[NTK2004] SDF J132440.6+273607 , the SIMBAD biblio

[NTK2004] SDF J132440.6+273607 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST10:29:16


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Title First 3 Authors
2004ApJ...613L...9N 43   K                 2 39 A strong Lyα emitter at z = 6.33 in the Subaru Deep Field selected as an i'-dropout. NAGAO T., TANIGUCHI Y., KASHIKAWA N., et al.
2005ApJ...631L...5N 38   K                 8 26 An observational pursuit for population III stars in a Lyα emitter at z = 6.33 through He II emission. NAGAO T., MOTOHARA K., MAIOLINO R., et al.
2005ApJ...634..142N 1 5 24 Spectroscopy of i'-dropout galaxies with an NB921-Band depression in the Subaru Deep Field. NAGAO T., KASHIKAWA N., MALKAN M.A., et al.
2007ApJ...660...47D 28 60 Spectroscopy of z ∼ 6 i-dropout galaxies: frequency of Lyα emission and the sizes of Lyα-emitting galaxies. DOW-HYGELUND C.C., HOLDEN B.P., BOUWENS R.J., et al.
2007A&A...468..877N 126       D     X         4 10 26 High-redshift Lyα emitters with a large equivalent width. Properties of i'-dropout galaxies with an NB921-band depression in the Subaru Deep Field. NAGAO T., MURAYAMA T., MAIOLINO R., et al.
2009MNRAS.399...37J 115               F     1 1 80 The first galaxies: signatures of the initial starburst. JOHNSON J.L., GREIF T.H., BROMM V., et al.
2011ARA&A..49..373B 112             C       1 5 368 The first galaxies. BROMM V. and YOSHIDA N.
2013ApJ...772...99J 15       D               1 68 51 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. I. Basic characteristics of the rest-frame UV continuum and Lyα emission. JIANG L., EGAMI E., MECHTLEY M., et al.
2013ApJ...773..153J 77               F     1 46 42 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. II. Morphology of the rest-frame UV continuum and Lyα emission. JIANG L., EGAMI E., FAN X., et al.
2015MNRAS.451.2050Z 95       D       C       2 9 20 Deep rest-frame far-UV spectroscopy of the giant Lyman α emitter `Himiko'. ZABL J., NORGAARD-NIELSEN H.U., FYNBO J.P.U., et al.
2016ApJ...816...16J 16       D               3 44 23 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. III. Stellar populations from SED modeling with secure Lyα emission and redshifts. JIANG L., FINLATOR K., COHEN S.H., et al.
2018PASJ...70S..15S 162           X C       3 104 117 SILVERRUSH. III. Deep optical and near-infrared spectroscopy for Lyα and UV-nebular lines of bright Lyα emitters at z = 6-7. SHIBUYA T., OUCHI M., HARIKANE Y., et al.

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