TOI-1743 b, TOI-5799 b, TOI-5799 c, and TOI-6223 b: TESS discovery and validation of four super-Earth to Neptune-sized planets around M dwarfs

Open Access

Table D.1

Exposure times and S/N obtained for each synthetic spectrum of JWST.

Instrument	Mode^a	Exposure	S/N
		Time
TOI-1743 b
MIRI	Slit Spectroscopy	930 s	400
NIRSpec	G140H/F070LP^b	1115 s	1195
	G140H/F100LP	1115 s	1165
	G235H/F170LP	1135 s	1225
	G395H/F290LP	1150 s	1050
NIRCam	F322W2	1145 s	1115
	F444W	1135 s	850
NIRISS	SUBSTRIP256^c	1155 s	1680
TOI-5799 b
MIRI	Slit Spectroscopy	1080 s	805
NIRSpec	G140H/F070LP	1630 s	2265
	G140H/F100LP	1630 s	2300
	G235H/F170LP	1625 s	2270
	G395H/F290LP	1630 s	1930
NIRCam	F322W2	1650 s	2160
	F444W	1660 s	1620
NIRISS	SUBSTRIP256	1650 s	3115
TOI-5799 c
MIRI	Slit Spectroscopy	1390 s	910
NIRSpec	G140H/F070LP	2085 s	2560
	G140H/F100LP	2090 s	2600
	G235H/F170LP	2085 s	2570
	G395H/F290LP	2095 s	2185
NIRCam	F322W2	2095 s	2435
	F444W	2085 s	1820
NIRISS	SUBSTRIP256	2080 s	3495
TOI-6223 b
MIRI	Slit Spectroscopy	2260 s	650
NIRSpec	G140H/F070LP	2465 s	1340
	G140H/F100LP	2440 s	1370
	G235H/F170LP	2435 s	1245
	G395H/F290LP	2475 s	1010
NIRCam	F322W2	2560 s	1165
	F444W	2460 s	795
NIRISS	SUBSTRIP256	2522 s	1895

^aInformation of the different modes, resolving power, and wave-length can be found at: https://jwst-docs.stsci.edu/

^bWe chose various disperser-filter combinations that can provide a high-resolution power of 2700. G = Grism, F = Filter.

^cSize of the subarray for single-object slitless spectroscopy.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.