J/MNRAS/511/1043    Sub-Neptunes transiting TOI-1064             (Wilson+, 2022)

A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS. Wilson T.G., Goffo E., Alibert Y., Gandolfi D., Bonfanti A., Persson C.M., Collier Cameron A., Fridlund M., Fossati L., Korth J., Benz W., Deline A., Floren H.-G., Guterman P., Adibekyan V., Hooton M.J., Hoyer S., Leleu A., Mustill A.J., Salmon S., Sousa S.G., Suarez O., Abe L., Agabi A., Alonso R., Anglada G., Asquier J., Barczy T., Barrado Navascues D., Barros S.C.C., Baumjohann W., Beck M., Beck T., Billot N., Bonfils X., Brandeker A., Broeg C., Bryant E.M., Burleigh M.R., Buttu M., Cabrera J., Charnoz S., Ciardi D.R., Cloutier R., Cochran W.D., Collins K.A., Colon K.D., Crouzet N., Csizmadia S., Davies M.B., Deleuil M., Delrez L., Demangeon O., Demory B.-O., Dragomir D., Dransfield G., Ehrenreich D., Erikson A., Fortier A., Gan T., Gill S., Gillon M., Gnilka C.L., Grieves N., Grziwa S., Gudel M., Guillot T., Haldemann J., Heng K., Horne K., Howell S.B., Isaak K.G., Jenkins J.M., Jensen E.L.N., Kiss L., Lacedelli G., Lam K., Laskar J., Latham D.W., Lecavelier des Etangs A., Lendl M., Lester K.V., Levine A.M., Livingston J., Lovis C., Luque R., Magrin D., Marie-Sainte W., Maxted P.F.L., Mayo A.W., McLean B., Mecina M., Mekarnia D., Nascimbeni V., Nielsen L.D., Olofsson G., Osborn H.P., Osborne H.L.M., Ottensamer R., Pagano I., Palle E., Peter G., Piotto G., Pollacco D., Queloz D., Ragazzoni R., Rando N., Rauer H., Redfield S., Ribas I., Ricker G.R., Rieder M., Santos N.C., Scandariato G., Schmider F.-X., Schwarz R.P., Scott N.J., Seager S., Segransan D., Serrano L.M., Simon A.E., Smith A.M.S., Steller M., Stockdale C., Szabo G., Thomas N., Ting E.B., Triaud A.H.M.J., Udry S., Van Eylen V., Van Grootel V., Vanderspek R.K., Viotto V., Walton N., Winn J.N. <Mon. Not. R. Astron. Soc., 511, 1043-1071 (2022)> =2022MNRAS.511.1043W 2022MNRAS.511.1043W (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Exoplanets ; Radial velocities ; Optical Keywords: techniques: photometric - techniques: radial velocities - planets and satellites: composition - planets and satellites: detection - planets and satellites: interiors - stars: individual: TOI-1064 (TIC 79748331; Gaia EDR3 6683371847364921088) Abstract: We report the discovery and characterization of a pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey Satellite (TESS) photometry. To characterize the system, we performed and retrieved the CHaracterising ExOPlanets Satellite (CHEOPS), TESS, and ground-based photometry, the High Accuracy Radial velocity Planet Searcher (HARPS) high-resolution spectroscopy, and Gemini speckle imaging. We characterize the host star and determine Teff,*=4734±67K, R*=0.726±0.007R, and M*=0.748±0.032M. We present a novel detrending method based on point spread function shape-change modelling and demonstrate its suitability to correct flux variations in CHEOPS data. We confirm the planetary nature of both bodies and find that TOI-1064 b has an orbital period of Pb=6.44387±0.00003d, a radius of Rb=2.59±0.04R, and a mass of Mb=13.5+1.7-1.8M, whilst TOI-1064 c has an orbital period of Pc=12.22657+0.00005-0.00004d, a radius of Rc=2.65±0.04R, and a 3σ upper mass limit of 8.5M. From the high-precision photometry we obtain radius uncertainties of ∼1.6 per cent, allowing us to conduct internal structure and atmospheric escape modelling. TOI-1064 b is one of the densest, well-characterized sub-Neptunes, with a tenuous atmosphere that can be explained by the loss of a primordial envelope following migration through the protoplanetary disc. It is likely that TOI-1064 c has an extended atmosphere due to the tentative low density, however further radial velocities are needed to confirm this scenario and the similar radii, different masses nature of this system. The high-precision data and modelling of TOI-1064 b are important for planets in this region of mass-radius space, and it allow us to identify a trend in bulk density-stellar metallicity for massive sub-Neptunes that may hint at the formation of this population of planets. Description: Raw and detrended data from CHEOPS, TESS, LCOGT, NGTS, ASTEP, ASAS-SN, WASP, HARPS, and