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Title: Cosmic reionization on computers. Ultraviolet continuum slopes and dust opacities in high redshift galaxies

Abstract

In this study, we compare the properties of stellar populations of model galaxies from the Cosmic Reionization On Computers (CROC) project with the exiting UV and IR data. Since CROC simulations do not follow cosmic dust directly, we adopt two variants of the dust-follows-metals ansatz to populate model galaxies with dust. Using the dust radiative transfer code Hyperion, we compute synthetic stellar spectra, UV continuum slopes, and IR fluxes for simulated galaxies. We find that the simulation results generally match observational measurements, but, perhaps, not in full detail. The differences seem to indicate that our adopted dust-follows-metals ansatzes are not fully sufficient. While the discrepancies with the exiting data are marginal, the future JWST data will be of much higher precision, rendering highly significant any tentative difference between theory and observations. It is, therefore, likely, that in order to fully utilize the precision of JWST observations, fully dynamical modeling of dust formation, evolution, and destruction may be required.

Authors:
 [1];  [2]
  1. Univ. of Chicago, Chicago, IL (United States)
  2. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
Publication Date:
Research Org.:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1244416
Report Number(s):
FERMILAB-PUB-16-018-A; arXiv:1601.00641
Journal ID: ISSN 1538-4357; 1412038
Grant/Contract Number:  
AC02-07CH11359
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 820; Journal Issue: 2; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; cosmology: theory; intergalactic medium; large-scale structure of universe; methods: numerical

Citation Formats

Khakhaleva-Li, Zimu, and Gnedin, Nickolay Y. Cosmic reionization on computers. Ultraviolet continuum slopes and dust opacities in high redshift galaxies. United States: N. p., 2016. Web. doi:10.3847/0004-637X/820/2/133.
Khakhaleva-Li, Zimu, & Gnedin, Nickolay Y. Cosmic reionization on computers. Ultraviolet continuum slopes and dust opacities in high redshift galaxies. United States. https://doi.org/10.3847/0004-637X/820/2/133
Khakhaleva-Li, Zimu, and Gnedin, Nickolay Y. Wed . "Cosmic reionization on computers. Ultraviolet continuum slopes and dust opacities in high redshift galaxies". United States. https://doi.org/10.3847/0004-637X/820/2/133. https://www.osti.gov/servlets/purl/1244416.
@article{osti_1244416,
title = {Cosmic reionization on computers. Ultraviolet continuum slopes and dust opacities in high redshift galaxies},
author = {Khakhaleva-Li, Zimu and Gnedin, Nickolay Y.},
abstractNote = {In this study, we compare the properties of stellar populations of model galaxies from the Cosmic Reionization On Computers (CROC) project with the exiting UV and IR data. Since CROC simulations do not follow cosmic dust directly, we adopt two variants of the dust-follows-metals ansatz to populate model galaxies with dust. Using the dust radiative transfer code Hyperion, we compute synthetic stellar spectra, UV continuum slopes, and IR fluxes for simulated galaxies. We find that the simulation results generally match observational measurements, but, perhaps, not in full detail. The differences seem to indicate that our adopted dust-follows-metals ansatzes are not fully sufficient. While the discrepancies with the exiting data are marginal, the future JWST data will be of much higher precision, rendering highly significant any tentative difference between theory and observations. It is, therefore, likely, that in order to fully utilize the precision of JWST observations, fully dynamical modeling of dust formation, evolution, and destruction may be required.},
doi = {10.3847/0004-637X/820/2/133},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 820,
place = {United States},
year = {Wed Mar 30 00:00:00 EDT 2016},
month = {Wed Mar 30 00:00:00 EDT 2016}
}

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Cited by: 9 works
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Works referenced in this record:

Toward a Complete Accounting of Energy and Momentum from Stellar Feedback in Galaxy Formation Simulations
journal, May 2013

  • Agertz, Oscar; Kravtsov, Andrey V.; Leitner, Samuel N.
  • The Astrophysical Journal, Vol. 770, Issue 1
  • DOI: 10.1088/0004-637X/770/1/25

The formation of disc galaxies in a ΛCDM universe: The formation of disc galaxies
journal, October 2010


Dust formation history of galaxies: A critical role of metallicity dust mass growth by accreting materials in the interstellar medium
journal, March 2013

