The High-energy Spectrum of the Young Planet Host V1298 Tau

V1298 Tau is a young pre-main-sequence star hosting four known exoplanets that are prime targets for transmission spectroscopy with current-generation instruments. This work pieces together observations from the NICER X-ray telescope, the Space Telescope Imaging Spectrograph and Cosmic Origins Spect...

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Main Authors: Girish M. Duvvuri, P. Wilson Cauley, Fernando Cruz Aguirre, Roy Kilgard, Kevin France, Zachory K. Berta-Thompson, J. Sebastian Pineda
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/acfa74
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author Girish M. Duvvuri
P. Wilson Cauley
Fernando Cruz Aguirre
Roy Kilgard
Kevin France
Zachory K. Berta-Thompson
J. Sebastian Pineda
author_facet Girish M. Duvvuri
P. Wilson Cauley
Fernando Cruz Aguirre
Roy Kilgard
Kevin France
Zachory K. Berta-Thompson
J. Sebastian Pineda
author_sort Girish M. Duvvuri
collection DOAJ
description V1298 Tau is a young pre-main-sequence star hosting four known exoplanets that are prime targets for transmission spectroscopy with current-generation instruments. This work pieces together observations from the NICER X-ray telescope, the Space Telescope Imaging Spectrograph and Cosmic Origins Spectrograph instruments aboard Hubble Space Telescope, and empirically informed models to create a panchromatic spectral energy distribution for V1298 Tau spanning 1–10 ^5 Å. We describe the methods and assumptions used to assemble the panchromatic spectrum and show that despite this star’s brightness, its high-energy spectrum is near the limit of present X-ray and ultraviolet observatories’ abilities to characterize. We conclude by using the V1298 Tau spectrum as a benchmark for the activity saturation stage of high-energy radiation from solar-mass stars to compare the lifetime cumulative high-energy irradiation of the V1298 Tau planets to other planets orbiting similarly massive stars.
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spelling doaj.art-93aa134c36db4c4ab53ca52ae6fd47542023-10-16T12:42:15ZengIOP PublishingThe Astronomical Journal1538-38812023-01-01166519610.3847/1538-3881/acfa74The High-energy Spectrum of the Young Planet Host V1298 TauGirish M. Duvvuri0https://orcid.org/0000-0002-7119-2543P. Wilson Cauley1https://orcid.org/0000-0001-9207-0564Fernando Cruz Aguirre2https://orcid.org/0000-0003-4628-8524Roy Kilgard3Kevin France4https://orcid.org/0000-0002-1002-3674Zachory K. Berta-Thompson5https://orcid.org/0000-0002-3321-4924J. Sebastian Pineda6https://orcid.org/0000-0002-4489-0135Department of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO 80309, USA ; girish.duvvuri@colorado.edu; Center for Astrophysics and Space Astronomy, University of Colorado , 593 UCB, Boulder, CO 80309, USA; Laboratory for Atmospheric and Space Physics, University of Colorado , 600 UCB, Boulder, CO 80309, USA; Department of Physics and Astronomy, Vanderbilt University , Nashville, TN 37235, USALaboratory for Atmospheric and Space Physics, University of Colorado , 600 UCB, Boulder, CO 80309, USADepartment of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO 80309, USA ; girish.duvvuri@colorado.edu; Laboratory for Atmospheric and Space Physics, University of Colorado , 600 UCB, Boulder, CO 80309, USA; The University of Iowa , Department of Physics & Astronomy, Van Allen Hall, Iowa City, IA 52242, USAAstronomy Department, Wesleyan University , Middletown, CT 06459, USADepartment of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO 80309, USA ; girish.duvvuri@colorado.edu; Center for Astrophysics and Space Astronomy, University of Colorado , 593 UCB, Boulder, CO 80309, USA; Laboratory for Atmospheric and Space Physics, University of Colorado , 600 UCB, Boulder, CO 80309, USADepartment of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO 80309, USA ; girish.duvvuri@colorado.edu; Center for Astrophysics and Space Astronomy, University of Colorado , 593 UCB, Boulder, CO 80309, USALaboratory for Atmospheric and Space Physics, University of Colorado , 600 UCB, Boulder, CO 80309, USAV1298 Tau is a young pre-main-sequence star hosting four known exoplanets that are prime targets for transmission spectroscopy with current-generation instruments. This work pieces together observations from the NICER X-ray telescope, the Space Telescope Imaging Spectrograph and Cosmic Origins Spectrograph instruments aboard Hubble Space Telescope, and empirically informed models to create a panchromatic spectral energy distribution for V1298 Tau spanning 1–10 ^5 Å. We describe the methods and assumptions used to assemble the panchromatic spectrum and show that despite this star’s brightness, its high-energy spectrum is near the limit of present X-ray and ultraviolet observatories’ abilities to characterize. We conclude by using the V1298 Tau spectrum as a benchmark for the activity saturation stage of high-energy radiation from solar-mass stars to compare the lifetime cumulative high-energy irradiation of the V1298 Tau planets to other planets orbiting similarly massive stars.https://doi.org/10.3847/1538-3881/acfa74Pre-main sequence starsX-ray astronomyUltraviolet astronomyStellar atmospheresStellar chromospheresStellar coronae
spellingShingle Girish M. Duvvuri
P. Wilson Cauley
Fernando Cruz Aguirre
Roy Kilgard
Kevin France
Zachory K. Berta-Thompson
J. Sebastian Pineda
The High-energy Spectrum of the Young Planet Host V1298 Tau
The Astronomical Journal
Pre-main sequence stars
X-ray astronomy
Ultraviolet astronomy
Stellar atmospheres
Stellar chromospheres
Stellar coronae
title The High-energy Spectrum of the Young Planet Host V1298 Tau
title_full The High-energy Spectrum of the Young Planet Host V1298 Tau
title_fullStr The High-energy Spectrum of the Young Planet Host V1298 Tau
title_full_unstemmed The High-energy Spectrum of the Young Planet Host V1298 Tau
title_short The High-energy Spectrum of the Young Planet Host V1298 Tau
title_sort high energy spectrum of the young planet host v1298 tau
topic Pre-main sequence stars
X-ray astronomy
Ultraviolet astronomy
Stellar atmospheres
Stellar chromospheres
Stellar coronae
url https://doi.org/10.3847/1538-3881/acfa74
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