Gemini-South; PSF and CCF SCALPELS data from CHEOPS and HARPS analyses. Objects: ----------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------- 19 44 00.95 -47 33 41.75 TOI-1064 = TIC 79748331 ----------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file cheoraw1.dat 187 440 CHEOPS visit 1 raw data cheoraw2.dat 187 278 CHEOPS visit 2 raw data cheoraw3.dat 187 282 CHEOPS visit 3 raw data cheoraw4.dat 187 254 CHEOPS visit 4 raw data cheoraw5.dat 187 231 CHEOPS visit 5 raw data cheoraw6.dat 187 762 CHEOPS visit 6 raw data cheopsf1.dat 621 440 CHEOPS visit 1 PSF SCALPELS data cheopsf2.dat 469 278 CHEOPS visit 2 PSF SCALPELS data cheopsf3.dat 599 282 CHEOPS visit 3 PSF SCALPELS data cheopsf4.dat 318 254 CHEOPS visit 4 PSF SCALPELS data cheopsf5.dat 665 231 CHEOPS visit 5 PSF SCALPELS data cheopsf6.dat 1001 762 CHEOPS visit 6 PSF SCALPELS data cheodet1.dat 55 440 CHEOPS visit 1 detrended data cheodet2.dat 55 278 CHEOPS visit 2 detrended data cheodet3.dat 55 282 CHEOPS visit 3 detrended data cheodet4.dat 55 254 CHEOPS visit 4 detrended data cheodet5.dat 55 231 CHEOPS visit 5 detrended data cheodet6.dat 55 762 CHEOPS visit 6 detrended data traws13.dat 59 17939 TESS sector 13 raw data traws27.dat 59 71703 TESS sector 27 raw data tdets13.dat 59 17939 TESS sector 13 detrended data tdets27.dat 59 71703 TESS sector 27 detrended data harpsraw.dat 98 26 HARPS raw data harpsccf.dat 107 26 HARPS CCF SCALPELS data ctiozs.dat 55 255 LCOGT CTIO Zs data saaob.dat 46 122 LCOGT SAAO B data saaozs1.dat 55 453 LCOGT SAAO Zs visit 1 data saaozs2.dat 55 368 LCOGT SAAO Zs visit 2 data saaozs3.dat 55 343 LCOGT SAAO Zs visit 4 data ngtsraw.dat 75 1811 NGTS raw data ngtsdet.dat 48 1811 NGTS detrended data astep1.dat 46 297 ASTEP visit 1 data astep2.dat 46 421 ASTEP visit 2 data astep3.dat 46 267 ASTEP visit 3 data astep4.dat 46 178 ASTEP visit 3 data asassn.dat 58 401 ASAS-SN data wasp.dat 59 66832 WASP data gems562.dat 19 119 Gemini-South 562 data gems832.dat 19 120 Gemini-South 832 data -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheoraw*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.10 d BJD Barycentric Julian date 20- 37 F18.16 --- Flux Normalised flux 39- 60 F22.20 --- e_Flux Normalised flux error 62- 75 E14.7 pix Xoffset X centroid position offset 77- 88 F12.9 pix Yoffset Y centroid position offset 90-108 F19.15 --- Roll Roll angle 110-129 F20.18 ct Contam Contamination 131-150 F20.18 ct Bckg Background 152-173 E22.16 ct Smear Smear 175-187 F13.10 --- DeltaT Delta temperature -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheopsf*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 F16.8 d BJD Barycentric Julian date 18- 34 F17.15 --- Flux Normalised flux 36- 52 F17.15 --- e_Flux Normalised flux error 54- 70 F17.15 --- Fluxd Normalised detrended flux 72- 88 F17.15 --- e_Fluxd Normalised detrended flux error 90- 106 F17.15 --- Fluxpsfmodel PSF SCALPELS PSF shape change model 108- 128 E21.13 --- Theta0 1st PSF SCALPELS principal component 130- 150 E21.12 --- Theta1 2nd PSF SCALPELS principal component 151- 168 F18.15 --- Theta2 3rd PSF SCALPELS principal component 170- 190 E21.13 --- Theta3 4th PSF SCALPELS principal component 192- 209 F18.15 --- Theta4 5th PSF SCALPELS principal component 211- 231 E21.13 --- Theta5 6th PSF SCALPELS principal component 233- 253 E21.13 --- Theta6 7th PSF SCALPELS principal component 255- 274 E20.12 --- Theta7 8th PSF SCALPELS principal component 276- 296 E21.13 --- Theta8 9th PSF SCALPELS principal component 298- 318 E21.13 --- Theta9 10th PSF SCALPELS principal component 320- 339 E20.12 --- Theta10 ? 11th PSF SCALPELS principal component 341- 361 E21.12 --- Theta11 ? 12th PSF SCALPELS principal component 362- 382 E21.13 --- Theta12 ? 13th PSF SCALPELS principal component 384- 404 E21.13 --- Theta13 ? 14th PSF SCALPELS principal component 406- 426 E21.13 --- Theta14 ? 15th PSF SCALPELS principal component 428- 448 E21.13 --- Theta15 ? 16th PSF SCALPELS principal component 449- 469 E21.13 --- Theta16 ? 17th PSF SCALPELS principal component 471- 491 E21.13 --- Theta17 ? 18th PSF SCALPELS principal component 493- 512 E20.12 --- Theta18 ? 