REBELS-27 , the SIMBAD biblio

REBELS-27 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:23:08

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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
2017ApJ...851...43S 135       D     X C       3 11 18 HST imaging of the brightest z ∼ 8-9 galaxies from UltraVISTA: the extreme bright end of the UV luminosity function. STEFANON M., LABBE I., BOUWENS R.J., et al.
2019ApJ...883...99S 263       D     X         7 24 84 The brightest z >= 8 galaxies over the Cosmos UltraVISTA field. STEFANON M., LABBE I., BOUWENS R.J., et al.
2020MNRAS.493.2059B 19       D               3 39 130 A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10. BOWLER R.A.A., JARVIS M.J., DUNLOP J.S., et al.
2022MNRAS.512...58F 402       D     X   F     9 18 38 The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≃ 7. FERRARA A., SOMMOVIGO L., DAYAL P., et al.
2022MNRAS.512..989D 20       D               1 17 58 The ALMA REBELS survey: the dust content of z ∼ 7 Lyman break galaxies. DAYAL P., FERRARA A., SOMMOVIGO L., et al.
2022ApJ...928...31S 189       D     X C       4 18 48 Significant Dust-obscured Star Formation in Luminous Lyman-break Galaxies at z ∼ 7-8. SCHOUWS S., STEFANON M., BOUWENS R., et al.
2022MNRAS.513.3122S 103       D         F     2 30 49 The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7. SOMMOVIGO L., FERRARA A., PALLOTTINI A., et al.
2022ApJ...931..160B 18       D               1 50 96 Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe. BOUWENS R.J., SMIT R., SCHOUWS S., et al.
2022MNRAS.515.3126I viz 102       D         F     7 55 45 The ALMA REBELS Survey: dust continuum detections at z > 6.5. INAMI H., ALGERA H.S.B., SCHOUWS S., et al.
2022MNRAS.517.5642E 443       D S   X   F     9 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.
2022A&A...667A..65K 17       D               1 25 14 COSMOS2020: UV-selected galaxies at z ≥ 7.5. KAUFFMANN O.B., ILBERT O., WEAVER J.R., et al.
2023MNRAS.518.6142A 87               F     1 47 27 The ALMA REBELS survey: the dust-obscured cosmic star formation rate density at redshift 7. ALGERA H.S.B., INAMI H., OESCH P.A., et al.
2024MNRAS.527.5808B 18       D               1 63 ~ The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z= 4-8 revealed by the IRX-β and M⋆ relations. BOWLER R.A.A., INAMI H., SOMMOVIGO L., 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.528.2407P 63       D     X         2 16 ~ Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations. PALLA M., DE LOOZE I., RELANO M., et al.
2025ApJ...980..138H 19       D               1 68 ~ JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe. HARIKANE Y., INOUE A.K., ELLIS R.S., et al.
2025ApJ...982....7N 19       D               1 14 ~ The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission. NARAYANAN D., STARK D.P., FINKELSTEIN S.L., et al.
2026ApJ...999...95E 370       D S   X         7 14 ~ REBELS-MOSFIRE: Weak C III] Emission Is Typical among Extremely UV-bright, Massive Galaxies at z ∼ 7. ENDSLEY R., SHAPLEY A.E., TOPPING M.W., et al.

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