The early maturity of high-redshift galaxies: Insights from sSFR, M/L, and SFHs at z ∼ 7─14
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Exploring the hardness of the ionising radiation with the infrared softness diagram. I. Similar effective temperature scales for starbursts and (ultra)luminous infrared galaxies
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The softness diagram for MaNGA star-forming regions: diffuse ionized gas contamination or local HOLMES predominance?
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