Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars
The Transiting Exoplanet Survey Satellite (TESS) follow-up of a large number of known transiting exoplanets provides a unique opportunity to study their physical properties more precisely. Being a space-based telescope, the TESS observations are devoid of any noise component resulting from the inter...
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| Format: | Article |
| Language: | English |
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IOP Publishing
2023-01-01
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| Series: | The Astrophysical Journal Supplement Series |
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| Online Access: | https://doi.org/10.3847/1538-4365/acdb6b |
| _version_ | 1797697140378566656 |
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| author | Suman Saha |
| author_facet | Suman Saha |
| author_sort | Suman Saha |
| collection | DOAJ |
| description | The Transiting Exoplanet Survey Satellite (TESS) follow-up of a large number of known transiting exoplanets provides a unique opportunity to study their physical properties more precisely. Being a space-based telescope, the TESS observations are devoid of any noise component resulting from the interference of Earth’s atmosphere. TESS also provides a greater probability to observe subsequent transit events owing to its longer uninterrupted time-series observations compared to ground-based telescopes. For the exoplanets around bright host stars in particular, TESS time-series observations provide high signal-to-noise ratio (S/N) lightcurves, which can be used for higher-precision studies for these exoplanets. In this work, I have studied the TESS transit photometric follow-up observations of 28 exoplanets around bright stars with V _mag ≤ 10. The already high-S/N lightcurves from TESS have been further processed with a critical noise-treatment algorithm, using the wavelet-denoising and the Gaussian-process regression techniques, to effectively reduce the noise components, both correlated and uncorrelated in time, which were then used to estimate the physical properties of these exoplanets. The study has resulted in very precise values for the physical properties of the target exoplanets, with the improvements in precision being significant for most of the cases compared to the previous studies. Also, since a comparatively large number of transit lightcurves from TESS observations were used to estimate these physical properties for each of the target exoplanets, which removes any bias due to the lack of sufficient data sets, these updated physical properties can be considered extremely accurate and reliable for future studies. |
| first_indexed | 2024-03-12T03:36:01Z |
| format | Article |
| id | doaj.art-bf0749c2d8a440339c3bb5de4949b2f9 |
| institution | Directory Open Access Journal |
| issn | 0067-0049 |
| language | English |
| last_indexed | 2024-03-12T03:36:01Z |
| publishDate | 2023-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| series | The Astrophysical Journal Supplement Series |
| spelling | doaj.art-bf0749c2d8a440339c3bb5de4949b2f92023-09-03T13:12:05ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492023-01-012681210.3847/1538-4365/acdb6bPrecise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright StarsSuman Saha0https://orcid.org/0000-0001-8018-0264Indian Institute of Astrophysics , II Block, Koramangala, Bengaluru, India ; suman.saha@iiap.res.in; Pondicherry University , R.V. Nagar, Kalapet, Puducherry, IndiaThe Transiting Exoplanet Survey Satellite (TESS) follow-up of a large number of known transiting exoplanets provides a unique opportunity to study their physical properties more precisely. Being a space-based telescope, the TESS observations are devoid of any noise component resulting from the interference of Earth’s atmosphere. TESS also provides a greater probability to observe subsequent transit events owing to its longer uninterrupted time-series observations compared to ground-based telescopes. For the exoplanets around bright host stars in particular, TESS time-series observations provide high signal-to-noise ratio (S/N) lightcurves, which can be used for higher-precision studies for these exoplanets. In this work, I have studied the TESS transit photometric follow-up observations of 28 exoplanets around bright stars with V _mag ≤ 10. The already high-S/N lightcurves from TESS have been further processed with a critical noise-treatment algorithm, using the wavelet-denoising and the Gaussian-process regression techniques, to effectively reduce the noise components, both correlated and uncorrelated in time, which were then used to estimate the physical properties of these exoplanets. The study has resulted in very precise values for the physical properties of the target exoplanets, with the improvements in precision being significant for most of the cases compared to the previous studies. Also, since a comparatively large number of transit lightcurves from TESS observations were used to estimate these physical properties for each of the target exoplanets, which removes any bias due to the lack of sufficient data sets, these updated physical properties can be considered extremely accurate and reliable for future studies.https://doi.org/10.3847/1538-4365/acdb6bTransit photometryExoplanetsHot JupitersGaussian Processes regressionWavelet analysis |
| spellingShingle | Suman Saha Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars The Astrophysical Journal Supplement Series Transit photometry Exoplanets Hot Jupiters Gaussian Processes regression Wavelet analysis |
| title | Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars |
| title_full | Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars |
| title_fullStr | Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars |
| title_full_unstemmed | Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars |
| title_short | Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars |
| title_sort | precise transit photometry using tess updated physical properties for 28 exoplanets around bright stars |
| topic | Transit photometry Exoplanets Hot Jupiters Gaussian Processes regression Wavelet analysis |
| url | https://doi.org/10.3847/1538-4365/acdb6b |
| work_keys_str_mv | AT sumansaha precisetransitphotometryusingtessupdatedphysicalpropertiesfor28exoplanetsaroundbrightstars |