New constraints on lyman-α opacity with a sample of 62 quasars at z > 5.7

Sarah E.I. Bosman, Xiaohui Fan, Linhua Jiang, Sophie Reed, Yoshiki Matsuoka, George Becker, Martin Haehnelt

Research output: Contribution to journalArticle

22 Citations (Scopus)

Abstract

We present measurements of the mean and scatter of the intergalactic medium (IGM) Lyman-a opacity at 4.9 < z < 6.1 along the lines of sight of 62 quasars at zsource> 5.7, the largest sample assembled at these redshifts to date by a factor of two. The sample size enables us to sample cosmic variance at these redshifts more robustly than ever before. The spectra used here were obtained by the Sloan Digital Sky Survey, Dark Energy Survey-VISTA Hemisphere Survey, and Subaru High-z Exploration of Low-Luminosity Quasars collaborations, drawn from the Echellette Spectrograph and Imager and X-Shooter archives, reused from previous studies or observed specifically for this work. We measure the effective optical depth of Lyman-α in bins of 10, 30, 50, and 70 cMpc h-1, construct cumulative distribution functions under two treatments of upper limits on flux and explore an empirical analytic fit to residual Lyman- a transmission. We verify the consistency of our results with those of previous studies via bootstrap resampling and confirm the existence of tails towards high values in the opacity distributions, which may persist down to z ~ 5.2. Comparing our results with predictions from cosmological simulations, we find further strong evidence against models that include a spatially uniform ionizing background and temperature-density relation. We also compare to IGM models that include either a fluctuating ultraviolet background dominated by rare quasars or temperature fluctuations due to patchy reionization. Although both models produce better agreement with the observations, neither fully captures the observed scatter in IGM opacity. Our sample of 62 z > 5.7 quasar spectra opens many avenues for future study of the reionization epoch.

Original languageEnglish (US)
Pages (from-to)1055-1076
Number of pages22
JournalMonthly Notices of the Royal Astronomical Society
Volume479
Issue number1
DOIs
StatePublished - Sep 1 2018

Fingerprint

opacity
quasars
intergalactic media
optical depth
hemispheres
temperature
dark energy
optical thickness
spectrographs
distribution functions
luminosity
time measurement
prediction
simulation
energy
predictions
distribution

Keywords

  • Dark ages, reionization, first stars
  • Intergalactic medium
  • Quasars: absorption lines

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

New constraints on lyman-α opacity with a sample of 62 quasars at z > 5.7. / Bosman, Sarah E.I.; Fan, Xiaohui; Jiang, Linhua; Reed, Sophie; Matsuoka, Yoshiki; Becker, George; Haehnelt, Martin.

In: Monthly Notices of the Royal Astronomical Society, Vol. 479, No. 1, 01.09.2018, p. 1055-1076.

Research output: Contribution to journalArticle

Bosman, SEI, Fan, X, Jiang, L, Reed, S, Matsuoka, Y, Becker, G & Haehnelt, M 2018, 'New constraints on lyman-α opacity with a sample of 62 quasars at z > 5.7', Monthly Notices of the Royal Astronomical Society, vol. 479, no. 1, pp. 1055-1076. https://doi.org/10.1093/mnras/sty1344
Bosman, Sarah E.I. ; Fan, Xiaohui ; Jiang, Linhua ; Reed, Sophie ; Matsuoka, Yoshiki ; Becker, George ; Haehnelt, Martin. / New constraints on lyman-α opacity with a sample of 62 quasars at z > 5.7. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 479, No. 1. pp. 1055-1076.
@article{0dccdbbbf81c4deb9a7ce981ae7aac36,
title = "New constraints on lyman-α opacity with a sample of 62 quasars at z > 5.7",
abstract = "We present measurements of the mean and scatter of the intergalactic medium (IGM) Lyman-a opacity at 4.9 < z < 6.1 along the lines of sight of 62 quasars at zsource> 5.7, the largest sample assembled at these redshifts to date by a factor of two. The sample size enables us to sample cosmic variance at these redshifts more robustly than ever before. The spectra used here were obtained by the Sloan Digital Sky Survey, Dark Energy Survey-VISTA Hemisphere Survey, and Subaru High-z Exploration of Low-Luminosity Quasars collaborations, drawn from the Echellette Spectrograph and Imager and X-Shooter archives, reused from previous studies or observed specifically for this work. We measure the effective optical depth of Lyman-α in bins of 10, 30, 50, and 70 cMpc h-1, construct cumulative distribution functions under two treatments of upper limits on flux and explore an empirical analytic fit to residual Lyman- a transmission. We verify the consistency of our results with those of previous studies via bootstrap resampling and confirm the existence of tails towards high values in the opacity distributions, which may persist down to z ~ 5.2. Comparing our results with predictions from cosmological simulations, we find further strong evidence against models that include a spatially uniform ionizing background and temperature-density relation. We also compare to IGM models that include either a fluctuating ultraviolet background dominated by rare quasars or temperature fluctuations due to patchy reionization. Although both models produce better agreement with the observations, neither fully captures the observed scatter in IGM opacity. Our sample of 62 z > 5.7 quasar spectra opens many avenues for future study of the reionization epoch.",
keywords = "Dark ages, reionization, first stars, Intergalactic medium, Quasars: absorption lines",
author = "Bosman, {Sarah E.I.} and Xiaohui Fan and Linhua Jiang and Sophie Reed and Yoshiki Matsuoka and George Becker and Martin Haehnelt",
year = "2018",
month = "9",
day = "1",
doi = "10.1093/mnras/sty1344",
language = "English (US)",
volume = "479",
pages = "1055--1076",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",

}

TY - JOUR

T1 - New constraints on lyman-α opacity with a sample of 62 quasars at z > 5.7

AU - Bosman, Sarah E.I.

AU - Fan, Xiaohui

AU - Jiang, Linhua

AU - Reed, Sophie

AU - Matsuoka, Yoshiki

AU - Becker, George

AU - Haehnelt, Martin

PY - 2018/9/1

Y1 - 2018/9/1

N2 - We present measurements of the mean and scatter of the intergalactic medium (IGM) Lyman-a opacity at 4.9 < z < 6.1 along the lines of sight of 62 quasars at zsource> 5.7, the largest sample assembled at these redshifts to date by a factor of two. The sample size enables us to sample cosmic variance at these redshifts more robustly than ever before. The spectra used here were obtained by the Sloan Digital Sky Survey, Dark Energy Survey-VISTA Hemisphere Survey, and Subaru High-z Exploration of Low-Luminosity Quasars collaborations, drawn from the Echellette Spectrograph and Imager and X-Shooter archives, reused from previous studies or observed specifically for this work. We measure the effective optical depth of Lyman-α in bins of 10, 30, 50, and 70 cMpc h-1, construct cumulative distribution functions under two treatments of upper limits on flux and explore an empirical analytic fit to residual Lyman- a transmission. We verify the consistency of our results with those of previous studies via bootstrap resampling and confirm the existence of tails towards high values in the opacity distributions, which may persist down to z ~ 5.2. Comparing our results with predictions from cosmological simulations, we find further strong evidence against models that include a spatially uniform ionizing background and temperature-density relation. We also compare to IGM models that include either a fluctuating ultraviolet background dominated by rare quasars or temperature fluctuations due to patchy reionization. Although both models produce better agreement with the observations, neither fully captures the observed scatter in IGM opacity. Our sample of 62 z > 5.7 quasar spectra opens many avenues for future study of the reionization epoch.

AB - We present measurements of the mean and scatter of the intergalactic medium (IGM) Lyman-a opacity at 4.9 < z < 6.1 along the lines of sight of 62 quasars at zsource> 5.7, the largest sample assembled at these redshifts to date by a factor of two. The sample size enables us to sample cosmic variance at these redshifts more robustly than ever before. The spectra used here were obtained by the Sloan Digital Sky Survey, Dark Energy Survey-VISTA Hemisphere Survey, and Subaru High-z Exploration of Low-Luminosity Quasars collaborations, drawn from the Echellette Spectrograph and Imager and X-Shooter archives, reused from previous studies or observed specifically for this work. We measure the effective optical depth of Lyman-α in bins of 10, 30, 50, and 70 cMpc h-1, construct cumulative distribution functions under two treatments of upper limits on flux and explore an empirical analytic fit to residual Lyman- a transmission. We verify the consistency of our results with those of previous studies via bootstrap resampling and confirm the existence of tails towards high values in the opacity distributions, which may persist down to z ~ 5.2. Comparing our results with predictions from cosmological simulations, we find further strong evidence against models that include a spatially uniform ionizing background and temperature-density relation. We also compare to IGM models that include either a fluctuating ultraviolet background dominated by rare quasars or temperature fluctuations due to patchy reionization. Although both models produce better agreement with the observations, neither fully captures the observed scatter in IGM opacity. Our sample of 62 z > 5.7 quasar spectra opens many avenues for future study of the reionization epoch.

KW - Dark ages, reionization, first stars

KW - Intergalactic medium

KW - Quasars: absorption lines

UR - http://www.scopus.com/inward/record.url?scp=85051549548&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85051549548&partnerID=8YFLogxK

U2 - 10.1093/mnras/sty1344

DO - 10.1093/mnras/sty1344

M3 - Article

AN - SCOPUS:85051549548

VL - 479

SP - 1055

EP - 1076

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -