J/A+A/664/A156 Young sub-Neptunes orbiting TOI-2076 light curves (Osborn+, 2022)

Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076. Osborn H.P., Bonfanti A., Gandolfi D., Hedges C., Leleu A., Fortier A., Futyan D., Gutermann P., Maxted P.F.L., Borsato L., Collins K.A., Gomes da Silva J., Gomez Maqueo Chew Y., Hooton M.J., Lendl M., Parviainen H., Salmon S., Schanche N., Serrano L.M., Sousa S.G., Tuson A., Ulmer-Moll S., Van Grootel V., Wells R.D., Wilson T.G., Alibert Y., Alonso R., Anglada G., Asquier J., Barrado y Navascues D., Baumjohann W., Beck T., Benz W., Biondi F., Bonfils X., Bouchy F., Brandeker A., Broeg C., Barczy T., Barros S.C.C., Cabrera J., Charnoz S., Collier Cameron A., Csizmadia S., Davies M.B., Deleuil M., Delrez L., Demory B.-O., Ehrenreich D., Erikson A., Fossati L., Fridlund M., Gillon M., Gomez-Munoz M.A., Guedel M., Heng K., Hoyer S., Isaak K.G., Kiss L., Laskar J., Lecavelier des Etangs A., Lovis C., Magrin D., Malavolta L., McCormac J., Nascimbeni V., Olofsson G., Ottensamer R., Pagano I., Palle E., Peter G., Piazza D., Piotto G., Pollacco D., Queloz D., Ragazzoni R., Rando N., Rauer H., Reimers C., Ribas I., Demangeon O.D.S., Smith A.M.S., Sabin L., Santos N., Scandariato G., Schroffenegger U., Schwarz R.P., Shporer A., Simon A.E., Steller M., Szabo G.M., Segransan D., Thomas N., Udry S., Walter I., Walton N. <Astron. Astrophys. 664, A156 (2022)> =2022A&A...664A.156O 2022A&A...664A.156O (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Exoplanets ; Photometry Keywords: planets and satellites: detection - stars: individual: TOI-2076 - techniques: photometric Abstract: TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G=8.9mag), young (340±80Myr) K-type star. Although a validated planetary system, the orbits of the two outer planets were unconstrained as only two non-consecutive transits were seen in TESS photometry. This left 11 and 7 possible period aliases for each. To reveal the true orbits of these two long-period planets, precise photometry targeted on the highest- probability period aliases is required. Long-term monitoring of transits in multi-planet systems can also help constrain planetary masses through TTV measurements. We used the MonoTools package to determine which aliases to follow, and then performed space-based and ground-based photometric follow-up of TOI-2076 c and d with CHEOPS, SAINT-EX, and LCO telescopes. CHEOPS observations revealed a clear detection for TOI-2076 c at P=21.01538+0.00084-0.00074d, and allowed us to rule out three of the most likely period aliases for TOI-2076 d. Ground-based photometry further enabled us to rule out remaining aliases and confirm the P=35.12537±0.00067d alias. These observations also improved the radius precision of all three sub- Neptunes to 2.518±0.036, 3.497±0.043, and 3.232±0.063 R. Our observations also revealed a clear anti-correlated TTV signal between planets b and c likely caused by their proximity to the 2:1 resonance, while planets c and d appear close to a 5:3 period commensurability, although model degeneracy meant we were unable to retrieve robust TTV masses. Their inflated radii, likely due to extended H-He atmospheres, combined with low insolation makes all three planets excellent candidates for future comparative transmission spectroscopy with JWST. Description: We present all space- and ground-based photometry observed of TOI-2076 which contributed the paper. This includes 4 visits with CHEOPS, and 6 ground-based lightcurves from LCO/McDonald (1m, z-band), Saint-Ex (1m, r-band), LCO/MuSCAT-3 (2m, g, r, i & z bands, each presented independently here). Objects: -------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------- 14 29 34.24 +39 47 25.5 TOI-2076 = BD+40 2790 -------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file cheops_0.dat 248 545 Cheops visit 4 photometry and best-fit models (File key CHPR110048TG003701_V0200) cheops_1.dat 320 502 Cheops visit 3 photometry and best-fit models (File key CHPR110048TG003601_V0200) cheops_2.dat 248 564 Cheops visit 2 photometry and best-fit models (File key CHPR110048TG003201_V0200) cheops_3.dat 324 415 Cheops visit 1 photometry and best-fit models (File key CHPR110048TG002501_V0200) g_lco.dat 430 404 LCO/MuSCAT3 photometry and best-fit models in g band r_lco.dat 426 639 LCO/MuSCAT3 photometry and best-fit models in r band i_lco.dat 423 693 LCO/MuSCAT3 photometry and best-fit models in i band z_lco.dat 424 598 LCO/MuSCAT3 photometry and best-fit models in z band r_sex.dat 322 490 Saint-Ex photometry and best-fit models in r band z_mcd.dat 136 458 LCO/1m McDonald photometry and best-fit models in z band -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheops_0.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 37 F18.14 deg phi CHEOPS spacecraft roll angle (in degrees) adjusted to be near-continuous 39- 61 F23.20 --- Flux Normalised aperture flux (in ppt) 63- 81 F19.17 --- e_Flux Flux standard deviation (in ppt) 83-105 E23.16 --- smear Vertical read-out smear as computed by the CHEOPS DRP 107-126 F20.17 --- deltaT Change in on-board CHEOPS temperature as computed by the DRP 128-150 F23.20 --- bg Background contaminant flux as computed by the CHEOPS DRP 152-173 F22.19 --- sinphi Sine of CHEOPS spacecraft roll angle 175-195 F21.18 --- cosphi Cosine of CHEOPS spacecraft roll angle 197-219 E23.16 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 221-240 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 242-244 F3.1 --- plxmed Best-fit planetary transit model (median) 246-248 F3.1 --- plxsd Error on best-fit planetary transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheops_1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 37 F18.14 deg phi CHEOPS spacecraft roll angle (in degrees) adjusted to be near-continuous 39- 59 F21.18 --- Flux Normalised aperture flux (in ppt) 61- 79 F19.17 --- e_Flux Flux standard deviation (in ppt) 81-103 E23.17 --- smear vertical read-out smear as computed by the CHEOPS DRP 105-124 F20.17 --- deltaT Change in on-board CHEOPS temperature as computed by the DRP 126-148 E23.17 --- bg Background contaminant flux as computed by the CHEOPS DRP 150-171 F22.19 --- sinphi Sine of CHEOPS spacecraft roll angle 173-193 F21.18 --- cosphi Cosine of CHEOPS spacecraft roll angle 195-215 F21.18 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 217-236 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 238-256 F19.16 --- plxmed Best-fit planetary transit model (median) 258-277 F20.18 --- plxsd Error on best-fit planetary transit model (standard deviation) 279-299 F21.18 --- summodxmed Best-fit combined flux correction and transit model (median) 301-320 F20.18 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheops_2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 37 F18.14 deg phi CHEOPS spacecraft roll angle (in degrees) adjusted to be near-continuous 39- 60 F22.19 --- Flux Normalised aperture flux (in ppt) 62- 80 F19.17 --- e_Flux Flux standard deviation (in ppt) 82-104 E23.17 --- smear vertical read-out smear as computed by the CHEOPS DRP 106-125 F20.17 --- deltaT Change in on-board CHEOPS temperature as computed by the DRP 127-150 E24.17 --- bg Background contaminant flux as computed by the CHEOPS DRP 152-172 F21.18 --- sinphi Sine of CHEOPS spacecraft roll angle 174-196 F23.20 --- cosphi Cosine of CHEOPS spacecraft roll angle 198-219 F22.19 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 221-240 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 242-244 F3.1 --- plxmed Best-fit planetary transit model (median) 246-248 F3.1 --- plxsd Error on best-fit planetary transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: cheops_3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 37 F18.14 deg phi CHEOPS spacecraft roll angle (in degrees) adjusted to be near-continuous 39- 59 F21.18 --- Flux Normalised aperture flux (in ppt) 61- 79 F19.17 --- e_Flux Flux standard deviation (in ppt) 81-102 E22.16 --- smear vertical read-out smear as computed