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Title: Implications of z ~ 6 Quasar Proximity Zones for the Epoch of Reionization and Quasar Lifetimes

Abstract

In this paper, we study quasar proximity zones in the redshift range $$5.77\leqslant z\leqslant 6.54$$ by homogeneously analyzing 34 medium-resolution spectra, encompassing both archival and newly obtained data, and exploiting recently updated systemic redshift and magnitude measurements. Whereas previous studies found strong evolution of proximity zone sizes with redshift and argued that this provides evidence for a rapidly evolving intergalactic medium (IGM) neutral fraction during reionization, we measure a much shallower trend $$\propto {(1+z)}^{-1.44}$$. We compare our measured proximity zone sizes to predictions from hydrodynamical simulations post-processed with one-dimensional radiative transfer and find good agreement between observations and theory, irrespective of the ionization state of the ambient IGM. This insensitivity to IGM ionization state has been previously noted, and results from the fact that the definition of proximity zone size as the first drop of the smoothed quasar spectrum below the 10% flux transmission level probes locations where the ionizing radiation from the quasar is an order of magnitude larger than the expected ultraviolet ionizing background that sets the neutral fraction of the IGM. Our analysis also uncovered three objects with exceptionally small proximity zones (two have $${R}_{p}\lt 1$$ proper Mpc), which constitute outliers from the observed distribution and are challenging to explain with our radiative transfer simulations. Finally, we consider various explanations for their origin, such as strong absorption line systems associated with the quasar or patchy reionization, but find that the most compelling scenario is that these quasars have been shining for ≲105 years.

Authors:
ORCiD logo [1];  [2]; ORCiD logo [2]; ORCiD logo [3];  [4];  [1]
  1. Max Planck Inst. for Astronomy, Heidelberg (Germany); Heidelberg Univ. (Germany)
  2. Max Planck Inst. for Astronomy, Heidelberg (Germany); Univ. of California, Santa Barbara, CA (United States)
  3. Univ. of California, Santa Cruz, CA (United States)
  4. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Org.:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR); USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1379826
Alternate Identifier(s):
OSTI ID: 1563931
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 840; Journal Issue: 1; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; dark ages; reionization; first stars; intergalactic medium; data analysis methods; quasar absorption lines

Citation Formats

Eilers, Anna-Christina, Davies, Frederick B., Hennawi, Joseph F., Prochaska, J. Xavier, Lukić, Zarija, and Mazzucchelli, Chiara. Implications of z ~ 6 Quasar Proximity Zones for the Epoch of Reionization and Quasar Lifetimes. United States: N. p., 2017. Web. doi:10.3847/1538-4357/aa6c60.
Eilers, Anna-Christina, Davies, Frederick B., Hennawi, Joseph F., Prochaska, J. Xavier, Lukić, Zarija, & Mazzucchelli, Chiara. Implications of z ~ 6 Quasar Proximity Zones for the Epoch of Reionization and Quasar Lifetimes. United States. https://doi.org/10.3847/1538-4357/aa6c60
Eilers, Anna-Christina, Davies, Frederick B., Hennawi, Joseph F., Prochaska, J. Xavier, Lukić, Zarija, and Mazzucchelli, Chiara. Tue . "Implications of z ~ 6 Quasar Proximity Zones for the Epoch of Reionization and Quasar Lifetimes". United States. https://doi.org/10.3847/1538-4357/aa6c60. https://www.osti.gov/servlets/purl/1379826.
@article{osti_1379826,
title = {Implications of z ~ 6 Quasar Proximity Zones for the Epoch of Reionization and Quasar Lifetimes},
author = {Eilers, Anna-Christina and Davies, Frederick B. and Hennawi, Joseph F. and Prochaska, J. Xavier and Lukić, Zarija and Mazzucchelli, Chiara},
abstractNote = {In this paper, we study quasar proximity zones in the redshift range $5.77\leqslant z\leqslant 6.54$ by homogeneously analyzing 34 medium-resolution spectra, encompassing both archival and newly obtained data, and exploiting recently updated systemic redshift and magnitude measurements. Whereas previous studies found strong evolution of proximity zone sizes with redshift and argued that this provides evidence for a rapidly evolving intergalactic medium (IGM) neutral fraction during reionization, we measure a much shallower trend $\propto {(1+z)}^{-1.44}$. We compare our measured proximity zone sizes to predictions from hydrodynamical simulations post-processed with one-dimensional radiative transfer and find good agreement between observations and theory, irrespective of the ionization state of the ambient IGM. This insensitivity to IGM ionization state has been previously noted, and results from the fact that the definition of proximity zone size as the first drop of the smoothed quasar spectrum below the 10% flux transmission level probes locations where the ionizing radiation from the quasar is an order of magnitude larger than the expected ultraviolet ionizing background that sets the neutral fraction of the IGM. Our analysis also uncovered three objects with exceptionally small proximity zones (two have ${R}_{p}\lt 1$ proper Mpc), which constitute outliers from the observed distribution and are challenging to explain with our radiative transfer simulations. Finally, we consider various explanations for their origin, such as strong absorption line systems associated with the quasar or patchy reionization, but find that the most compelling scenario is that these quasars have been shining for ≲105 years.},
doi = {10.3847/1538-4357/aa6c60},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 840,
place = {United States},
year = {Tue May 02 00:00:00 EDT 2017},
month = {Tue May 02 00:00:00 EDT 2017}
}

