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Sowing the CEERS of Supermassive Black Holes in the Early Universe

Sowing the CEERS of Supermassive Black Holes in the Early Universe

by Sarah Bodansky | Sep 20, 2023 | Daily Paper Summaries

How did supermassive black holes grow in the early universe? Finding faint and distant AGN with JWST may help us unravel this mystery!

Gardens of the Galaxy: Has JWST Confirmed the Existence of Heavy Supermassive Black Hole Seeds?

Gardens of the Galaxy: Has JWST Confirmed the Existence of Heavy Supermassive Black Hole Seeds?

by Lucas Brown | Aug 15, 2023 | Daily Paper Summaries

A recent observation of an extremely distant quasar sheds some (X-ray) light on the long-standing mystery of supermassive black hole formation.

Tracking Down the Quasar Light Switch

Tracking Down the Quasar Light Switch

by Delaney Dunne | May 27, 2023 | Daily Paper Summaries

We’re still not sure what causes quasars, some of the brightest objects in the universe, to switch on. Today’s authors present a compelling case for galaxy mergers being the culprit!

X-raying Quasar Titans in the Distant Universe

X-raying Quasar Titans in the Distant Universe

by Megan Masterson | May 12, 2023 | Daily Paper Summaries

Journey to the distant universe with today’s paper, as we discover what the X-ray emission from high-redshift quasars can tell us about their formation and accretion physics!

Far, Farther, Quasars – One Step Closer to the Early Formation of Supermassive Objects

Far, Farther, Quasars – One Step Closer to the Early Formation of Supermassive Objects

by Lina Kimmig | Mar 25, 2023 | Daily Paper Summaries

The existence of distant quasars requires the formation of supermassive stars in the very early universe. But is it possible to form supermassive stars so early? Find out in today’s bite!

A Galactic Prison Break: Tracing Lyα Escape at High Redshift

A Galactic Prison Break: Tracing Lyα Escape at High Redshift

by Delaney Dunne | Mar 11, 2023 | Daily Paper Summaries

Astrophysics is a lot like life in that sometimes the journey matters more than the destination. In today’s paper, which looks at the Hydrogen Lyman-α spectral line in a high-redshift protocluster, that’s absolutely the case!

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