Multi-band Spectral and Astrometric Characterization of the HIP 99770 b Planet with SCExAO/CHARIS and Gaia∗ Article Swipe
Danielle Bovie
,
Thayne Currie
,
Mona El Morsy
,
Brianna Lacy
,
Masayuki Kuzuhara
,
Jeffrey Chilcote
,
Taylor Tobin
,
Olivier Guyon
,
Tyler D. Groff
,
Julien Lozi
,
Sébastien Vievard
,
Vincent Déo
,
Frantz Martinache
,
Yiting Li
,
Motohide Tamura
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ae0195
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ae0195
We present and analyze follow-up, higher resolution ( R ∼ 70) H and K band integral field spectroscopy of the superjovian exoplanet HIP 99770 b with SCExAO/CHARIS. Our new data recover the companion at a high SNR in both bandpasses and more than double the astrometric baseline for its orbital motion. Jointly modeling HIP 99770 b’s position and the star’s astrometry from Hipparcos and Gaia yields orbital parameters consistent with those from the discovery paper, albeit with smaller errors, and a slight preference for a smaller semimajor axis (∼15.7–15.8 au) and a larger eccentricity (∼0.28–0.29), disfavoring a circular orbit. We revise its dynamical mass slightly downwards to 15.0 M Jup for a flat prior and 13.1 M Jup for a more standard log-uniform mass prior, where the inclusion of its relative radial-velocity measurement is primarily responsible for these changes. We find consistent results for HIP 99770 b’s dynamical mass, including recent VLTI/GRAVITY astrometry, albeit with a slightly smaller, better constrained eccentricity of e ∼ 0.22 . HIP 99770 b is a ∼1300 K object at the L/T transition with a gravity intermediate between that of the HR 8799 planets and older, more massive field brown dwarfs with similar temperatures but with hints of equilibrium chemistry. HIP 99770 b is particularly well suited for spectroscopic follow-up with Roman Coronagraph Instrument during the technology demonstration phase at 730 nm to further constrain its metallicity and chemistry; JWST thermal infrared observations could likewise explore the planet’s carbon chemistry, metallicity, and clouds.
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- Landing Page
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- OA Status
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- Cited By
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Multi-band Spectral and Astrometric Characterization of the HIP 99770 b Planet with SCExAO/CHARIS and Gaia∗Work title
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articleOpenAlex work type
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enPrimary language
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2025Year of publication
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2025-10-06Full publication date if available
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Danielle Bovie, Thayne Currie, Mona El Morsy, Brianna Lacy, Masayuki Kuzuhara, Jeffrey Chilcote, Taylor Tobin, Olivier Guyon, Tyler D. Groff, Julien Lozi, Sébastien Vievard, Vincent Déo, Frantz Martinache, Yiting Li, Motohide TamuraList of authors in order
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goldOpen access status per OpenAlex
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2Total citation count in OpenAlex
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| abstract_inverted_index.Instrument | 264 |
| abstract_inverted_index.astrometry | 61 |
| abstract_inverted_index.bandpasses | 40 |
| abstract_inverted_index.chemistry, | 290 |
| abstract_inverted_index.chemistry. | 250 |
| abstract_inverted_index.chemistry; | 279 |
| abstract_inverted_index.consistent | 69, 172 |
| abstract_inverted_index.follow-up, | 5 |
| abstract_inverted_index.parameters | 68 |
| abstract_inverted_index.planet’s | 288 |
| abstract_inverted_index.preference | 83 |
| abstract_inverted_index.resolution | 7 |
| abstract_inverted_index.technology | 267 |
| abstract_inverted_index.transition | 223 |
| abstract_inverted_index.</mml:math> | 123, 146, 210 |
| abstract_inverted_index.</mml:mrow> | 117, 121, 140, 144, 204, 208 |
| abstract_inverted_index.<mml:mrow/> | 113, 136, 200 |
| abstract_inverted_index.Coronagraph | 263 |
| abstract_inverted_index.astrometric | 46 |
| abstract_inverted_index.astrometry, | 183 |
| abstract_inverted_index.constrained | 190 |
| abstract_inverted_index.disfavoring | 96 |
| abstract_inverted_index.equilibrium | 249 |
| abstract_inverted_index.log-uniform | 153 |
| abstract_inverted_index.measurement | 163 |
| abstract_inverted_index.metallicity | 277 |
| abstract_inverted_index.responsible | 166 |
| abstract_inverted_index.superjovian | 21 |
| abstract_inverted_index.VLTI/GRAVITY | 182 |
| abstract_inverted_index.eccentricity | 94, 191 |
| abstract_inverted_index.intermediate | 227 |
| abstract_inverted_index.metallicity, | 291 |
| abstract_inverted_index.observations | 283 |
| abstract_inverted_index.particularly | 255 |
| abstract_inverted_index.spectroscopy | 18 |
| abstract_inverted_index.temperatures | 244 |
| abstract_inverted_index.<mml:msubsup> | 112, 135, 199 |
| abstract_inverted_index.demonstration | 268 |
| abstract_inverted_index.spectroscopic | 259 |
| abstract_inverted_index.</mml:msubsup> | 122, 145, 209 |
| abstract_inverted_index.SCExAO/CHARIS. | 27 |
| abstract_inverted_index.(∼15.7–15.8 | 89 |
| abstract_inverted_index.radial-velocity | 162 |
| abstract_inverted_index.(∼0.28–0.29), | 95 |
| abstract_inverted_index.<mml:mo>+</mml:mo> | 119, 142, 206 |
| abstract_inverted_index.overflow="scroll"> | 111, 134, 198 |
| abstract_inverted_index.<mml:mn>4.4</mml:mn> | 116 |
| abstract_inverted_index.<mml:mn>4.5</mml:mn> | 120 |
| abstract_inverted_index.<mml:mn>4.8</mml:mn> | 143 |
| abstract_inverted_index.<mml:mn>5.2</mml:mn> | 139 |
| abstract_inverted_index.<mml:mo>−</mml:mo> | 115, 138, 202 |
| abstract_inverted_index.<mml:mn>0.10</mml:mn> | 207 |
| abstract_inverted_index.<mml:mn>0.13</mml:mn> | 203 |
| abstract_inverted_index.xmlns:mml="http://www.w3.org/1998/Math/MathML" | 110, 133, 197 |
| cited_by_percentile_year.max | 97 |
| cited_by_percentile_year.min | 95 |
| corresponding_author_ids | https://openalex.org/A5075917998, https://openalex.org/A5075421385, https://openalex.org/A5032861079, https://openalex.org/A5108125229, https://openalex.org/A5033911713, https://openalex.org/A5085344522, https://openalex.org/A5035585472, https://openalex.org/A5089666756, https://openalex.org/A5024494164, https://openalex.org/A5110803736, https://openalex.org/A5100670474, https://openalex.org/A5063356742, https://openalex.org/A5024510333, https://openalex.org/A5024083887, https://openalex.org/A5073141775 |
| countries_distinct_count | 3 |
| institutions_distinct_count | 15 |
| corresponding_institution_ids | https://openalex.org/I107639228, https://openalex.org/I1294671590, https://openalex.org/I1306266525, https://openalex.org/I138006243, https://openalex.org/I154570441, https://openalex.org/I185103710, https://openalex.org/I24262253, https://openalex.org/I27837315, https://openalex.org/I4210115062, https://openalex.org/I4210126779, https://openalex.org/I4210159940, https://openalex.org/I45438204, https://openalex.org/I74801974 |
| citation_normalized_percentile.value | 0.93568585 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |