J/AJ/162/82   IRD and HPF spectra of TRAPPIST-1b,e and f  (Krishnamurthy+, 2021)

Nondetection of Helium in the Upper Atmospheres of TRAPPIST-1b, e, and f. Krishnamurthy V., Hirano T., Stefansson G., Ninan J.P., Mahadevan S., Gaidos E., Kopparapu R., Sato B., Hori Y., Bender C.F., Canas C.I., Diddams S.A., Halverson S., Harakawa H., Hawley S., Hearty F., Hebb L., Hodapp K., Jacobson S., Kanodia S., Konishi M., Kotani T., Kowalski A., Kudo T., Kurokawa T., Kuzuhara M., Lin A., Maney M., Metcalf A.J., Morris B., Nishikawa J., Omiya M., Robertson P., Roy A., Schwab C., Serizawa T., Tamura M., Ueda A., Vievard S., Wisniewski J. <Astron. J., 162, 82 (2021)> =2021AJ....162...82K 2021AJ....162...82K
ADC_Keywords: Exoplanets; Spectra, infrared; Photometry, SDSS Keywords: Exoplanets ; Transmission spectroscopy ; Exoplanet atmospheres Abstract: We obtained high-resolution spectra of the ultracool M-dwarf TRAPPIST-1 during the transit of its planet "b" using two high-dispersion near-infrared spectrographs, the Infrared Doppler (IRD) instrument on the Subaru 8.2m telescope, and the Habitable Zone Planet Finder (HPF) instrument on the 10m Hobby-Eberly Telescope. These spectroscopic observations are complemented by a photometric transit observation for planet "b" using the APO/ARCTIC, which assisted us in capturing the correct transit times for our transit spectroscopy. Using the data obtained by the new IRD and HPF observations, as well as the prior transit observations of planets "b," "e" and "f" from IRD, we attempt to constrain the atmospheric escape of the planet using the Hei triplet 10830Å absorption line. We do not detect evidence for any primordial extended H-He atmospheres in all three planets. To limit any planet-related absorption, we place an upper limit on the equivalent widths of <7.754mÅ for planet "b," <10.458mÅ for planet "e," <4.143mÅ for planet "f" at 95% confidence from the IRD data, and <3.467mÅ for planet "b" at 95% confidence from HPF data. Using these limits along with a solar- like composition isothermal Parker wind model, we attempt to constrain the mass-loss rates for the three planets. For TRAPPIST-1b, our models exclude the highest possible energy-limited rate for a wind temperature <5000K. This nondetection of extended atmospheres with low mean-molecular weights in all three planets aids in further constraining their atmospheric composition by steering the focus toward the search of high-molecular-weight species in their atmospheres. Description: We observed a photometric transit of TRAPPIST-1b on the night of UT 2020 September 5 using the Astrophysical Research Consortium Telescope Imaging Camera (ARCTIC) on the 3.5m Astrophysical Research Consortium Telescope at Apache Point Observatory. We adopted the SDSS filter using an exposure time of 18s in the 4x4 binning fast-readout mode. We observed the transit of TRAPPIST-1b on the night of UT 2020 September 17 using Infrared Doppler (IRD), which has a spectral resolution of ∼70000 in the operating wavelength range of 0.95-1.75µm, mounted on the 8.2m Subaru Telescope on Maunakea, Hawaii. Habitable Planet Finder (HPF) is a fiber-fed high-resolution (R=55000) spectrograph on the 10m Hobby-Eberly Telescope (HET) at McDonald Observatory in Texas. Using HPF, we obtained three transits on the nights of UT 2018 October 2, 2019 July 31, and 2020 September 5. Objects: ---------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------- 