[PFV2011] BDF-2203 , the SIMBAD biblio

[PFV2011] BDF-2203 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST19:24:09


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Title First 3 Authors
2011ApJ...743..132P 19       D               1 32 270 Spectroscopic confirmation of z ∼ 7 Lyman break galaxies: probing the earliest galaxies and the epoch of reionization. PENTERICCI L., FONTANA A., VANZELLA E., et al.
2018ApJ...859...84H 17       D               1 87 105 SILVERRUSH. V. Census of Lyα, [O III] λ5007, Hα, and [C II] 158 µm line emission with ∼1000 LAEs at z = 4.9-7.0 revealed with Subaru/HSC. HARIKANE Y., OUCHI M., SHIBUYA T., et al.
2018MNRAS.478.1170C 419       D     X C       10 41 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2019MNRAS.487.1689P 86               F     1 15 87 Deep into the structure of the first galaxies: SERRA views. PALLOTTINI A., FERRARA A., DECATALDO D., et al.
2019MNRAS.487.3007K 18       D               1 26 66 Kinematics of z >= 6 galaxies from [C II] line emission. KOHANDEL M., PALLOTTINI A., FERRARA A., et al.
2019ApJ...881..124M 17       D               3 37 73 Resolved UV and [C II] structures of luminous galaxies within the epoch of reionization. MATTHEE J., SOBRAL D., BOOGAARD L.A., et al.
2019ApJ...887..107F 142       D     X C       3 20 93 First identification of 10 kpc [C II] 158 µm halos around star-forming galaxies at z = 5-7. FUJIMOTO S., OUCHI M., FERRARA A., et al.
2020ApJ...896...93H 18       D               1 50 106 Large population of ALMA galaxies at z > 6 with very high [O III] 88 µm to [C II] 158 µm flux ratios: evidence of extremely high ionization parameter or PDR deficit? HARIKANE Y., OUCHI M., INOUE A.K., et al.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024MNRAS.534.2062V 18       D               1 72 ~ Characterising the contribution of dust-obscured star formation at ≳ 5 using 18 serendipitously identified [C II] emitters. VAN LEEUWEN I.F., BOUWENS R.J., VAN DER WERF P.P., et al.

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