Student or educator? Sign up with your school email and get 6 months of Pro free.
Cited by 599

The DOI matches its Crossref record.

A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225

Open access
Gehrels, N., Sarazin, C. L., O'Brien, P. T., Zhang, B., Barbier, L., Barthelmy, S. D., Blustin, A., Burrows, D. N., Cannizzo, J., Cummings, J. R., Goad, M., Holland, S. T., Hurkett, C. P., Kennea, J. A., Levan, A., Markwardt, C. B., Mason, K. O., Meszaros, P., Page, M., Palmer, D. M., Rol, E., Sakamoto, T., Willingale, R., Angelini, L., Beardmore, A., Boyd, P. T., Breeveld, A., Campana, S., Chester, M. M., Chincarini, G., Cominsky, L. R., Cusumano, G., de Pasquale, M., Fenimore, E. E., Giommi, P., Gronwall, C., Grupe, D., Hill, J. E., Hinshaw, D., Hjorth, J., Hullinger, D., Hurley, K. C., Klose, S., Kobayashi, S., Kouveliotou, C., Krimm, H. A., Mangano, V., Marshall, F. E., McGowan, K., Moretti, A., Mushotzky, R. F., Nakazawa, K., Norris, J. P., Nousek, J. A., Osborne, J. P., Page, K., Parsons, A. M., Patel, S., Perri, M., Poole, T., Romano, P., Roming, P. W. A., Rosen, S., Sato, G., Schady, P., Smale, A. P., Sollerman, J., Starling, R., Still, M., Suzuki, M., Tagliaferri, G., Takahashi, T., Tashiro, M., Tueller, J., Wells, A. A., White, N. E., Wijers, R. A. M. J.·2005·Nature

Abstract

Gamma-ray bursts (GRBs) come in two classes: long (> 2 s), soft-spectrum bursts and short, hard events. Most progress has been made on understanding the long GRBs, which are typically observed at high redshift (z ≈ 1) and found in subluminous star-forming host galaxies. They are likely to be produced in core-collapse explosions of massive stars. In contrast, no short GRB had been accurately (< 10″) and rapidly (minutes) located. Here we report the detection of the X-ray afterglow from—and the localization of—the short burst GRB 050509B. Its position on the sky is near a luminous, non-star-forming elliptical galaxy at a redshift of 0.225, which is the location one would expect if the origin of this GRB is through the merger of neutron-star or black-hole binaries. The X-ray afterglow was weak and faded below the detection limit within a few hours; no optical afterglow was detected to stringent limits, explaining the past difficulty in localizing short GRBs.

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 · 10.1038/nature04142

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.

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

Cited by

See all 599

Metadata

Authors
Gehrels, N., Sarazin, C. L., O'Brien, P. T., Zhang, B., Barbier, L., Barthelmy, S. D., Blustin, A., Burrows, D. N., Cannizzo, J., Cummings, J. R., Goad, M., Holland, S. T., Hurkett, C. P., Kennea, J. A., Levan, A., Markwardt, C. B., Mason, K. O., Meszaros, P., Page, M., Palmer, D. M., Rol, E., Sakamoto, T., Willingale, R., Angelini, L., Beardmore, A., Boyd, P. T., Breeveld, A., Campana, S., Chester, M. M., Chincarini, G., Cominsky, L. R., Cusumano, G., de Pasquale, M., Fenimore, E. E., Giommi, P., Gronwall, C., Grupe, D., Hill, J. E., Hinshaw, D., Hjorth, J., Hullinger, D., Hurley, K. C., Klose, S., Kobayashi, S., Kouveliotou, C., Krimm, H. A., Mangano, V., Marshall, F. E., McGowan, K., Moretti, A., Mushotzky, R. F., Nakazawa, K., Norris, J. P., Nousek, J. A., Osborne, J. P., Page, K., Parsons, A. M., Patel, S., Perri, M., Poole, T., Romano, P., Roming, P. W. A., Rosen, S., Sato, G., Schady, P., Smale, A. P., Sollerman, J., Starling, R., Still, M., Suzuki, M., Tagliaferri, G., Takahashi, T., Tashiro, M., Tueller, J., Wells, A. A., White, N. E., & Wijers, R. A. M. J.
Venue
Nature
Published
2005-10
Volume
437
Issue
7060
Pages
851-854
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W2167504726
Cited by
599
References
0
FWCI
36.70
Type
journal article
Language
en
Open access
green

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: A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225. https://app.cochat.ai/papers/10.1038/nature04142
The paper
Gehrels, N., Sarazin, C. L., O'Brien, P. T., Zhang, B., Barbier, L., Barthelmy, S. D., Blustin, A., Burrows, D. N., Cannizzo, J., Cummings, J. R., Goad, M., Holland, S. T., Hurkett, C. P., Kennea, J. A., Levan, A., Markwardt, C. B., Mason, K. O., Meszaros, P., Page, M., . . . Wijers, R. A. M. J. (2005). A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225. Nature. https://doi.org/10.1038/nature04142

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.