Scientists and other hungry-minded people are getting a lot of images and data from the james wbb space telescope The telescope has shown us the Pillars of Creation, the details of very young stars as they grow inside their dense cloaks of gas, and a Deep Field that has taken over from the Hubble's ground-breaking Deep Field and It is only the beginning.

The JWST has peered back in time to the Universe's earliest galaxies to look for clues to how they assemble and evolve.

The prime extragalactic areas for reionization and lensing science is one of the programs that the telescope observes. A team of researchers explained the program in a new paper. The paper is called "JWST PEARLS" The project overview and first results of the prime extragalactic areas for reionization and lensing science.

A mouthful of words, but we can break it down to figure out how relevant it is.

There is only one way to understand the Universe and what happened to us. We have to wind the clock back to before the Earth, the Sun, our Solar System, or even the Milky Way. All the other galaxies have vanished over the observational horizon because the Universe hasn't expanded yet.

“The main goal of PEARLS is to study the epoch of galaxy assembly, active galactic nucleus (AGN) growth, and First Light.”

From the paper “JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results.”

The light from ancient galaxies and the Universe's early days is only now reaching us after 13 billion years. The only way to look back in time and see the faintest, most red-shifted galaxies was to build a powerful telescope that could look back in time. They wanted to build a telescope that could see in theIR.

The JWST has met expectations so far.

“Webb’s images are truly phenomenal, really beyond my wildest dreams.”

Rogier Windhorst, lead author, JWST PEARLS.

There was a need to look back in time to the beginning of the universe. The program is called Extragalactic because it looks at fields of galaxies instead of individual galaxies. The Universe can be reionized to make it transparent. The end of the Dark Ages and the appearance of the first light were signaled by that. The light from objects behind a cluster can be amplified by the gravity of the structure. Astronomers can study objects at even longer distances.

Milestones in the history of the Universe (not to scale). The intergalactic gas was in a neutral state from about 300,000 years after the Big Bang until the light from the first generation of stars and galaxies began to ionize it. That brought an end to the Universe's Dark Age. The gas was completely ionized after 1 billion years. Image Credit: NAOJ.
Milestones in the history of the Universe (not to scale). The intergalactic gas was in a neutral state from about 300,000 years after the Big Bang until the light from the first generation of stars and galaxies began to ionize it. That brought an end to the Universe’s Dark Age. The gas was completely ionized after 1 billion years. Image Credit: NAOJ.

You get Pearls if you add it all together. The main goal of PEARLS is to study the first light. The main science goals of PEARLS are First Light and Reionization and Assembly of Galaxies.

The PEARLS images were assembled into large mosaics by a research astronomer at theSTScI. The PEARLS field allows us to see very rare galaxies at the beginning of the universe.

One of the first wide-field images of the universe has been captured. The North Ecliptic Pole is in the sky. The images show how distant objects can be seen from the foreground. The distant objects interact with each other. There are regions at the center of the universe where black holes can fall. SMBHs are an extremely active area of research and the AGN images should give clues to how they grow.

PEARLS has captured one of the first medium-deep wide-field images of the cosmos. This image is only one-quarter the size of the final image and features interacting galaxies with active nuclei. Click the image for a much larger, zoomable, version of the image. It's filled with red-shifted objects that date from the Universe's early days. Image Credit: SCIENCE: NASA, ESA, CSA, Rolf A. Jansen (ASU), Jake Summers (ASU), Rosalia O'Brien (ASU), Rogier Windhorst (ASU), Aaron Robotham (UWA), Anton M. Koekemoer (STScI), Christopher Willmer (University of Arizona), JWST PEARLS Team
IMAGE PROCESSING: Rolf A. Jansen (ASU), Alyssa Pagan (STScI)
PEARLS has captured one of the first medium-deep wide-field images of the cosmos. This image is only one-quarter the size of the final image and features interacting galaxies with active nuclei. Click the image for a much larger, zoomable version of the image. It’s filled with red-shifted objects that date from the Universe’s early days. Image Credit: SCIENCE: NASA, ESA, CSA, Rolf A. Jansen (ASU), Jake Summers (ASU), Rosalia O’Brien (ASU), Rogier Windhorst (ASU), Aaron Robotham (UWA), Anton M. Koekemoer (STScI), Christopher Willmer (University of Arizona), JWST PEARLS Team
IMAGE PROCESSING: Rolf A. Jansen (ASU), Alyssa Pagan (STScI)

One of the paper's co- authors is a research scientist. The earliest galaxies formed and how they evolved into what they are today is studied by him. The first PEARLS images blew my mind. When I chose this field near the North Ecliptic Pole, I didn't know that it would yield a treasure trove of distant galaxies and that we would get direct clues about the processes by which galaxies assemble and grow.

The same regions of the sky will be observed by PEARLS four different times.

This image is the PEARLS NIRCam image of the IRAC Dark Field (JWIDF) Epoch-1 at the north Ecliptic pole. The IRAC Dark Field is one of two fields PEARLS will observe, and it's considered a blank field that's suited to time domain surveys. PEARLS will observe this field and its other targets up to four times in one year. Image Credit: STScI/Windhorst et al. 2023.
This image is the PEARLS NIRCam image of the IRAC Dark Field (JWIDF) Epoch-1 at the north Ecliptic pole. The IRAC Dark Field is one of two fields PEARLS will observe, and it’s considered a blank field that’s suited to time domain surveys. PEARLS will observe this field and its other targets up to four times in one year. Image Credit: STScI/Windhorst et al. 2023.

