James Webb Space Telescope

By J. McDowell. 2004

642 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/1f9c3c0ef1ede530d39087562e52eef84e897341

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Citations in the corpus

Active galactic nuclei: what’s in a name? (2017, methodology): “it/tgevcat To complement the 2FHL sample, and in an effort to construct a much larger list of targets for VHE observations, Chang et al. (2017) assembled the 2WHSP catalogue, a very large sample of confirmed and candidate blazars of the HSP”
CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results (2022, background): “The thirteen ERS programs cover a wide range of science topics and together have provided a wealth of information about early JWST performance and calibration.”
Unveiling the gravitational universe at μ-Hz frequencies (2019, background): “eration of X-ray missions, like the ESA L2 Advanced Telescope for High Energy Astrophysics (Athena, [189]) and the proposed NASA Lynx [115], will probe the emergence of the first quasars; the James Webb Space Telescope (JWST, [114])”
The physics of the intergalactic medium (2007, background): “Much improved Lyα emitter statistics are anticipated with current or upcoming narrow band surveys which may make it possible to realize these tests (Gardner et al., 2006; Horton et al., 2004; Ouchi et al., 2008; Stark et al., 2007b).”
Cosmic X-ray surveys of distant active galaxies (2015, background): “The ELTs will complement JWST in an analogous manner to how the current 8–10 m telescopes complement HST, with innovative instruments and ultra-deep imaging and spectroscopy over large FOVs.11”
LSST: From Science Drivers to Reference Design and Anticipated Data Products (2008, background): “Last but not least, the huge samples of various astronomical source populations will yield extremely rare objects for investigations by powerful facilities such as JWST (Gardner et al. 2006) and the next generation of 20-40 meter telescopes.”
Gravitational probes of dark matter physics (2017, unknown): “Astrometry (space based) Gaia(6) [470] JWST(7) [471] WFIRST [472]”
Distant radio galaxies and their environments (2008, background): “…detailed history of the formation and evolution of HzRGS and the surrounding protoclusters will be helped enormously with the advent of 30m -class ground-based telescopes in the optical and near-infrared and the James Webb Space Telescope (JWST) (Gardner et al 2006) in the near and mid-infrared.”
The Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Lyα Emission from Galaxies (2017, methodology): “Predictions for JWST JWST will be uniquely equipped to observe Lyα and rest-frame optical emission lines into Cosmic Dawn, with extremely sensitive spectrometers NIRSpec and NIRISS covering 1− 5µm in a large field of view (Gardner et al. 2006; Stiavelli et al. 2007).”
The James Webb Space Telescope Mission (2023, methodology): “We summarize the history, concept, scientific program, and technical performance of the James Webb Space Telescope (JWST, Webb; Gardner et al. 2006).”
Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure (2022, unknown): “The infrared instruments aboard the James Webb Space Telescope (Gardner et al. 2006; Beichman et al. 2012; Artigau et al. 2014; 3 Rieke et al. 2015; Labiano et al. 2021) will search for confirmation and spectral classification of this distant star to define its place on the Hertzsprung–Russell…”