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AstroSat's Insights into the Ultraviolet Universe

AstroSat reveals over 102,000 light sources in the ultraviolet spectrum.

Swagat Bordoloi, P. Shalima, Rupjyoti Gogoi, Jayant Murthy

― 5 min read


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Have you ever looked up at the night sky and wondered what you could see if you had a superpowered telescope? Well, scientists in India did just that. They launched a satellite named AstroSat that took a closer look at ultraviolet light from stars and galaxies. This satellite has helped create a big list of points in the sky where we can find various celestial objects. Let's break down what that means and why it matters.

What is AstroSat?

AstroSat is India's first satellite designed for astronomy. Launched in 2015, it has different tools, or payloads, for observing the universe in various light frequencies. One of its key instruments is the Ultra Violet Imaging Telescope (UVIT). It helps us see in ultraviolet light, which is like the light that gives you a sunburn but comes from stars instead of the sun.

How UVIT Works

UVIT has two telescopes on board. One telescope looks at far ultraviolet light, while the other splits the light into near ultraviolet and visible light. This lets the scientists look for different types of light coming from stars. Imagine trying to find hidden treasures-UVIT is like a treasure map that helps find everything from bright young stars to old, faded ones, but in the spectrum of ultraviolet light.

What Did They Find?

The researchers looked at a big chunk of the sky-about 63 square degrees, which is like pointing a flashlight at a large part of your ceiling. After observing multiple areas, they found over 102,000 sources of light, or point sources, in the sky. You can think of these sources as individual "stars" on their starry map.

Making Sense of the Data

To gather all this information, the scientists needed to take a lot of pictures and look at them carefully. They took images using different filters, much like wearing sunglasses with different tints. Each filter helps to capture different details from the light coming from the sources.

They observed 428 areas using far ultraviolet light and 54 areas using Near Ultraviolet Light. It’s like taking lots of selfies at different angles and times to find the best one.

The Catalog of Sources

Once they had all the images, the researchers needed to put everything into a neat catalog, which is like a giant playlist of all the best songs-except these are all the best sources seen in ultraviolet light.

The catalog includes technical details about each source, like how bright it is and what kind of light it gives off. This information is essential for scientists who want to study different objects in the universe.

Why Does It Matter?

This catalog can help scientists learn about a variety of cosmic objects, such as young galaxies, black holes, and even white dwarfs, which are remnants of stars. Each object tells a story about the history and makeup of our universe.

Having such a catalog is important because most existing Catalogs focus on visible light. Observing ultraviolet light gives scientists new insights, much like how using a special lens helps to spot things we usually miss.

Learning from the Catalog

With years of observations under its belt, UVIT is a powerful tool for figuring out where things are in the universe. The researchers used clever techniques to find and correct the positions of the point sources, ensuring that they are accurate. Think of it like using a GPS to find the right place when your map doesn’t quite match up.

Challenges Faced

The researchers didn’t have it easy. Some images needed adjustments since the initial positions were incorrect. They had to create custom catalogs using existing data to help correct the mistakes. Sometimes, you need to roll up your sleeves and do a bit more digging to find the right answer.

A Bigger Picture

The work with UVIT is part of a larger effort to create a multi-dimensional view of the universe. The scientists aim to correlate this data with other wavelengths-like infrared or X-ray observations-to get a full picture of cosmic events. Combining different types of light is like putting together a jigsaw puzzle; each piece is important to see the entire picture.

Future Plans

The researchers aren’t done yet. They plan to expand the catalog further, including more fields and different types of data. With more observations, they will continue to learn about the vast universe. Who knows what cool new discoveries await?

Conclusion

What started as a satellite floating in space has turned into a treasure trove of information about our universe. With over 102,000 sources cataloged, scientists can keep digging into the mysteries of the cosmos. AstroSat and its UVIT instrument have opened doors to new findings that can help us better understand the stars and galaxies near and far.

So next time you gaze up at the stars, remember there are hardworking scientists out there using some pretty awesome tech to uncover the secrets of the universe, one ultraviolet ray at a time.

Original Source

Title: A sky survey of ultraviolet sources observed through AstroSat's UVIT: A point source catalog

Abstract: The Ultra Violet Imaging Telescope (UVIT) onboard India's first dedicated multiwavelength satellite \textit{AstroSat} observed a significant fraction of the sky in the ultraviolet with a spatial resolution of 1.4\arcsec. We present a catalog of the point sources observed by UVIT in the far ultraviolet (FUV; 1300-1800 \AA) and near ultraviolet (NUV; 2000-3000 \AA). We carried out astrometry and photometry of 428 field pointings in the FUV and 54 field pointings in the NUV band, observed in 5 filter bands in each channel respectively, covering an area of about 63 square degrees. The final catalog contains about 102,773 sources. The limiting magnitude(AB) of the F148W band filter, that has the largest number of detections is $\sim21.3$. For the NUV channel, we find the limiting magnitude at around $\sim23$. We describe the final catalog and present the results of the statistical analysis.

Authors: Swagat Bordoloi, P. Shalima, Rupjyoti Gogoi, Jayant Murthy

Last Update: 2024-11-04 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.01809

Source PDF: https://arxiv.org/pdf/2411.01809

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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