IOK 1 , the SIMBAD biblio

IOK 1 , the SIMBAD biblio (55 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:34:06

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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
2006Natur.443..186I 24 4 292 A galaxy at a redshift z = 6.96. IYE M., OTA K., KASHIKAWA N., et al.
2008ApJ...677...12O 1214       D S   X C       31 12 176 Reionization and galaxy evolution probed by z = 7 Lyα emitters. OTA K., IYE M., KASHIKAWA N., et al.
2008ApJ...685..705R 39           X         1 20 102 A Hubble and Spitzer Space Telescope Survey for gravitationally lensed galaxies: further evidence for a significant population of low-luminosity galaxies beyond z=7. RICHARD J., STARK D.P., ELLIS R.S., et al.
2009ApJ...697L..33W 712     A D     X C F     18 8 15 The molecular gas content of z > 6.5 lyman-α emitters. WAGG J., KANEKAR N. and CARILLI C.L.
2009A&A...505...97M 40           X         1 8 59 Discovery of a redshift 6.13 quasar in the UKIRT infrared deep sky survey. MORTLOCK D.J., PATEL M., WARREN S.J., et al.
2009ApJ...706.1136O 303       D     X C       7 5 266 Large area survey for z = 7 galaxies in SDF and GOODS-N: implications for galaxy formation and cosmic reionization. OUCHI M., MOBASHER B., SHIMASAKU K., et al.
2010ApJ...708..117B 77           X         2 7 32 On the origin of the highest redshift gamma-ray bursts. BELCZYNSKI K., HOLZ D.E., FRYER C.L., et al.
2010PASJ...62.1167O 2886     A     X C       76 3 10 Spitzer Space Telescope constraint on the stellar mass of a z = 6.96 Lyα emitter. OTA K., LY C., MALKAN M.A., et al.
2011MNRAS.412.2579N 38           X         1 20 17 Lyα emitters at z= 6.5 in the SSA22 field: an area more neutral or void at the end of the re-ionization epoch. NAKAMURA E., INOUE A.K., HAYASHINO T., et al.
2011ApJ...736L..28C 1052 T   A     X C       26 2 26 Probing population III stars in galaxy
IOK-1 at z = 6.96 through He II emission. 		CAI Z., FAN X., JIANG L., et al.
2011ApJ...741..101H 115           X         3 9 18 Search for z ∼ 6.96 Lyα emitters with Magellan/IMACS in the COSMOS field. HIBON P., MALHOTRA S., RHOADS J., et al.
2012ApJ...744...83O 728     A D     X C       19 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.
2012MNRAS.421.3266V 78             C       1 2 9 Molecular hydrogen in Lyman alpha emitters. VALLINI L., DAYAL P. and FERRARA A.
2012MNRAS.423..444O 153           X C       3 10 6 Subaru FOCAS survey of z = 7–7.1 Lyα emitters: a test for z ≳ 7 Lyα photometric luminosity functions. OTA K. and IYE M.
2012ApJ...752L..28R 40           X         1 4 20 A Lyα galaxy at redshift z = 6.944 in the COSMOS field. RHOADS J.E., HIBON P., MALHOTRA S., et al.
2012ApJ...752...93W 840     A D     X C       22 11 43 Evidence for low extinction in actively star-forming galaxies at z > 6.5. WALTER F., DECARLI R., CARILLI C., et al.
2012ApJ...752..114S 81           X         2 13 132 The first systematic survey for Lyα emitters at z = 7.3 with red-sensitive Subaru/Suprime-Cam. SHIBUYA T., KASHIKAWA N., OTA K., et al.
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.
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.
2014MNRAS.438.2483M 15       D               2 13 14 Extreme galaxies during reionization: testing ISM and disc models. MUNOZ J.A. and FURLANETTO S.R.
2014ApJ...784...99G 1045   K A D     X C       27 24 31 Search for [C II] emission in z = 6.5-11 star-forming galaxies. GONZALEZ-LOPEZ J., RIECHERS D.A., DECARLI R., et al.
2014MNRAS.440.2498P 62           X         1 2 95 Simulating cosmic metal enrichment by the first galaxies. PALLOTTINI A., FERRARA A., GALLERANI S., et al.
2014ApJ...792...34O 4744     A     X C       122 34 104 ALMA observation of 158 µm [C II] line and dust continuum of a z = 7 normally star-forming galaxy in the epoch of reionization. OTA K., WALTER F., OHTA K., et al.