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Cited by: 97 works
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Figures / Tables:

TABLE 1 TABLE 1: Overview of the observations of the 34 quasars in our data sample.

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journal, January 2019

  • Greig, Bradley; Mesinger, Andrei; Bañados, Eduardo
  • Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 4
  • DOI: 10.1093/mnras/stz230

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). VIII. A less biased view of the early co-evolution of black holes and host galaxies
journal, September 2019

  • Izumi, Takuma; Onoue, Masafusa; Matsuoka, Yoshiki
  • Publications of the Astronomical Society of Japan, Vol. 71, Issue 6
  • DOI: 10.1093/pasj/psz096

The Faint End of the z = 5 Quasar Luminosity Function from the CFHTLS
journal, February 2018

  • McGreer, Ian D.; Fan, Xiaohui; Jiang, Linhua
  • The Astronomical Journal, Vol. 155, Issue 3
  • DOI: 10.3847/1538-3881/aaaab4

Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
journal, July 2018


An ALMA [C ii] Survey of 27 Quasars at z > 5.94
journal, February 2018

  • Decarli, Roberto; Walter, Fabian; Venemans, Bram P.
  • The Astrophysical Journal, Vol. 854, Issue 2
  • DOI: 10.3847/1538-4357/aaa5aa

A New Method to Measure the Post-reionization Ionizing Background from the Joint Distribution of Ly α and Ly β Forest Transmission
journal, March 2018

  • Davies, Frederick B.; Hennawi, Joseph F.; Eilers, Anna-Christina
  • The Astrophysical Journal, Vol. 855, Issue 2
  • DOI: 10.3847/1538-4357/aaaf70

Modeling the He ii Transverse Proximity Effect: Constraints on Quasar Lifetime and Obscuration
journal, July 2018

  • Schmidt, Tobias M.; Hennawi, Joseph F.; Worseck, Gábor
  • The Astrophysical Journal, Vol. 861, Issue 2
  • DOI: 10.3847/1538-4357/aac8e4

The Opacity of the Intergalactic Medium Measured along Quasar Sightlines at z ∼ 6
journal, August 2018

  • Eilers, Anna-Christina; Davies, Frederick B.; Hennawi, Joseph F.
  • The Astrophysical Journal, Vol. 864, Issue 1
  • DOI: 10.3847/1538-4357/aad4fd

Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7
journal, September 2018

  • Davies, Frederick B.; Hennawi, Joseph F.; Bañados, Eduardo
  • The Astrophysical Journal, Vol. 864, Issue 2
  • DOI: 10.3847/1538-4357/aad6dc

Predicting Quasar Continua near Ly α with Principal Component Analysis
journal, September 2018

  • Davies, Frederick B.; Hennawi, Joseph F.; Bañados, Eduardo
  • The Astrophysical Journal, Vol. 864, Issue 2
  • DOI: 10.3847/1538-4357/aad7f8

First Spectroscopic Study of a Young Quasar
journal, October 2018

  • Eilers, Anna-Christina; Hennawi, Joseph F.; Davies, Frederick B.
  • The Astrophysical Journal, Vol. 867, Issue 1
  • DOI: 10.3847/1538-4357/aae081

No Evidence for Millimeter Continuum Source Overdensities in the Environments of z ≳ 6 Quasars
journal, November 2018

