| --- |
| license: apache-2.0 |
| language: |
| - en |
| base_model: |
| - nasa-impact/nasa-smd-ibm-v0.1 |
| pipeline_tag: text-classification |
| tags: |
| - unified |
| - astronomy |
| - thesaurus |
| - uat |
| widget: |
| - text: Solar Observations by Angelo Secchi. I. Digitization of Original Documents |
| and Analysis of Group Numbers over the Period of 1853-1878. Angelo Secchi, an |
| Italian Jesuit and prominent scientist of the 19th century, and one of the founders |
| of modern astrophysics, observed the Sun regularly at the Collegio Romano in Rome, |
| Italy, for more than 25 yr. Results from his observations are reported in articles |
| published in the scientific journals of the time, as well as in drawings and personal |
| notebooks that are stored in the historical archive of the Istituto Nazionale |
| di Astrofisica Osservatorio Astronomico di Roma. The latter material, which reports |
| solar observations performed from 1853-1878, includes original documents from |
| Secchi and from a few of his close collaborators. The above unique material has |
| recently been digitized for preservation purposes and for allowing the scientific |
| exploitation of data not easily accessible so far. A total of more than 5400 digital |
| images have been produced. Here we present the archival material and the new digital |
| data derived from it. We also present results obtained from our primary analysis |
| of the new digital data. In particular, we produced new measurements of the group |
| number from 1853-1878, which will be available for future recalibration of the |
| group number series. |
| example_title: Solar Observations by Angelo Secchi |
| - text: 'Disk-resolved Photometric Properties of Pluto and the Coloring Materials |
| across its Surface. A multiwavelength regionally dependent photometric analysis |
| of Pluto''s anti-Charon-facing hemisphere using images collected by New Horizons'' |
| Multispectral Visible Imaging Camera (MVIC) reveals large variations in the absolute |
| value and spectral slope of the single-scattering albedo. Four regions of interest |
| are analyzed: the dark equatorial belt, Pluto''s north pole, nitrogen-rich regions, |
| and the mid-latitude terrains. Regions dominated by volatile ices such as Lowell |
| Regio and Sputnik Planitia present single-scattering albedos of ∼0.98 at 492 nm, |
| almost neutral across MVIC''s visible wavelength range (400-910 nm), indicating |
| limited contributions from tholin materials. Pluto''s dark equatorial regions, |
| informally named Cthulhu and Krun Maculae, have single-scattering albedos of ∼0.16 |
| at 492 nm and are the reddest regions. Applying the Hapke radiative transfer model |
| to combined MVIC and Linear Etalon Imaging Spectral Array (LEISA) spectra (400-2500 |
| nm) of Cthulhu Macula and Lowell Regio successfully reproduces the spectral properties |
| of these two regions of dramatically disparate coloration, composition, and morphology. |
| Since this model uses only a single coloring agent, very similar to the Titan-like |
| tholin of Khare et al., to account for all of Pluto''s colors, this result supports |
| the Grundy et al. conclusion that Pluto''s coloration is the result of photochemical |
| products mostly produced in the atmosphere. Although cosmic rays and extreme ultraviolet |
| photons reach Pluto''s surface where they can drive chemical processing, observations |
| of diverse surface colors do not require different chemical products produced |
| in different environments. We report a correction scaling factor in the LEISA |
| radiometric calibration of 0.74 ± 0.05.' |
| example_title: Photometric Properties of Pluto |
| --- |
| |
| # KAILAS |
| KAILAS (aka Keyword Labeler At SciX aka Indus-UAT-Labeler aka nasa-smd-ibm-v0.1_UAT_Labeler) is a RoBERTa-based, Encoder-only transformer model, domain-adapted for NASA Science Mission Directorate (SMD) applications. It's fine-tuned on scientific journals and articles relevant to NASA SMD, aiming to enhance natural language technologies like information retrieval and intelligent search. |
| This specific fork was finetuned on SciX Digital Library (https://scixplorer.org/, formerly NASA-ADS) proprietary data to label text with UAT labels (https://astrothesaurus.org/) |
|
|
| ## Model Details |
| - **Base Model**: RoBERTa |
| - **Tokenizer**: Custom |
| - **Parameters**: 125M |
| - **UAT Version used**: [5.1](https://github.com/astrothesaurus/UAT/releases/tag/v.5.1.0) |
|
|
| ## Training Data |
| - 18K titles, abstracts, body and acknowledgments from recent, quality astronomy papers |
| - approximately 217M tokens |
|
|
| # Contact |
| KAILAS is maintained by [Dr. Felix Grezes](https://scixplorer.org/scixabout/team/team/fgrezes.html) and [Dr. Jennifer Lynn Bartlett](https://scixplorer.org/scixabout/team/team/jbartlett.html). |
| <!-- ## Note --> |
|
|
| <!-- ## Citation --> |
| <!-- If you find this work useful, please cite using the following bibtex citation: --> |
|
|
| <!-- ## Disclaimer --> |
