KAILAS version 3

README.md

@@ -9,54 +9,49 @@ tags:
 - astronomy
 - uat
 - KAILAS-v02
+- v3
 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.
+- 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.
+- 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
 ---
 

config.json

@@ -1,5 +1,5 @@
 {
-  "_name_or_path": "../astroBERT-Tasks/Finetuning_4_UAT/trained_models/m.INDUS_d.expanded_v.005/checkpoint-630576/",
+  "_name_or_path": "../astroBERT-Tasks/Finetuning_4_UAT/trained_models/m.INDUS_d.expanded_astro_only_v.006/checkpoint-810471/",
   "architectures": [
     "RobertaForSequenceClassification"
   ],

model.safetensors

@@ -1,3 +1,3 @@
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