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High-definition imaging of a filamentary connection between a close quasar pair at z = 3

Tornotti, Davide; Fumagalli, Michele; Fossati, Matteo; Benitez-Llambay, Alejandro; Izquierdo-Villalba, David; Travascio, Andrea; Arrigoni Battaia, Fabrizio; Cantalupo, Sebastiano; Beckett, Alexander; Bonoli, Silvia; Dayal, Pratika; D’Odorico, Valentina; Dutta, Rajeshwari; Lusso, Elisabeta; Peroux, Celine; Rafelski, Marc; Revalski, Mitchell; Spinoso, Daniele; Swinbank, Mark

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Authors

Davide Tornotti

Matteo Fossati

Alejandro Benitez-Llambay

David Izquierdo-Villalba

Andrea Travascio

Fabrizio Arrigoni Battaia

Sebastiano Cantalupo

Silvia Bonoli

Pratika Dayal

Valentina D’Odorico

Rajeshwari Dutta

Celine Peroux

Marc Rafelski

Mitchell Revalski

Daniele Spinoso



Abstract

Filaments connecting haloes are a long-standing prediction of cold-dark-matter theories. Here we present a detection of the cosmic web emission connecting two quasar-host galaxies at redshift z ≈ 3.22 in the MUSE Ultra Deep Field (MUDF), observed with the Multi Unit Spectroscopic Explorer (MUSE) instrument. The very deep observations unlock a high-definition view of the filament morphology, a measure of the transition radius between the intergalactic and circumgalactic medium, and the characterization of the surface brightness profiles along the filament and in the transverse direction. Through systematic comparisons with simulations, we validate the filaments’ typical density predicted in the current cold-dark-matter model. Our analysis of the MUDF, an excellent laboratory for quantitatively studying filaments in emission, opens a new avenue to constrain the physical properties of the cosmic web and to trace the distribution of dark matter on large scales.

Citation

Tornotti, D., Fumagalli, M., Fossati, M., Benitez-Llambay, A., Izquierdo-Villalba, D., Travascio, A., Arrigoni Battaia, F., Cantalupo, S., Beckett, A., Bonoli, S., Dayal, P., D’Odorico, V., Dutta, R., Lusso, E., Peroux, C., Rafelski, M., Revalski, M., Spinoso, D., & Swinbank, M. (online). High-definition imaging of a filamentary connection between a close quasar pair at z = 3. Nature Astronomy, https://doi.org/10.1038/s41550-024-02463-w

Journal Article Type Article
Acceptance Date Nov 29, 2024
Online Publication Date Jan 29, 2025
Deposit Date Mar 27, 2025
Publicly Available Date Mar 27, 2025
Journal Nature Astronomy
Electronic ISSN 2397-3366
Publisher Nature Research
Peer Reviewed Peer Reviewed
DOI https://doi.org/10.1038/s41550-024-02463-w
Public URL https://durham-repository.worktribe.com/output/3743014
Other Repo URL https://arxiv.org/abs/2406.17035

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