HORuS transmission spectroscopy and revised planetary parameters of KELT-7 b Article Swipe
H. M. Tabernero
,
M. R. Zapatero Osorio
,
Carlos Allende Prieto
,
E. González-Álvarez
,
J. Sanz‐Forcada
,
Álvaro López-Gallifa
,
D. Montes
,
C. del Burgo
,
J. I. Gónzalez Hernández
,
R. Rébolo
·
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stac1759
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stac1759
We report on the high-resolution spectroscopic observations of two planetary transits of the hot Jupiter KELT-7b (Mp = 1.28 ± 0.17MJup, Teq = 2028 K) observed with the High Optical Resolution Spectrograph (HORuS) mounted on the 10.4-m Gran Telescopio Canarias (GTC). A new set of stellar parameters are obtained for the rapidly rotating parent star from the analysis of the spectra. Using the newly derived stellar mass and radius, and the planetary transit data of the Transiting Exoplanet Survey Satellite (TESS) together with the HORuS velocities and the photometric and spectroscopic data available in the literature, we update and improve the ephemeris of KELT-7b. Our results indicate that KELT-7 has an angle λ = −10.55 ± 0.27 deg between the sky projections of the star’s spin axis and the planet’s orbital axis. By combining this angle and our newly derived stellar rotation period of 1.38 ± 0.05 d, we obtained a 3D obliquity ψ = 12.4 ± 11.7 deg (or 167.6 deg), thus reinforcing that KELT-7 is a well-aligned planetary system. We search for the presence of Hα, Li i, Na i, Mg i, and Ca ii features in the transmission spectrum of KELT-7b but we are only able to determine upper limits of 0.08–1.4 per cent on their presence after accounting for the contribution of the stellar variability to the extracted planetary spectrum. We also discuss the impact of stellar variability on the planetary data. Our results reinforce the importance of monitoring the parent star when performing high-resolution transmission spectroscopy of the planetary atmosphere in the presence of stellar activity.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stac1759
- https://academic.oup.com/mnras/article-pdf/515/1/1247/45045276/stac1759.pdf
- OA Status
- hybrid
- Cited By
- 6
- References
- 126
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4283456831
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- OpenAlex ID
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https://openalex.org/W4283456831Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.1093/mnras/stac1759Digital Object Identifier
- Title
-
HORuS transmission spectroscopy and revised planetary parameters of KELT-7 bWork title
- Type
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articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2022Year of publication
- Publication date
-
2022-07-19Full publication date if available
- Authors
-
H. M. Tabernero, M. R. Zapatero Osorio, Carlos Allende Prieto, E. González-Álvarez, J. Sanz‐Forcada, Álvaro López-Gallifa, D. Montes, C. del Burgo, J. I. Gónzalez Hernández, R. RéboloList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/stac1759Publisher landing page
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https://academic.oup.com/mnras/article-pdf/515/1/1247/45045276/stac1759.pdfDirect link to full text PDF
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://academic.oup.com/mnras/article-pdf/515/1/1247/45045276/stac1759.pdfDirect OA link when available
- Concepts
