Lyα EMITTER GALAXIES at z ∼ 2.8 in the EXTENDED CHANDRA DEEP FIELD SOUTH. I. TRACING the LARGE-SCALE STRUCTURE VIA Lyα IMAGING

Zhen Ya Zheng, Sangeeta Malhotra, James E. Rhoads, Steven L. Finkelstein, Jun Xian Wang, Chun Yan Jiang, Zheng Cai

Research output: Contribution to journalArticle

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Abstract

We present a narrowband survey with three adjacent filters for z =2.8-2.9 Lyman alpha (Lyα) emitter (LAE) galaxies in the Extended Chandra Deep Field South (ECDFS), along with spectroscopic follow-up. With a complete sample of 96 LAE candidates in the narrowband NB466, we confirm the large-scale structure at z ∼ 2.8 suggested by previous spectroscopic surveys. Compared to the blank field detected with the other two narrowband filters NB470 and NB475, the LAE-density excess in NB466 (900 arcmin2) is ∼ 6.00.8 times the standard deviation expected at z ∼ 2.8, assuming a linear bias of 2. The overdense large-scale structure in NB466 can be decomposed into four protoclusters, whose overdensities (each within an equivalent comoving volume 153 Mpc3) relative to the blank field (NB470+NB475) are in the range of 4.6-6.6. These four protoclusters are expected to evolve into a Coma-like cluster (M ≥ 1015Mo) at z ∼ 0. We also investigate the various properties of LAEs at z = 2.8-2.9 and their dependence on the environment. The average star formation rates derived from the Lyα, rest-frame UV, and X-ray bands are ∼4, 10, and <16 M o yr-1, respectively, implying a Lyα escape fraction of 25% ≲ ≲ 40% and a UV continuum escape fraction of 62% for LAEs at z ∼ 2.8. The Lyα photon density calculated from the integrated Lyα luminosity function in the overdense field (NB466) is ∼50% higher than that in the blank field (NB470+NB475), and more bright LAEs are found in the overdense field. The three brightest LAEs, including a quasar at z = 2.81, are all detected in the X-ray band and in NB466. These three LAE-active galactic nuclei contribute an extra 20%-30% Lyα photon density compared to other LAE galaxies. Furthermore, we find that LAEs in overdense regions have larger equivalent width values, bluer U - B and V - R (∼2-3σ) colors compared with those in lower density regions, indicating that LAEs in overdense regions are younger and possible less dusty. We conclude that the structure at z ∼ 2.8 in the ECDFS field is a very significant and rare density peak similar to the SSA22 protocluster, and narrowband imaging is an efficient method of detecting and studying such structures in the high-z universe.

Original languageEnglish (US)
Article number23
JournalAstrophysical Journal, Supplement Series
Volume226
Issue number2
DOIs
StatePublished - Oct 1 2016

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tracing
narrowband
blanks
photon density
escape
galaxies
filters
coma
filter
star formation rate
active galactic nuclei
quasars
standard deviation
emitters
x rays
universe
luminosity
continuums
color

Keywords

  • galaxies: evolution
  • galaxies: high-redshift
  • galaxies: luminosity function
  • galaxies: structure
  • mass function

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Lyα EMITTER GALAXIES at z ∼ 2.8 in the EXTENDED CHANDRA DEEP FIELD SOUTH. I. TRACING the LARGE-SCALE STRUCTURE VIA Lyα IMAGING. / Zheng, Zhen Ya; Malhotra, Sangeeta; Rhoads, James E.; Finkelstein, Steven L.; Wang, Jun Xian; Jiang, Chun Yan; Cai, Zheng.

In: Astrophysical Journal, Supplement Series, Vol. 226, No. 2, 23, 01.10.2016.

Research output: Contribution to journalArticle

Zheng, Zhen Ya ; Malhotra, Sangeeta ; Rhoads, James E. ; Finkelstein, Steven L. ; Wang, Jun Xian ; Jiang, Chun Yan ; Cai, Zheng. / Lyα EMITTER GALAXIES at z ∼ 2.8 in the EXTENDED CHANDRA DEEP FIELD SOUTH. I. TRACING the LARGE-SCALE STRUCTURE VIA Lyα IMAGING. In: Astrophysical Journal, Supplement Series. 2016 ; Vol. 226, No. 2.
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abstract = "We present a narrowband survey with three adjacent filters for z =2.8-2.9 Lyman alpha (Lyα) emitter (LAE) galaxies in the Extended Chandra Deep Field South (ECDFS), along with spectroscopic follow-up. With a complete sample of 96 LAE candidates in the narrowband NB466, we confirm the large-scale structure at z ∼ 2.8 suggested by previous spectroscopic surveys. Compared to the blank field detected with the other two narrowband filters NB470 and NB475, the LAE-density excess in NB466 (900 arcmin2) is ∼ 6.00.8 times the standard deviation expected at z ∼ 2.8, assuming a linear bias of 2. The overdense large-scale structure in NB466 can be decomposed into four protoclusters, whose overdensities (each within an equivalent comoving volume 153 Mpc3) relative to the blank field (NB470+NB475) are in the range of 4.6-6.6. These four protoclusters are expected to evolve into a Coma-like cluster (M ≥ 1015Mo) at z ∼ 0. We also investigate the various properties of LAEs at z = 2.8-2.9 and their dependence on the environment. The average star formation rates derived from the Lyα, rest-frame UV, and X-ray bands are ∼4, 10, and <16 M o yr-1, respectively, implying a Lyα escape fraction of 25{\%} ≲ ≲ 40{\%} and a UV continuum escape fraction of 62{\%} for LAEs at z ∼ 2.8. The Lyα photon density calculated from the integrated Lyα luminosity function in the overdense field (NB466) is ∼50{\%} higher than that in the blank field (NB470+NB475), and more bright LAEs are found in the overdense field. The three brightest LAEs, including a quasar at z = 2.81, are all detected in the X-ray band and in NB466. These three LAE-active galactic nuclei contribute an extra 20{\%}-30{\%} Lyα photon density compared to other LAE galaxies. Furthermore, we find that LAEs in overdense regions have larger equivalent width values, bluer U - B and V - R (∼2-3σ) colors compared with those in lower density regions, indicating that LAEs in overdense regions are younger and possible less dusty. We conclude that the structure at z ∼ 2.8 in the ECDFS field is a very significant and rare density peak similar to the SSA22 protocluster, and narrowband imaging is an efficient method of detecting and studying such structures in the high-z universe.",
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T1 - Lyα EMITTER GALAXIES at z ∼ 2.8 in the EXTENDED CHANDRA DEEP FIELD SOUTH. I. TRACING the LARGE-SCALE STRUCTURE VIA Lyα IMAGING

