The DOI matches its Crossref record.
The Discovery of Rapid X-Ray Oscillations in the Tail of the SGR 1806-20 Hyperflare
Open accessAbstract
We have discovered rapid quasi-periodic oscillations (QPOs) in RXTE /PCA measurements of the pulsating tail of the 2004 December 27 giant flare of SGR 1806-20. QPOs at ~92.5 Hz are detected in a 50 s interval starting 170 s after the onset of the giant flare. These QPOs appear to be associated with increased emission by a relatively hard unpulsed component and are seen only over phases of the 7.56 s spin period pulsations away from the main peak. QPOs at ~18 and ~30 Hz are also detected ~200-300 s after the onset of the giant flare. This is the first time that QPOs are unambiguously detected in the flux of a soft gamma-ray repeater or any other magnetar candidate. We interpret the highest QPOs in terms of the coupling of toroidal seismic modes with Alfvén waves propagating along magnetospheric field lines. The lowest frequency QPO might instead provide indirect evidence on the strength of the internal magnetic field of the magnetar.
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.
Integrity signals
Registry
Cites
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.
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
Cited by
Color superconductivity in dense quark matter
Alford, M. G., Schmitt, A., Rajagopal, K., & Schäfer, T. (2008) · Reviews of Modern Physics · doi:10.1103/revmodphys.80.1455 · Cited by 1,443
The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars
Mereghetti, S. (2008) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-008-0011-z · Cited by 673
Magnetars: the physics behind observations. A review
Turolla, R., Zane, S., & Watts, A. L. (2015) · Reports on Progress in Physics · doi:10.1088/0034-4885/78/11/116901 · Cited by 447
Discovery of Fast X-Ray Oscillations during the 1998 Giant Flare from SGR 1900+14
Strohmayer, T. E., & Watts, A. L. (2005) · The Astrophysical Journal · doi:10.1086/497911 · Cited by 273
The tensor-vector-scalar theory and its cosmology
Skordis, C. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/14/143001 · Cited by 184
Metadata
- Authors
- Israel, G. L., Belloni, T., Stella, L., Rephaeli, Y., Gruber, D. E., Casella, P., Dall'Osso, S., Rea, N., Persic, M., & Rothschild, R. E.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2005-06-27
- Volume
- 628
- Issue
- 1
- Pages
- L53-L56
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2029327327
- Cited by
- 373
- References
- 0
- FWCI
- 13.86
- 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 Discovery of Rapid X-Ray Oscillations in the Tail of the SGR 1806-20 Hyperflare. https://app.cochat.ai/papers/10.1086/432615
- The paper
- Israel, G. L., Belloni, T., Stella, L., Rephaeli, Y., Gruber, D. E., Casella, P., Dall'Osso, S., Rea, N., Persic, M., & Rothschild, R. E. (2005). The Discovery of Rapid X-Ray Oscillations in the Tail of the SGR 1806-20 Hyperflare. The Astrophysical Journal. https://doi.org/10.1086/432615
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.