J/MNRAS/510/4857         WASP-94A light curves                    (Ahrer+, 2022)

LRG-BEASTS: Sodium absorption and Rayleigh scattering in the atmosphere of WASP-94A b using NTT/EFOSC2. Ahrer E., Wheatley P. J., Kirk J., Gandhi S., King G. W., Louden T. <Mon. Not. R. Astron. Soc. 510, 4857-4871 (2022)> =2022MNRAS.510.4857A 2022MNRAS.510.4857A (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Exoplanets ; Spectra, optical Keywords: methods: observational - techniques: spectroscopic - planets and satellites: atmospheres - planets and satellites: individual: WASP-94Ab Abstract: We present an optical transmission spectrum for WASP-94A b, the first atmospheric characterization of this highly-inflated hot Jupiter. The planet has a reported radius of 1.72+0.06-0.05RJup, a mass of only 0.456+0.032-0.036MJup, and an equilibrium temperature of 1508±75K. We observed the planet transit spectroscopically with the EFOSC2 instrument on the ESO New Technology Telescope (NTT) at La Silla, Chile: the first use of NTT/EFOSC2 for transmission spectroscopy. We achieved an average transit-depth precision of 128ppm for bin widths of ∼200Å. This high precision was achieved in part by linking Gaussian Process hyperparameters across all wavelength bins. The resulting transmission spectrum, spanning a wavelength range of 3800-7140Å, exhibits a sodium absorption with a significance of 4.9σ, suggesting a relatively cloud-free atmosphere. The sodium signal may be broadened, with a best-fitting width of 78+67-32Å in contrast to the instrumental resolution of 27.2±0.2Å. We also detect a steep slope in the blue end of the transmission spectrum, indicating the presence of Rayleigh scattering in the atmosphere of WASP-94A b. Retrieval models show evidence for the observed slope to be super-Rayleigh and potential causes are discussed. Finally, we find narrow absorption cores in the CaII H&K lines of WASP-94A, suggesting the star is enshrouded in gas escaping the hot Jupiter. Description: These tables contain the wavelength binned and white-light light curves of the transit of WASP-94Ab observed with the EFOSC2 instrument on the New Technology Telescope (NTT) on the nights of 14 August 2017. Objects: --------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------- 20 55 07.94 -34 08 08.0 WASP-94A = CD-34 14724A --------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file lc.dat 1020 477 Light curves -------------------------------------------------------------------------------- Byte-by-byte Description of file:lc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 20 F20.14 d Time Time in MJD 22- 45 E24.18 --- Flux1 Normalised flux in 220Å-wide bin centred on 3910Å 47- 70 E24.18 --- e_Flux1 Error in flux in 220Å-wide bin centred on 3910Å 72- 95 E24.18 --- Flux2 Normalised flux in 200Å-wide bin centred on 4120Å 97-120 E24.18 --- e_Flux2 Error in flux in 200Å-wide bin centred on 4120Å 122-145 E24.18 --- Flux3 Normalised flux in 200Å-wide bin centred on 4320Å 147-170 E24.18 --- e_Flux3 Error in flux in 200Å-wide bin centred on 4320Å 172-195 E24.18 --- Flux4 Normalised flux in 210Å-wide bin centred on 4525Å 197-220 E24.18 --- e_Flux4 Error in flux in 210Å-wide bin centred on 4525Å 222-245 E24.18 --- Flux5 Normalised flux in 180Å-wide bin centred on 4720Å 247-270 E24.18 --- e_Flux5 Error in flux in 180Å-wide bin centred on 4720Å 272-295 E24.18 --- Flux6 Normalised flux in 170Å-wide bin centred on 4895Å 297-320 E24.18 --- e_Flux6 Error in flux in 170Å-wide bin centred on 4895Å 322-345 E24.18 --- Flux7 Normalised flux in 220Å-wide bin centred on 5090Å 347-370 E24.18 --- e_Flux7 Error in flux in 220Å-wide bin centred on 5090Å 372-395 E24.18 --- Flux8 Normalised flux in 200Å-wide bin centred on 5300Å 397-420 E24.18 --- e_Flux8 Error in flux in 200Å-wide bin centred on 5300Å 422-445 E24.18 --- Flux9 Normalised flux in 210Å-wide bin centred on 5505Å 447-470 E24.18 --- e_Flux9 Error in flux in 210Å-wide bin centred on 5505Å 472-495 E24.18 --- Flux10 Normalised flux in 208Å-wide bin centred on 5714Å 497-520 E24.18 --- e_Flux10 Error in flux in 208Å-wide bin centred on 5714Å 522-545 E24.18 --- Flux11 Normalised flux in 50Å-wide bin centred on 5843Å 547-570 E24.18 --- e_Flux11 Error in flux in 50Å-wide bin centred on 5843Å 572-595 E24.18 --- Flux12 Normalised flux in 50Å-wide bin centred on 5893Å 597-620 E24.18 --- e_Flux12 Error in flux in 50Å-wide bin centred on 5893Å 622-645 E24.18 --- Flux13 Normalised flux in 50Å-wide bin centred on 5943Å 647-670 E24.18 --- e_Flux13 Error in flux in 50Å-wide bin centred on 5943Å 672-695 E24.18 --- Flux14 Normalised flux in 162Å-wide bin centred on 6049Å 697-720 E24.18 --- e_Flux14 Error in flux in 162Å-wide bin centred on 6049Å 722-745 E24.18 --- Flux15 Normalised flux in 210Å-wide bin centred on 6235Å 747-770 E24.18 --- e_Flux15 Error in flux in 210Å-wide bin centred on 6235Å 772-795 E24.18 --- Flux16 Normalised flux in 180Å-wide bin centred on 6430Å 797-820 E24.18 --- e_Flux16 Error in flux in 180Å-wide bin centred on 6430Å 822-845 E24.18 --- Flux17 Normalised flux in 220Å-wide bin centred on 6630Å 847-870 E24.18 --- e_Flux17 Error in flux in 220Å-wide bin centred on 6630Å 872-895 E24.18 --- Flux18 Normalised flux in 200Å-wide bin centred on 6840Å 897-920 E24.18 --- e_Flux18 Error in flux in 200Å-wide bin centred on 6840Å 922-945 E24.18 --- Flux19 Normalised flux in 200Å-wide bin centred on 7040Å 947-970 E24.18 --- e_Flux19 Error in flux in 200Å-wide bin centred on 7040Å 972-995 E24.18 --- FluxWL Normalised white-light flux excluding bin 1 (4020-7140 Å) 997-1020 E24.18 --- e_FluxWL Error in white-light flux excluding bin 1 (4020-7140 Å) -------------------------------------------------------------------------------- Acknowledgements: Eva-Maria Ahrer, eva-maria.ahrer(at)warwick.ac.uk
(End) Patricia Vannier [CDS] 22-Feb-2022
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