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Physics, Exoplanet, Ephemeris, Hot Jupiter, Astrophysics, Spectrograph, Planetary system, Planet, Astronomy, Stellar rotation, Transit (satellite), Spectral line, Stars, Satellite, Public transport, Law, Political scienceTop concepts (fields/topics) attached by OpenAlex
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6Total citation count in OpenAlex
- Citations by year (recent)
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2025: 1, 2024: 4, 2023: 1Per-year citation counts (last 5 years)
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126Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.of | 8, 12, 45, 59, 75, 103, 123, 144, 177, 193, 204, 216, 230, 242, 252, 259 |
| abstract_inverted_index.on | 3, 35, 208, 233 |
| abstract_inverted_index.to | 200, 220 |
| abstract_inverted_index.we | 97, 149, 196 |
| abstract_inverted_index.± | 20, 116, 146, 157 |
| abstract_inverted_index.λ | 113 |
| abstract_inverted_index.ψ | 154 |
| abstract_inverted_index.(Mp | 17 |
| abstract_inverted_index.(or | 160 |
| abstract_inverted_index.Our | 105, 237 |
| abstract_inverted_index.Teq | 22 |
| abstract_inverted_index.and | 68, 70, 87, 90, 99, 128, 137, 185 |
| abstract_inverted_index.are | 48, 197 |
| abstract_inverted_index.but | 195 |
| abstract_inverted_index.deg | 118, 159 |
| abstract_inverted_index.for | 50, 174, 213 |
| abstract_inverted_index.has | 110 |
| abstract_inverted_index.hot | 14 |
| abstract_inverted_index.new | 43 |
| abstract_inverted_index.our | 138 |
| abstract_inverted_index.per | 206 |
| abstract_inverted_index.set | 44 |
| abstract_inverted_index.sky | 121 |
| abstract_inverted_index.the | 4, 13, 28, 36, 51, 57, 60, 63, 71, 76, 84, 88, 95, 101, 120, 124, 129, 175, 190, 214, 217, 221, 228, 234, 240, 244, 253, 257 |
| abstract_inverted_index.two | 9 |
| abstract_inverted_index.0.05 | 147 |
| abstract_inverted_index.0.27 | 117 |
| abstract_inverted_index.1.28 | 19 |
| abstract_inverted_index.1.38 | 145 |
| abstract_inverted_index.11.7 | 158 |
| abstract_inverted_index.12.4 | 156 |
| abstract_inverted_index.2028 | 24 |
| abstract_inverted_index.Gran | 38 |
| abstract_inverted_index.High | 29 |
| abstract_inverted_index.Hα, | 178 |
| abstract_inverted_index.able | 199 |
| abstract_inverted_index.also | 226 |
| abstract_inverted_index.axis | 127 |
| abstract_inverted_index.cent | 207 |
| abstract_inverted_index.data | 74, 92 |
| abstract_inverted_index.from | 56 |
| abstract_inverted_index.mass | 67 |
| abstract_inverted_index.only | 198 |
| abstract_inverted_index.spin | 126 |
| abstract_inverted_index.star | 55, 246 |
| abstract_inverted_index.that | 108, 165 |
| abstract_inverted_index.this | 135 |
| abstract_inverted_index.thus | 163 |
| abstract_inverted_index.when | 247 |
| abstract_inverted_index.with | 27, 83 |
| abstract_inverted_index.167.6 | 161 |
| abstract_inverted_index.HORuS | 85 |
| abstract_inverted_index.Using | 62 |
| abstract_inverted_index.after | 211 |
| abstract_inverted_index.angle | 112, 136 |
| abstract_inverted_index.axis. | 132 |
| abstract_inverted_index.data. | 236 |
| abstract_inverted_index.deg), | 162 |
| abstract_inverted_index.newly | 64, 139 |
| abstract_inverted_index.their | 209 |
| abstract_inverted_index.upper | 202 |
| abstract_inverted_index.(GTC). | 41 |
| abstract_inverted_index.(TESS) | 81 |
| abstract_inverted_index.10.4-m | 37 |
| abstract_inverted_index.KELT-7 | 109, 166 |
| abstract_inverted_index.Survey | 79 |
| abstract_inverted_index.impact | 229 |
| abstract_inverted_index.limits | 203 |
| abstract_inverted_index.parent | 54, 245 |
| abstract_inverted_index.period | 143 |
| abstract_inverted_index.report | 2 |
| abstract_inverted_index.search | 173 |
