VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic Pole Article Swipe
K. G. Strassméier
,
M. Weber
,
D. Gruner
,
I. Ilyin
,
M. Steffen
,
M. Baratella
,
S. Järvinen
,
T. Granzer
,
S. A. Barnes
,
T. A. Carroll
,
M. Mallonn
,
D. Sablowski
,
P. Gabor
,
D. Brown
,
C. J. Corbally
,
M. Franz
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2302.01794
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2302.01794
We embarked on a high-resolution optical spectroscopic survey of bright Transiting Exoplanet Survey Satellite (TESS) stars around the Northern Ecliptic Pole (NEP), dubbed the Vatican-Potsdam-NEP (VPNEP) survey. Our NEP coverage comprises 1067 stars, of which 352 are bona fide dwarf stars and 715 are giant stars, all cooler than spectral type F0 and brighter than V=8. m 5. Our aim is to characterize these stars for the benefit of future studies in the community. We analyzed the spectra via comparisons with synthetic spectra. Particular line profiles were analyzed by means of eigen-profiles, equivalent widths, and relative emission-line fluxes (when applicable). Two R=200 000 spectra were obtained for each of the dwarf stars with the Vatican Advanced Technology Telescope (VATT) and the Potsdam Echelle Polarimetric and Spectroscopic Instrument (PEPSI), with typically three R=55 000 spectra obtained for the giant stars with STELLA and the STELLA Echelle Spectrograph (SES). Combined with V-band magnitudes, Gaia eDR3 parallaxes, and isochrones from the Padova and Trieste Stellar Evolutionary Code, the spectra can be used to obtain radial velocities, effective temperatures, gravities, rotational and turbulence broadenings, stellar masses and ages, and abundances for 27 chemical elements, as well as isotope ratios for lithium and carbon, line bisector spans, convective blue-shifts (when feasible), and levels of magnetic activity from Hα, Hβ, and the Ca ii infrared triplet. In this initial paper, we discuss our analysis tools and biases, presenting our first results from a pilot sub-sample of 54 stars (27 bona-fide dwarf stars observed with VATT+PEPSI and 27 bona-fide giant stars observed with STELLA+SES) and making all reduced spectra available to the community.
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Metadata
- Type
- preprint
- Language
- en
- Landing Page
- https://doi.org/10.48550/arxiv.2302.01794
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4319323759
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4319323759Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.48550/arxiv.2302.01794Digital Object Identifier
- Title
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VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic PoleWork title
- Type
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-02-03Full publication date if available
- Authors
-
K. G. Strassméier, M. Weber, D. Gruner, I. Ilyin, M. Steffen, M. Baratella, S. Järvinen, T. Granzer, S. A. Barnes, T. A. Carroll, M. Mallonn, D. Sablowski, P. Gabor, D. Brown, C. J. Corbally, M. FranzList of authors in order
- Landing page
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https://doi.org/10.48550/arxiv.2302.01794Publisher landing page
- Open access
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YesWhether a free full text is available
- OA status
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greenOpen access status per OpenAlex
- OA URL
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https://doi.org/10.48550/arxiv.2302.01794Direct OA link when available
- Concepts
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Ecliptic, Characterization (materials science), Astronomy, Astrobiology, Physics, Geology, Optics, Nuclear physics, Solar wind, PlasmaTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.Survey | 12 |
| abstract_inverted_index.V-band | 149 |
| abstract_inverted_index.around | 16 |
| abstract_inverted_index.bright | 9 |
| abstract_inverted_index.cooler | 47 |
| abstract_inverted_index.dubbed | 22 |
| abstract_inverted_index.fluxes | 97 |
| abstract_inverted_index.future | 69 |
| abstract_inverted_index.levels | 207 |
| abstract_inverted_index.making | 258 |
| abstract_inverted_index.masses | 181 |
| abstract_inverted_index.obtain | 170 |
| abstract_inverted_index.paper, | 223 |