19th PSF SCALPELS principal component 514- 534 E21.13 --- Theta19 ? 20th PSF SCALPELS principal component 536- 556 E21.13 --- Theta20 ? 21st PSF SCALPELS principal component 558- 578 E21.13 --- Theta21 ? 22nd PSF SCALPELS principal component 580- 599 E20.12 --- Theta22 ? 23rd PSF SCALPELS principal component 601- 621 E21.13 --- Theta23 ? 24th PSF SCALPELS principal component 623- 643 E21.13 --- Theta24 ? 25th PSF SCALPELS principal component 645- 665 E21.13 --- Theta25 ? 26th PSF SCALPELS principal component 667- 686 E20.12 --- Theta26 ? 27th PSF SCALPELS principal component 688- 707 E20.12 --- Theta27 ? 28th PSF SCALPELS principal component 709- 729 E21.13 --- Theta28 ? 29th PSF SCALPELS principal component 731- 751 E21.13 --- Theta29 ? 30th PSF SCALPELS principal component 753- 773 E21.13 --- Theta30 ? 31st PSF SCALPELS principal component 775- 795 E21.13 --- Theta31 ? 32nd PSF SCALPELS principal component 797- 814 F18.15 --- Theta32 ? 33rd PSF SCALPELS principal component 816- 836 E21.13 --- Theta33 ? 34th PSF SCALPELS principal component 838- 855 F18.15 --- Theta34 ? 35th PSF SCALPELS principal component 857- 876 E20.12 --- Theta35 ? 36th PSF SCALPELS principal component 878- 895 F18.15 --- Theta36 ? 37th PSF SCALPELS principal component 897- 917 E21.13 --- Theta37 ? 38th PSF SCALPELS principal component 919- 939 E21.13 --- Theta38 ? 39th PSF SCALPELS principal component 941- 961 E21.13 --- Theta39 ? 40th PSF SCALPELS principal component 963- 982 E20.12 --- Theta40 ? 41st PSF SCALPELS principal component 984-1001 F18.15 --- Theta41 ? 42nd PSF SCALPELS principal component -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheodet*.dat ngtsdet.dat tdets*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.10 d BJD Barycentric Julian date 20- 37 F18.16 --- Flux Normalised detrended flux 39- 59 F21.19 --- e_Flux Normalised flux error -------------------------------------------------------------------------------- Byte-by-byte Description of file: [acs]*.dat traw*.dat wasp.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.10 d BJD Barycentric Julian date 20- 37 F18.16 --- Flux Normalised flux 39- 59 F21.19 --- e_Flux Normalised flux error -------------------------------------------------------------------------------- Byte-by-byte Description of file: ngtsraw.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 F16.8 d BJD Barycentric Julian date 18- 27 F10.8 --- Flux Normalised flux 29- 38 F10.8 --- e_Flux Normalised flux error 40- 47 F8.6 --- Airmass Airmass 49- 57 F9.3 ct SkyBkg Sky background 59- 66 F8.3 pix X X centroid position 68- 75 F8.3 pix Y Y centroid position -------------------------------------------------------------------------------- Byte-by-byte Description of file: harpsraw.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 F16.8 d BJD Barycentric Julian date 18- 33 F16.10 m/s RV Radial velocity 35- 50 F16.14 m/s e_RV Radial velocity error 52- 55 F4.1 m/s BIS Bisector span of the CCF 57- 62 F6.1 m/s FWHM FWHM of the CCF 64- 70 F7.4 --- Contrast Contrast of the CCF 72- 77 F6.4 --- Sindex S index 79- 84 F6.4 --- Halpha Hα activity index 86- 91 F6.4 --- NaD1 Na D1 activity index 93- 98 F6.4 --- NaD2 Na D2 activity index -------------------------------------------------------------------------------- Byte-by-byte Description of file: harpsccf.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 F16.8 d BJD Barycentric Julian date 18- 33 F16.10 m/s RV Radial velocity 35- 50 F16.14 m/s e_RV Radial velocity error 52- 69 F18.15 --- Theta0 1st CCF SCALPELS principal component 71- 88 F18.15 --- Theta1 2nd CCF SCALPELS principal component 90-107 F18.15 --- Theta2 3rd CCF SCALPELS principal component -------------------------------------------------------------------------------- Byte-by-byte Description of file: gems562.dat gems832.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 nm lambda Wavelength (562 or 832) 5- 11 F7.5 arcsec Sep Separation 13- 19 F7.5 --- Deltamag Delta magnitude -------------------------------------------------------------------------------- Acknowledgements: Thomas G. Wilson, tgw1(at)st-andrews.ac.uk
(End) Patricia Vannier [CDS] 26-Apr-2022
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