Spectroscopic confirmation of an ultra-faint galaxy at the epoch of reionization
Journal
Date Issued
2017
Author(s)
Hoag, Austin
•
Bradač, Maruša
•
Trenti, Michele
•
Treu, Tommaso
•
Schmidt, Kasper B.
•
Huang, Kuang-Han
•
Lemaux, Brian C.
•
He, Julie
•
Bernard, Stephanie R.
•
Abramson, Louis E.
•
Mason, Charlotte A.
•
Morishita, Takahiro
•
•
Schrabback, Tim
Abstract
Within one billion years of the Big Bang, intergalactic hydrogen was ionized by sources emitting ultraviolet and higher energy photons. This was the final phenomenon to globally affect all the baryons (visible matter) in the Universe. It is referred to as cosmic reionization and is an integral component of cosmology. It is broadly expected that intrinsically faint galaxies were the primary ionizing sources due to their abundance in this epoch1,2. However, at the highest redshifts (z > 7.5 lookback time 13.1 Gyr), all galaxies with spectroscopic confirmations to date are intrinsically bright and, therefore, not necessarily representative of the general population3. Here, we report the unequivocal spectroscopic detection of a low luminosity galaxy at z > 7.5. We detected the Lyman-α emission line at ∼10,504 Å in two separate observations with MOSFIRE4 on the Keck I Telescope and independently with the Hubble Space Telescope's slitless grism spectrograph, implying a source redshift of z = 7.640 ± 0.001. The galaxy is gravitationally magnified by the massive galaxy cluster MACS J1423.8+2404 (z = 0.545), with an estimated intrinsic luminosity of MAB = -19.6 ± 0.2 mag and a stellar mass of M☉=3.0-0.8+1.5×108 solar masses. Both are an order of magnitude lower than the four other Lyman-α emitters currently known at z > 7.5, making it probably the most distant representative source of reionization found to date.
Volume
1
Issue
5
Start page
0091
Issn Identifier
2397-3366
Ads BibCode
2017NatAs...1E..91H
Rights
open.access
File(s)![Thumbnail Image]()
![Thumbnail Image]()
Loading...
Name
Nat. Astr. s41550-017-0091.pdf
Description
PDF editoriale
Size
1.15 MB
Format
Adobe PDF
Checksum (MD5)
5b6b652a9c5b49ffd1b8216e75a33036
Loading...
Name
1704.02970.pdf
Description
preprint
Size
7.25 MB
Format
Adobe PDF
Checksum (MD5)
2a78ccc8ea07a3ffd9fd7f58f817d345