| abstract_inverted_index.update | 98 |
| abstract_inverted_index.(HORuS) | 33 |
| abstract_inverted_index.Jupiter | 15 |
| abstract_inverted_index.KELT-7b | 16, 194 |
| abstract_inverted_index.Optical | 30 |
| abstract_inverted_index.between | 119 |
| abstract_inverted_index.derived | 65, 140 |
| abstract_inverted_index.discuss | 227 |
| abstract_inverted_index.improve | 100 |
| abstract_inverted_index.mounted | 34 |
| abstract_inverted_index.orbital | 131 |
| abstract_inverted_index.radius, | 69 |
| abstract_inverted_index.rapidly | 52 |
| abstract_inverted_index.results | 106, 238 |
| abstract_inverted_index.stellar | 46, 66, 141, 218, 231, 260 |
| abstract_inverted_index.system. | 171 |
| abstract_inverted_index.transit | 73 |
| abstract_inverted_index.ABSTRACT | 0 |
| abstract_inverted_index.Canarias | 40 |
| abstract_inverted_index.KELT-7b. | 104 |
| abstract_inverted_index.analysis | 58 |
| abstract_inverted_index.features | 188 |
| abstract_inverted_index.indicate | 107 |
| abstract_inverted_index.observed | 26 |
| abstract_inverted_index.obtained | 49, 150 |
| abstract_inverted_index.presence | 176, 210, 258 |
| abstract_inverted_index.rotating | 53 |
| abstract_inverted_index.rotation | 142 |
| abstract_inverted_index.spectra. | 61 |
| abstract_inverted_index.spectrum | 192 |
| abstract_inverted_index.star’s | 125 |
| abstract_inverted_index.together | 82 |
| abstract_inverted_index.transits | 11 |
| abstract_inverted_index.−10.55 | 115 |
| abstract_inverted_index.0.17MJup, | 21 |
| abstract_inverted_index.Exoplanet | 78 |
| abstract_inverted_index.Satellite | 80 |
| abstract_inverted_index.activity. | 261 |
| abstract_inverted_index.available | 93 |
| abstract_inverted_index.combining | 134 |
| abstract_inverted_index.determine | 201 |
| abstract_inverted_index.ephemeris | 102 |
| abstract_inverted_index.extracted | 222 |
| abstract_inverted_index.obliquity | 153 |
| abstract_inverted_index.planetary | 10, 72, 170, 223, 235, 254 |
| abstract_inverted_index.reinforce | 239 |
| abstract_inverted_index.spectrum. | 224 |
| abstract_inverted_index.0.08–1.4 | 205 |
| abstract_inverted_index.Resolution | 31 |
| abstract_inverted_index.Telescopio | 39 |
| abstract_inverted_index.Transiting | 77 |
| abstract_inverted_index.accounting | 212 |
| abstract_inverted_index.atmosphere | 255 |
| abstract_inverted_index.importance | 241 |
| abstract_inverted_index.monitoring | 243 |
| abstract_inverted_index.parameters | 47 |
| abstract_inverted_index.performing | 248 |
| abstract_inverted_index.planet’s | 130 |
| abstract_inverted_index.velocities | 86 |
| abstract_inverted_index.literature, | 96 |
| abstract_inverted_index.photometric | 89 |
| abstract_inverted_index.projections | 122 |
| abstract_inverted_index.reinforcing | 164 |
| abstract_inverted_index.variability | 219, 232 |
| abstract_inverted_index.Spectrograph | 32 |
| abstract_inverted_index.contribution | 215 |
| abstract_inverted_index.observations | 7 |
| abstract_inverted_index.spectroscopy | 251 |
| abstract_inverted_index.transmission | 191, 250 |
| abstract_inverted_index.well-aligned | 169 |
| abstract_inverted_index.spectroscopic | 6, 91 |
| abstract_inverted_index.high-resolution | 5, 249 |
| cited_by_percentile_year.max | 98 |
| cited_by_percentile_year.min | 89 |
| corresponding_author_ids | https://openalex.org/A5076041127 |
| countries_distinct_count | 2 |
| institutions_distinct_count | 10 |
| corresponding_institution_ids | https://openalex.org/I4210129022 |
| citation_normalized_percentile.value | 0.78742759 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |