Systematic survey of extended Lyα sources over z ∼ 3-5

Tomoki Saito, Kazuhiro Shimasaku, Sadanori Okamura, Masami Ouchi, Masayuki Akiyama, Michitoshi Yoshida

Research output: Contribution to journalReview articlepeer-review

67 Citations (Scopus)

Abstract

Spatially extended Lyα sources that are faint and compact in continuum are candidates for extremely young (≲107 yr) galaxies at high redshifts. We carried out a systematic survey for extended Lyα sources, using deep intermediate-band imaging data taken with the Suprime-Cam on the Subaru Telescope. Our survey covers a field of view of 33′ × 25× and a redshift range of 3.24 ≲ z ≲ 4.95, down to a Lyα flux of ∼1 × 10-17 ergs cm-2 s-1. We identified 41 extended Lyα sources. The redshift distribution of these sources shows that this kind of object is common in the early universe over the surveyed redshift range. The identified objects have typical sizes of ∼10-15 kpc and luminosities of ∼1042 ergs s-1. Follow-up spectroscopy made for 7 of the 41 objects showed that our sample suffers from little contamination. All 7 objects have large equivalent widths of Lyα emission line, all but one exceeding 240 Å in the rest frame. The large equivalent widths suggest that their extended Lyα emissions are unlikely to be due to normal starbursts, but possibly originate from very young galaxies. All 41 objects in our sample have much smaller Lyα luminosities than the two Lyα blobs (LABs) found at a z ≃ 3.1 protocluster, in spite of our much larger survey volume. This suggests that large and luminous extended Lyα objects like the two LABs are very rare and are clustered in overdense regions.

Original languageEnglish
Pages (from-to)54-66
Number of pages13
JournalAstrophysical Journal
Volume648
Issue number1 I
DOIs
Publication statusPublished - 2006 Sep 1
Externally publishedYes

Keywords

  • Galaxies: formation
  • Galaxies: high-redshift

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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