Stripping in the Adiabatic Limit2207.00604v2 · Jens Stucker, Go Ogiya, Raul E. Angulo et al.2022 · 31 citationsarXiv
Evolution of Massive Black Hole Binaries in Collisionally Relaxed Nuclear Star Clusters -- Impact of Mass Segregation2205.12289v2 · Diptajyoti Mukherjee, Qirong Zhu, Go Ogiya et al.2022 · 8 citationsarXiv
Dark matter cores in massive high- galaxies formed by baryonic clumps2205.04577v1 · Go Ogiya, Daisuke Nagai2022 · 12 citationsarXiv
On the Tidal Formation of Dark Matter Deficient Galaxies2111.12104v2 · Go Ogiya, Frank C. van den Bosch, Andreas Burkert2021 · 33 citationsarXiv
Evolution of subhalo orbits in a smoothly-growing host halo potential2102.02786v1 · Go Ogiya, James E. Taylor, Michael J. Hudson2021 · 18 citationsarXiv
Dynamical self-friction: how mass loss slows you down2001.06489v1 · Tim B. Miller, Frank C. van den Bosch, Sheridan B. Green et al.2020 · 28 citationsMNRAS 495, 4496 (2020)
Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters1911.11526v2 · Go Ogiya, Oliver Hahn, Chiara M. F. Mingarelli et al.2019 · 33 citationsarXiv
DASH: a library of dynamical subhalo evolution1901.08601v1 · Go Ogiya, Frank C. van den Bosch, Oliver Hahn et al.2019 · 54 citationsMNRAS 485, 189 (2019)
Tidal stripping as a possible origin of the ultra diffuse galaxy lacking dark matter1804.06421v2 · Go Ogiya2018 · 106 citationsarXiv
Physical and numerical stability and instability of AGN bubbles in a hot intracluster medium1802.02177v1 · Go Ogiya, Pawel Biernacki, Oliver Hahn et al.2018 · 2 citationsarXiv
Dark Matter Substructure in Numerical Simulations: A Tale of Discreteness Noise, Runaway Instabilities, and Artificial Disruption1801.05427v1 · Frank C. van den Bosch, Go Ogiya2018 · 289 citationsarXiv
Disruption of Dark Matter Substructure: Fact or Fiction?1711.05276v1 · Frank C. van den Bosch, Go Ogiya, Oliver Hahn et al.2017 · 315 citationsarXiv
What sets the central structure of dark matter haloes?1707.07693v2 · Go Ogiya, Oliver Hahn2017 · 46 citationsarXiv
Universal dark halo scaling relation for the dwarf spheroidal satellites1703.02604v1 · Kohei Hayashi, Tomoaki Ishiyama, Go Ogiya et al.2017 · 7 citationsarXiv
Dynamical Evolution of Primordial Dark Matter Haloes through Mergers1604.02866v2 · Go Ogiya, Daisuke Nagai, Tomoaki Ishiyama2016 · 41 citationsarXiv
Dynamical friction and scratches of orbiting satellite galaxies on host systems1510.07892v2 · Go Ogiya, Andreas Burkert2015 · 23 citationsarXiv
Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores1408.6444v2 · Go Ogiya, Andreas Burkert2014 · 27 citationsarXiv
The connection between the cusp-to-core transformation and observational universalities of DM halos1309.1646v2 · Go Ogiya, Masao Mori, Tomoaki Ishiyama et al.2013 · 26 citationsarXiv
The Core-Cusp Problem in Cold Dark Matter Halos and Supernova Feedback: Effects of Oscillation1206.5412v3 · Go Ogiya, Masao Mori2012 · 66 citationsApJ, 793, 46 (2014)
Astrophysical Particle Simulations on Heterogeneous CPU-GPU Systems1206.1199v1 · Naohito Nakasato, Go Ogiya, Yohei Miki et al.2012 · 7 citationsarXiv
The core-cusp problem in cold dark matter halos and supernova feedback: Effects of Mass Loss1106.2864v1 · Go Ogiya, Masao Mori2011 · 49 citationsarXiv
Career total: 53 works. 33 are in this corpus.
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