The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
The Space Telescope Imaging Spectrograph Design
Open accessAbstract
The Space Telescope Imaging Spectrograph (STIS) instrument was installed on the Hubble Space Telescope ( HST ) during the second servicing mission, in 1997 February. Four bands cover the wavelength range of 115–1000 nm, with spectral resolving powers between 26 and 200,000. Camera modes are used for target acquisition and deep imaging. Correction for HST 's spherical aberration and astigmatism is included. The 115–170 nm range is covered by a CsI MAMA (Multianode Microchannel Array) detector and the 165–310 nm range by a Cs 2 Te MAMA, each with a format of 2048 × 2048 pixels, while the 305–555 and 550–1000 nm ranges are covered by a single CCD with a format of 1024 × 1024 pixels. The multiplexing advantage of using these two‐dimensional detectors compared with the 1 × 512 pixel detectors of the first‐generation spectrographs is 1 or 2 orders of magnitude, depending on the mode used. The relationship between the scientific goals and the instrument specifications and design is discussed.
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
Cites
The On-Orbit Performance of the Space Telescope Imaging Spectrograph
Kimble, R. A., Woodgate, B. E., Bowers, C. W., Kraemer, S. B., Kaiser, M. E., Gull, T. R., Heap, S. R., Danks, A. C., Boggess, A., Green, R. F., et al. (1998) · The Astrophysical Journal · doi:10.1086/311102 · Cited by 268
Self-citation
Cited by
Overview of the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Mission
Moos, H. W., Cash, W. C., Cowie, L. L., Davidsen, A. F., Dupree, A. K., Feldman, P. D., Friedman, S. D., Green, J. C., Green, R. F., Gry, C., et al. (2000) · The Astrophysical Journal · doi:10.1086/312795 · Cited by 666
Self-citationA probable giant planet imaged in the β Pictoris disk: VLT/NaCo deep L'-band imaging
Lagrange, A.-M., Gratadour, D., Chauvin, G., Fusco, T., Ehrenreich, D., Mouillet, D., Rousset, G., Rouan, D., Allard, F., Gendron, É., et al. (2009) · Astronomy & Astrophysics · doi:10.1051/0004-6361:200811325 · Cited by 572
THE COSMIC ORIGINS SPECTROGRAPH
Green, J. C., Froning, C. S., Osterman, S., Ebbets, D., Heap, S. H., Leitherer, C., Linsky, J. L., Savage, B. D., Sembach, K., Michael Shull, J., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/744/1/60 · Cited by 485
Self-citationFilippazzo, J. C., Rice, E. L., Faherty, J., Cruz, K. L., Van Gordon, M. M., & Looper, D. L. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/810/2/158 · Cited by 362
STIS CORONAGRAPHIC IMAGING OF FOMALHAUT: MAIN BELT STRUCTURE AND THE ORBIT OF FOMALHAUT b
Kalas, P., Graham, J. R., Fitzgerald, M. P., & Clampin, M. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/775/1/56 · Cited by 158
Metadata
- Authors
- Woodgate, B. E., Kimble, R. A., Bowers, C. W., Kraemer, S., Kaiser, M. E., Danks, A. C., Grady, J. F., Loiacono, J. J., Brumfield, M., Feinberg, L., Gull, T. R., Heap, S. R., Maran, S. P., Lindler, D., Hood, D., Meyer, W., VanHouten, C., Argabright, V., Franka, S., Bybee, R., Dorn, D., Bottema, M., Woodruff, R., Michika, D., Sullivan, J., Hetlinger, J., Ludtke, C., Stocker, R., Delamere, A., Rose, D., Becker, I., Garner, H., Timothy, J. G., Blouke, M., Joseph, C. L., Hartig, G., Green, R. F., Jenkins, E. B., Linsky, J. L., Hutchings, J. B., Moos, H. W., Boggess, A., Roesler, F., & Weistrop, D.
- Venue
- Publications of the Astronomical Society of the Pacific
- Publisher
- IOP Publishing
- Published
- 1998-10
- Volume
- 110
- Issue
- 752
- Pages
- 1183-1204
- ISSN
- 0004-6280 (ISSN-L)
- 1538-3873
- OpenAlex
- W1993217083
- Cited by
- 379
- References
- 1
- FWCI
- 66.22
- 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 Space Telescope Imaging Spectrograph Design. https://app.cochat.ai/papers/10.1086/316243
- The paper
- Woodgate, B. E., Kimble, R. A., Bowers, C. W., Kraemer, S., Kaiser, M. E., Danks, A. C., Grady, J. F., Loiacono, J. J., Brumfield, M., Feinberg, L., Gull, T. R., Heap, S. R., Maran, S. P., Lindler, D., Hood, D., Meyer, W., VanHouten, C., Argabright, V., Franka, S., . . . Weistrop, D. (1998). The Space Telescope Imaging Spectrograph Design. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/316243
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.