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The First Ionized Bubblesin the Cosmic Dawn
James Rhoads & Sangeeta MalhotraNASA Goddard Space Flight Center
and Vithal S. TilviArizona State University
[email protected] (mobile: 480-278-0192); [email protected]; [email protected]
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A Sketch of Cosmic History
Big Bang Now13.8 billion years ago
Cosmic microwave background Cosmic
Dawn
Dark Ages
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Growth of Ionized Bubbles
Simulation by M. Alvarez, R. Kaehler, and T. Abel
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Lyman Alpha
• A particular wavelength of light, produced by young galaxies.
• Before reionization – it is scattered, like headlights in fog.
• After reionization– we can see it clearly now.
By looking for Lyman alpha from galaxies we can determine if their surroundings are neutral or ionized..
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The Cosmic DAWN SurveyWe undertook sensitive infrared imaging from the KittPeak National Observatory’s 4m Mayall Telescope + NEWFIRM camera.
We looked for Lyman alpha light from galaxies in the epoch of cosmic dawn.
We took spectra of DAWN survey galaxies with the Keck telescope on Maunakea, Hawai`i.
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The Group EGS77 in the Cosmic DAWN Survey
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Galaxy Group EGS77Lyman alpha light - bright
Redder starlight –detected but faint
Bluer light –galaxies not detected
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Galaxy Group EGS77 in Cosmic History
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EGS 77 bubbles in contxt
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Summary
• Reionization was the last time that anything interesting happened to a typical atom, and we want to understand its history.
• We have found an ionized bubble, traced by the earliest known galaxy group (EGS77), when the universe was 5% of its current age.
• This sheds new light on Cosmic Dawn.• There is a bright future for studying EGS77 with JWST, and
finding more like it with [email protected] (mobile: 480-278-0192); [email protected]; [email protected]
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The Cosmic DAWN Survey Team
These results are described in more detail in a manuscript submitted to The Astrophysical Journal Letters and led by V. Tilvi.
The DAWN team consists ofJames Rhoads, Sangeeta Malhotra, Vithal S. Tilvi, Alicia Coughlin, Ronald Probst, Sylvain Veilleux, Steven L. Finkelstein, Bahram Mobasher, Pascale Hibon, Tianxing Jiang, Bhavin Joshi, John Pharo, Rob Swaters, Junxian Wang, Huan Yang, Johannes Zabl, and Zhenya Zheng.