Locating dust and molecules in the inner circumstellar environment of R Sculptoris with MATISSE

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Table A.2

List of the calibrator targets used for R Scl sorted by their decreasing effective temperature.

Name	Sp. Type	T_eff (K)	θ_UD (mas)	F_L (Jy)	F_N (Jy)
HD 10144	B6V	15216 ± 100^a	1.8 ± 0.2	120 ± 14	18 ± 4
HD 48915	A1V	9711 ± 23^b	6.2 ± 0.5	996 ± 55	118 ± 14
HD 6805	K2-IIIb	4687 ± 85^c	3.3 ± 0.3	135 ± 3	20 ± 2
HD 39425	K1III	4631 ± 120^d	3.7 ± 0.4	178 ± 24	23 ± 4
HD 32887	K4III	4243 ± 25^e	6.0 ± 0.6	403 ± 42	56 ± 7
HD 23614	M1III	3 841 ±100^a	5.3 ± 0.5	199 ± 36	28 ± 4
HD 1038	M1III	3 802 ± 100^a	5.6 ± 0.6	255 ± 45	41 ± 10
HD 51799	M1III	3 780 ± 100^a	4.7 ± 0.6	183 ± 38	29 ± 6
HD 11695	M4III	3 550 ± 50^b	9.3 ± 1.2	224 ± 198	69 ± 19

Notes: The values of the uniform-disk angular diameter are reported in the II/346 VizieR catalog (Bourgés et al. 2014), those of the L- and N-band fluxes in the II/361 catalog (Cruzalèbes et al. 2019).

^a Chandler et al. (2016)

^b Huang et al. (2015)

^c Sousa et al. (2018)

^d Stevens et al. (2017)

^e Jofré et al. (2015)

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