Wide-Field InfraRed Survey Telescope WFIRST Final Report

By J. Green, C. Hirata, L. Hillenbrand, G. Helou, R. Cutri. 2012

166 citations recorded by the source corpus.

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Citations in the corpus

Enabling Dark Energy Science with Deep Generative Models of Galaxy Images (2016, background): “Yet we lack an understanding of what dark energy actually is, which provides one of the main motivations behind the next generation of cosmological surveys such as LSST LSST Science Collaboration et al. (2009), Euclid Laureijs et al. (2011) and WFIRST Green et al. (2012).”
Predictions of the WFIRST Microlensing Survey. I. Bound Planet Detection Rates (2018, methodology): “A new SDT was assembled to produce an AFTA DRM, which added a coronagraphic instrument channel to the mission (Spergel et al. 2013).”
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of f(z)σ8(z) on constraining dark energy (2013, background): “3 z 2.7 over 3400 deg2, with a larger area possible with an extended mission (Green et al.2012).”
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering (2013, background): “The proposed WFIRST3 satellite would map 17 million galaxies in the redshift range 1.3 < z < 2.7 over 3400 deg2, with a larger area possible with an extended mission (Green et al. 2012).”
EFFECT OF A HIGH OPACITY ON THE LIGHT CURVES OF RADIOACTIVELY POWERED TRANSIENTS FROM COMPACT OBJECT MERGERS (2013, methodology): “The construction of space based facilities such as WFIRST (Green et al. 2012) and Euclid (Amendola et al. 2012) would be of particular interest.”
RADIOACTIVITY AND THERMALIZATION IN THE EJECTA OF COMPACT OBJECT MERGERS AND THEIR IMPACT ON KILONOVA LIGHT CURVES (2016, background): “Euclid (Amendola et al. 2012) and WFIRST (Green et al. 2012), each which will have an H-band depth of ∼25, could detect a typical NS2 kilonova, located at 100 Mpc, out to ~t 15 days.”
RADIATIVE TRANSFER SIMULATIONS OF NEUTRON STAR MERGER EJECTA (2013, background): “The Wide-Field Infrared Survey Telescope (WFIRST; Green et al. 2012) and the Wide-field Imaging Surveyor for High-redshift (WISH; Yamada et al. 2012) are planned to perform wide-field surveys at NIR wavelengths.”