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• W4309201923 abstract "We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg$^2$ NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5$sigma$ point source depths ranging $sim$27.5-28.2 magnitudes. In parallel, we will obtain 0.19 deg$^2$ of MIRI imaging in one filter (F770W) reaching 5$sigma$ point source depths of $sim$25.3-26.0 magnitudes. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization ($6<z<11$) and map reionization's spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at $z>4$ and place constraints on the formation of the Universe's most massive galaxies ($M_star>10^{10}$,M$_odot$), and (3) directly measure the evolution of the stellar mass to halo mass relation using weak gravitational lensing out to $zsim2.5$ and measure its variance with galaxies' star formation histories and morphologies. In addition, we anticipate COSMOS-Web's legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool sub-dwarf stars in the Galactic halo, and possibly the identification of $z>10$ pair-instability supernovae. In this paper we provide an overview of the survey's key measurements, specifications, goals, and prospects for new discovery." @default.
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• W4309201923 date "2022-11-14" @default.
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• W4309201923 title "COSMOS-Web: An Overview of the JWST Cosmic Origins Survey" @default.
• W4309201923 doi "https://doi.org/10.48550/arxiv.2211.07865" @default.
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