MINDS: Water reservoirs of compact planet-forming dust discs - A diversity of H2O distributions

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Volume 699 (July 2025)

A&A, 699 (2025) A134

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Table F.1

Integrated fluxes for the lines tracing the cold, intermediate, and hot H₂O reservoirs.

Source	F_1448K	F_1615K	F_3646K	F_6052K	$F_{1500 K}^{α}$ $F_{1500\text{K}}^{\alpha}$
BPTau	10.67±0.07	10.43±0.04	6.68±0.05	3.15±0.05	21.09±0.08
CX Tau	0.99±0.02	0.93±0.02	0.49±0.03	0.09±0.03	1.91±0.03
CY Tau	1.17±0.01	1.22±0.01	1.02±0.01	0.60±0.01	2.40±0.01
DN Tau	1.29±0.03	1.49±0.05	0.57±0.02	0.13±0.02	2.78±0.06
DR Tau	36.38±0.20	33.89±0.16	24.94±3.17	13.49±0.26	70.27±0.26
FT Tau	8.60±0.03	6.99±0.03	2.81±0.03	2.13±0.03	15.59±0.05
RNO90	66.03±0.26	66.65±0.22	40.82±0.19	24.72±0.27	132.68±0.34
XX Cha	4.23±0.01	3.88±0.02	1.54±0.01	1.09±0.01	8.11±0.02

Notes. The fluxes are given in × 10⁻¹⁵ erg s⁻¹ cm⁻².

^α: The F_1500K flux is the summation of the fluxes of the 1448 K and 1615

K lines, following Banzatti et al. (2025).

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