Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS - Insights into the Neptunian desert around M dwarfs

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Table E.1

Sample used for the study of the Neptunian desert boundaries.

Planet	a	T_eff	R_*	M_*	L	S	P_orb	R_p/R_*	R_p	^Tdur	δ	N^†	N_S^‡	σ_CDPP	S/N	P⁻¹_trans	P⁻¹_det	w
	(au)	(K)	(R_⊙)	(M_⊙)	(L_⊙)	(S_⊕)	(days)		(R_⊕)	(hrs)	(^*)			(^§)
K00752.01	0.086	5610	0.90	0.94	0.73	99	9.49	0.022	2.20	3.59	0.00050	142		207.29	287.63	20.43	1.03	20.99
K00752.02	0.275	5610	0.90	0.94	0.73	10	54.42	0.028	2.76	5.36	0.00078	25		184.96	211.70	65.46	1.03	67.27
K00755.01	0.036	5660	0.92	0.94	0.79	630	2.53	0.024	2.42	1.74	0.00058	515		325.80	404.22	8.28	1.03	8.51
K00756.01	0.098	5837	1.03	1.03	1.12	116	11.09	0.037	4.14	3.66	0.00136	95		235.39	561.33	20.53	1.03	21.10
K00756.02	0.051	5837	1.03	1.03	1.12	431	4.13	0.026	2.94	2.04	0.00068	240		299.06	354.53	10.63	1.03	10.93
								⋮
toi892.01	0.100	6163	1.33	1.19	2.32	231	10.63	0.079	11.48	5.42	7530.0	2	1	220.61	51.60	16.19	1.03	16.64
toi905.01	0.046	5434	0.93	0.95	0.69	319	3.74	0.131	13.30	2.04	15256.9	42	6	1943.18	332.65	10.73	1.03	11.02
toi942.01	0.049	5043	0.83	0.83	0.40	169	4.32	0.040	3.61	3.18	1480.0	6	1	556.19	6.55	12.71	10.09	128.16
toi954.01	0.052	5932	1.78	1.35	3.62	1361	3.68	0.046	8.98	4.54	2070.0	7	1	178.90	30.81	6.22	1.03	6.39
toi966.01	0.046	6231	1.19	1.15	1.93	892	3.41	0.107	13.84	3.21	16294.4	22	3	1748.80	208.27	8.43	1.03	8.66

The sample is described in Section 6 and depicted in Fig. E.1. This table is truncated (error columns are omitted and precisions are reduced); the full version can be found on the Strasbourg astronomical Data Center (CDS).

^*It is important to note that the depth, δ, is reported in units of ppm×10⁻⁶ for the Kepler planets, and ppm for the TESS planets, to match the differing units for the Kepler and TESS rms CDPP values.

^†The number of transits, N, for the TESS targets is the total number of transits across all sectors; more specifically, we take an average number of transits in a sector based on planet period and the length of each sector, then sum over all sectors.

^‡For TESS targets, the total number of sectors in which the planet transits is given as N_S.

^§The rms CDPP computed at the transit duration, σ_CDPP, is reported in units of ppm×10⁻⁶ for Kepler; for TESS it is reported in units of ppm. In this table, the value we give for σ_CDPP for the TESS targets is rather the denominator of Equ. 11, i.e. $\sqrt{\sum_{i} N_{i} σ_{C D P P, i}^{2}}$ $Mathematical equation: $\sqrt{\sum_i N_i \sigma^2_{{\rm CDPP}, i}}$$ .

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