Masanao Sumiyoshi

Photometric H alpha and [O II] Luminosity Function of SDF and SXDF Galaxies: Implications for Future Baryon Oscillation Surveys (2009)

Sumiyoshi, Masanao, Totani, Tomonori, Oshige, Shunsuke, Glazebrook, Karl, Akiyama, Masayuki, Morokuma, Tomoki, ...

Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy using the baryon...

CCD Photometry of a Newly Confirmed SU UMa-Type Dwarf Nova, NSV 4838 (2009)

Imada, Akira, Yasuda, Tatsuki, Omodaka, Toshihiro, Oizumi, Shota, Yamamoto, Hiroyuki, Tanada, Shunsuke, ...

We present time-resolved CCD photometry of a dwarf nova NSV 4838 (UMa 8, SDSS J102320.27+440509.8) during the 2005 June and 2007 February outburst. Both light curves showed superhumps with a mean...

Photometric H alpha and [O II] luminosity function of SDF and SXDF galaxies: implications for future baryon oscillation surveys (2009)

Sumiyoshi, Masanao, Totani, Tomonori, Oshige, Shunsuke, Glazebrook, Karl, Akiyama, Masayuki, Morokuma, Tomoki, ...

Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy using the baryon...

Photometric H alpha and [O II] luminosity function of SDF and SXDF galaxies: implications for future baryon oscillation surveys (2009)

Sumiyoshi, Masanao, Totani, Tomonori, Oshige, Shunsuke, Glazebrook, Karl, Akiyama, Masayuki, Morokuma, Tomoki, ...

Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy using the baryon...