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Dataset of "Activity-stability relationship in magnetron co-sputtered bimetallic catalysts for proton exchange membrane fuel cells"
<p>In the present study, magnetron sputtered PtxM100-x (M = Co, Cu, Y; x = 25, 50, 75 and 100) bimetallic alloys were investigated as PEMFC cathodes. Accurate composition control enabled a systematic study of the correlation between alloy composition, activity, and stability. The catalysts underwent thorough characterization, employing a diverse portfolio of characterization techniques such as scanning electron microscopy, energy-dispersive X-ray spectroscopy, X-ray photoelectron spectroscopy and cyclic voltammetry. The activity of all investigated alloys was tested directly in a fuel cell device, while stability was assessed through potentiodynamic cycling in a half-cell. <br>The activity-stability index, considering experimental results for both activity and stability, was calculated and compared for all investigated catalysts. All alloys exhibited a volcano-type trend in activity-stability index as a function of the concentration of alloying element with peaks observed at Pt50Co50, Pt50Cu50 and Pt75Y25 for respective alloys, surpassing that of monometallic platinum. Overall, Pt50Co50 emerged as a catalyst with the highest activity-stability ratio.</p>
Geoarchaeological dataset for the hinterland of Ravenna
<p><strong>Geoarchaeological dataset with 8798 archaeological sites and geological layers and known extent of 591 archaeological sites collected for the hinterland of Ravenna, Italy.</strong></p> <p>The dataset includes:</p> <ul> <li><em>Ravenna_hinterland_geoarchaeological_data.csv</em> = text file with the full geoarchaeological dataset</li> <li><em>Ravenna_hinterland_geoarchaeological_data.gpkg</em> = vector file with the full geoarchaeological dataset</li> <li><em>Ravenna_hinterland_geoarchaeological_site.gpkg</em> = vector file with archaeological sites extent</li> <li><em>Ravenna_hinterland_geoarchaeological_data_metadata.txt = </em>text file with metadata of geoarchaeological dataset</li> <li><em>Ravenna_hinterland_geoarchaeological_dataset_bibliography.odt </em>= text file with bibliographical references of geoarchaeological dataset</li> <li><em>Ravenna_hinterland_geoarchaeological_dataset_archaeological_reports.odt</em> = reference file with the list of unpublished archaeological reports collected from SABAP-RA and SABAP-BO</li> <li><em>Ravenna_hinterland_geoarchaeological_dataset_archaeological_reports.bib</em> = reference file with the list of unpublished archaeological reports collected from SABAP-RA and SABAP-BO</li> <li><em>Ravenna_hinterland_geoarchaeological_dataset_geological_reports.bib</em> = reference file with the list of raw geological reports from SGSS available online</li> </ul> <p> </p> <p>-------------------------------------------------------------------------------</p> <p>SABAP-RA = Soprintendenza Archeologia, Belle Arti e Paesaggio per le province di Ravenna, Forlì-Cesena e Rimini</p> <p>SABAP-BO = Soprintendenza Archeologia belle arti e paesaggio per la città metropolitana di Bologna e le province di Modena, Reggio Emilia e Ferrara</p> <p>SGSS = Servizio Geologico Sismico e dei Suoli, Regione Emilia-Romagna</p>
FULFILL dataset - diet policy acceptability - efficacy and acceptability framing Denmark
<p>This dataset represents survey data on sufficiency-oriented policy acceptability in regard to dietary consumption. The study was part of the second round surveys in Denmark in 2023 within the FULFILL project - Fundamental Decarbonisation Through Sufficiency By Lifestyle Changes.</p> <p>As part of Work Package 3 (WP3) in the FULFILL project, we collected quantitative data from two countries: Denmark and Germany, with representative sampling (age, income, gender, current region). In this survey on the acceptability of sufficiency-oriented diet policies we recruited a representative sample with approximately 800 participants from Denmark and Germany, taking into account primarily the individual perspective, added by some questions on the household level.</p> <p>The central part of the survey includes a framing experiment including three groups with participants being randomly assigned to. We were interested in peoples' acceptability on three majorly discussed and sufficiency-relevant policies, i.e. meat tax, carbon label or meat-free day at public canteens. We investigated if an information on either the efficacy of the measures or a combination of information with acceptance information or none of these information could influence people's acceptability (overall, self vs. others perspective). We measured several control variables (socio-economics such as age, gender, income, education, household size, life stage, ideological measures such as political orientation or attitudinal measures such as sufficiency orientation and climate change denial). A quantitative assessment of the carbon footprint in the food consumption domain was also included.</p>
FULFILL dataset round 2 Delhi and Mumbai (India)
<p>This dataset and codebook correspond to the second round of survey data gathered in Delhi and Mumbai (India) in 2024, within the project FULFILL - Fundamental Decarbonisation Through Sufficiency By Lifestyle Changes. </p> <p>As part of Work Package 3 (WP3) in the FULFILL project, we collected quantitative data from six countries: Denmark, France, Germany, Italy, Latvia, and India. The first round of the survey, consisted of recruiting a representative sample of approximately 2000 households in each country. In this second survey round, we recruit around 1000 respondents from the initial survey round, ensuring representativity is maintained.</p> <p>In order to consider sufficiency-oriented lifestyles not only in Europe but also in the Global South, we conducted a similar survey in India. More specifically, we adjusted the survey to fit the context (e.g., including cooling) and, due to the large size and diversity within India, we focused data collection on two Mega Cities (>10Mio inhabitants), namely Mumbai and Delhi. Due to the different cultural context and in exchange with Indian researchers and the supporting market research institute, we decided to change the methodology for data collection from an online survey to face-to-face interviews. The survey includes a quantitative assessment of the carbon footprint in various domains of life, such as housing, mobility, and diet. In addition to this, the survey also measures socio-economic factors such as age, gender, income, education, household size, life stage, and political orientation. Furthermore, the survey includes measures of quality of life, encompassing aspects such as health and well-being, environmental quality, financial security, and comfort.</p>
