SDSS J015952.75+075148.9 , the SIMBAD biblio

SDSS J015952.75+075148.9 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST01:35:40


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Title First 3 Authors
2017MNRAS.471..548I 534       D     X C       13 9 53 LBT observations of compact star-forming galaxies with extremely high [O III]/[O II] flux ratios: He I emission-line ratios as diagnostics of Lyman continuum leakage. IZOTOV Y.I., THUAN T.X. and GUSEVA N.G.
2018MNRAS.473.1956I 247           X C F     4 11 72 J0811+4730: the most metal-poor star-forming dwarf galaxy known. IZOTOV Y.I., THUAN T.X., GUSEVA N.G., et al.
2020MNRAS.491..468I 390       D     X C       9 12 46 Diverse properties of Ly α emission in low-redshift compact star-forming galaxies with extremely high [O III]/[O II] ratios. IZOTOV Y.I., SCHAERER D., WORSECK G., et al.
2020MNRAS.497.4293G 125           X   F     2 12 26 Properties of five z ∼ 0.3-0.4 confirmed LyC leakers: VLT/XShooter observations. GUSEVA N.G., IZOTOV Y.I., SCHAERER D., et al.
2021ApJ...913L..15K 17       D               1 38 6 The atomic gas mass of Green Pea galaxies. KANEKAR N., GHOSH T., RHOADS J., et al.
2022MNRAS.511.4377D 43           X         1 12 5 On the use of sulphur as a tracer for abundances in galaxies. DIAZ A.I. and ZAMORA S.
2023MNRAS.520.5903H 17       D               1 75 7 Spectral shapes of the Ly α emission from galaxies - II. The influence of stellar properties and nebular conditions on the emergent Ly α profiles. HAYES M.J., RUNNHOLM A., SCARLATA C., et al.
2023RAA....23f5006L 17       D               1 37 ~ The H I Gas Fraction Scaling Relation of the Green Pea Galaxies. LIU S., LUO A.-L., ZHANG W., et al.
2024ApJ...961...49X 18       D               2 29 ~ EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely Metal-poor Galaxies. XU Y., OUCHI M., ISOBE Y., et al.
2025ApJ...988....4J 485       D     X C       10 7 ~ Local Analogs of Potential Ionizers of the Intergalactic Medium: Compact Star-forming Galaxies with Intense C IVλ1550 Emission. JUNG I., RAVINDRANATH S., JASKOT A.E., et al.

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