  • Asano, Ryosuke S.; Takeuchi, Tsutomu T.; Hirashita, Hiroyuki
  • Earth, Planets and Space, Vol. 65, Issue 3
  • DOI: 10.5047/eps.2012.04.014

Hydrogen reionization in the Illustris universe
journal, September 2015

  • Bauer, Andreas; Springel, Volker; Vogelsberger, Mark
  • Monthly Notices of the Royal Astronomical Society, Vol. 453, Issue 4
  • DOI: 10.1093/mnras/stv1893

UV Luminosity Functions at z ∼4, 5, and 6 from the Hubble Ultra Deep Field and Other Deep Hubble Space Telescope ACS Fields: Evolution and Star Formation History
journal, December 2007

  • Bouwens, R. J.; Illingworth, G. D.; Franx, Marijn
  • The Astrophysical Journal, Vol. 670, Issue 2
  • DOI: 10.1086/521811

UV CONTINUUM SLOPE AND DUST OBSCURATION FROM z ∼ 6 TO z ∼ 2: THE STAR FORMATION RATE DENSITY AT HIGH REDSHIFT
journal, October 2009


VERY BLUE UV-CONTINUUM SLOPE β OF LOW LUMINOSITY z ∼ 7 GALAXIES FROM WFC3/IR: EVIDENCE FOR EXTREMELY LOW METALLICITIES?
journal, December 2009


UV-CONTINUUM SLOPES OF >4000 z ∼ 4-8 GALAXIES FROM THE HUDF/XDF, HUDF09, ERS, CANDELS-SOUTH, AND CANDELS-NORTH FIELDS
journal, September 2014


UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS
journal, April 2015


The bright end of the galaxy luminosity function at z≃7: before the onset of mass quenching?
journal, April 2014

  • Bowler, R. A. A.; Dunlop, J. S.; McLure, R. J.
  • Monthly Notices of the Royal Astronomical Society, Vol. 440, Issue 3
  • DOI: 10.1093/mnras/stu449

THE BRIGHTEST OF REIONIZING GALAXIES SURVEY: CONSTRAINTS ON THE BRIGHT END OF THE z ∼ 8 LUMINOSITY FUNCTION
journal, November 2012


Thin disc, thick disc and halo in a simulated galaxy: Disc galaxy decomposition
journal, September 2012


SKIRT: An advanced dust radiative transfer code with a user-friendly architecture
journal, March 2015


Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission
journal, June 2015


The Propagation of Uncertainties in Stellar Population Synthesis Modeling. iii. Model Calibration, Comparison, and Evaluation
journal, March 2010


The Propagation of Uncertainties in Stellar Population Synthesis Modeling. ii. the Challenge of Comparing Galaxy Evolution Models to Observations
journal, December 2009


Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
journal, July 2007

  • Draine, B. T.; Dale, D. A.; Bendo, G.
  • The Astrophysical Journal, Vol. 663, Issue 2
  • DOI: 10.1086/518306

Low-mass galaxy formation and the ionizing photon budget during reionization
journal, August 2014

  • Duffy, Alan R.; Wyithe, J. Stuart B.; Mutch, Simon J.
  • Monthly Notices of the Royal Astronomical Society, Vol. 443, Issue 4
  • DOI: 10.1093/mnras/stu1328

The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field
journal, September 2014

  • Duncan, K.; Conselice, C. J.; Mortlock, A.
  • Monthly Notices of the Royal Astronomical Society, Vol. 444, Issue 3
  • DOI: 10.1093/mnras/stu1622

A critical analysis of the ultraviolet continuum slopes (β) of high-redshift galaxies: no evidence (yet) for extreme stellar populations at z > 6: The UV slopes of high-redshift galaxies
journal, December 2011


The UV continua and inferred stellar populations of galaxies at z ≃ 7–9 revealed by the Hubble Ultra-Deep Field 2012 campaign
journal, May 2013

  • Dunlop, J. S.; Rogers, A. B.; McLure, R. J.
  • Monthly Notices of the Royal Astronomical Society, Vol. 432, Issue 4
  • DOI: 10.1093/mnras/stt702

The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxies
journal, April 2015

  • Feldmann, Robert
  • Monthly Notices of the Royal Astronomical Society, Vol. 449, Issue 3
  • DOI: 10.1093/mnras/stv552