23 06 29.37 -05 02 29.0 TRAPPIST-1b = TRAPPIST-1b 23 06 29.3 -05 02 29.0 TRAPPIST-1e = TRAPPIST-1e 23 06 29.4 -05 02 29.0 TRAPPIST-1f = TRAPPIST-1f ---------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig1.dat 108 556 APO/ARCTIC Transit and modeling of TRAPPIST-1b fig2a.dat 182 107 Transmission spectra of TRAPPIST-1b,e,f from IRD fig2b.dat 60 94 Transmission spectra of TRAPPIST-1b from HPF -------------------------------------------------------------------------------- See also: J/A+A/632/A24 : HeI IR triplet measurements for M dwarfs (Fuhrmeister+, 2019) J/A+A/640/A112 : TRAPPIST-1 transit timings (Ducrot+, 2020) J/AJ/159/100 : Flux & RVs of the dwarf G9-40 with K2 & HPF (Stefansson+,2020) J/AJ/160/192 : Photometry and RVs of K2-25b with HPF (Stefansson+, 2020) J/AJ/159/278 : He-filter obs. of WASP-69b & WASP-52b (Vissapragada+, 2020) Byte-by-byte Description of file: fig1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 F18.10 d BJD [2459097/2459098] Barycentric Julian Date at TDB 20- 31 F12.10 --- flux [0.98/1.01] Normalized flux 33- 44 F12.10 --- e_flux [0.002/0.004] flux uncertainty 46- 57 F12.10 --- model1 [0.99/1.01] Best-fit transit model, with Gaussian Process 59- 70 F12.10 --- gp [1/1.01] Best-fit Gaussian-Process model only 72- 89 F18.16 --- flux2 [0.98/1.01] detrended flux, removing Gaussian Process 91-108 F18.16 --- model2 [0.99/1.01] best-fit transit fit, no Gaussian Process -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig2a.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.6 nm waveb [1083/1084] Wavelength for TRAPPIST-1b (IRD) 13- 23 F11.9 --- tb [0.6/1.7] median-combined normalized flux during transit of TRAPPIST-1b from IRD 25- 35 F11.9 --- ntb [0.6/2] median-combined normalized flux outside the transit of TRAPPIST-1b from IRD 37- 48 F12.9 --- ratiob [-0.54/0.77] Flux ratio TRAPPIST-1b IRD (in/out-1) 50- 60 F11.9 --- e_ratiob [0.009/0.4] Error in Flux ratio of TRAPPIST-1b 62- 72 F11.6 nm wavee [1083/1084] Wavelength in nm for TRAPPIST-1e (IRD) 74- 84 F11.9 --- te [0.59/1.9] median-combined normalized flux during transit of TRAPPIST-1e from IRD 86- 96 F11.9 --- nte [0.6/2] median-combined normalized flux outside the transit of TRAPPIST-1e from IRD 98-109 F12.9 --- ratioe [-0.11/0.06] Flux ratio TRAPPIST-1e IRD (in/out-1) 111-121 F11.9 --- e_ratioe [0.01/0.5] Error in Flux ratio of TRAPPIST-1e 123-133 F11.6 nm wavef [1083/1084] Wavelength in nm for TRAPPIST-1f (IRD) 135-145 F11.9 --- tf [0.59/1.6] median-combined normalized flux during transit of TRAPPIST-1f from IRD 147-157 F11.9 --- ntf [0.6/2] median-combined normalized flux outside the transit of TRAPPIST-1f from IRD 159-170 F12.9 --- ratiof [-0.21/0.07] Flux ratio TRAPPIST-1f IRD (in/out-1) 172-182 F11.9 --- e_ratiof [0.01/0.5] Error in Flux ratio of TRAPPIST-1f -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig2b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.6 nm waveb [1083/1084] Wavelength from HPF 13- 23 F11.9 --- tb [0.37/1.1] Median-combined normalized flux during transit of TRAPPIST-1b from HPF 25- 35 F11.9 --- ntb [0.65/1.2] Median-combined normalized flux outside the transit of TRAPPIST-1b from HPF 37- 48 F12.9 --- ratiob [-0.58/0.09] Flux ratio TRAPPIST-1b HPF (in/out-1) 50- 60 F11.9 --- e_ratiob [0.02/9.5] Error in Flux ratio of TRAPPIST-1b -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 23-Nov-2021
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