A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy
arXiv:1603.00461 · doi:10.3847/0004-637X/819/2/129
Abstract
We present Hubble WFC3/IR slitless grism spectra of a remarkably bright galaxy candidate, GN-z11, identified initially from CANDELS/GOODS-N imaging data. A significant spectroscopic continuum break is detected at m. The new grism data, combined with the photometric data, rule out all plausible lower redshift solutions for this source. The only viable solution is that this continuum break is the Ly break redshifted to , just 400 Myr after the Big Bang. This observation extends the current spectroscopic frontier by 150 Myr to well before the Planck (instantaneous) cosmic reionization peak at z~8.8, demonstrating that galaxy build-up was well underway early in the reionization epoch at z>10. GN-z11 is remarkably and unexpectedly luminous for a galaxy at such an early time: its UV luminosity is 3x larger than L* measured at z~6-8. The Spitzer IRAC detections up to 4.5 m of this galaxy are consistent with a stellar mass of . This spectroscopic redshift measurement suggests that the James Webb Space Telescope (JWST) will be able to similarly and easily confirm such sources at z>10 and characterize their physical properties through detailed spectroscopy. Furthermore, WFIRST, with its wide-field near-IR imaging, would find large numbers of similar galaxies and contribute greatly to JWST's spectroscopy, if it is launched early enough to overlap with JWST.
arXiv comment12 pages, 11 figures, accepted for publication in ApJ
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- The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries
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- First Light: Switching on Stars at the Dawn of Time
- A Comprehensive JWST/NIRSpec Census of Broad-line Active Galactic Nuclei: Faint, Low-mass Accretors and a Population of Little Red Dots
- The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
- The BUFFALO HST Survey
- The FLARE mission: Deep and Wide-field 1-5m Imaging and Spectroscopy for the Early Universe: a proposal for M5 Cosmic Vision call
- The AGEL Survey: Spectroscopic Confirmation of Strong Gravitational Lenses in the DES and DECaLS Fields Selected Using Convolutional Neural Networks
- Finding High-Redshift Galaxies with JWST
- GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
- Astro2020 Science White Paper: Exploration and characterization of the earliest epoch of galaxy formation: beyond the re-ionization era