Dataset of "Molecular dynamics of evaporative cooling of water clusters"
<p>The cooling of water clusters through evaporation into a vacuum is studied using classical molecular dynamics with the SPC water model, and the results are compared with semimacroscopic theory. A model based on the Hertz–Knudsen equation underestimates the cooling rates. A modified approach, which accounts for the Kelvin equation, provides better results. While the rotational temperature of the clusters is in equilibrium with their internal temperature, the translational temperature of the clusters “as individual particles” remains unchanged.</p>
CLDF dataset of the Enggano word list from 1895 in Stokhof and Almanar's (1987) Holle List
<p>The repository for the digitised Enggano word list from 1895 (see Stokhof and Almanar 1987 for the original source) that has been matched with the <a href="https://engganolang.github.io/digitised-holle-list/">digitised Holle List</a> (Rajeg 2023a; cf. Stokhof 1980), providing the English and Indonesian glosses for the Enggano forms. The data set <a href="https://github.com/engganolang/holle-list-enggano-1895/actions/workflows/cldf-validation.yml">conforms</a> to the Wordlist module of the Cross-Linguistic Data Format (<a href="https://cldf.clld.org/">CLDF</a>) (Forkel et al. 2018).</p> <p><em>The work in this repository is part of the <a href="https://gtr.ukri.org/project/8AB0C3DC-F1C9-4CFA-BB4D-5BE748213372">AHRC-funded research</a> on <strong>Lexical resources for Enggano, a threatened language of Indonesia</strong> (visit the <a href="https://enggano.ling-phil.ox.ac.uk/">central webpage of the Enggano research</a> and the specific repository of the <a href="https://portal.sds.ox.ac.uk/Lexical_resources_for_Enggano">Lexical Resources for Enggano</a> project as well the <a href="https://portal.sds.ox.ac.uk/Enggano/groups">main Enggano repository</a> on the University of Oxford's Sustainable Digital Scholarship (SDS))</em></p> <h1>Updates in version 2.0.0</h1> <p>The following items summarise the major updates in version 2.0.0:</p> <ul> <li> <p><strong>Adding <a href="https://github.com/engganolang/holle-list-enggano-1895/blob/main/cldf/media.csv">MediaTable</a></strong> to accommodate <a href="https://github.com/engganolang/holle-list-enggano-1895/tree/main/img">images</a> in/for note ID <26> (commits <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/dab95401f128bd4203a81294f2e9f4620d45b145">dab9540</a> & <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/a0040038e2577cb37ff8ad3ac68e8bbdedc26291">a004003</a> <a href="https://github.com/engganolang/holle-list-enggano-1895/blob/a0040038e2577cb37ff8ad3ac68e8bbdedc26291/code/Enggano-Holle-List-with-NBL.R#L229-L232">at this line</a> and <a href="https://github.com/engganolang/holle-list-enggano-1895/blob/2aab3ab385fc82c0613de2aacb5947ca4981b417/code/Enggano-Holle-List-with-NBL.R#L370-L397">these lines</a>)</p> </li> <li> <p><strong>Splitting multiple forms in a cell</strong> into their own rows, both for the original list and the forms in the Notes (commit <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/39cdc663843b265aa8f3c5bbdcb11628fcc17b5e">39cdc66</a> at <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/39cdc663843b265aa8f3c5bbdcb11628fcc17b5e#diff-ac46f8a3edb85868970d77f55bb86c5f0449feb25c37295895c4a9e560564301R83">this line</a> and <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/39cdc663843b265aa8f3c5bbdcb11628fcc17b5e#diff-ac46f8a3edb85868970d77f55bb86c5f0449feb25c37295895c4a9e560564301R83">this line</a>, and commit <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/a0040038e2577cb37ff8ad3ac68e8bbdedc26291">a004003</a> at <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/a0040038e2577cb37ff8ad3ac68e8bbdedc26291#diff-5b59e4a74b953f80c8867a60c422bd8405c9d6236bd61239a0d3f20b0d582b78R69">this line</a>)</p> </li> <li> <p><strong>Orthography transliteration</strong> into Enggano's common orthography and IPA (across several commits and [closed] issues [#1 #3 #4 #5 #7], but see <a href="https://github.com/engganolang/holle-list-enggano-1895/blob/2aab3ab385fc82c0613de2aacb5947ca4981b417/code/Enggano-Holle-List-with-NBL.R#L32-L93">these lines</a> for retrieving the existing orthography profile and doing the editing, and <a href="https://github.com/engganolang/holle-list-enggano-1895/blob/2aab3ab385fc82c0613de2aacb5947ca4981b417/code/Enggano-Holle-List-with-NBL.R#L220-L306">these lines</a> for running the transliteration using the <a href="https://cran.r-project.org/web/packages/qlcData/index.html">qlcData</a> R package [Moran & Cysouw 2018; Cysouw 2024])</p> <ul> <li>In the <a href="https://github.com/engganolang/holle-list-enggano-1895/blob/main/cldf/forms.csv">FormTable</a>, the <code>Form</code> column contains the Enggano forms in their common orthography; the <code>Value</code> column contains their original transcription/orthography, with their tokenised/segmented formats available under the <code>Graphemes</code> column; the <code>Segments</code> column, finally, contains the segmented IPA transliteration of the Enggano forms (cf. #6 ). The <code>Comment</code> column is derived from the contents of the Notes. It includes, if any, Enggano forms in their original transcription followed by their segmented/tokenised forms in IPA in square brackets, their glosses in English (<strong>EN</strong>) and/or Indonesian (<strong>ID</strong>) inside the bracket, and finally the ID of the Notes in the original document inside angular brackets. The <code>English</code> and <code>Indonesian</code> columns respectively are glosses of the given language from the master/main Holle List (Stokhof 1980) that has been digitised (Rajeg 2023a).