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ZENODO
Dataset . 2025
License: CC BY
Data sources: ZENODO
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
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CRIRES+ and CARMENES reduced spectroscopic observations of TOI-2109

Authors: Lavail, Alexis;

CRIRES+ and CARMENES reduced spectroscopic observations of TOI-2109

Abstract

CRIRES+ and CARMENES reduced spectroscopic observations of TOI-2109 This records contains the reduced data as used in the publication of Cont et al. 2025 "Retrieving day- and nightside atmospheric properties of the ultra-hot Jupiter TOI-2109b. Detection of Fe and CO emission lines and evidence for inefficient heat transport" currently in press with Astronomy & Astrophysics and available as preprint on arXiv. Links to the publication: ADS: TBD arXiv: TBD The data reduction steps for CRIRES+ and CARMENES data are explained in sect. 2 of the article Acknowledgements If you make use of this data in your research, please cite the Cont et al. 2025 article and this record with its DOI (10.5281/zenodo.15037659) and its reference, the bibtex reference is: @dataset{lavail_2025_15037659, author = {Lavail, Alexis}, title = {CRIRES+ and CARMENES reduced spectroscopic observations of TOI-2109 }, month = mar, year = 2025, publisher = {Zenodo}, version = {1.0}, doi = {10.5281/zenodo.15037659}, url = {https://doi.org/10.5281/zenodo.15037659},} Note also that ESO requests an acknowledgement, which in this case would be: "Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 113.26GE". This data is released under a Creative Commons Attribution 4.0 International license. CRIRES+ data The CRIRES+ data is following the same format as other records such as https://zenodo.org/records/11637332. The CRIRES+ data files are the following : 240408_TOI2109.pickle 240408_TOI2109_order1.pickle 240409_TOI2109.pickle 240409_TOI2109-order1.pickle 240526_TOI2109.pickle 240526_TOI2109-order1.pickle The standard files for each date are named YYMMDD_TOI2109.pickle. They contain the full spectrum, except the part of the first spectral order on the left-most detector. That wavelength segment is not reduced by default by the pipeline because it is slightly out of the detector on one of the nodding position. We used a custom reduction to be able to reduce this order, and it is contained in the YYMMDD_TOI2109-order1.pickle files. The reduction was done on a restricted fraction of the slit. CARMENES data The CARMENES reduced spectra are in the TOI2109.zip archive. The archive contains a README file (README_TOI2109.txt) explaining the data.

Keywords

Exoplanetology, Astronomy, Spectroscopy

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
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