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On the narrowband detection properties of high-redshift Lyman-alpha emitters
Stockholm University, Faculty of Science, Department of Astronomy.
Stockholm University, Faculty of Science, Department of Astronomy.
2006 (English)In: Astronomy & Astrophysics, ISSN 0004-6361, Vol. 460, no 3, 681-694 p.Article in journal (Refereed) Published
Abstract [en]

Context: Numerous surveys are currently underway or planned that aim to exploit the strengths of the Lyman-alpha emission line for cosmological purposes. Today, narrowband imaging surveys are frequently used as a probe of the distant universe.

Aims: To investigate the reliability of the results of such high-z Lyα studies, and the validity of the conclusions that are based upon them. To determine whether reliable Lyα fluxes (FLyα) and equivalent widths (WLyα) can be estimated from narrowband imaging surveys and whether any observational biases may be present.

Methods: We have developed software to simulate the observed line and continuum properties of synthetic Lyα galaxies in the distant universe by adopting various typical observational survey techniques. This was used to investigate how detected FLyα and WLyα vary with properties of the host galaxy or intergalactic medium: internal dust reddening; intervening Lyα absorption systems; the presence of underlying stellar populations.

Results: None of the techniques studied are greatly susceptible to underlying stellar populations or the relative contribution of nebular gas. We find that techniques that use one off-line filter on the red side of Lyα result in highly inaccurate measurements of WLyα under all tests. Adopting two off-line filters to estimate continuum at Lyα is an improvement but is still unreliable when dust extinction is considered. Techniques that employ single narrow- and broad-band filters with the same central wavelength are not susceptible to internal dust, but Lyα absorption in the IGM can cause WLyα to be overestimated by factors of up to 2: at z=6, the median WLyα is overestimated by ~25%. The most robust approach is a SED fitting technique that fits EB-V and burst-age from synthetic models - broadband observations are needed that sample the UV continuum slope, 2175 Å dust feature, and the 4000 Å discontinuity. We also notice a redshift-dependent incompleteness that results from DLA systems close to the target LAEs, amounting to ˜ 10% at z=6.

Place, publisher, year, edition, pages
2006. Vol. 460, no 3, 681-694 p.
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:su:diva-20157DOI: doi:10.1051/0004-6361:20065493OAI: diva2:186682
Available from: 2007-02-27 Created: 2007-02-27 Last updated: 2011-01-11Bibliographically approved

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