2014ApJ...796...96B 232           X C       5 31 13 ALMA observations of the host galaxy of GRB 090423 at z = 8.23: deep limits on obscured star formation 630 million years after the Big Bang. BERGER E., ZAUDERER B.A., CHARY R.-R., et al.
2015ApJ...799L..19C 80           X         2 2 11 Constraining very high mass population III stars through He II emission in galaxy BDF-521 at z = 7.01. CAI Z., FAN X., JIANG L., et al.
2015A&A...574A..19S 742     A D     X         20 23 69 New constraints on dust emission and UV attenuation of z = 6.5-7.5 galaxies from millimeter observations. SCHAERER D., BOONE F., ZAMOJSKI M., et al.
2015Natur.519..327W 15 9 282 A dusty, normal galaxy in the epoch of reionization. WATSON D., CHRISTENSEN L., KNUDSEN K.K., et al.
2015A&A...577A..80M 214       D   O X         6 13 97 Dust production 680-850 million years after the Big Bang. MICHALOWSKI M.J.
2015ApJ...807..180W 45           X         1 11 148 Star formation and the interstellar medium in z > 6 UV-luminous Lyman-break galaxies. WILLOTT C.J., CARILLI C.L., WAGG J., et al.
2015MNRAS.450.1618L 39           X         1 2 ~ The effects of convection criteria on the evolution of Population III stars and the detectability of their supernovae. LAWLOR T.M., YOUNG T.R., TEFFS J., 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.
2015MNRAS.451.2050Z 17       D               1 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.
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.
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.
2016ApJS..222....1F viz 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.
2016MNRAS.457.1842S 39           X         1 9 17 The dust content of the most metal-poor star-forming galaxies. SCHNEIDER R., HUNT L. and VALIANTE R.
2017MNRAS.465.2540P 52           X         1 4 100 Zooming on the internal structure of z ~= 6 galaxies. PALLOTTINI A., FERRARA A., GALLERANI S., et al.
2017ApJ...844...85O 1009       D     X C       25 28 38 A new constraint on reionization from the evolution of the Lyα luminosity function at z ∼ 6-7 probed by a Deep census of z = 7.0 Lyα emitter candidates to 0.3L*. OTA K., IYE M., KASHIKAWA N., et al.
2017ApJ...846..105O viz 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.
2017ApJ...851..145M 49           X         1 5 91 ALMA reveals metals yet no dust within multiple components in CR7. MATTHEE J., SOBRAL D., BOONE F., et al.
2017MNRAS.471.4128P 89             C       1 4 85 The impact of chemistry on the structure of high-z galaxies. PALLOTTINI A., FERRARA A., BOVINO S., et al.
2017MNRAS.471.5018F 42           X         1 5 23 The infrared-dark dust content of high redshift galaxies. FERRARA A., HIRASHITA H., OUCHI M., et al.
2018MNRAS.473.5363W 202           X   F     4 11 16 Dust-obscured star-forming galaxies in the early universe. WILKINS S.M., FENG Y., DI MATTEO T., et al.
2017MNRAS.472..772M viz 95       D     X         3 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               2 41 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2019A&A...623A.157S 18       D               1 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.
2019PASJ...71...71H 225       D     X C       5 31 193 Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O III] 88 μm, [C II] 158 μm, and dust continuum with ALMA. HASHIMOTO T., INOUE A.K., MAWATARI K., 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.
2023MNRAS.525.4976M 87               F     1 6 ~ Dust attenuation in galaxies at cosmic dawn from the FirstLight simulations. MUSHTAQ M., CEVERINO D., KLESSEN R.S., et al.
2024MNRAS.528..499L 63       D     X         2 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024A&A...683A.238J viz 90           X         2 95 ~ JADES: The emergence and evolution of Lyα emission and constraints on the intergalactic medium neutral fraction. JONES G.C., BUNKER A.J., SAXENA A., et al.

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