</li> <li>The output files of the orthography profiling and transliteration (commit <a href="https://github.com/engganolang/holle-list-enggano-1895/commit/2aab3ab385fc82c0613de2aacb5947ca4981b417">2aab3ab</a>) are available in <a href="https://github.com/engganolang/holle-list-enggano-1895/tree/main/data-raw">data-raw</a> with the file names prefixed with <code>ortho-...</code>.</li> </ul> </li> </ul> <h2>References</h2> <p>Cysouw, Michael. 2024. qlcData: Processing Data for Quantitative Language Comparison. https://cran.r-project.org/web/packages/qlcData/index.html. (25 December, 2024). Version 0.3</p> <p>Forkel, Robert, Johann-Mattis List, Simon J. Greenhill, Christoph Rzymski, Sebastian Bank, Michael Cysouw, Harald Hammarström, Martin Haspelmath, Gereon A. Kaiping & Russell D. Gray. 2018. Cross-Linguistic Data Formats, advancing data sharing and re-use in comparative linguistics. Scientific Data. Nature Publishing Group 5(1). 180205. https://doi.org/10.1038/sdata.2018.205.</p> <p>Moran, Steven & Michael Cysouw. 2018. The Unicode cookbook for linguists: Managing writing systems using orthography profiles (Translation and Multilingual Natural Language Processing 10). Berlin: Language Science Press. https://doi.org/10.5281/zenodo.1296780.</p> <p>Rajeg, Gede Primahadi Wijaya. 2023a. Digitised, Searchable Holle List in Stokhof (1980) [Data set]. (1.3.0). Zenodo. https://doi.org/10.5281/ZENODO.7972273. https://engganolang.github.io/digitised-holle-list/. https://ora.ox.ac.uk/objects/uuid:a511951b-86fb-4019-94d4-280efa83de02</p> <p>Rajeg, Gede Primahadi Wijaya. 2023b. CLDF dataset of the Enggano word list from 1895 in Stokhof and Almanar's (1987) Holle List [Data set]. https://github.com/engganolang/holle-list-enggano-1895 https://doi.org/10.25446/oxford.23515788</p> <p>Stokhof, W. A. L., ed. 1980. Holle Lists, Vocabularies in Languages of Indonesia, Vol. 1: Introductory Volume. Vol. Materials in Languages of Indonesia. Canberra, A.C.T., Australia: Dept. of Linguistics, Research School of Pacific Studies, The Australian National University. https://core.ac.uk/reader/159464813.</p> <p>Stokhof, W. A. L., and Alma E. Almanar. 1987. Holle Lists, Vocabularies in Languages of Indonesia, Vol. 10/3: Islands Off the West Coast of Sumatra. Vol. Materials in Languages of Indonesia. Pacific Linguistics (Series d) 76. Canberra, A.C.T., Australia: Dept. of Linguistics, Research School of Pacific Studies, The Australian National University. http://hdl.handle.net/1885/144589.</p>
Dataset of "MoO3-xNiMoO4 nanorods synthetized using NiO nanoparticles for hydrogen evolution in anion exchange membrane water electrolysis"
<p>Novel method of Mo-Ni catalyst for hydrogen evolution reaction in anion exchange membrane water electrolysis was used. Complete physico-chemical and electrochemical characterization was done. Prepared material showed enhanced performance when compared to the similar Ni based materials. Physico-chemical characterization showed, that final material is formed by NiMoO4 nanorods coverd on the surface by the layer of the MoO3-x.</p>
Permafrost Thaw Settlement Dataset
<p>The Permafrost Thaw Settlement Dataset comprises four data files containing measurements, properties and derived parameters related to permafrost thaw settlement tests. This dataset is intended to support research on mechanical properties of permafrost, particularly in understanding the relationship between soil properties and thaw settlement behavior.</p> <h3><strong>Data Paper Reference</strong></h3> <p>A detailed description of the dataset, including methodology, data sources, and analysis, is provided in the accompanying data paper submitted to <em>Earth System Science Data</em>:</p> <div> <div>Mohammadi, Z., Hayley, J.L., 2025. Compilation and Analysis of Thaw Settlement Test Results: Implications for Prediction Tools and Stress-Strain Characterization in Permafrost. <a href="https://doi.org/10.5194/essd-2024-514">https://doi.org/10.5194/essd-2024-514</a></div> </div> <p>An <strong>updated GitHub repository</strong> containing fully reproducible R code and figures: → <a href="https://github.com/Zucchii/ThawSettlement_DataPaper/releases/tag/essd-pts-final">https://github.com/Zucchii/ThawSettlement_DataPaper/releases/tag/essd-pts-final</a></p> <p> </p> <p>The GitHub repository includes:</p> <ul> <li> <p>R scripts for data processing, analysis, and figure generation</p> </li> <li> <p>Pre-generated figures and processed datasets for convenience</p> </li> <li> <p>Detailed instructions for reproducing all results</p> </li> </ul>
Probabilistic-deterministic storm surge return level dataset for the Bengal delta
<p>Bengal delta shoreline, spanning Bangladesh and India, gets hit every 3 years on average by a major tropical cyclone. Although their occurrence is relatively moderate compared to other tropical regions (accounting for only 5% of global cyclones), the impact of these events is major, accounting for 50% of the victims recorded worldwide. This is due to the very low topography of the delta above sea level (less than 5 meters), high storm surge induced water level and flooding, combined with the high density of the vulnerable population. </p> <p>On one hand, the unavailability of long-term reliable water level data on a sparse tide-gauge network along the coastline has hindered the assessment of storm surge hazards. The application of hydrodynamic modelling to fill the data gap also suffers from the unavailability of a reliable long-term storm dataset over the region. The complex topography of the Bengal delta, with defence structures, and a dense network of rivers presents another modelling challenge. Finally, the interaction of tide, surge and wave further complicate the numerical complexity, needing a coupled modelling framework. </p> <p>Thanks to advancements made to acquire high-quality regional nearshore bathymetry and topography (Krien et al. 2016, Khan et al. 2019), as well as coupled storm surge modelling (Krien et al. 2017, Khan et al. 2021), the tidal and storm surge dynamics over the Bengal delta is now well captured by recent high-resolution coupled SCHISM-WWM Bay of Bengal model (Khan et al. 2021). To estimate the risk of storm surge and associated flooding across the Bengal delta, we have integrated the wave-coupled hydrodynamic model of Khan et al. (2021) for a large ensemble (~3600 cyclones, ~5000 years of storm activity) of synthetic cyclones generated through the statistical-deterministic method of Emanuel (2006). Our storm and surge ensemble covers the whole range of natural variability of storm frequency, size, intensity and track location, with a dense spatial distribution. The interactions among the tide, surge, and waves are modelled explicitly at high spatial resolution. The storm surge-induced water level at various return periods, up to 500 years, is then determined at high spatial resolution (250m at the coast) using a ranking-based technique.