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  • 1506.02670v1

    Rights statement: This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version I. Oteo, D. Sobral, R. J. Ivison, I. Smail, P. N. Best, J. Cepa, and A. M. Pérez-García On the nature of Hα emitters at z~ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence MNRAS 2015 452: 2018-2033. is available online at: http://mnras.oxfordjournals.org/content/452/2/2018

    Accepted author manuscript, 2.51 MB, PDF document

    Available under license: CC BY: Creative Commons Attribution 4.0 International License

  • 1506.02670v1

    Accepted author manuscript, 2.51 MB, PDF document

    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

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On the nature of H$α$ emitters at $z \sim 2$ from the HiZELS survey: physical properties, Ly$α$ escape fraction, and main sequence

Research output: Contribution to journalJournal articlepeer-review

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  • I. Oteo
  • D. Sobral
  • R. J. Ivison
  • I. Smail
  • P. N. Best
  • J. Cepa
  • A. M. Perez-Garcia
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<mark>Journal publication date</mark>11/09/2015
<mark>Journal</mark>Monthly Notices of the Royal Astronomical Society
Issue number2
Volume452
Number of pages16
Pages (from-to)2018-2033
Publication StatusPublished
Early online date21/07/15
<mark>Original language</mark>English

Abstract

We present a detailed multi-wavelength study (from rest-frame UV to far-IR) of narrow-band (NB) selected, star-forming (SF) H$\alpha$ emitters (HAEs) at $z \sim 2.23$ taken from the High Redshift(Z) Emission Line Survey (HiZELS). We find that HAEs have similar SED-derived properties and colors to $sBzK$ galaxies and probe a well-defined portion of the SF population at $z \sim 2$. This is not true for Ly$\alpha$ emitters (LAEs), which are strongly biased towards blue, less massive galaxies (missing a significant percentage of the SF population). Combining our H$\alpha$ observations with matched, existing Ly$\alpha$ data we determine that the Ly$\alpha$ escape fraction ($f_{\rm esc}$) is low (only $\sim$ 4.5\% of HAEs show Ly$\alpha$ emission) and decreases with increasing dust attenuation, UV continuum slope, stellar mass, and star formation rate (SFR). This suggests that Ly$\alpha$ preferentially escapes from blue galaxies with low dust attenuation. However, a small population of red and massive LAEs is also present in agreement with previous works. This indicates that dust and Ly$\alpha$ are not mutually exclusive. Using different and completely independent measures of the total SFR we show that the H$\alpha$ emission is an excellent tracer of star formation at $z \sim 2$ with deviations typically lower than 0.3 dex for individual galaxies. We find that the slope and zero-point of the HAE main-sequence (MS) at $z \sim 2$ strongly depend on the dust correction method used to recover SFR, although they are consistent with previous works when similar assumptions are made.

Bibliographic note

This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version I. Oteo, D. Sobral, R. J. Ivison, I. Smail, P. N. Best, J. Cepa, and A. M. Pérez-García On the nature of Hα emitters at z~ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence MNRAS 2015 452: 2018-2033. is available online at: http://mnras.oxfordjournals.org/content/452/2/2018