  • Champagne, Jaclyn B.; Decarli, Roberto; Casey, Caitlin M.
  • The Astrophysical Journal, Vol. 867, Issue 2
  • DOI: 10.3847/1538-4357/aae396

Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6
journal, December 2018

  • Matsuoka, Yoshiki; Strauss, Michael A.; Kashikawa, Nobunari
  • The Astrophysical Journal, Vol. 869, Issue 2
  • DOI: 10.3847/1538-4357/aaee7a

The Evolution of the He ii-ionizing Background at Redshifts 2.3 < z < 3.8 Inferred from a Statistical Sample of 24 HST /COS He ii Ly α Absorption Spectra
journal, April 2019

  • Worseck, Gábor; Davies, Frederick B.; Hennawi, Joseph F.
  • The Astrophysical Journal, Vol. 875, Issue 2
  • DOI: 10.3847/1538-4357/ab0fa1

High Star Formation Rates of Low Eddington Ratio Quasars at z ≳ 6
journal, July 2019


Anomaly in the Opacity of the Post-reionization Intergalactic Medium in the Ly α and Ly β Forest
journal, August 2019

  • Eilers, Anna-Christina; Hennawi, Joseph F.; Davies, Frederick B.
  • The Astrophysical Journal, Vol. 881, Issue 1
  • DOI: 10.3847/1538-4357/ab2b3f

Mapping Quasar Light Echoes in 3D with Ly α Forest Tomography
journal, September 2019

  • Schmidt, Tobias M.; Hennawi, Joseph F.; Lee, Khee-Gan
  • The Astrophysical Journal, Vol. 882, Issue 2
  • DOI: 10.3847/1538-4357/ab2fcb

A Metal-poor Damped Ly α System at Redshift 6.4
journal, October 2019

  • Bañados, Eduardo; Rauch, Michael; Decarli, Roberto
  • The Astrophysical Journal, Vol. 885, Issue 1
  • DOI: 10.3847/1538-4357/ab4129

X-Ray Observations of a z ∼ 6.2 Quasar/Galaxy Merger
journal, December 2019

  • Connor, Thomas; Bañados, Eduardo; Stern, Daniel
  • The Astrophysical Journal, Vol. 887, Issue 2
  • DOI: 10.3847/1538-4357/ab5585

The REQUIEM Survey. I. A Search for Extended Ly α Nebular Emission Around 31 z > 5.7 Quasars
journal, December 2019

  • Farina, Emanuele Paolo; Arrigoni-Battaia, Fabrizio; Costa, Tiago
  • The Astrophysical Journal, Vol. 887, Issue 2
  • DOI: 10.3847/1538-4357/ab5847

Most Lensed Quasars at z > 6 are Missed by Current Surveys
journal, January 2019


Evidence for Low Radiative Efficiency or Highly Obscured Growth of z > 7 Quasars
journal, October 2019

  • Davies, Frederick B.; Hennawi, Joseph F.; Eilers, Anna-Christina
  • The Astrophysical Journal, Vol. 884, Issue 1
  • DOI: 10.3847/2041-8213/ab42e3

Supermassive black holes in the early Universe
journal, December 2015

  • Melia, F.; McClintock, T. M.
  • Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 471, Issue 2184
  • DOI: 10.1098/rspa.2015.0449

Supermassive black holes in the early universe
journal, March 2004

  • Dietrich, M.; Hamann, F.
  • Proceedings of the International Astronomical Union, Vol. 2004, Issue IAUS222
  • DOI: 10.1017/s1743921304003084

Modeling the HeII Transverse Proximity Effect: Constraints on Quasar Lifetime and Obscuration
text, January 2017


The Faint End of the z=5 Quasar Luminosity Function from the CFHTLS
text, January 2017


Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
text, January 2018


The Opacity of the Intergalactic Medium Measured Along Quasar Sightlines at $z\sim 6$
text, January 2018


No Evidence for Millimeter Continuum Source Overdensities in the Environments of $z\gtrsim6$ Quasars
text, January 2018


Nuisance hardened data compression for fast likelihood-free inference
text, January 2019


Discovery of intergalactic bridges connecting two faint $z\sim3$ quasars
text, January 2019


X-ray Observations of a $z\sim6.2$ Quasar/Galaxy Merger
text, January 2019