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Exoplanet Transit Spectroscopy with JWST NIRSpec: Diagnostics and Homogeneous Case Study of WASP-39 b

By Keith Cowing
Status Report
May 15, 2024
Filed under , , , , , , , ,
Exoplanet Transit Spectroscopy with JWST NIRSpec: Diagnostics and Homogeneous Case Study of WASP-39 b
The obtained NIRSpec Prism and G395H transmission spectra of WASP-39 b, shown as errorbars with green and blue centres, respectively. Also shown is a nominal model assuming 10× solar elemental abundances and Mie scattering aerosols, as discussed in section 7. The observations are binned to R∼100 for visual clarity, while the grey area denotes the persistent saturation region for NIRSpec Prism as shown in Figure 2 — astro-ph.EP

The JWST has ushered in a new era of exoplanet transit spectroscopy. Among the JWST instruments, the Near-Infrared Spectrograph (NIRSpec) has the most extensive set of configurations for exoplanet time series observations.

The NIRSpec Prism and G395H grating represent two extremes in NIRSpec instrument modes, with the Prism spanning a wider spectral range (0.6-5.3 μm at lower resolution (R∼100) compared to G395H (2.87-5.14 μm; R∼2700).

In this work, we develop a new data reduction framework, JexoPipe, to conduct a homogeneous assessment of the two NIRSpec modes for exoplanet spectroscopy. We use observations of the hot Saturn WASP-39 b obtained as part of the JWST Transiting Exoplanets ERS program to assess the spectral quality and stability between the two instrument modes at different epochs.

We explore the noise sources, effect of saturation, and offsets in transmission spectra between the different instrument modes and also between the two G395H NRS detectors. We find an inter-detector offset in G395H of ∼ 40-50 ppm, consistent with recent studies. We find evidence for correlated noise in the Prism white light curve.

We find the G395H spectrum to be of higher precision compared to the Prism at the same resolution. We also compare the JexoPipe spectra with those reported from other pipelines. Our work underscores the need for robust assessment of instrument performance and identification of optimal practices for JWST data reduction and analyses.

Subhajit Sarkar, Nikku Madhusudhan, Savvas Constantinou, Måns Holmberg

Comments: 27 pages, 23 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2405.06737 [astro-ph.EP] (or arXiv:2405.06737v1 [astro-ph.EP] for this version)
Submission history
From: Subhajit Sarkar
[v1] Fri, 10 May 2024 18:00:00 UTC (11,640 KB)

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