CANDELS: THE EVOLUTION OF GALAXY REST-FRAME ULTRAVIOLET COLORS FROM z = 8 TO 4
journal, August 2012


The James Webb Space Telescope
book, January 2009


Cosmic Reionization on Computers. i. Design and Calibration of Simulations
journal, September 2014


Escape of Ionizing Radiation from High‐Redshift Galaxies
journal, January 2008

  • Gnedin, Nickolay Y.; Kravtsov, Andrey V.; Chen, Hsiao‐Wen
  • The Astrophysical Journal, Vol. 672, Issue 2
  • DOI: 10.1086/524007

Implementing the dc mode in Cosmological Simulations with Supercomoving Variables
journal, June 2011

  • Gnedin, Nickolay Y.; Kravtsov, Andrey V.; Rudd, Douglas H.
  • The Astrophysical Journal Supplement Series, Vol. 194, Issue 2
  • DOI: 10.1088/0067-0049/194/2/46

Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows
journal, January 2010


The visibility of Lyman α emitters: constraining reionization, ionizing photon escape fractions and dust
journal, May 2014

  • Hutter, Anne; Dayal, Pratika; Partl, Adrian M.
  • Monthly Notices of the Royal Astronomical Society, Vol. 441, Issue 4
  • DOI: 10.1093/mnras/stu791

Simulating cosmic reionization: how large a volume is large enough?
journal, January 2014

  • Iliev, Ilian T.; Mellema, Garrelt; Ahn, Kyungjin
  • Monthly Notices of the Royal Astronomical Society, Vol. 439, Issue 1
  • DOI: 10.1093/mnras/stt2497

Evolution of Dust-to-Metal Ratio in Galaxies
journal, October 2003

  • Inoue, Akio K.
  • Publications of the Astronomical Society of Japan, Vol. 55, Issue 5
  • DOI: 10.1093/pasj/55.5.901

The origin of dust in galaxies revisited: the mechanism determining dust content
journal, October 2011


SUNRISE: polychromatic dust radiative transfer in arbitrary geometries
journal, October 2006


High-resolution panchromatic spectral models of galaxies including photoionization and dust
journal, March 2010


Constrained Simulations of the Real Universe. II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region
journal, June 2002

  • Kravtsov, Andrey V.; Klypin, Anatoly; Hoffman, Yehuda
  • The Astrophysical Journal, Vol. 571, Issue 2
  • DOI: 10.1086/340046

THE CO-TO-H 2 CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUP
journal, July 2011


Preparing Red‐Green‐Blue Images from CCD Data
journal, February 2004

  • Lupton, Robert; Blanton, Michael R.; Fekete, George
  • Publications of the Astronomical Society of the Pacific, Vol. 116, Issue 816
  • DOI: 10.1086/382245

Cosmic Reionization After Planck: Could Quasars do it all?
journal, October 2015


Dust Absorption and the Ultraviolet Luminosity Density at z  ≈ 3 as Calibrated by Local Starburst Galaxies
journal, August 1999

  • Meurer, Gerhardt R.; Heckman, Timothy M.; Calzetti, Daniela
  • The Astrophysical Journal, Vol. 521, Issue 1
  • DOI: 10.1086/307523

Fully Coupled Simulation of Cosmic Reionization. i. Numerical Methods and Tests
journal, January 2015

  • Norman, Michael L.; Reynolds, Daniel R.; So, Geoffrey C.
  • The Astrophysical Journal Supplement Series, Vol. 216, Issue 1
  • DOI: 10.1088/0067-0049/216/1/16

THE BRIGHT END OF THE ULTRAVIOLET LUMINOSITY FUNCTION AT z ∼ 8: NEW CONSTRAINTS FROM CANDELS DATA IN GOODS-SOUTH
journal, October 2012


PROBING THE DAWN OF GALAXIES AT z ∼ 9-12: NEW CONSTRAINTS FROM HUDF12/XDF AND CANDELS DATA
journal, July 2013


THE MOST LUMINOUS z ∼ 9-10 GALAXY CANDIDATES YET FOUND: THE LUMINOSITY FUNCTION, COSMIC STAR-FORMATION RATE, AND THE FIRST MASS DENSITY ESTIMATE AT 500 Myr
journal, April 2014


