ULISSE: Determination of the star formation rate and stellar mass based on the one-shot galaxy imaging technique

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Volume 701 (September 2025)

A&A, 701 (2025) A162

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Table 5

ULISSE efficiency in separately retrieving SFR and ℳ_* for different classes of galaxies.

Target object sample	$M_{}^{t a r g} - ⟨ M_{}^{n e i g} ⟩$ $\mathcal{M}_{\ast}^{\rm targ} - \langle\mathcal{M}_{\ast}^{\rm neig}\rangle$	$M_{}^{t a r g} - M_{}^{n o r m}$ $\mathcal{M}_{\ast}^{\rm targ} - \mathcal{M}_{\ast}^{\rm norm}$	SFR^targ - ⟨SFR_neig⟩	SFR^targ - SFR^norm
All	94.1% [81.4%]	93.8% [61.0%]	81.0% [70.7%]	73.4% [57.2%]

SFG	92.2% [79.5%]	91.2% [62.9%]	80.0% [70.2%]	76.1% [54.1%]
QG	98.8% [85.9%]	100.0% [56.5%]	83.5% [71.8%]	67.1% [63.5%]

Notes. The fraction of target objects with the mean, $⟨ M_{*}^{n e i g} ⟩$ $\langle\mathcal{M}_{\ast}^{\rm neig}\rangle$ or ⟨SFR^neig⟩, or normalised mean, ℳ_*^norm or SFR^norm, values for the retrieved neighbours within 1 dex/ $\sqrt{2}$ $/\sqrt{2}$ from the $M_{*}^{t a r g}$ $\mathcal{M}_{\ast}^{\rm targ}$ or SFR^targ estimations of the target.

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