Several rich galaxy clusters that boost the signal of faint, high-redshift objects will be imaged by PEARls. The PEARLS were able to observe a number of galaxy clusters. The authors say that all of their clusters show arcs.

This image is of the El Gordo cluster, a cluster of galaxies chosen for its enormous mass. This image doesn't show the center of the cluster, but it has a
This image is of the El Gordo cluster, a cluster of galaxies chosen for its enormous mass. This image doesn’t show the center of the cluster, but it has a “rich collection of distant lensed source candidates,” according to the authors. STScI/Windhorst et al. 2023.

Jake is a co-author. The images from the JWST far exceed what I expected. I was surprised by their resolution.

There are two types of structures in the Universe, the second one being a galaxy cluster. Two young clusters will be observed by PEARLS. The embryonic cluster is called TNJ 1338-1942. It is about 1.5 billion years old.

This image shows the TNJ1338-1942 protocluster, the most distant known protocluster. It contains a luminous, steep-spectrum radio source. The radio source is an active galactic nucleus, and a future JWST observing program will study it in more detail. The radio source is the irregular orange object in the center. Image Credit: STScI/Windhorst et al. 2023.
This image shows the TNJ1338-1942 protocluster, the most distant known protocluster. It contains a luminous, steep-spectrum radio source. The radio source is an active galactic nucleus, and a future JWST observing program will study it in more detail. The radio source is the irregular orange object in the center. Image Credit: STScI/Windhorst et al. 2023.

The pair of galaxies were imaged by PEARls. When the Hubble looked at this area, they were invisible. That shows the capabilities of the JWST.

There is an elliptical galaxy on the left and a spiral galaxy on the right in this picture. There is a distant galaxy that can be seen from the south.

The PEARLS NIRCam image of the VV 191 system. VV 191a on the left is gravitationally lensing the red galaxy at 10 o'clock and stretching its light into a curve. Image Credit: STScI/Windhorst et al. 2023.
The PEARLS NIRCam image of the VV 191 system. VV 191a on the left is gravitationally lensing the red galaxy at 10 o’clock and stretching its light into a curve. Image Credit: STScI/Windhorst et al. 2023.

Over the course of two decades, I have worked with a large international team of scientists. bb's images are beyond my expectations They allow us to measure the total amount of light produced and the number of stars in the sky. The light is not as bright as the sky between the galaxies.

There are a lot of Galaxies in the images. As far away as the Moon, there are objects as small as 10 fireflies. That is an accomplishment. The faintest red objects in the images are hundreds of millions of years old.

Astronomers are interested in the light in between stars. Unexplained light is not accepted by scientists. A small amount of light remains when astronomer remove all the light from known sources. The source of the light is being investigated. The sky may be related to missing faint galaxies. They should be found if they are there.

One of the paper's co- authors is a third-year astrophysics graduate student. The light between the stars and the galaxies is faint.

The history of the universe is affected by the diffuse light that Imeasured between stars and galaxies. I feel fortunate to be starting my career right now, and I am excited about the opportunities and challenges that come with it.

Throughout the mission, the fields that PEARL is in will be monitored. Pearl will look at the region four times in a year. The region's accessibility and desirability make it a target for others.

The field will be monitored throughout the mission to see objects that move, vary in brightness or briefly flare up, like distant exploding supernovae or accretion gas around black holes.

This is Centaurus A, the nearest galaxy with an active nucleus. The active nucleus is where a supermassive black hole (SMBH) resides. One of the questions in astrophysics is how SMBHs grow so large, and the JWST should help answer that question by looking at more ancient active nuclei. Image Credit: By ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray) - http://www.eso.org/public/images/eso0903a/, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=5821706
This is Centaurus A, the nearest galaxy with an active nucleus. The active nucleus is where a supermassive black hole (SMBH) resides. One of the questions in astrophysics is how SMBHs grow so large, and the JWST should help answer that question by looking at more ancient active nuclei. Image Credit: By ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray) – http://www.eso.org/public/images/eso0903a/, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=5821706

The time-domain legacy, area covered, and depth reached can only get better with time.

This is just the beginning of what the JWST has to offer. The authors explain how the new space telescope will help us understand the early Universe.

The galaxy cluster SMACS 0723 as seen by NIRCam on JWST (Not part of PEARL.) Its gravitational lensing properties (from its mass and from the mass of dark matter) are helping astronomers identify 88 distant galaxies in this field of view for further study. These distant galaxies are the most ancient and are critical to understanding how the Universe takes the shape it does today. JWST images like this also show evidence of dark matter, another question waiting for an answer. Courtesy NASA, ESA, CSA, STScI
The galaxy cluster SMACS 0723 as seen by NIRCam on JWST (Not part of PEARL.) Its gravitational lensing properties (from its mass and from the mass of dark matter) are helping astronomers identify 88 distant galaxies in this field of view for further study. These distant galaxies are the most ancient and are critical to understanding how the Universe takes the shape it does today. JWST images like this also show evidence of dark matter, another question waiting for an answer. Courtesy NASA, ESA, CSA, STScI

Young scientists just starting their careers are not the only lucky ones. For people who grew up with Hubble images, the James Webb is a source of excitement. Researchers are making progress on long-standing questions and it will be enjoyable to watch.

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