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The Intermediate-band Dropout Method: A New Method to Search for High-Redshift Galaxies

Yasuhiro Shioya·Yoshiaki Taniguchi·Masaru Ajiki·Tohru Nagao·Takashi Murayama·Shunji Sasaki·Ryoko Sumiya·Yuichiro Hatakeyama
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Abstract

We propose a new method to search for high-redshift galaxies that is based on an intermediate-band dropout technique rather than the usual broad-band dropout one. In this method, we use an intermediate-band filter whose central wavelength is longer than 7000 Å. This new method makes it possible to distinguish both very late-type stars such as L and T dwarfs and dusty galaxies at intermediate redshift from real high-$z$ Lyman break galaxies. The reason for this is that such interlopers do not show strong intermediate-band depression although they have very red broad-band colors that are indicative of Lyman break galaxies. Applying our new method to imaging data sets obtained with the Suprime-Cam on the Subaru Telescope, we find a new sample of Lyman break galaxies at $z \simeq 5$.

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Yasuhiro Shioya, Yoshiaki Taniguchi, Masaru Ajiki, Tohru Nagao, Takashi Murayama, Shunji Sasaki, Ryoko Sumiya, Yuichiro Hatakeyama. 2005-02-17. The Intermediate-band Dropout Method: A New Method to Search for High-Redshift Galaxies. https://doi.org/10.1093/pasj%2F57.2.287

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