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| [CFP2010] BDF 521 , the SIMBAD biblio (25 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:09:01 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2010A&A...524A..28C | 18 | D | 1 | 11 | 71 | The bright end of the z ∼ 7 UV luminosity function from a wide and deep HAWK-I survey. | CASTELLANO M., FONTANA A., PARIS D., et al. | ||
| 2011ApJ...730L..35V | 346 | D | X C | 8 | 3 | 172 | Spectroscopic confirmation of two Lyman break galaxies at redshift beyond 7. | VANZELLA E., PENTERICCI L., FONTANA A., et al. | |
| 2012ApJ...744...83O | 18 | D | 1 | 53 | 350 | Spectroscopic confirmation of three z-dropout galaxies at z = 6.844-7.213: demographics of Lyα emission in z ∼ 7 galaxies. | ONO Y., OUCHI M., MOBASHER B., et al. | ||
| 2013Natur.502..524F | 12 | 9 | 226 | A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51. | FINKELSTEIN S.L., PAPOVICH C., DICKINSON M., et al. | ||||
| 2015MNRAS.451L..70M | 21 | D | 1 | 11 | 123 | The dust mass in z > 6 normal star-forming galaxies. | MANCINI M., SCHNEIDER R., GRAZIANI L., et al. | ||
| 2015ApJ...813...36V | 83 | C | 1 | 14 | 144 | On the [CII]-SFR relation in high redshift galaxies. | VALLINI L., GALLERANI S., FERRARA A., et al. | ||
| 2015MNRAS.452...54M | 103 | D | X | 3 | 10 | 186 | The assembly of `normal' galaxies at z ∼ 7 probed by ALMA. | MAIOLINO R., CARNIANI S., FONTANA A., et al. | |
| 2015A&A...584A..78C | 161 | X | 4 | 6 | 69 | ALMA constraints on the faint millimetre source number counts and their contribution to the cosmic infrared background. | CARNIANI S., MAIOLINO R., DE ZOTTI G., et al. | ||
|
2016ApJS..222....1F |
1 | 40 | 108 | ALMA census of faint 1.2 mm sources down to ∼ 0.02 mJy: extragalactic background light and dust-poor, high-z galaxies. | FUJIMOTO S., OUCHI M., ONO Y., et al. | ||||
| 2016ApJ...818L...3C | 599 | X C | 14 | 3 | 59 | First observational support for overlapping reionized bubbles generated by a galaxy overdensity. | CASTELLANO M., DAYAL P., PENTERICCI L., et al. | ||
| 2017MNRAS.464..469S | 28 | D | 1 | 11 | 281 | Lyα and C III] emission in z = 7-9 Galaxies: accelerated reionization around luminous star-forming systems? | STARK D.P., ELLIS R.S., CHARLOT S., et al. | ||
|
2017ApJ...846..105O |
17 | D | 2 | 36 | 76 | SIGAME simulations of the [C II], [O I] and [O III] line emission from star-forming galaxies at z ~= 6. | OLSEN K., GREVE T.R., NARAYANAN D., et al. | ||
|
2017MNRAS.472..772M |
16 | D | 2 | 48 | 66 | Spectroscopic properties of luminous Ly α emitters at z ~= 6-7 and comparison to the Lyman-break population. | MATTHEE J., SOBRAL D., DARVISH B., 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 | 18 | D | 3 | 41 | 108 | Kiloparsec-scale gaseous clumps and star formation at z = 5-7. | CARNIANI S., MAIOLINO R., AMORIN R., et al. | ||
| 2018ApJ...863L...3C | 16 | D | 1 | 17 | 10 | Spectroscopic investigation of a reionized galaxy overdensity at z = 7. | CASTELLANO M., PENTERICCI L., VANZELLA E., et al. | ||
| 2019A&A...623A.157S | 2 | 27 | 57 | Predicting Lyα escape fractions with a simple observable. Lyα in emission as an empirically calibrated star formation rate indicator. | SOBRAL D. and MATTHEE J. | ||||
| 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. | ||
| 2020MNRAS.494.1071G | 100 | D | F | 2 | 54 | 62 | The assembly of dusty galaxies at z >= 4: statistical properties. | GRAZIANI L., SCHNEIDER R., GINOLFI M., 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. | ||
| 2021MNRAS.503.4242R | 268 | D | X F | 6 | 18 | ~ | Is the Bremer Deep Field reionized, at z ∼ 7? | RODRIGUEZ ESPINOSA J.M., MAS-HESSE J.M. and CALVI R. | |
| 2022A&A...662A.115C | 1152 | T A | D | X C | 26 | 4 | 13 | The ionizing properties of two bright Lyα emitters in the Bremer Deep Field reionized bubble at z = 7. | CASTELLANO M., PENTERICCI L., CUPANI G., et al. |
| 2022MNRAS.517.5642E | 17 | D | 1 | 31 | 29 | The REBELS ALMA Survey: efficient Ly α transmission of UV-bright z ≃ 7 galaxies from large velocity offsets and broad line widths. | ENDSLEY R., STARK D.P., BOUWENS R.J., 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. |