A NEW APPROACH TO ANALYZING HST SPATIAL SCANS: THE TRANSMISSION SPECTRUM OF HD 209458 b

By Angelos Tsiaras, Ingo P. Waldmann, Marco Rocchetto, Ryan Varley, G. Morello, M. Damiano, Giovanna Tinetti. 2015

50 citations recorded by the source corpus.

The Wide Field Camera 3 on the Hubble Space Telescope is currently one of the most widely used instruments for observing exoplanetary atmospheres, especially with the use of the spatial scanning technique. An increasing number of exoplanets have been studied using this technique as it enables the observation of bright targets without saturating the sensitive detectors. In this work, we present a new pipeline for analyzing the data obtained with the spatial scanning technique, starting from the raw data provided by the instrument. In addition to commonly used correction techniques, we take into account the geometric distortions of the instrument, the impact of which may become important when they are combined with the scanning process. Our approach can improve the photometric precision for existing data and also extend the limits of the spatial scanning technique, as it allows the analysis of even longer spatial scans. As an application of our method and pipeline, we present the results from a reanalysis of the spatially scanned transit spectrum of HD 209458 b. We calculate the transit depth per wavelength channel with an average relative uncertainty of 40 ppm. We interpret the final spectrum with -REx, our fully Bayesian spectral retrieval code, which confirms the presence of water vapor and clouds in the atmosphere of HD 209458 b. The narrow wavelength range limits our ability to disentangle the degeneracies between the fitted atmospheric parameters. Additional data over a broader spectral range are needed to address this issue.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

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Citations in the corpus

HD 209458b in new light: evidence of nitrogen chemistry, patchy clouds and sub-solar water (2017, background): “In another effort, Tsiaras et al. (2016b) also detected H2O but were unable to robustly constrain its abundance.”
DETECTION OF AN ATMOSPHERE AROUND THE SUPER-EARTH 55 CANCRI E (2015, methodology): “We refer the reader to Tsiaras et al. (2015) for a detailed discussion of our pipeline, which was conceived to reduce spatially scanned spectra.”
A Population Study of Gaseous Exoplanets (2017, methodology): “…Morello et al. 2015) and super-Earths (e.g. Bean et al. 2010; Berta et al. 2012; Knutson et al. 2014b; Kreidberg et al. 2014b; Demory et al. 2016; Tsiaras et al. 2016b) allow us to learn important properties of the planets analysed, we can only gain a limited insight into the global population…”