We present the first results on the search for very bright (M_AB~-21) z~8
galaxies from the Brightest of Reionizing Galaxies (BoRG) survey. BoRG is a
Hubble Space Telescope Wide Field Camera 3 pure-parallel survey that is
obtaining images on random lines of sight at high Galactic latitudes in four
filters (F606W, F098M, F125W, F160W), with integration times optimized to
identify galaxies at z>7.5 as F098M-dropouts. We discuss here results from a
search area of ~130 arcmin^2 over 23 BoRG fields, complemented by 6 other
pure-parallel WFC3 fields with similar filters. This new search area is >2X
wider compared to previous WFC3 observations at z~8. We identify four
F098M-dropout candidates with high statistical confidence (detected at >8 sigma
in F125W). These sources are among the brightest candidates currently known at
z~8 and ~10x brighter than the z=8.56 galaxy UDFy-38135539. They thus represent
ideal targets for spectroscopic followup observations and could potentially
lead to a redshift record as our color selection includes objects up to z~ 9.
However, the expected contamination rate of our sample is ~30% higher than
typical searches for dropout galaxies in legacy fields, such as the GOODS and
HUDF, where more extended wavelength coverage is available both in the optical
and in the infrared.
Description
The Brightest Of Reionizing Galaxies Survey: Design and Preliminary
Results
%0 Generic
%1 Trenti2010
%A Trenti, M.
%A Bradley, L. D.
%A Stiavelli, M.
%A Oesch, P.
%A Treu, T.
%A Bouwens, R. J.
%A Shull, J. M.
%A MacKenty, J. W.
%A Carollo, C. M.
%A Illingworth, G. D.
%D 2010
%K arxiv reionizing
%T The Brightest Of Reionizing Galaxies Survey: Design and Preliminary
Results
%U http://arxiv.org/abs/1011.4075
%X We present the first results on the search for very bright (M_AB~-21) z~8
galaxies from the Brightest of Reionizing Galaxies (BoRG) survey. BoRG is a
Hubble Space Telescope Wide Field Camera 3 pure-parallel survey that is
obtaining images on random lines of sight at high Galactic latitudes in four
filters (F606W, F098M, F125W, F160W), with integration times optimized to
identify galaxies at z>7.5 as F098M-dropouts. We discuss here results from a
search area of ~130 arcmin^2 over 23 BoRG fields, complemented by 6 other
pure-parallel WFC3 fields with similar filters. This new search area is >2X
wider compared to previous WFC3 observations at z~8. We identify four
F098M-dropout candidates with high statistical confidence (detected at >8 sigma
in F125W). These sources are among the brightest candidates currently known at
z~8 and ~10x brighter than the z=8.56 galaxy UDFy-38135539. They thus represent
ideal targets for spectroscopic followup observations and could potentially
lead to a redshift record as our color selection includes objects up to z~ 9.
However, the expected contamination rate of our sample is ~30% higher than
typical searches for dropout galaxies in legacy fields, such as the GOODS and
HUDF, where more extended wavelength coverage is available both in the optical
and in the infrared.
@misc{Trenti2010,
abstract = { We present the first results on the search for very bright (M_AB~-21) z~8
galaxies from the Brightest of Reionizing Galaxies (BoRG) survey. BoRG is a
Hubble Space Telescope Wide Field Camera 3 pure-parallel survey that is
obtaining images on random lines of sight at high Galactic latitudes in four
filters (F606W, F098M, F125W, F160W), with integration times optimized to
identify galaxies at z>7.5 as F098M-dropouts. We discuss here results from a
search area of ~130 arcmin^2 over 23 BoRG fields, complemented by 6 other
pure-parallel WFC3 fields with similar filters. This new search area is >2X
wider compared to previous WFC3 observations at z~8. We identify four
F098M-dropout candidates with high statistical confidence (detected at >8 sigma
in F125W). These sources are among the brightest candidates currently known at
z~8 and ~10x brighter than the z=8.56 galaxy UDFy-38135539. They thus represent
ideal targets for spectroscopic followup observations and could potentially
lead to a redshift record as our color selection includes objects up to z~ 9.
However, the expected contamination rate of our sample is ~30% higher than
typical searches for dropout galaxies in legacy fields, such as the GOODS and
HUDF, where more extended wavelength coverage is available both in the optical
and in the infrared.
},
added-at = {2010-11-19T02:55:23.000+0100},
author = {Trenti, M. and Bradley, L. D. and Stiavelli, M. and Oesch, P. and Treu, T. and Bouwens, R. J. and Shull, J. M. and MacKenty, J. W. and Carollo, C. M. and Illingworth, G. D.},
biburl = {https://www.bibsonomy.org/bibtex/2b8fc85572265a09f4e88256b56788401/jimmies},
description = {The Brightest Of Reionizing Galaxies Survey: Design and Preliminary
Results},
interhash = {3802dff5bf765b90607bbe8d42e2e0b8},
intrahash = {b8fc85572265a09f4e88256b56788401},
keywords = {arxiv reionizing},
note = {cite arxiv:1011.4075
Comment: 6 pages, 3 figures, 2 tables, ApJL submitted},
timestamp = {2010-11-19T02:55:23.000+0100},
title = {The Brightest Of Reionizing Galaxies Survey: Design and Preliminary
Results},
url = {http://arxiv.org/abs/1011.4075},
year = 2010
}