The team will measure everything that is between us and the quasars with NIRSpec. Only after the first billion years of the universe did the gas become fully transparent, allowing light to travel more easily. What was the universe like 700 or 800 million years after the big bang? This was a period known as the Era of Reionization, when the gas between galaxies was largely opaque. Webb's expansive, high-resolution observations will help the team characterize the galaxies that are in the neighborhood by employing Webb's Near-Infrared Imager and Slitless Spectrograph (NIRISS) and NIRCam.įinally, the researchers will also sample the large-scale environments around the quasars-the characteristics of the gas and dust. They will also 'zoom out' to see galaxies near these quasars. Although no one can watch a complete feedback loop in real time (it takes millions of years!), they can sample what's present with NIRSpec and begin to observe the connections between the quasars and their host galaxies. The team will also obtain spectra of both the quasars and their host galaxies to trace how gas is moving in the host galaxies and determine if the active supermassive black holes are sending out hot winds that heat the galaxies' gas. Were these ancient galaxies more compact? Do their stars contain more than hydrogen and helium? Webb will certainly yield new insights. No one can fully predict what they'll learn. The team will also obtain spectra with Webb's Mid-Infrared Instrument (MIRI). The final, processed images will give them the first views of the light from the stars in the host galaxies. They will take very deep, detailed images of each target with Webb's Near-Infrared Camera (NIRCam) and then use computer models to remove the quasars' light from each. Next, they will focus on revealing the galaxies behind the quasars' bright light.

This will allow the team to produce more accurate black hole masses.

To increase the precision of existing measurements from other observatories, they'll turn to spectra-data that detail an object's physical properties, including mass and chemical composition, delivered by Webb's Near-Infrared Spectrograph (NIRSpec). 'We want to obtain more accurate measurements of their masses to improve our understanding of how they formed and grew so quickly.' 'The existence of these black holes challenges theoretical models,' Yang said.

First, they will refine the measurements of the mass of each supermassive black hole. 'That is why we want to provide the best characterization possible of each with Webb.'įan, Yang, and Bañados are wasting no opportunity: They will use almost every available instrument on Webb to observe these quasars. 'These quasars are very special objects,' explained Bañados.

The team plans to observe and analyze the data on three scales: closely examining the quasars themselves, studying the stars in the surrounding host galaxies after removing the quasars' light, and classifying the galaxies that lie nearby. Webb has unmatched sensitivity and spatial resolution, which will reveal complex structures in these distant objects. Webb's sensitivity to infrared light-including mid-infrared wavelengths that can only be captured from space-will allow the team to observe these objects, whose light has traveled for 13 billion years and has had its wavelengths stretched from ultraviolet and visible light into infrared light. 'We structured this program to learn everything we could think of so our team and the greater astronomical community can fully explore these quasars.' 'These are really valuable objects,' Fan said. These are questions Xiaohui Fan and Jinyi Yang, both of the University of Arizona, and Eduardo Bañados, of the Max Planck Institute for Astronomy in Heidelberg, Germany, with an international team of astronomers, will pursue with observations taken by the James Webb Space Telescope.

Quasar galaxy