Article 5WRCC To Find the First Galaxies, Webb Space Telescope Pays Attention to Detail and Theory

To Find the First Galaxies, Webb Space Telescope Pays Attention to Detail and Theory

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To Find the First Galaxies, Webb Space Telescope Pays Attention to Detail and Theory:

As the Webb team continues to make progress in aligning the telescope, other successful activities include the calibration of the NIRISS filter wheel and pupil wheel tuning for NIRCam. There are hundreds of activities like these planned during the commissioning process, and each is as important as the next to ensure that Webb can achieve its ambitious science goals. One such goal - detecting the earliest galaxies - also requires a lot of planning and theory to prepare for the observations. L.Y. Aaron Yung, a postdoc at NASA's Goddard Space Flight Center, tells us more about the important theoretical work that helps plan for and then analyze galaxy surveys:

"This summer, Webb will start searching for galaxies in the distant universe. These highly anticipated observations are the key to unlocking the secrets in galaxy evolution and our universe's history. Depending on the specific science goal of an observing program, the best-suited survey configurations can vary a lot.

"For instance, galaxy surveys going after the faintest and most distant galaxies require long exposure times (e.g., NGDEEP, PRIMER), but surveys for large-scale cosmological structure would require large survey areas (e.g., COSMOS-Web). Inputs from physically motivated simulations are essential to developing optimal observing strategies to achieve the specific scientific goals.

"To create a simulated universe, we first lay the foundation with dark matter concentrations, or halos, extracted from cosmological simulations. Dark matter accounts for 85% of the matter in the universe and has a dominant effect on the spatial distributions of galaxies across the universe. We then simulate the galaxies forming inside these dark matter halos based on astrophysical processes we learned from past observations.

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