| abstract_inverted_index.radial | 171 |
| abstract_inverted_index.ratios | 194 |
| abstract_inverted_index.spans, | 201 |
| abstract_inverted_index.stars, | 32, 45 |
| abstract_inverted_index.survey | 7 |
| abstract_inverted_index.(VPNEP) | 25 |
| abstract_inverted_index.Echelle | 122, 144 |
| abstract_inverted_index.Potsdam | 121 |
| abstract_inverted_index.Stellar | 161 |
| abstract_inverted_index.Trieste | 160 |
| abstract_inverted_index.Vatican | 114 |
| abstract_inverted_index.benefit | 67 |
| abstract_inverted_index.biases, | 230 |
| abstract_inverted_index.carbon, | 198 |
| abstract_inverted_index.discuss | 225 |
| abstract_inverted_index.initial | 222 |
| abstract_inverted_index.isotope | 193 |
| abstract_inverted_index.lithium | 196 |
| abstract_inverted_index.optical | 5 |
| abstract_inverted_index.reduced | 260 |
| abstract_inverted_index.results | 234 |
| abstract_inverted_index.spectra | 77, 103, 133, 165, 261 |
| abstract_inverted_index.stellar | 180 |
| abstract_inverted_index.studies | 70 |
| abstract_inverted_index.survey. | 26 |
| abstract_inverted_index.widths, | 93 |
| abstract_inverted_index.(PEPSI), | 127 |
| abstract_inverted_index.Advanced | 115 |
| abstract_inverted_index.Combined | 147 |
| abstract_inverted_index.Ecliptic | 19 |
| abstract_inverted_index.Northern | 18 |
| abstract_inverted_index.activity | 210 |
| abstract_inverted_index.analysis | 227 |
| abstract_inverted_index.analyzed | 75, 87 |
| abstract_inverted_index.bisector | 200 |
| abstract_inverted_index.brighter | 53 |
| abstract_inverted_index.chemical | 188 |
| abstract_inverted_index.coverage | 29 |
| abstract_inverted_index.embarked | 1 |
| abstract_inverted_index.infrared | 218 |
| abstract_inverted_index.magnetic | 209 |
| abstract_inverted_index.observed | 246, 254 |
| abstract_inverted_index.obtained | 105, 134 |
| abstract_inverted_index.profiles | 85 |
| abstract_inverted_index.relative | 95 |
| abstract_inverted_index.spectra. | 82 |
| abstract_inverted_index.spectral | 49 |
| abstract_inverted_index.triplet. | 219 |
| abstract_inverted_index.Exoplanet | 11 |
| abstract_inverted_index.Satellite | 13 |
| abstract_inverted_index.Telescope | 117 |
| abstract_inverted_index.available | 262 |
| abstract_inverted_index.bona-fide | 243, 251 |
| abstract_inverted_index.comprises | 30 |
| abstract_inverted_index.effective | 173 |
| abstract_inverted_index.elements, | 189 |
| abstract_inverted_index.synthetic | 81 |
| abstract_inverted_index.typically | 129 |
| abstract_inverted_index.Instrument | 126 |
| abstract_inverted_index.Particular | 83 |
| abstract_inverted_index.Technology | 116 |
| abstract_inverted_index.Transiting | 10 |
| abstract_inverted_index.VATT+PEPSI | 248 |
| abstract_inverted_index.abundances | 185 |
| abstract_inverted_index.community. | 73, 265 |
| abstract_inverted_index.convective | 202 |
| abstract_inverted_index.equivalent | 92 |
| abstract_inverted_index.feasible), | 205 |
| abstract_inverted_index.gravities, | 175 |
| abstract_inverted_index.isochrones | 155 |
| abstract_inverted_index.presenting | 231 |
| abstract_inverted_index.rotational | 176 |
| abstract_inverted_index.sub-sample | 238 |
| abstract_inverted_index.turbulence | 178 |
| abstract_inverted_index.STELLA+SES) | 256 |
| abstract_inverted_index.blue-shifts | 203 |
| abstract_inverted_index.comparisons | 79 |
| abstract_inverted_index.magnitudes, | 150 |
| abstract_inverted_index.parallaxes, | 153 |
| abstract_inverted_index.velocities, | 172 |
| abstract_inverted_index.Evolutionary | 162 |
| abstract_inverted_index.Polarimetric | 123 |
| abstract_inverted_index.Spectrograph | 145 |
| abstract_inverted_index.applicable). | 99 |
| abstract_inverted_index.broadenings, | 179 |
| abstract_inverted_index.characterize | 62 |
| abstract_inverted_index.Spectroscopic | 125 |
| abstract_inverted_index.emission-line | 96 |
| abstract_inverted_index.spectroscopic | 6 |
| abstract_inverted_index.temperatures, | 174 |
| abstract_inverted_index.eigen-profiles, | 91 |
| abstract_inverted_index.high-resolution | 4 |
| abstract_inverted_index.Vatican-Potsdam-NEP | 24 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 16 |
| citation_normalized_percentile.value | 0.01482372 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |