cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.21223/km16bh/zhbs8w
title: 1026814.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/afixdb
title: 1026871.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/dnyd6a
title: 1026864.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/eydnos
title: 1026872.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/fhuspq
title: 1026869.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/gqikld
title: 1026868.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/icxvvr
title: 1026867.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/ymicfv
title: 1026865.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/ysa8td
title: 1026866.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/73eubm
title: 1026880.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/cq7d77
title: 1026875.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/ex0enr
title: 1026878.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/hj3ouv
title: 1026874.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/mzwobg
title: 1026879.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/qwyzxo
title: 1026876.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/tmrtwn
title: 1026877.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/vquezn
title: 1026873.FASTQ.gz

description: :unav
DOI: 10.5281/zenodo.3560761
title: Supplemental Materials for "Humanities Data Analysis"

description: Data discussed in the manuscript "Humanities Data Analysis: Case Studies with Python". Each folder in this dataset contains data used or discussed in one chapter. The data itself resides in a ``data`` directory inside each folder. Each ``data`` directory contains a ``README`` file which describes the files found in the directory. Most of the data are texts published before 1900. These texts are in the public domain.
DOI: 10.21223/km16bh/35m1is
title: 1026881.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/9lwxp9
title: 1026887.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/btzhei
title: 1026888.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/gksork
title: 1026886.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/jiav74
title: 1026882.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/mhueg7
title: 1026884.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/r8jbn0
title: 1026883.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/wnq0qq
title: 1026885.FASTQ.gz

description: :unav
DOI: 10.5281/zenodo.3560852
title: Villa Nylander in Haukipudas: 3D laser scanning survey and post production

description: This report shows some of the drawings elaborated for the 3d laser scanning documentation of an Art art Nouveau Villa situated in Haukipudas, Oulu, Finland.
DOI: 10.5281/zenodo.3560853
title: Villa Nylander in Haukipudas: 3D laser scanning survey and post production

description: This report shows some of the drawings elaborated for the 3d laser scanning documentation of an Art art Nouveau Villa situated in Haukipudas, Oulu, Finland.
DOI: 10.21223/km16bh/9nspfz
title: 1026889.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/hbihfa
title: 1026854.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/hn8k53
title: 1026857.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/ktz7gf
title: 1026856.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/lzwnvr
title: 1026853.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/ofvxip
title: 1026855.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/q4xoy0
title: 1026858.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/qmz3fn
title: 1026890.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/sgop9g
title: 1026891.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/vpgtp9
title: 1026852.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/5746e6
title: 1026900.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/6xzp5j
title: 1026904.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/bbmgth
title: 1026902.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/hzjtdh
title: 1026903.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/oyjzjw
title: 1026901.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/zimdbu
title: 1026859.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/cytfgs
title: 1026906.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/eugkdg
title: 1026911.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/gxtznv
title: 1026907.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/hx9iz8
title: 1026910.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/lnqpok
title: 1026913.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/rbtqsl
title: 1026909.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/xqlprt
title: 1026908.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/yv3ksy
title: 1026912.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/yxkbjn
title: 1026905.FASTQ.gz

description: :unav
DOI: 10.25345/c5rt0m
title: MassIVE MSV000084654 - EGFR inhibition triggers an adaptive response by co-opting antiviral signaling pathways in lung cancer
title: HCC827 cells were treated with 0.1 microM erlotinib for 0, 2, 6, and 24 hours. Cell lysates were immunoprecipitated with TBK1 antibody. Antibody enriched protein samples were run on SDS-PAGE gels and submitted to UT Southwestern Proteomics Core Facility for Mass Spectrometry. Protein gel pieces were digested overnight with trypsin (Pierce) following reduction and alkylation with DTT and iodoacetamide (Sigma Aldrich. The samples then underwent solid-phase extraction cleanup with Oasis HLB microelution plates (Waters) and the resulting samples were analyzed by LC-MS-MS, using an Orbitrap Fusion Lumos mass spectrometer (Thermo Electron) coupled to an Ultimate 3000 RSLC-Nano liquid chromatography systems (Dionex).
DOI: 10.21223/km16bh/01biyk
title: 1026915.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/2e9yuk
title: 1026918.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/bvwpv7
title: 1026919.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/pcf64q
title: 1026916.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/r9bfjx
title: 1026921.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/tafslh
title: 1026917.FASTQ.gz