</p> <p>The dataset distributed here represents the storm surge water level estimate (e.g. total water level from the tide, surge, and wave computed dynamically through the model) at 25 to 500 year return period (25-year step). The corresponding variable in the self-describing netCDF data file is 'maxelev'. The estimated storm surge water level values are interpolated in a 30" (~1km at the equator) structured grid over the Bengal delta from the original unstructured-grid model outputs (250m resolution at the coast). </p> <p>This dataset is a part of a manuscript, currently being submitted to Natural Hazards and Earth System Sciences (https://nhess.copernicus.org/). Please cite the original paper, along with the dataset if used in your work as - Khan, M. J. U., Durand, F., Emanuel, K., Krien, Y., Testut, L., and Islam, A. K. M. S.: Storm surge hazard over Bengal delta: A probabilistic-deterministic modelling approach, Nat. Hazards Earth Syst. Sci. Discuss. [preprint], https://doi.org/10.5194/nhess-2021-329, in review, 2021.</p>
WageIndicator Collective Agreements Database Dataset with Full Texts and Selected Clauses
<p>Since 2012, the <a href="https://wageindicator.org/">WageIndicator Foundation</a> has maintained a <a href="https://wageindicator.org/cbadatabase">Collective Agreements Database</a>, where the texts of 1600 collective agreements (CBAs) from 61 countries and in 27 languages have been uploaded, coded and annotated. This database is a unique example at global level: collective agreements are documents containing conditions of employment that result from negotiations between independent unions and employers, and their content is often surrounded by an atmosphere of secrecy. Under the <a href="https://sshopencloud.eu/">SSHOC project</a> and with the support of the <a href="https://www.clarin.eu/">CLARIN Research Infrastructure</a>, the agreements have been manually and automatically annotated on several levels: for each agreement, the team answers a series of questions and selects the appropriate piece of text (clause) for each. </p> <p>One of the results of the collective agreements' annotation process is the dataset which is available here and includes all the clauses selected for each variable (WageIndicator_CBADatabase_Selected_Clauses). The full collective agreements' texts are stored in another dataset, also available here (WageIndicator_CBADatabase_Full_Texts_211019). A codebook is also included (210125-wageindicator-cba-codebook.pdf).</p>
The MoLLIST dataset for 16O1H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/OH/16O-1H/MoLLIST.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check OH_16O1H_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>16O-1H__MoLLIST.def</strong>[5.59 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/OH/16O-1H/MoLLIST/">https://exomol.com/models/OH/16O-1H/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>16O-1H__MoLLIST.trans.bz2</strong>[584.47 KB]<br>MoLLIST (16O)(1H) line list: Transition file, compiled by Yixin Wang</p> <p><strong>16O-1H__MoLLIST.states.bz2</strong>[16.51 KB]<br>MoLLIST (16O)(1H) line list: States, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 1. Brooke, J. S. A., Bernath, P. F., Western, C. M., Sneden, C., Afşar, M., Li, G., Gordon, I. E., "Line strengths of rovibrational and rotational transitions in the Χ2Π ground state of OH", Journal of Quantitative Spectroscopy and Radiative Transfer 138, 142-157 (2016). <a href="[http://dx.doi.org/10.1016/j.jqsrt.2015.07.021]">[http://dx.doi.org/10.1016/j.jqsrt.2015.07.021]</a>[16BrBeWe.OH]<br> 2. Yousefi, M., Bernath, P. F., Hodges, J., Masseron, T., "A new line list for the A2 S - X2 electronic transition of OH", Journal of Quantitative Spectroscopy & Radiative Transfer 217, 416-424 (2018). <a href="[https://doi.org/10.1016/j.jqsrt.2018.06.016]">[https://doi.org/10.1016/j.jqsrt.2018.06.016]</a><br> 3. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br></p> </blockquote> <strong>MoLLIST: partition function</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>16O-1H__MoLLIST.pf</strong>[122.07 KB]<br>MoLLIST (16O)(1H) line list: Partition function, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 1. Yousefi, M., Bernath, P. F., Hodges, J., Masseron, T., "A new line list for the A2 S - X2 electronic transition of OH", Journal of Quantitative Spectroscopy & Radiative Transfer 217, 416-424 (2018). <a href="[https://doi.org/10.1016/j.jqsrt.2018.06.016]">[https://doi.org/10.1016/j.jqsrt.2018.06.016]</a><br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>16O-1H__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[437.21 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (16O)(1H) line list.</p> <p><strong>16O-1H__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (16O)(1H) line list.</p> <p><strong>16O-1H__MoLLIST.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: MoLLIST (16O)(1H) line list.</p> <p><strong>16O-1H__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (16O)(1H) line list.</p> <p><strong>References:</strong><br> 1. Brooke, J. S. A., Bernath, P. F., Western, C. M., Sneden, C., Afşar, M., Li, G., Gordon, I. E., "Line strengths of rovibrational and rotational transitions in the Χ2Π ground state of OH", Journal of Quantitative Spectroscopy and Radiative Transfer 138, 142-157 (2016). <a href="[http://dx.doi.org/10.1016/j.jqsrt.2015.07.021]">[http://dx.doi.org/10.1016/j.jqsrt.2015.07.021]</a>[16BrBeWe.OH]<br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 3. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The LaTY dataset for 31P1H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/PH/31P-1H/LaTY.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check PH_31P1H_LaTY.