by the CHEOPS DRP 104-123 F20.17 --- deltaT Change in on-board CHEOPS temperature as computed by the DRP 125-147 E23.17 --- bg Background contaminant flux as computed by the CHEOPS DRP 149-169 F21.18 --- sinphi Sine of CHEOPS spacecraft roll angle 171-192 F22.19 --- cosphi Cosine of CHEOPS spacecraft roll angle 194-215 F22.19 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 217-236 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 238-258 F21.18 --- plxmed Best-fit planetary transit model (median) 260-280 E21.16 --- plxsd Error on best-fit planetary transit model (standard deviation) 282-303 F22.19 --- summodxmed Best-fit combined flux correction and transit model (median) 305-324 F20.18 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: g_lco.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 44 F25.20 --- Flux Normalised aperture flux (in ppt) 46- 63 F18.16 --- e_Flux Flux standard deviation (in ppt) 65- 86 F22.19 --- Airmass Airmass of star 88-109 F22.19 --- Entropy PSF fit model entropy from MuSCAT DRP 111-132 F22.19 --- Width PSF with from AstroImageJ 134-155 F22.19 --- X PSF x-centroid from AIJ 157-178 F22.19 --- Y PSF y-centroid from AIJ 180-200 F21.18 --- FWHM PSF full-width-half-maximum from AIJ 202-223 F22.19 --- compcts Total comparison star flux counts as computed with AIJ 225-246 F22.19 --- g/r Interpolated weighted flux normalised colour ratio between MuSCAT3 bands g & r 248-269 F22.19 --- r/i Interpolated weighted flux normalised colour ratio between MuSCAT3 bands r & i 271-292 F22.19 --- i/z Interpolated weighted flux normalised colour ratio between MuSCAT3 bands i & z 294-317 F24.19 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 319-338 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 340-361 F22.19 --- plxmed Best-fit planetary transit model (median) 363-384 E22.17 --- plxsd Error on best-fit planetary transit model (standard deviation) 386-409 F24.19 --- summodxmed Best-fit combined flux correction and transit model (median) 411-430 F20.18 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: r_lco.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 41 F22.18 --- Flux Normalised aperture flux (in ppt) 43- 60 F18.16 --- e_Flux Flux standard deviation (in ppt) 62- 82 F21.18 --- Airmass Airmass of star 84-105 F22.19 --- Entropy PSF fit model entropy from MuSCAT DRP 107-128 F22.19 --- Width PSF with from AstroImageJ 130-151 E22.16 --- X PSF x-centroid from AIJ 153-174 F22.19 --- Y PSF y-centroid from AIJ 176-196 F21.18 --- FWHM PSF full-width-half-maximum from AIJ 198-219 F22.19 --- compcts Total comparison star flux counts as computed with AIJ 221-242 F22.19 --- g/r Interpolated weighted flux normalised colour ratio between MuSCAT3 bands g & r 244-266 F23.20 --- r/i Interpolated weighted flux normalised colour ratio between MuSCAT3 bands r & i 268-288 F21.18 --- i/z Interpolated weighted flux normalised colour ratio between MuSCAT3 bands i & z 290-313 F24.20 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 315-334 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 336-357 F22.19 --- plxmed Best-fit planetary transit model (median) 359-380 E22.17 --- plxsd Error on best-fit planetary transit model (standard deviation) 382-405 F24.20 --- summodxmed Best-fit combined flux correction and transit model (median) 407-426 F20.18 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: i_lco.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 41 F22.18 --- Flux Normalised aperture flux (in ppt) 43- 60 F18.16 --- e_Flux Flux standard deviation (in ppt) 62- 83 F22.19 --- Airmass Airmass of star 85-106 F22.19 --- Entropy PSF fit model entropy from MuSCAT DRP 108-129 F22.19 --- Width PSF with from AstroImageJ 131-152 F22.19 --- X PSF x-centroid from AIJ 154-175 F22.19 --- Y PSF y-centroid from AIJ 177-198 F22.19 --- FWHM PSF full-width-half-maximum from AIJ 200-222 F23.20 --- compcts Total comparison star flux counts as computed with AIJ 224-244 F21.18 --- g/r Interpolated weighted flux normalised