FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4327957062> ?p ?o ?g. }

• W4327957062 endingPage "167" @default.
• W4327957062 startingPage "167" @default.
• W4327957062 abstract "Abstract Characterizing the bulk compositions of transiting exoplanets within the M dwarf radius valley offers a unique means to establish whether the radius valley emerges from an atmospheric mass-loss process or is imprinted by planet formation itself. We present the confirmation of such a planet orbiting an early-M dwarf ( T mag = 11.0294 ± 0.0074, M s = 0.513 ± 0.012 M ⊙ , R s = 0.515 ± 0.015 R ⊙ , and T eff = 3690 ± 50 K): TOI-1695 b ( P = 3.13 days and <?CDATA ${R}_{p}={1.90}_{-0.14}^{+0.16} {R}_{oplus }$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow> <mml:mi>R</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>p</mml:mi> </mml:mrow> </mml:msub> <mml:mo>=</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>1.90</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.14</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.16</mml:mn> </mml:mrow> </mml:msubsup> <mml:mspace width=0.33em /> <mml:msub> <mml:mrow> <mml:mi>R</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊕</mml:mo> </mml:mrow> </mml:msub> </mml:math> ). TOI-1695 b’s radius and orbital period situate the planet between model predictions from thermally driven mass loss versus gas depleted formation, offering an important test case for radius valley emergence models around early-M dwarfs. We confirm the planetary nature of TOI-1695 b based on five sectors of TESS data and a suite of follow-up observations including 49 precise radial velocity measurements taken with the HARPS-N spectrograph. We measure a planetary mass of 6.36 ± 1.00 M ⊕ , which reveals that TOI-1695 b is inconsistent with a purely terrestrial composition of iron and magnesium silicate, and instead is likely a water-rich planet. Our finding that TOI-1695 b is not terrestrial is inconsistent with the planetary system being sculpted by thermally driven mass loss. We present a statistical analysis of seven well-characterized planets within the M dwarf radius valley demonstrating that a thermally driven mass-loss scenario is unlikely to explain this population." @default.
• W4327957062 created "2023-03-21" @default.
• W4327957062 creator A5000486542 @default.
• W4327957062 creator A5004341810 @default.
• W4327957062 creator A5005103000 @default.
• W4327957062 creator A5006342170 @default.
• W4327957062 creator A5006919346 @default.
• W4327957062 creator A5008522406 @default.
• W4327957062 creator A5013019436 @default.
• W4327957062 creator A5017318517 @default.
• W4327957062 creator A5022129586 @default.
• W4327957062 creator A5022799398 @default.
• W4327957062 creator A5023734359 @default.
• W4327957062 creator A5023878393 @default.
• W4327957062 creator A5029531592 @default.
• W4327957062 creator A5036163493 @default.
• W4327957062 creator A5038444269 @default.
• W4327957062 creator A5043746848 @default.
• W4327957062 creator A5044238721 @default.
• W4327957062 creator A5045522063 @default.
• W4327957062 creator A5045664975 @default.
• W4327957062 creator A5046626315 @default.
• W4327957062 creator A5047272660 @default.
• W4327957062 creator A5049263167 @default.
• W4327957062 creator A5051898788 @default.
• W4327957062 creator A5053613581 @default.
• W4327957062 creator A5054806694 @default.
• W4327957062 creator A5056033867 @default.
• W4327957062 creator A5056356825 @default.
• W4327957062 creator A5063065836 @default.
• W4327957062 creator A5064622518 @default.
• W4327957062 creator A5066527569 @default.
• W4327957062 creator A5066955570 @default.
• W4327957062 creator A5076152149 @default.
• W4327957062 creator A5076329760 @default.
• W4327957062 creator A5080099403 @default.
• W4327957062 creator A5082502116 @default.
• W4327957062 creator A5084594696 @default.
• W4327957062 creator A5085340454 @default.
• W4327957062 creator A5085415923 @default.
• W4327957062 creator A5087654538 @default.
• W4327957062 creator A5088359901 @default.
• W4327957062 creator A5089730601 @default.
• W4327957062 creator A5090526973 @default.
• W4327957062 date "2023-03-20" @default.
• W4327957062 modified "2023-10-17" @default.
• W4327957062 title "TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley" @default.
• W4327957062 cites W1531115531 @default.
• W4327957062 cites W1942108275 @default.
• W4327957062 cites W1964084984 @default.
• W4327957062 cites W1965898507 @default.
• W4327957062 cites W1990546575 @default.
• W4327957062 cites W1991102845 @default.
• W4327957062 cites W1992188543 @default.
• W4327957062 cites W1992355897 @default.
• W4327957062 cites W2044560189 @default.
• W4327957062 cites W2063103184 @default.
• W4327957062 cites W2068032877 @default.
• W4327957062 cites W2079641157 @default.
• W4327957062 cites W2082329580 @default.
• W4327957062 cites W2099879414 @default.
• W4327957062 cites W2106231443 @default.
• W4327957062 cites W2111817932 @default.
• W4327957062 cites W2118385536 @default.
• W4327957062 cites W2129944627 @default.
• W4327957062 cites W2135625048 @default.
• W4327957062 cites W2152687544 @default.
• W4327957062 cites W2159561097 @default.
• W4327957062 cites W2197745694 @default.
• W4327957062 cites W2233380899 @default.
• W4327957062 cites W2304135995 @default.
• W4327957062 cites W2488660279 @default.
• W4327957062 cites W2499105366 @default.
• W4327957062 cites W2572441160 @default.
• W4327957062 cites W2605775362 @default.
• W4327957062 cites W2606686133 @default.
• W4327957062 cites W2616480584 @default.
• W4327957062 cites W2621237140 @default.
• W4327957062 cites W2743656798 @default.
• W4327957062 cites W2761986865 @default.
• W4327957062 cites W2765226415 @default.
• W4327957062 cites W2767848202 @default.
• W4327957062 cites W2787745239 @default.
• W4327957062 cites W2809733166 @default.
• W4327957062 cites W2883837929 @default.
• W4327957062 cites W2900224735 @default.
• W4327957062 cites W2905357997 @default.
• W4327957062 cites W2905464296 @default.
• W4327957062 cites W2919249415 @default.
• W4327957062 cites W2943428116 @default.
• W4327957062 cites W2953485706 @default.
• W4327957062 cites W2963604282 @default.
• W4327957062 cites W2980421020 @default.
• W4327957062 cites W3006267693 @default.
• W4327957062 cites W3023360297 @default.
• W4327957062 cites W3034291645 @default.
• W4327957062 cites W3098601396 @default.
• W4327957062 cites W3098790947 @default.

• next