The DOI matches its Crossref record.
Readout modes and automated operation of the Swift X-ray Telescope
Abstract
The Swift X-ray Telescope (XRT) is designed to make astrometric, spectroscopic, and photometric observations of X-ray emission from Gamma-ray Bursts and their afterglows in the energy band 0.2-10 keV. In order to provide rapid-response, automated observations of these randomly occurring objects without ground intervention, the XRT must be able to observe objects covering some seven orders of magnitude in flux, extracting the maximum possible science from each one. This requires a variety of readout modes designed to optimise the information collected in response to shifting scientific priorities as the flux from the burst diminishes. The XRT will support four major readout modes: imaging, two timing modes and photon-counting, with several sub-modes. We describe in detail the readout modes of the XRT. We describe the flux ranges over which each mode will operate, the automated mode switching that will occur and the methods used for collection of bias information for this instrument. We also discuss the data products produced from each mode.
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
Burrows, D. N., Hill, J. E., Nousek, J. A., Kennea, J. A., Wells, A., Osborne, J. P., Abbey, A. F., Beardmore, A., Mukerjee, K., Short, A. D. T., et al. (2005) · Space Science Reviews · doi:10.1007/s11214-005-5097-2 · Cited by 2,641
Self-citationShappee, B. J., Prieto, J. L., Grupe, D., Kochanek, C. S., Stanek, K. Z., De Rosa, G., Mathur, S., Zu, Y., Peterson, B. M., Pogge, R. W., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/788/1/48 · Cited by 1,887
THE SPECTRAL ENERGY DISTRIBUTION OF FERMI BRIGHT BLAZARS
Abdo, A. A., Ackermann, M., Agudo, I., Ajello, M., Aller, H. D., Aller, M. F., Angelakis, E., Arkharov, A. A., Axelsson, M., Bach, U., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/716/1/30 · Cited by 1,019
Self-citationAn online repository of Swift/XRT light curves of $\vec \gamma$-ray bursts
Evans, P. A., Beardmore, A. P., Page, K. L., Tyler, L. G., Osborne, J. P., Goad, M. R., O'Brien, P. T., Vetere, L., Racusin, J., Morris, D., et al. (2007) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20077530 · Cited by 891
Self-citationThe Early X‐Ray Emission from GRBs
O’Brien, P. T., Willingale, R., Osborne, J., Goad, M. R., Page, K. L., Vaughan, S., Rol, E., Beardmore, A., Godet, O., Hurkett, C. P., et al. (2006) · The Astrophysical Journal · doi:10.1086/505457 · Cited by 414
Self-citation
Metadata
- Authors
- Hill, J. E., Burrows, D. N., Nousek, J. A., Abbey, A. F., Ambrosi, R. M., Brauninger, H. W., Burkert, W., Campana, S., Cheruvu, C., Cusumano, G., Freyberg, M. J., Hartner, G. D., Klar, R., Mangels, C., Moretti, A., Mori, K., Morris, D. C., Short, A. D. T., Tagliaferri, G., Watson, D. J., Wood, P., & Wells, A. A.
- Venue
- SPIE Proceedings
- Publisher
- SPIE
- Published
- 2004-02-03
- Volume
- 5165
- Pages
- 217
- ISSN
- 0277-786X (ISSN-L)
- OpenAlex
- W2134413610
- Cited by
- 210
- References
- 0
- FWCI
- 27.44
- Type
- conference paper
- Language
- en
- Open access
- closed
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: Readout modes and automated operation of the Swift X-ray Telescope. https://app.cochat.ai/papers/10.1117/12.505728
- The paper
- Hill, J. E., Burrows, D. N., Nousek, J. A., Abbey, A. F., Ambrosi, R. M., Brauninger, H. W., Burkert, W., Campana, S., Cheruvu, C., Cusumano, G., Freyberg, M. J., Hartner, G. D., Klar, R., Mangels, C., Moretti, A., Mori, K., Morris, D. C., Short, A. D. T., Tagliaferri, G., . . . Wells, A. A. (2004). Readout modes and automated operation of the Swift X-ray Telescope. SPIE Proceedings. https://doi.org/10.1117/12.505728
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.