colour ratio between MuSCAT3 bands g & r 246-267 F22.19 --- r/i Interpolated weighted flux normalised colour ratio between MuSCAT3 bands r & i 269-289 F21.18 --- i/z Interpolated weighted flux normalised colour ratio between MuSCAT3 bands i & z 291-312 F22.18 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 314-333 F20.18 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 335-356 F22.19 --- plxmed Best-fit planetary transit model (median) 358-379 E22.17 --- plxsd Error on best-fit planetary transit model (standard deviation) 381-402 F22.18 --- summodxmed Best-fit combined flux correction and transit model (median) 404-423 F20.18 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: z_lco.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 41 F22.18 --- Flux Normalised aperture flux (in ppt) 43- 60 F18.16 --- e_Flux Flux standard deviation (in ppt) 62- 83 F22.19 --- Airmass Airmass of star 85-106 F22.19 --- Entropy PSF fit model entropy from MuSCAT DRP 108-129 F22.19 --- Width PSF with from AstroImageJ 131-152 F22.19 --- X PSF x-centroid from AIJ 154-176 F23.20 --- Y PSF y-centroid from AIJ 178-199 F22.19 --- FWHM PSF full-width-half-maximum from AIJ 201-222 F22.19 --- compcts Total comparison star flux counts as computed with AIJ 224-245 F22.19 --- g/r Interpolated weighted flux normalised colour ratio between MuSCAT3 bands g & r 247-269 F23.20 --- r/i Interpolated weighted flux normalised colour ratio between MuSCAT3 bands r & i 271-292 F22.19 --- i/z Interpolated weighted flux normalised colour ratio between MuSCAT3 bands i & z 294-315 F22.18 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 317-335 F19.17 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 337-358 F22.19 --- plxmed Best-fit planetary transit model (median) 360-381 E22.17 --- plxsd Error on best-fit planetary transit model (standard deviation) 383-404 F22.18 --- summodxmed Best-fit combined flux correction and transit model (median) 406-424 F19.17 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: r_sex.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 42 F23.19 --- Flux Normalised aperture flux (in ppt) 44- 61 F18.15 --- e_Flux Flux standard deviation (in ppt) 63- 84 F22.19 --- Airmass Airmass of star 86-107 F22.19 --- Width PSF with from AstroImageJ 109-130 F22.19 --- X PSF x-centroid from AIJ 132-152 F21.18 --- Y PSF y-centroid from AIJ 154-174 F21.18 --- FWHM PSF full-width-half-maximum from AIJ 176-196 F21.18 --- compcts Total comparison star flux counts as computed with AIJ 198-219 F22.18 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 221-238 F18.16 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 240-260 F21.18 --- plxmed Best-fit planetary transit model (median) 262-281 F20.18 --- plxsd Error on best-fit planetary transit model (standard deviation) 283-303 F21.17 --- summodxmed Best-fit combined flux correction and transit model (median) 305-322 F18.16 --- summodxsd Error on best-fit combined flux correction and transit model (standard deviation) -------------------------------------------------------------------------------- Byte-by-byte Description of file: z_mcd.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.13 d Time Barycentric Julian Date (BJD-2457000) 20- 42 F23.19 --- Flux Normalised aperture flux (in ppt) 44- 61 F18.13 --- e_Flux [] Flux standard deviation (in ppt) 63- 84 F22.19 --- Airmass Airmass of star 86-109 E24.17 --- Fluxcmed Best-fit flux correction model from linear decorrelation of meta data (median) 111-128 F18.16 --- Fluxcsd Error on best-fit flux correction model from linear decorrelation of meta data (standard deviation) 130-132 F3.1 --- plxmed Best-fit planetary transit model (median) 134-136 F3.1 --- plxsd Error on best-fit planetary transit model (standard deviation) -------------------------------------------------------------------------------- Acknowledgements: Hugh Osborn, hugh.osborn(at)unibe.ch
(End) Patricia Vannier [CDS] 07-Mar-2022
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