J/MNRAS/529/3323               HD 77946 RV curves            (Palethorpe+, 2024)

Confronting compositional confusion through the characterization of the sub-Neptune orbiting HD 77946. Palethorpe L., Anna John A., Mortier A., Davoult J., Wilson T. G., Rice K., Cameron A. C., Alibert Y., Buchhave L., Malavolta L., Cadman J., Lopez-Morales M., Dumusque X., Silva A. M., Quinn S. N., Van Eylen V., Vissapragada S., Affer L., Charbonneau D., Cosentino R., Ghedina A., Haywood R. D., Latham D. W., Lienhard F., Martinez Fiorenzano A. F., Pedani M., Pepe F., Pinamonti M., Sozzetti A., Stalport M., Udry S., Vanderburg A. <Mon. Not. R. Astron. Soc., 529, 3323-3341> =2024MNRAS.529.3323P 2024MNRAS.529.3323P (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Exoplanets ; Radial velocities ; Optical Keywords: techniques: photometric - techniques: radial velocities - techniques: spectroscopic - planets and satellites: composition - planets and satellites: fundamental parameters - stars: individual (HD 77946) Abstract: We report on the detailed characterization of the HD 77946 planetary system. HD 77946 is an F5 (M*=1.17M, R*=1.31R) star, which hosts a transiting planet recently discovered by NASA's Transiting Exoplanet Survey Satellite (TESS), classified as TOI-1778 b. Using TESS photometry, high-resolution spectroscopic data from HARPS-N, and photometry from CHEOPS, we measure the radius and mass from the transit and radial velocity observations, and find that the planet, HD 77946 b, orbits with period Pb=6.527282-0.000020+0.000015d, has a mass of Mb=8.38±1.32M, and a radius of Rb=2.705-0.081+0.086R. From the combination of mass and radius measurements, and the stellar chemical composition, the planet properties suggest that HD 77946 b is a sub-Neptune with a ∼1 per cent H/He atmosphere. However, a degeneracy still exists between water-world and silicate/iron-hydrogen models, and even though interior structure modelling of this planet favours a sub-Neptune with a H/He layer that makes up a significant fraction of its radius, a water-world composition cannot be ruled out, as with Teq= 1248+40-38K, water may be in a supercritical state. The characterization of HD 77946 b, adding to the small sample of well-characterized sub-Neptunes, is an important step forwards on our journey to understanding planetary formation and evolution pathways. Furthermore, HD 77946 b has one of the highest transmission spectroscopic metrics for small planets orbiting hot stars, thus transmission spectroscopy of this key planet could prove vital for constraining the compositional confusion that currently surrounds small exoplanets. Description: Table1 contains the DRS reduced radial velocities and activity indicators for HD 77946 obtained by HARPS-N. Table2 contains the s-BART reduced radial velocities for HD 77946 obtained by HARPS-N. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 09 07 06.73 +46 40 21.3 HD 77946 = TOI-1778 ------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 93 102 HARPS-N RV DRS reduced data table2.dat 28 102 HARPS-N RV s-BART reduced data -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 F15.7 d BJD Barycentric Julian date 17- 24 F8.2 m/s RV Radial velocity 26- 29 F4.2 m/s e_RV Error in radial velocity 31- 36 F6.3 m/s BIS Bisector inverse span 38- 41 F4.2 m/s e_BIS Error in bisector inverse span 43- 49 F7.5 km/s FWHM Full-width-at-half-maximum of the CCF 51- 57 F7.5 km/s e_FWHM Error in Full-width-at-half-maximum of the CCF 59- 66 F8.6 --- Halpha Halpha index 68- 75 F8.6 --- e_Halpha Error in Halpha index 77- 84 F8.5 --- logRHK RHK activity index 86- 93 F8.6 --- e_logRHK Error in RHK activity index -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.6 d BJD Barycentric Julian date 16- 23 F8.2 m/s RV Radial velocity 25- 28 F4.2 m/s e_RV Error in radial velocity -------------------------------------------------------------------------------- Acknowledgements: Larissa Palethorpe, larissa.palethorpe(at)ed.ac.uk
(End) Patricia Vannier [CDS] 03-Jun-2024
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line