AU - Zheng, Zhen Ya

AU - Malhotra, Sangeeta

AU - Rhoads, James E.

AU - Finkelstein, Steven L.

AU - Wang, Jun Xian

AU - Jiang, Chun Yan

AU - Cai, Zheng

PY - 2016/10/1

Y1 - 2016/10/1

N2 - We present a narrowband survey with three adjacent filters for z =2.8-2.9 Lyman alpha (Lyα) emitter (LAE) galaxies in the Extended Chandra Deep Field South (ECDFS), along with spectroscopic follow-up. With a complete sample of 96 LAE candidates in the narrowband NB466, we confirm the large-scale structure at z ∼ 2.8 suggested by previous spectroscopic surveys. Compared to the blank field detected with the other two narrowband filters NB470 and NB475, the LAE-density excess in NB466 (900 arcmin2) is ∼ 6.00.8 times the standard deviation expected at z ∼ 2.8, assuming a linear bias of 2. The overdense large-scale structure in NB466 can be decomposed into four protoclusters, whose overdensities (each within an equivalent comoving volume 153 Mpc3) relative to the blank field (NB470+NB475) are in the range of 4.6-6.6. These four protoclusters are expected to evolve into a Coma-like cluster (M ≥ 1015Mo) at z ∼ 0. We also investigate the various properties of LAEs at z = 2.8-2.9 and their dependence on the environment. The average star formation rates derived from the Lyα, rest-frame UV, and X-ray bands are ∼4, 10, and <16 M o yr-1, respectively, implying a Lyα escape fraction of 25% ≲ ≲ 40% and a UV continuum escape fraction of 62% for LAEs at z ∼ 2.8. The Lyα photon density calculated from the integrated Lyα luminosity function in the overdense field (NB466) is ∼50% higher than that in the blank field (NB470+NB475), and more bright LAEs are found in the overdense field. The three brightest LAEs, including a quasar at z = 2.81, are all detected in the X-ray band and in NB466. These three LAE-active galactic nuclei contribute an extra 20%-30% Lyα photon density compared to other LAE galaxies. Furthermore, we find that LAEs in overdense regions have larger equivalent width values, bluer U - B and V - R (∼2-3σ) colors compared with those in lower density regions, indicating that LAEs in overdense regions are younger and possible less dusty. We conclude that the structure at z ∼ 2.8 in the ECDFS field is a very significant and rare density peak similar to the SSA22 protocluster, and narrowband imaging is an efficient method of detecting and studying such structures in the high-z universe.

AB - We present a narrowband survey with three adjacent filters for z =2.8-2.9 Lyman alpha (Lyα) emitter (LAE) galaxies in the Extended Chandra Deep Field South (ECDFS), along with spectroscopic follow-up. With a complete sample of 96 LAE candidates in the narrowband NB466, we confirm the large-scale structure at z ∼ 2.8 suggested by previous spectroscopic surveys. Compared to the blank field detected with the other two narrowband filters NB470 and NB475, the LAE-density excess in NB466 (900 arcmin2) is ∼ 6.00.8 times the standard deviation expected at z ∼ 2.8, assuming a linear bias of 2. The overdense large-scale structure in NB466 can be decomposed into four protoclusters, whose overdensities (each within an equivalent comoving volume 153 Mpc3) relative to the blank field (NB470+NB475) are in the range of 4.6-6.6. These four protoclusters are expected to evolve into a Coma-like cluster (M ≥ 1015Mo) at z ∼ 0. We also investigate the various properties of LAEs at z = 2.8-2.9 and their dependence on the environment. The average star formation rates derived from the Lyα, rest-frame UV, and X-ray bands are ∼4, 10, and <16 M o yr-1, respectively, implying a Lyα escape fraction of 25% ≲ ≲ 40% and a UV continuum escape fraction of 62% for LAEs at z ∼ 2.8. The Lyα photon density calculated from the integrated Lyα luminosity function in the overdense field (NB466) is ∼50% higher than that in the blank field (NB470+NB475), and more bright LAEs are found in the overdense field. The three brightest LAEs, including a quasar at z = 2.81, are all detected in the X-ray band and in NB466. These three LAE-active galactic nuclei contribute an extra 20%-30% Lyα photon density compared to other LAE galaxies. Furthermore, we find that LAEs in overdense regions have larger equivalent width values, bluer U - B and V - R (∼2-3σ) colors compared with those in lower density regions, indicating that LAEs in overdense regions are younger and possible less dusty. We conclude that the structure at z ∼ 2.8 in the ECDFS field is a very significant and rare density peak similar to the SSA22 protocluster, and narrowband imaging is an efficient method of detecting and studying such structures in the high-z universe.

KW - galaxies: evolution

KW - galaxies: high-redshift

KW - galaxies: luminosity function

KW - galaxies: structure

KW - mass function

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