Generating Cosmological Gaussian Random Fields
journal, December 1997

  • Pen, Ue-Li
  • The Astrophysical Journal, Vol. 490, Issue 2
  • DOI: 10.1086/311042

HYPERION: an open-source parallelized three-dimensional dust continuum radiative transfer code
journal, December 2011


The colour distribution of galaxies at redshift five
journal, April 2014

  • Rogers, A. B.; McLure, R. J.; Dunlop, J. S.
  • Monthly Notices of the Royal Astronomical Society, Vol. 440, Issue 4
  • DOI: 10.1093/mnras/stu558

Effects of Baryons and Dissipation on the Matter Power Spectrum
journal, January 2008

  • Rudd, Douglas H.; Zentner, Andrew R.; Kravtsov, Andrey V.
  • The Astrophysical Journal, Vol. 672, Issue 1
  • DOI: 10.1086/523836

THE UV LUMINOSITY FUNCTION OF STAR-FORMING GALAXIES VIA DROPOUT SELECTION AT REDSHIFTS z ∼ 7 AND 8 FROM THE 2012 ULTRA DEEP FIELD CAMPAIGN
journal, April 2013

  • Schenker, Matthew A.; Robertson, Brant E.; Ellis, Richard S.
  • The Astrophysical Journal, Vol. 768, Issue 2
  • DOI: 10.1088/0004-637X/768/2/196

Initial Conditions to Cosmological N ‐Body Simulations, or, How to Run an Ensemble of Simulations
journal, December 2005

  • Sirko, Edwin
  • The Astrophysical Journal, Vol. 634, Issue 2
  • DOI: 10.1086/497090

Fully Coupled Simulation of Cosmic Reionization. ii. Recombinations, Clumping Factors, and the Photon Budget for Reionization
journal, June 2014

  • So, Geoffrey C.; Norman, Michael L.; Reynolds, Daniel R.
  • The Astrophysical Journal, Vol. 789, Issue 2
  • DOI: 10.1088/0004-637X/789/2/149

The Metallicity and dust Content of a Redshift 5 Gamma-Ray Burst host Galaxy
journal, April 2014


Making Galaxies In a Cosmological Context: the need for early stellar feedback
journal, October 2012

  • Stinson, G. S.; Brook, C.; Macciò, A. V.
  • Monthly Notices of the Royal Astronomical Society, Vol. 428, Issue 1
  • DOI: 10.1093/mnras/sts028

Feedback and the formation of dwarf galaxy stellar haloes
journal, May 2009


Scorch. i. the Galaxy–Halo Connection in the First Billion Years
journal, October 2015


A dusty, normal galaxy in the epoch of reionization
journal, March 2015

  • Watson, Darach; Christensen, Lise; Knudsen, Kirsten Kraiberg
  • Nature, Vol. 519, Issue 7543
  • DOI: 10.1038/nature14164

Dust Grain–Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud
journal, February 2001

  • Weingartner, Joseph C.; Draine, B. T.
  • The Astrophysical Journal, Vol. 548, Issue 1
  • DOI: 10.1086/318651

The ultraviolet properties of star-forming galaxies - I. HST WFC3 observations of very high redshift galaxies: The UV properties of star-forming galaxies - I
journal, August 2011

  • Wilkins, Stephen M.; Bunker, Andrew J.; Stanway, Elizabeth
  • Monthly Notices of the Royal Astronomical Society, Vol. 417, Issue 1
  • DOI: 10.1111/j.1365-2966.2011.19315.x

AN EXPONENTIAL DECLINE AT THE BRIGHT END OF THE z = 6 GALAXY LUMINOSITY FUNCTION
journal, November 2012

  • Willott, Chris J.; McLure, Ross J.; Hibon, Pascale
  • The Astronomical Journal, Vol. 145, Issue 1
  • DOI: 10.1088/0004-6256/145/1/4

The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
journal, December 2013


Works referencing / citing this record:

Interpreting the evolution of galaxy colours from z  = 8 to 5
journal, July 2016

  • Mancini, Mattia; Schneider, Raffaella; Graziani, Luca
  • Monthly Notices of the Royal Astronomical Society, Vol. 462, Issue 3
  • DOI: 10.1093/mnras/stw1783