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Strong Emission-Line Galaxies at Low Redshift in the Field around the Quasar SDSSp J104433.04-012502.2

Masaru Ajiki·Yasuhiro Shioya·Yoshiaki Taniguchi·Takashi Murayama·Tohru Nagao·Shunji S. Sasaki·Ryoko Sumiya·Taichi Morioka·Yuichiro Hatakeyama·Asuka Yokouchi·Mari I. Takahashi·Osamu Koizumi
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Abstract

We discuss observational properties of strong emission-line galaxies at low redshift found by our deep imaging survey for high-redshift Ly alpha emitters. In our surveys, we used the narrowband filter, NB816 (lambda_center=8150A with FWHM = 120A), and the intermediate-band filter, IA827 (lambda_center = 8270A with FWHM = 340A). In this survey, 62 NB816-excess (> 0.9 mag) and 21 IA827-excess (> 0.8 mag) objects were found. Among them, we found 20 NB816-excess and 4 IA827-excess Ly alpha emitter candidates. Therefore, it turns out that 42 NB816-excess and 17 IA827-excess objects are strong emission-line objects at lower redshift. Since 4 objects in the two low-z samples are common, the total number of strong low-z emitters is 55. Applying our photometric redshift technique, we identify 7 H alpha emitters at z~0.24, 20 H beta-[OIII] ones at z~0.65, and 11 [OII] ones at z~1.19. However, we cannot determine reliable photometric redshifts of the remaining 17 emitters. The distributions of their rest frame equivalent widths are consistently understood with recent studies of galaxy evolution from z~1 to z~0.

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Masaru Ajiki, Yasuhiro Shioya, Yoshiaki Taniguchi, Takashi Murayama, Tohru Nagao, Shunji S. Sasaki, Ryoko Sumiya, Taichi Morioka, Yuichiro Hatakeyama, Asuka Yokouchi, Mari I. Takahashi, Osamu Koizumi. 2005-11-16. Strong Emission-Line Galaxies at Low Redshift in the Field around the Quasar SDSSp J104433.04-012502.2. https://doi.org/10.1093/pasj%2F58.1.113

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