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>31P-1H__LaTY.def</strong>[5.97 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/PH/31P-1H/LaTY/">https://exomol.com/models/PH/31P-1H/LaTY/</a><br></p> </blockquote> <strong>LaTY: line list</strong> <p><em>An empirical line list for PH covering the ground and 1st exited electronic states</em><br></p> <blockquote> <p><strong>31P-1H__LaTY.states</strong>[204.91 KB]<br>LaTY (31P)(1H) line list States file.</p> <p><strong>31P-1H__LaTY.trans</strong>[3.59 MB]<br>LaTY (31P)(1H) line list Transition file.</p> <p><strong>References:</strong><br> 1. Langleben, J., Tennyson, J., Yurchenko, S. N., Bernath, P., "ExoMol line list – XXXIV. A rovibrational line list for phosphinidene (PH) in its X 3Σ− and a 1Δ electronic states", Monthly Notices of the Royal Astronomical Society 488, 2332-2342 (2019). <a href="[https://doi.org/10.1093/mnras/stz1856]">[https://doi.org/10.1093/mnras/stz1856]</a>[19LaTeYu.PH]<br></p> </blockquote> <strong>LaTY: partition function</strong> <p><em>An empirical line list for PH covering the ground and 1st exited electronic states</em><br></p> <blockquote> <p><strong>31P-1H__LaTY.pf</strong>[97.66 KB]<br>LaTY (31P)(1H) line list Partition Function.</p> <p><strong>References:</strong><br> 1. Langleben, J., Tennyson, J., Yurchenko, S. N., Bernath, P., "ExoMol line list – XXXIV. A rovibrational line list for phosphinidene (PH) in its X 3Σ− and a 1Δ electronic states", Monthly Notices of the Royal Astronomical Society 488, 2332-2342 (2019). <a href="[https://doi.org/10.1093/mnras/stz1856]">[https://doi.org/10.1093/mnras/stz1856]</a>[19LaTeYu.PH]<br></p> </blockquote> <strong>LaTY: opacity</strong> <p><em>An empirical line list for PH covering the ground and 1st exited electronic states</em><br></p> <blockquote> <p><strong>31P-1H__LaTY.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[420.52 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): LaTY (31P)(1H) line list.</p> <p><strong>31P-1H__LaTY.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: LaTY (31P)(1H) line list.</p> <p><strong>31P-1H__LaTY.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: LaTY (31P)(1H) line list.</p> <p><strong>31P-1H__LaTY.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: LaTY (31P)(1H) line list.</p> <p><strong>References:</strong><br> 1. Langleben, J., Tennyson, J., Yurchenko, S. N., Bernath, P., "ExoMol line list – XXXIV. A rovibrational line list for phosphinidene (PH) in its X 3Σ− and a 1Δ electronic states", Monthly Notices of the Royal Astronomical Society 488, 2332-2342 (2019). <a href="[https://doi.org/10.1093/mnras/stz1856]">[https://doi.org/10.1093/mnras/stz1856]</a>[19LaTeYu.PH]<br> 2. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The MoLLIST dataset for 14N1H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/NH/14N-1H/MoLLIST.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check NH_14N1H_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>14N-1H__MoLLIST.def</strong>[6.0 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/NH/14N-1H/MoLLIST/">https://exomol.com/models/NH/14N-1H/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>14N-1H__MoLLIST.trans.bz2</strong>[236.11 KB]<br>MoLLIST (14N)(1H) line list: Transition file. The data are from Brooke et al (2015), http://dx.doi.org/10.1063/1.4923422, converted to ExoMol by Geronimo Villanueva (NASA/GSFC) Feb/2019.</p> <p><strong>14N-1H__MoLLIST.states.bz2</strong>[11.57 KB]<br>MoLLIST (14N)(1H) line list: States from Brooke et al (2015), http://dx.doi.org/10.1063/1.4923422, converted to ExoMol by Geronimo Villanueva (NASA/GSFC) Feb/2019.</p> <p><strong>14N-1H__MoLLIST.readme</strong>[2.09 KB]<br>MoLLIST's line list: readme file</p> <p><strong>References:</strong><br> 1. Brooke, J. S. A., Bernath, P. F., Western, C. M., van Hemert, M. C., Groenenboom, G. C., "Line strengths of rovibrational and rotational transitions within the X3Σ- ground state of NH", Journal of Chemical Physics 141, 54310 (2014). <a href="[http://dx.doi.org/10.1063/1.4891468]">[http://dx.doi.org/10.1063/1.4891468]</a>[14BrBeWe.NH]<br> 2. Fernando, A. M., Bernath, P. F., Hodges, J. N., Masseron, T., "A new linelist for the A3 P - X3 transition of the NH free radical", Journal of Quantitative Spectroscopy & Radiative Transfer 217, 29-34 (2018). <a href="[https://doi.org/10.1016/j.jqsrt.2018.05.021]">[https://doi.org/10.1016/j.jqsrt.2018.05.021]</a><br> 3. Brooke, J. S. A., Bernath, P. F., Western, C. M., "Note: Improved line strengths of rovibrational and rotational transitions within the X 3Σ− ground state of NH", The Journal of Chemical Physics 143, 026101/1-3 (2015). <a href="[https://doi.org/10.1063/1.4923422]">[https://doi.org/10.1063/1.4923422]</a>[15BrBeWe.NH]<br> 4. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br></p> </blockquote> <strong>MoLLIST: partition function</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>14N-1H__MoLLIST.pf</strong>[122.07 KB]<br>MoLLIST (14N)(1H) line list: partition function, data are from Brooke et al (2015), http://dx.doi.org/10.1063/1.4923422, compiled by Geronimo Villanueva (NASA/GSFC) Feb/2019.</p> <p><strong>References:</strong><br> 1. Sauval, A. J., Tatum, J. B., "A set of partition functions and equilibrium constants for 300 diatomic molecules of astrophysical interest", Astrophysical Journal Supplement Series 56, 193-209 (1984). <a href="[http://dx.doi.org/10.1086/190980]">[http://dx.doi.org/10.1086/190980]</a>[84SaTaxx.FeH]<br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>14N-1H__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[351.22 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (14N)(1H) line list.</p> <p><strong>14N-1H__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (14N)(1H) line list.</p> <p><strong>14N-1H__MoLLIST.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: MoLLIST (14N)(1H) line list.</p> <p><strong>14N-1H__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (14N)(1H) line list.</p> <p><strong>References:</strong><br> 1. Brooke, J. S. A., Bernath, P. F., Western, C. M., van Hemert, M. C., Groenenboom, G. C., "Line strengths of rovibrational and rotational transitions within the X3Σ- ground state of NH", Journal of Chemical Physics 141, 54310 (2014). <a href="[http://dx.doi.org/10.1063/1.4891468]">[http://dx.doi.org/10.1063/1.4891468]</a>[14BrBeWe.NH]<br> 2. Brooke, J. S. A., Bernath, P. F., Western, C. M., "Note: Improved line strengths of rovibrational and rotational transitions within the X 3Σ− ground state of NH", The Journal of Chemical Physics 143, 026101/1-3 (2015). <a href="[https://doi.org/10.1063/1.4923422]">[https://doi.org/10.1063/1.4923422]</a>[15BrBeWe.NH]<br> 3. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 4. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The MoLLIST dataset for 12C1H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CH/12C-1H/MoLLIST.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check CH_12C1H_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>12C-1H__MoLLIST.def</strong>[5.87 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/CH/12C-1H/MoLLIST/">https://exomol.com/models/CH/12C-1H/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>12C-1H__MoLLIST.trans.bz2</strong>[560.2 KB]<br>MoLLIST empirical (12C)(1H) line list transition file by T. Masseron et al. (2014)</p> <p><strong>12C-1H__MoLLIST.states.bz2</strong>[22.74 KB]<br>MoLLIST empirical (12C)(1H) line list states file from T. Masseron et al. (2014)</p> <p><strong>12C-1H__MoLLIST.readme</strong>[1.98 KB]<br>MoLLIST (12C)(1H) line list: Readme file</p> <p><strong>References:</strong><br> 1. Masseron, T., Plez, B., Van Eck, S., Colin, R., Daoutidis, I., Godefroid, M., Coheur, P. -F., Bernath, P., Jorissen, A., Christlieb, N., "CH in stellar atmospheres: an extensive linelist", Astronomy and Astrophysics 571, A47 (2014). <a href="[http://dx.doi.org/10.1051/0004-6361/201423956]">[http://dx.doi.org/10.1051/0004-6361/201423956]</a>[14MaPlVa.CH]<br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br></p> </blockquote> <strong>MoLLIST: partition function</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>12C-1H__MoLLIST.pf</strong>[115.97 KB]<br>MoLLIST (12C)(1H) line list: partition function by T. Masseron et al. (2014). Partition functions where computed by population addition up to 500K and then patched with the values obtained using Sauval and Tatum, ApJSS 56, 193 (1984).</p> <p><strong>References:</strong><br> 1. Masseron, T., Plez, B., Van Eck, S., Colin, R., Daoutidis, I., Godefroid, M., Coheur, P. -F., Bernath, P., Jorissen, A., Christlieb, N., "CH in stellar atmospheres: an extensive linelist", Astronomy and Astrophysics 571, A47 (2014). <a href="[http://dx.doi.org/10.1051/0004-6361/201423956]">[http://dx.doi.org/10.1051/0004-6361/201423956]</a>[14MaPlVa.CH]<br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>12C-1H__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[384.32 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (12C)(1H) line list.</p> <p><strong>12C-1H__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (12C)(1H) line list.</p> <p><strong>12C-1H__MoLLIST.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: MoLLIST (12C)(1H) line list.</p> <p><strong>12C-1H__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (12C)(1H) line list.</p> <p><strong>References:</strong><br> 1. Masseron, T., Plez, B., Van Eck, S., Colin, R., Daoutidis, I., Godefroid, M., Coheur, P. -F., Bernath, P., Jorissen, A., Christlieb, N., "CH in stellar atmospheres: an extensive linelist", Astronomy and Astrophysics 571, A47 (2014). <a href="[http://dx.doi.org/10.1051/0004-6361/201423956]">[http://dx.doi.org/10.1051/0004-6361/201423956]</a>[14MaPlVa.CH]<br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 3. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The SiGHTLY dataset for 28Si1H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/SiH/28Si-1H/SiGHTLY.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check SiH_28Si1H_SiGHTLY.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>28Si-1H__SiGHTLY.def</strong>[6.58 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/SiH/28Si-1H/SiGHTLY/">https://exomol.com/models/SiH/28Si-1H/SiGHTLY/</a><br></p> </blockquote> <strong>SiGHTLY: line list</strong> <p><em>ExoMol line lists XXIV: A new hot line list for silicon monohyrdide, SiH</em><br></p> <blockquote> <p><strong>28Si-1H__SiGHTLY.states.bz2</strong>[188.13 KB]<br>The states file (energy levels list) for the SiGHTLY line list for (28Si)(1H).</p> <p><strong>28Si-1H__SiGHTLY.trans.bz2</strong>[18.92 MB]<br>The trans file (transition list) for the SiGHTLY line list for (28Si)(1H).</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Sinden, F., Lodi, L., Hill, C., Gorman, M. N., Tennyson, J., "ExoMol line lists XXIV: A new hot line list for silicon monohydride, SiH", Monthly Notices of the Royal Astronomical Society 473, 5324-5333 (2018). <a href="[https://doi.org/10.1093/mnras/stx2738]">[https://doi.org/10.1093/mnras/stx2738]</a>[18YuSiLo.SiH]<br></p> </blockquote> <strong>SiGHTLY: partition function</strong> <p><em>ExoMol line lists XXIV: A new hot line list for silicon monohyrdide, SiH</em><br></p> <blockquote> <p><strong>28Si-1H__SiGHTLY.pf</strong>[126.95 KB]<br>The partition function file for the line list SiGHTLY for (28Si)(1H).</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Sinden, F., Lodi, L., Hill, C., Gorman, M. N., Tennyson, J., "ExoMol line lists XXIV: A new hot line list for silicon monohydride, SiH", Monthly Notices of the Royal Astronomical Society 473, 5324-5333 (2018). <a href="[https://doi.org/10.1093/mnras/stx2738]">[https://doi.org/10.1093/mnras/stx2738]</a>[18YuSiLo.SiH]<br></p> </blockquote> <strong>SiGHTLY: opacity</strong> <p><em>ExoMol line lists XXIV: A new hot line list for silicon monohyrdide, SiH</em><br></p> <blockquote> <p><strong>28Si-1H__SiGHTLY.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[438.18 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): SiGHTLY (28Si)(1H) line list.</p> <p><strong>28Si-1H__SiGHTLY.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: SiGHTLY (28Si)(1H) line list.</p> <p><strong>28Si-1H__SiGHTLY.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: SiGHTLY (28Si)(1H) line list.</p> <p><strong>28Si-1H__SiGHTLY.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: SiGHTLY (28Si)(1H) line list.</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Sinden, F., Lodi, L., Hill, C., Gorman, M. N., Tennyson, J., "ExoMol line lists XXIV: A new hot line list for silicon monohydride, SiH", Monthly Notices of the Royal Astronomical Society 473, 5324-5333 (2018). <a href="[https://doi.org/10.1093/mnras/stx2738]">[https://doi.org/10.1093/mnras/stx2738]</a>[18YuSiLo.SiH]<br> 2. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The GYT dataset for 32S1H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/SH/32S-1H/GYT.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check SH_32S1H_GYT.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>32S-1H__GYT.def</strong>[6.58 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/SH/32S-1H/GYT/">https://exomol.com/models/SH/32S-1H/GYT/</a><br></p> </blockquote> <strong>GYT: line list</strong> <p><em>ExoMol line lists -- XXXVI: line lists for the X-X and A-X bands of SH.</em><br></p> <blockquote> <p><strong>32S-1H__GYT.states.bz2</strong>[123.34 KB]<br>GYT (32S)(1H) line list states containing the X-X and A-X bands.</p> <p><strong>32S-1H__GYT.trans.bz2</strong>[6.23 MB]<br>Transitions of the GYT (32S)(1H) line list containing the X-X and A-X bands.</p> <p><strong>References:</strong><br> 1. Gorman, M. N., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists XXXVI: X 2Π - X 2Π and X 2Σ - X 2Π transitions of SH", Monthly Notices of the Royal Astronomical Society 490, 1652-1665 (2019). <a href="[https://doi.org/10.1093/mnras/stz2517]">[https://doi.org/10.1093/mnras/stz2517]</a>[19GoYuTe.SH]<br></p> </blockquote> <strong>GYT: partition function</strong> <p><em>ExoMol line lists -- XXXVI: line lists for the X-X and A-X bands of SH.</em><br></p> <blockquote> <p><strong>32S-1H__GYT.pf</strong>[122.07 KB]<br>Partition function for the GYT (32S)(1H) line list containing the X-X and A-X bands.</p> <p><strong>References:</strong><br> 1. Gorman, M. N., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists XXXVI: X 2Π - X 2Π and X 2Σ - X 2Π transitions of SH", Monthly Notices of the Royal Astronomical Society 490, 1652-1665 (2019). <a href="[https://doi.org/10.1093/mnras/stz2517]">[https://doi.org/10.1093/mnras/stz2517]</a>[19GoYuTe.SH]<br></p> </blockquote> <strong>GYT: opacity</strong> <p><em>ExoMol line lists -- XXXVI: line lists for the X-X and A-X bands of SH.</em><br></p> <blockquote> <p><strong>32S-1H__GYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[446.08 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): GYT (32S)(1H) line list.</p> <p><strong>32S-1H__GYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: GYT (32S)(1H) line list.</p> <p><strong>32S-1H__GYT.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: GYT (32S)(1H) line list.</p> <p><strong>32S-1H__GYT.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: GYT (32S)(1H) line list.</p> <p><strong>References:</strong><br> 1. Gorman, M. N., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists XXXVI: X 2Π - X 2Π and X 2Σ - X 2Π transitions of SH", Monthly Notices of the Royal Astronomical Society 490, 1652-1665 (2019). <a href="[https://doi.org/10.1093/mnras/stz2517]">[https://doi.org/10.1093/mnras/stz2517]</a>[19GoYuTe.SH]<br> 2. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The YT34to10 dataset for 12C1H4
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CH4/12C-1H4/YT34to10.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check CH4_12C1H4_YT34to10.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>12C-1H4__YT34to10.def</strong>[21.85 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/CH4/12C-1H4/YT34to10/">https://exomol.com/models/CH4/12C-1H4/YT34to10/</a><br></p> </blockquote> <strong>YT34to10: line list</strong> <p><strong>NB: These data are not included in the current version on Zenodo because the data are over Zenodo upload cap, 50GB</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/CH4/12C-1H4/YT34to10<br></p> <blockquote> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Tennyson, J., "ExoMol line lists IV: The rotation-vibration spectrum of methane up to 1500 K", Monthly Notices of the Royal Astronomical Society 440, 1649-1661 (2014). <a href="[http://http://dx.doi.org/10.1093/mnras/stu326]">[http://http://dx.doi.org/10.1093/mnras/stu326]</a>[14YuTexx.CH4]<br> 2. Yurchenko, S. N., Amundsen, D. S., Tennyson, J., Waldmann, I. P., "A hybrid line list for CH4 and hot methane continuum", Astronomy and Astrophysics 605, A95/1-9 (2017). <a href="[https://doi.org/10.1051/0004-6361/201731026]">[https://doi.org/10.1051/0004-6361/201731026]</a>[17YuAmTe.CH4]<br></p> </blockquote> <strong>YT34to10: partition function</strong> <p><em>Calculated line list and energy levels for (12C)(1H)4</em><br></p> <blockquote> <p><strong>12C-1H4__YT34to10.pf</strong>[25.39 KB]<br>Partition function of (12C)(1H)4 in 3 K intervals to 2000 K</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Tennyson, J., "ExoMol line lists IV: The rotation-vibration spectrum of methane up to 1500 K", Monthly Notices of the Royal Astronomical Society 440, 1649-1661 (2014). <a href="[http://http://dx.doi.org/10.1093/mnras/stu326]">[http://http://dx.doi.org/10.1093/mnras/stu326]</a>[14YuTexx.CH4]<br> 2. Yurchenko, S. N., Amundsen, D. S., Tennyson, J., Waldmann, I. P., "A hybrid line list for CH4 and hot methane continuum", Astronomy and Astrophysics 605, A95/1-9 (2017). <a href="[https://doi.org/10.1051/0004-6361/201731026]">[https://doi.org/10.1051/0004-6361/201731026]</a>[17YuAmTe.CH4]<br></p> </blockquote> <strong>YT34to10: opacity</strong> <p><em>Calculated line list and energy levels for (12C)(1H)4</em><br></p> <blockquote> <p><strong>12C-1H4__YT34to10.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[353.53 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): YT34to10 (12C)(1H)4 line list.</p> <p><strong>12C-1H4__YT34to10.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: YT34to10 (12C)(1H)4 line list.</p> <p><strong>12C-1H4__YT34to10.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: YT34to10 (12C)(1H)4 line list.</p> <p><strong>12C-1H4__YT34to10.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: YT34to10 (12C)(1H)4 line list.</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Amundsen, D. S., Tennyson, J., Waldmann, I. P., "A hybrid line list for CH4 and hot methane continuum", Astronomy and Astrophysics 605, A95/1-9 (2017). <a href="[https://doi.org/10.1051/0004-6361/201731026]">[https://doi.org/10.1051/0004-6361/201731026]</a>[17YuAmTe.CH4]<br> 2. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The ATP dataset for 26Al16O
