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MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M-UV similar to-15

Title
MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M-UV similar to-15
Type
Article in International Scientific Journal
Year
2018
Authors
Maseda, MV
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Bacon, R
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Franx, M
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J. Brinchmann
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Schaye, J
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Boogaard, LA
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Bouche, N
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Bouwens, RJ
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Cantalupo, S
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Contini, T
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Hashimoto, T
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Inami, H
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Marino, RA
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Muzahid, S
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Nanayakkara, T
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Richard, J
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Schmidt, KB
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Verhamme, A
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Wisotzki, L
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Journal
Vol. 865
Final page: L1
ISSN: 2041-8205
Other information
Authenticus ID: P-00P-MMC
Abstract (EN): Using an ultra-deep blind survey with the MUSE integral field spectrograph on the European Southern Observatory Very Large Telescope, we obtain spectroscopic redshifts to a depth never before explored: galaxies with observed magnitudes m(AB) greater than or similar to 30-32. Specifically, we detect objects via Ly alpha emission at 2.9 < z < 6.7 without individual continuum counterparts in areas covered by the deepest optical/near-infrared imaging taken by the Hubble Space Telescope, the Hubble Ultra Deep Field. In total, we find 102 such objects in 9 square arcminutes at these redshifts. Detailed stacking analyses confirm the Ly alpha emission as well as the 1216 angstrom breaks and faint ultraviolet continua (M-UV similar to -15). This makes them the faintest spectroscopically confirmed objects at these redshifts, similar to the sources believed to reionize the universe. A simple model for the expected fraction of detected/undetected Ly alpha emitters as a function of luminosity is consistent with these objects being the high-equivalent width tail of the normal Ly alpha-emitter population at these redshifts.
Language: English
Type (Professor's evaluation): Scientific
No. of pages: 7
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