CaltechAUTHORS
  A Caltech Library Service

The Keck Lyman Continuum Spectroscopic Survey (KLCS): The Emergent Ionizing Spectrum of Galaxies at z ∼ 3

Steidel, Charles C. and Bogosavljević, Milan and Shapley, Alice E. and Reddy, Naveen A. and Rudie, Gwen C. and Pettini, Max and Trainor, Ryan F. and Strom, Allison L. (2018) The Keck Lyman Continuum Spectroscopic Survey (KLCS): The Emergent Ionizing Spectrum of Galaxies at z ∼ 3. Astrophysical Journal, 869 (2). Art. No. 123. ISSN 1538-4357. http://resolver.caltech.edu/CaltechAUTHORS:20181129-135236660

[img] PDF - Published Version
Creative Commons Attribution.

12Mb
[img] PDF - Submitted Version
See Usage Policy.

5Mb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20181129-135236660

Abstract

We present results of a deep spectroscopic survey quantifying the statistics of the escape of ionizing radiation from star-forming galaxies at z ~ 3. We measure the ratio of ionizing to non-ionizing UV flux density 〈f_(900)/f_(1500) 〉_(obs), where f_(900) is the mean flux density evaluated over the range [880, 910] Å. We quantify the emergent ratio of ionizing to non-ionizing UV flux density by analyzing high signal-to-noise ratio composite spectra formed from subsamples with common observed properties and numbers sufficient to reduce the statistical uncertainty in the modeled IGM+CGM correction to obtain precise values of 〈f_(900)/f_(1500) 〉_(out), including a full-sample average 〈f_(900)/f_(1500) 〉_(out) = 0.057 ± 0.006. We show that 〈f_(900)/f_(1500) 〉_(out) increases monotonically with W_ λ(Lyα), inducing an inverse correlation with UV luminosity as a by-product. We fit the composite spectra using stellar spectral synthesis together with models of the ISM in which a fraction f c of the stellar continuum is covered by gas with column density N_(H1). We show that the composite spectra simultaneously constrain the intrinsic properties of the stars (L_(900)/L_(1500))_(int) along with f_c , N_(H1), E(B - V), and f_(esc,abs), the absolute escape fraction of ionizing photons. We find a sample-averaged f-(esc,abs) = 0.09 ± 0.01, with subsamples falling along a linear relation 〈f_(esc,abs) 〉 ≃ 0.75[W_ λ(Lyα)/110 Å]. Using the far-UV luminosity function, the distribution function n(W(Lyα)), and the relationship between W_ λ(Lyα) and f_(900)/f_(1500) 〉_(out), we estimate the total ionizing emissivity of z ~ 3 star-forming galaxies with M_(uv) ≤ −19.5, which exceeds the contribution of quasi-stellar objects by a factor of ~3, and accounts for ~50% of the total ϵ_(LyC) at z ~ 3 estimated using indirect methods.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/aaed28DOIArticle
https://arxiv.org/abs/1805.06071arXivDiscussion Paper
ORCID:
AuthorORCID
Steidel, Charles C.0000-0002-4834-7260
Shapley, Alice E.0000-0003-3509-4855
Reddy, Naveen A.0000-0001-9687-4973
Rudie, Gwen C.0000-0002-8459-5413
Trainor, Ryan F.0000-0002-6967-7322
Strom, Allison L.0000-0001-6369-1636
Additional Information:© 2018 The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 2018 May 16; revised 2018 October 18; accepted 2018 October 27; published 2018 December 18. Based on data obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, and was made possible by the generous financial support of the W.M. Keck Foundation. This work has been supported in part by the US National Science Foundation through grants AST-0606912, AST-0908805, and AST-1313472 (M.B., C.C.S., G.C.R., R.F.T., A.L.S.). C.C.S. acknowledges additional support from the John D. and Catherine T. MacArthur Foundation, the David and Lucile Packard Foundation, and the JPL/Caltech President's and Director's program. We thank J. J. Eldridge and Elizabeth Stanway for their continued work developing the BPASS SPS models and for many illuminating conversations. We are grateful to the dedicated staff of the W.M. Keck Observatory who keep the instruments and telescopes running effectively. We wish to extend thanks to those of Hawaiian ancestry on whose sacred mountain we are privileged to be guests.
Funders:
Funding AgencyGrant Number
NSFAST-0606912
NSFAST-0908805
NSFAST-1313472
John D. and Catherine T. MacArthur FoundationUNSPECIFIED
David and Lucile Packard FoundationUNSPECIFIED
JPL President and Director's FundUNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:cosmology: observations – galaxies: evolution – galaxies: high-redshift – intergalactic medium – ultraviolet: galaxies
Record Number:CaltechAUTHORS:20181129-135236660
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20181129-135236660
Official Citation:Charles C. Steidel et al 2018 ApJ 869 123
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91336
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:30 Nov 2018 15:07
Last Modified:18 Dec 2018 19:09

Repository Staff Only: item control page