TY - JOUR
T1 - A search for population iii galaxies in clash. I. singly imaged candidates at high redshift
AU - Rydberg, Claes Erik
AU - Zackrisson, Erik
AU - Zitrin, Adi
AU - Guaita, Lucia
AU - Melinder, Jens
AU - Asadi, Saghar
AU - Gonzalez, Juan
AU - Ostlin, Goran
AU - Strom, Tina
N1 - Publisher Copyright:
© 2015. The American Astronomical Society. All rights reserved..
PY - 2015/5/1
Y1 - 2015/5/1
N2 - 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 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.
AB - 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 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.
KW - dark ages, reionization, first stars
KW - galaxies: high-redshift
KW - gravitational lensing: strong
KW - stars: Population III
UR - http://www.scopus.com/inward/record.url?scp=84946185354&partnerID=8YFLogxK
U2 - 10.1088/0004-637X/804/1/13
DO - 10.1088/0004-637X/804/1/13
M3 - Article
AN - SCOPUS:84946185354
SN - 0004-637X
VL - 804
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 13
ER -