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/AlO/26Al-16O/ATP.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check AlO_26Al16O_ATP.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>26Al-16O__ATP.def</strong>[6.59 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/AlO/26Al-16O/ATP/">https://exomol.com/models/AlO/26Al-16O/ATP/</a><br></p> </blockquote> <strong>ATP: line list</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>ATP_README.txt</strong>[5.08 KB]<br>Documentation for the AlO line list of the ATP dataset</p> <p><strong>26Al-16O__ATP.states.bz2</strong>[1.07 MB]<br>Labelled rovibrational states of (26Al)(16O). Some calculated (Ca) energy levels were replaced with Pseudo-experimental correction (PE) values.</p> <p><strong>26Al-16O__ATP.trans.bz2</strong>[53.57 MB]<br>Frequency ordered transitions of (26Al)(16O)</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br></p> </blockquote> <strong>ATP: partition function</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>ATP_README.txt</strong>[5.08 KB]<br>Documentation for the AlO line list of the ATP dataset</p> <p><strong>26Al-16O__ATP.pf</strong>[22.85 KB]<br>Partition function for (26Al)(16O)</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br></p> </blockquote> <strong>ATP: opacity</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>27Al-16O__ATP.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[444.15 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): ATP (27Al)(16O) line list.</p> <p><strong>27Al-16O__ATP.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: ATP (27Al)(16O) line list.</p> <p><strong>27Al-16O__ATP.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: ATP (27Al)(16O) line list.</p> <p><strong>27Al-16O__ATP.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: ATP (27Al)(16O) line list.</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br> 2. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote> <strong>ATP: other States files</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/AlO/26Al-16O/ATP<br></p>
The ATP dataset for 27Al18O
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/AlO/27Al-18O/ATP.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check AlO_27Al18O_ATP.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>27Al-18O__ATP.def</strong>[6.48 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/AlO/27Al-18O/ATP/">https://exomol.com/models/AlO/27Al-18O/ATP/</a><br></p> </blockquote> <strong>ATP: line list</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>ATP_README.txt</strong>[5.08 KB]<br>Documentation for the AlO line list of the ATP dataset</p> <p><strong>27Al-18O__ATP.states.bz2</strong>[1.13 MB]<br>Labelled rovibrational states of (27Al)(18O). Some calculated (Ca) energy levels were replaced with Pseudo-experimental correction (PE) values.</p> <p><strong>27Al-18O__ATP.trans.bz2</strong>[59.06 MB]<br>Frequency ordered transitions of (27Al)(18O)</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br></p> </blockquote> <strong>ATP: partition function</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>ATP_README.txt</strong>[5.08 KB]<br>Documentation for the AlO line list of the ATP dataset</p> <p><strong>27Al-18O__ATP.pf</strong>[22.85 KB]<br>Partition function for (27Al)(18O)</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br></p> </blockquote> <strong>ATP: other States files</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/AlO/27Al-18O/ATP<br></p>
The ATP dataset for 27Al16O
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/AlO/27Al-16O/ATP.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check AlO_27Al16O_ATP.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>27Al-16O__ATP.def</strong>[6.48 KB]<br></p> <p><strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/AlO/27Al-16O/ATP/">https://exomol.com/models/AlO/27Al-16O/ATP/</a><br></p> </blockquote> <strong>ATP: line list</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>ATP_README.txt</strong>[5.08 KB]<br>Documentation for the AlO line list of the ATP dataset</p> <p><strong>27Al-16O__ATP.states.bz2</strong>[1.09 MB]<br>Labelled rovibrational states of (27Al)(16O). Many calculated (Ca) energy levels were replaced with Marvelised (Ma), Effective Hamiltonian (EH), Predicted shift (PS) and Pseudo-experimental correction (PE) values.</p> <p><strong>27Al-16O__ATP.trans.bz2</strong>[31.11 MB]<br>Frequency ordered transitions of (27Al)(16O)</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br> 2. Bowesman, C. A., Shuai, M., Yurchenko, S. N., Tennyson, J., "A high resolution line list for AlO", Monthly Notices of the Royal Astronomical Society Submitted (2021).<br></p> </blockquote> <strong>ATP: partition function</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>ATP_README.txt</strong>[5.08 KB]<br>Documentation for the AlO line list of the ATP dataset</p> <p><strong>27Al-16O__ATP.pf</strong>[22.85 KB]<br>Partition function for (27Al)(16O)</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br></p> </blockquote> <strong>ATP: other States files</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/AlO/27Al-16O/ATP<br></p> <strong>ATP: opacity</strong> <p><em>Line lists for four isotopes of aluminium monoxide covering the pure rotation, rotation–vibration and electronic (B − X blue–green and A − X infrared bands) spectrum. States file updated 20-11-2015.</em><br></p> <blockquote> <p><strong>27Al-16O__ATP.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[444.15 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): ATP (27Al)(16O) line list.</p> <p><strong>27Al-16O__ATP.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: ATP (27Al)(16O) line list.</p> <p><strong>27Al-16O__ATP.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: ATP (27Al)(16O) line list.</p> <p><strong>27Al-16O__ATP.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: ATP (27Al)(16O) line list.</p> <p><strong>References:</strong><br> 1. Patrascu, A. T., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists: IX The spectrum of AlO", Monthly Notices of the Royal Astronomical Society 449, 3613-3619 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv507]">[http://dx.doi.org/10.1093/mnras/stv507]</a>[15PaYuTe.AlO]<br></p> </blockquote>
ScienceDex guides
Understand access before you commit
These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.