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Cited by 282

The DOI matches its Crossref record; 226 of the 226 references it cites were found in a registry or an index.

Unveiling the gravitational universe at μ-Hz frequencies

Open access
Sesana, Alberto, Korsakova, Natalia, Sedda, Manuel Arca, Baibhav, Vishal, Barausse, Enrico, Barke, Simon, Berti, Emanuele, Bonetti, Matteo, Capelo, Pedro R., Caprini, Chiara, Garcia-Bellido, Juan, Haiman, Zoltan, Jani, Karan, Jennrich, Oliver, Johansson, Peter H., Khan, Fazeel Mahmood, Korol, Valeriya, Lamberts, Astrid, Lupi, Alessandro, Mangiagli, Alberto, Mayer, Lucio, Nardini, Germano, Pacucci, Fabio, Petiteau, Antoine, Raccanelli, Alvise, Rajendran, Surjeet, Regan, John, Shao, Lijing, Spallicci, Alessandro, Tamanini, Nicola, Volonteri, Marta, Warburton, Niels, Wong, Kaze, Zumalacarregui, Miguel·2021·Experimental Astronomy
DOI 10.1007/s10686-021-09709-9
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Abstract

We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.

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Metadata

Authors
Sesana, A., Korsakova, N., Sedda, M. A., Baibhav, V., Barausse, E., Barke, S., Berti, E., Bonetti, M., Capelo, P. R., Caprini, C., Garcia-Bellido, J., Haiman, Z., Jani, K., Jennrich, O., Johansson, P. H., Khan, F. M., Korol, V., Lamberts, A., Lupi, A., Mangiagli, A., Mayer, L., Nardini, G., Pacucci, F., Petiteau, A., Raccanelli, A., Rajendran, S., Regan, J., Shao, L., Spallicci, A., Tamanini, N., Volonteri, M., Warburton, N., Wong, K., & Zumalacarregui, M.
Venue
Experimental Astronomy
Publisher
Springer Science and Business Media LLC
Published
2021-06
Volume
51
Issue
3
Pages
1333-1383
ISSN
  • 0922-6435 (ISSN-L)
  • 1572-9508
DOI
10.1007/s10686-021-09709-9
OpenAlex
W3196450357
Cited by
282
References
226
FWCI
21.25
Type
journal article
Language
en
Open access
hybrid

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CoChat. (2026). Citation check: Unveiling the gravitational universe at μ-Hz frequencies. https://app.cochat.ai/papers/10.1007/s10686-021-09709-9
The paper
Sesana, A., Korsakova, N., Sedda, M. A., Baibhav, V., Barausse, E., Barke, S., Berti, E., Bonetti, M., Capelo, P. R., Caprini, C., Garcia-Bellido, J., Haiman, Z., Jani, K., Jennrich, O., Johansson, P. H., Khan, F. M., Korol, V., Lamberts, A., Lupi, A., . . . Zumalacarregui, M. (2021). Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy. https://doi.org/10.1007/s10686-021-09709-9

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.