Student or educator? Sign up with your school email and get 6 months of Pro free.
CoChat
Sign Up
Cited by 2,355

The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.

The Einstein Telescope: a third-generation gravitational wave observatory

Open access
Punturo, M, Abernathy, M, Acernese, F, Allen, B, Andersson, N, Arun, K, Barone, F, Barr, B, Barsuglia, M, Beker, M, Beveridge, N, Birindelli, S, Bose, S, Bosi, L, Braccini, S, Bradaschia, C, Bulik, T, Calloni, E, Cella, G, Mottin, E Chassande, Chelkowski, S, Chincarini, A, Clark, J, Coccia, E, Colacino, C, Colas, J, Cumming, A, Cunningham, L, Cuoco, E, Danilishin, S, Danzmann, K, De Luca, G, De Salvo, R, Dent, T, De Rosa, R, Di Fiore, L, Di Virgilio, A, Doets, M, Fafone, V, Falferi, P, Flaminio, R, Franc, J, Frasconi, F, Freise, A, Fulda, P, Gair, J, Gemme, G, Gennai, A, Giazotto, A, Glampedakis, K, Granata, M, Grote, H, Guidi, G, Hammond, G, Hannam, M, Harms, J, Heinert, D, Hendry, M, Heng, I, Hennes, E, Hild, S, Hough, J, Husa, S, Huttner, S, Jones, G, Khalili, F, Kokeyama, K, Kokkotas, K, Krishnan, B, Lorenzini, M, Lück, H, Majorana, E, Mandel, I, Mandic, V, Martin, I, Michel, C, Minenkov, Y, Morgado, N, Mosca, S, Mours, B, Müller–Ebhardt, H, Murray, P, Nawrodt, R, Nelson, J, Oshaughnessy, R, Ott, C D, Palomba, C, Paoli, A, Parguez, G, Pasqualetti, A, Passaquieti, R, Passuello, D, Pinard, L, Poggiani, R, Popolizio, P, Prato, M, Puppo, P, Rabeling, D, Rapagnani, P, Read, J, Regimbau, T, Rehbein, H, Reid, S, Rezzolla, L, Ricci, F, Richard, F, Rocchi, A, Rowan, S, Rüdiger, A, Sassolas, B, Sathyaprakash, B, Schnabel, R, Schwarz, C, Seidel, P, Sintes, A, Somiya, K, Speirits, F, Strain, K, Strigin, S, Sutton, P, Tarabrin, S, Thüring, A, van den Brand, J, van Leewen, C, van Veggel, M, van den Broeck, C, Vecchio, A, Veitch, J, Vetrano, F, Vicere, A, Vyatchanin, S, Willke, B, Woan, G, Wolfango, P, Yamamoto, K·2010·Classical and Quantum Gravity
DOI 10.1088/0264-9381/27/19/194002
Open this paper in CoChat — free account

Abstract

Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improved sensitivity of the third generation of gravitational wave observatories could permit detailed measurements of the sources' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sources obtained through other kinds of telescopes. This paper describes the progress of the ET project which is currently in its design study phase.

Overview

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1088/0264-9381/27/19/194002

Cites

14 of 14 references verified0 citation errors · 0 not checkable

Statistics

Verification

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Citations

Cites

Show all 14 references

Cited by

See all 2,355

Metadata

Authors
Punturo, M., Abernathy, M., Acernese, F., Allen, B., Andersson, N., Arun, K., Barone, F., Barr, B., Barsuglia, M., Beker, M., Beveridge, N., Birindelli, S., Bose, S., Bosi, L., Braccini, S., Bradaschia, C., Bulik, T., Calloni, E., Cella, G., Mottin, E. C., Chelkowski, S., Chincarini, A., Clark, J., Coccia, E., Colacino, C., Colas, J., Cumming, A., Cunningham, L., Cuoco, E., Danilishin, S., Danzmann, K., De Luca, G., De Salvo, R., Dent, T., De Rosa, R., Di Fiore, L., Di Virgilio, A., Doets, M., Fafone, V, Falferi, P., Flaminio, R., Franc, J., Frasconi, F., Freise, A., Fulda, P., Gair, J., Gemme, G., Gennai, A., Giazotto, A., Glampedakis, K., Granata, M., Grote, H., Guidi, G., Hammond, G., Hannam, M., Harms, J., Heinert, D., Hendry, M., Heng, I., Hennes, E., Hild, S., Hough, J., Husa, S., Huttner, S., Jones, G., Khalili, F., Kokeyama, K., Kokkotas, K., Krishnan, B., Lorenzini, M., Lück, H., Majorana, E., Mandel, I., Mandic, V, Martin, I., Michel, C., Minenkov, Y., Morgado, N., Mosca, S., Mours, B., Müller–Ebhardt, H., Murray, P., Nawrodt, R., Nelson, J., Oshaughnessy, R., Ott, C. D., Palomba, C., Paoli, A., Parguez, G., Pasqualetti, A., Passaquieti, R., Passuello, D., Pinard, L., Poggiani, R., Popolizio, P., Prato, M., Puppo, P., Rabeling, D., Rapagnani, P., Read, J., Regimbau, T., Rehbein, H., Reid, S., Rezzolla, L., Ricci, F., Richard, F., Rocchi, A., Rowan, S., Rüdiger, A., Sassolas, B., Sathyaprakash, B., Schnabel, R., Schwarz, C., Seidel, P., Sintes, A., Somiya, K., Speirits, F., Strain, K., Strigin, S., Sutton, P., Tarabrin, S., Thüring, A., van den Brand, J., van Leewen, C., van Veggel, M., van den Broeck, C., Vecchio, A., Veitch, J., Vetrano, F., Vicere, A., Vyatchanin, S., Willke, B., Woan, G., Wolfango, P., & Yamamoto, K.
Venue
Classical and Quantum Gravity
Publisher
IOP Publishing
Published
2010-09-21
Volume
27
Issue
19
Pages
194002
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
DOI
10.1088/0264-9381/27/19/194002
OpenAlex
W2061083933
Cited by
2,355
References
14
FWCI
14.95
Type
journal article
Language
en
Open access
bronze

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review

How to cite

Cite CoChat for the checks on this page, and the paper for its own findings.

This page
CoChat. (2026). Citation check: The Einstein Telescope: a third-generation gravitational wave observatory. https://app.cochat.ai/papers/10.1088/0264-9381/27/19/194002
The paper
Punturo, M., Abernathy, M., Acernese, F., Allen, B., Andersson, N., Arun, K., Barone, F., Barr, B., Barsuglia, M., Beker, M., Beveridge, N., Birindelli, S., Bose, S., Bosi, L., Braccini, S., Bradaschia, C., Bulik, T., Calloni, E., Cella, G., . . . Yamamoto, K. (2010). The Einstein Telescope: a third-generation gravitational wave observatory. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/27/19/194002

Data sources

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.