The DOI matches its Crossref record.
GLAST: the next-generation high energy gamma-ray astronomy mission
Overview
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Citations
Cited by
Domínguez, A., Primack, J. R., Rosario, D. J., Prada, F., Gilmore, R. C., Faber, S. M., Koo, D. C., Somerville, R. S., Pérez-Torres, M. A., Pérez-González, P., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17631.x · Cited by 710
The inert doublet model: an archetype for dark matter
Honorez, L. L., Nezri, E., Oliver, J. F., & Tytgat, M. H. G. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/02/028 · Cited by 667
Dark matter and collider phenomenology of universal extra dimensions
Hooper, D., & Profumo, S. (2007) · Physics Reports · doi:10.1016/j.physrep.2007.09.003 · Cited by 358
Cosmic ray nuclei, antiprotons and gamma rays in the galaxy: a new diffusion model
Evoli, C., Gaggero, D., Grasso, D., & Maccione, L. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/10/018 · Cited by 313
THE FERMI HAZE: A GAMMA-RAY COUNTERPART TO THE MICROWAVE HAZE
Dobler, G., Finkbeiner, D. P., Cholis, I., Slatyer, T., & Weiner, N. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/717/2/825 · Cited by 285
“The LAT (Large Area Telescope) on Fermi (see Gehrels & Michelson 1999 as well as the Fermi homepage9) is a pair-conversion telescope consisting of 16 layers of tungsten on top of a calorimeter with a thickness of 7 radiation lengths.”
Background
Metadata
- Authors
- GLAST Facility Science Team, Gehrels, N., & Michelson, P.
- Venue
- Astroparticle Physics
- Publisher
- Elsevier BV
- Published
- 1999-06
- Volume
- 11
- Issue
- 1-2
- Pages
- 277-282
- ISSN
- 0927-6505 (ISSN-L)
- OpenAlex
- W2069638808
- Cited by
- 249
- References
- 0
- FWCI
- 8.29
- Type
- journal article
- 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.
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How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: GLAST: the next-generation high energy gamma-ray astronomy mission. https://app.cochat.ai/papers/10.1016/s0927-6505(99)00066-3
- The paper
- GLAST Facility Science Team, Gehrels, N., & Michelson, P. (1999). GLAST: the next-generation high energy gamma-ray astronomy mission. Astroparticle Physics. https://doi.org/10.1016/s0927-6505(99)00066-3
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.