A Search for Population III Galaxies in CLASH. I. Singly-imaged Candidates at High Redshift
Abstract
Population III (Pop III) galaxies are predicted to exist at high redshifts and may be rendered sufficiently bright for detection with current telescopes when gravitationally lensed by a foreground galaxy cluster. Pop III galaxies that exhibit strong Lyα emission should furthermore be identifiable from broadband photometry because of their unusual colors. Here, we report on a search for such objects at z ≳ 6 in the imaging data from the Cluster Lensing And Supernova survey with Hubble (CLASH), covering 25 galaxy clusters in 16 filters. Our selection algorithm returns five singly imaged candidates with Lyα-like color signatures, for which ground-based spectroscopy with current 8–10 m class telescopes should be able to test the predicted strength of the Lyα line. None of these five objects have been included in previous CLASH compilations of high-redshift galaxy candidates. However, when large grids of spectral synthesis models are applied to the study of these objects, we find that only two of these candidates are significantly better fitted by Pop III models than by more mundane, low-metallicity stellar populations.
Additional Information
© 2015 American Astronomical Society. Received 2014 November 26; accepted 2015 February 5; published 2015 April 24. C. E. R. acknowledges funding from the Swedish National Space Board and the Royal Swedish Academy of Sciences. E. Z. acknowledges funding from the Swedish National Space Board and the Swedish Research Council (Project 2011–5349). E. Z. and J. G. acknowledge funding from the Wenner-Gren foundations. Support for A. Z. was provided by NASA through Hubble Fellowship grant #HST-HF2–51334.001 A awarded by STScI.Attached Files
Published - 0004-637X_804_1_13.pdf
Submitted - 1411.5691v2.pdf
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Additional details
- Eprint ID
- 58052
- Resolver ID
- CaltechAUTHORS:20150605-133327263
- Swedish National Space Board (SNSB)
- Royal Swedish Academy of Sciences
- Swedish Research Council
- Project 2011–5349
- Wenner-Gren Foundation
- NASA Hubble Fellowship
- HST-HF2–51334.001 A
- Created
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2015-06-06Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field