HSCS J100004+015835 , the SIMBAD biblio

HSCS J100004+015835 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST05:29:33


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Title First 3 Authors
2021MNRAS.500.5229E 18       D               1 103 111 The [O III]+H β equivalent width distribution at z ≃ 7: implications for the contribution of galaxies to reionization. ENDSLEY R., STARK D.P., CHEVALLARD J., et al.
2021MNRAS.502.6044E 603       D     X C       14 36 52 MMT spectroscopy of Lyman-alpha at z ≃ 7: evidence for accelerated reionization around massive galaxies. ENDSLEY R., STARK D.P., CHARLOT S., et al.
2022ApJS..259...20H viz 17       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., 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     3 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 826       D S   X C F     17 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.
2023MNRAS.519.5859W 105       D         F     3 36 43 Star formation histories of UV-luminous galaxies at z ≃ 6.8: implications for stellar mass assembly at early cosmic times. WHITLER L., STARK D.P., ENDSLEY 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.
2024ApJ...974..212P 45           X         1 2 ~ Lyα Profile Shape as an Escape-fraction Diagnostic at High Redshift. PAHL A., SHAPLEY A., STEIDEL C.C., 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.

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