description: :unav
DOI: 10.21223/km16bh/zugyck
title: 1026920.FASTQ.gz

description: :unav
DOI: 10.17876/plate/dr.4/envelopes/208_112319
title: Digital object identifier (DOI) for the envelope 112319 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112320
title: Digital object identifier (DOI) for the envelope 112320 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112321
title: Digital object identifier (DOI) for the envelope 112321 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112322
title: Digital object identifier (DOI) for the envelope 112322 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112323
title: Digital object identifier (DOI) for the envelope 112323 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112324
title: Digital object identifier (DOI) for the envelope 112324 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112325
title: Digital object identifier (DOI) for the envelope 112325 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112326
title: Digital object identifier (DOI) for the envelope 112326 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112327
title: Digital object identifier (DOI) for the envelope 112327 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112328
title: Digital object identifier (DOI) for the envelope 112328 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112329
title: Digital object identifier (DOI) for the envelope 112329 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112330
title: Digital object identifier (DOI) for the envelope 112330 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112331
title: Digital object identifier (DOI) for the envelope 112331 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112332
title: Digital object identifier (DOI) for the envelope 112332 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112333
title: Digital object identifier (DOI) for the envelope 112333 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112334
title: Digital object identifier (DOI) for the envelope 112334 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112335
title: Digital object identifier (DOI) for the envelope 112335 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112336
title: Digital object identifier (DOI) for the envelope 112336 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112337
title: Digital object identifier (DOI) for the envelope 112337 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112338
title: Digital object identifier (DOI) for the envelope 112338 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112339
title: Digital object identifier (DOI) for the envelope 112339 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112340
title: Digital object identifier (DOI) for the envelope 112340 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112341
title: Digital object identifier (DOI) for the envelope 112341 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112342
title: Digital object identifier (DOI) for the envelope 112342 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112343
title: Digital object identifier (DOI) for the envelope 112343 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112344
title: Digital object identifier (DOI) for the envelope 112344 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112345
title: Digital object identifier (DOI) for the envelope 112345 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112346
title: Digital object identifier (DOI) for the envelope 112346 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112347
title: Digital object identifier (DOI) for the envelope 112347 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112348
title: Digital object identifier (DOI) for the envelope 112348 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112349
title: Digital object identifier (DOI) for the envelope 112349 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112350
title: Digital object identifier (DOI) for the envelope 112350 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112351
title: Digital object identifier (DOI) for the envelope 112351 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112352
title: Digital object identifier (DOI) for the envelope 112352 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112353
title: Digital object identifier (DOI) for the envelope 112353 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112354
title: Digital object identifier (DOI) for the envelope 112354 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112355
title: Digital object identifier (DOI) for the envelope 112355 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112356
title: Digital object identifier (DOI) for the envelope 112356 in archive 208 from the APPLAUSE DR4
DOI: 10.48577/jpl.nprqm4
title: Forcing of Slow Density Waves in the C Ring by Saturn’s Quasi-Toroidal Normal Modes

description: We calculate Saturn’s quasi-toroidal normal modes of azimuthal order three for several candidate models for the interior stratification. We propose that these oscillations are responsible for exciting a class of slowly propagating spiral density waves observed in the C ring possessing the same azimuthal symmetry and pattern speeds that cluster near the rotation rate of the planet. Both prograde and retrograde propagation relative to the planetary rotation are observed. We find that we can construct interior models for which the pattern speeds of the normal modes align with those of a majority of the slow density waves. Excitation of the retrograde density waves requires retrograde toroidal modes with matching pattern speeds. We find that in order to support such modes, the interior model must include a layer of positive static stability in the molecular hydrogen envelope. The model that performs best places the peak of the static stability at a fractional radius of 0.85, near the radius of the semi-conductive layer where Saturn’s zonal jets are inferred to decay, but we cannot rule out models that place the peak stability somewhat deeper. The properties of the toroidal modes are less sensitive to the stratification in the deep interior, hence our results neither confirm nor contradict the presence of a dilute core. When differential rotation is included in the form of zonal winds based on analysis of Cassini gravity and magnetic field data, we find that several toroidal modes become inertially unstable, raising the possibility that this instability is the principal mechanism for their excitation. However, while we are able to construct interior models that align the pattern speeds of a few unstable retrograde modes with those of prominent density waves in the ring, the same models fail with respect to the unstable prograde modes. Consequently, the significance of the instability mechanism remains an open question. Our results suggest that the interaction of Saturn’s quasi-toroidal modes with the C ring provides an important source of new, complementary constraints on the planet’s internal stratification and that further study of these modes is warranted.
DOI: 10.17876/plate/dr.4/envelopes/208_112357
title: Digital object identifier (DOI) for the envelope 112357 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112358
title: Digital object identifier (DOI) for the envelope 112358 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112359
title: Digital object identifier (DOI) for the envelope 112359 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112360
title: Digital object identifier (DOI) for the envelope 112360 in archive 208 from the APPLAUSE DR4
DOI: 10.48577/jpl.gprang
title: Finite Element Modeling of Rigid-Flex PCB Origami Robotics Subjected to Large-Scale Deformations

description: Rigid-flex PCB robotics have been investigated for exploring planetary terrain currently inaccessible to traditional aluminum body rovers. In order to push the technology to flightreadiness, there must be rigorous methodologies for modeling these structures. This paper presents a modeling methodology for rigid-flex PCB robots subjected to large deformations, failure criteria for each component of the robot (PCB, Nomex hinges, flex cable), validation with drop testing of the rigid-flex PCB robot PUFFER, and an application of the method to assess survivability under Lunar impact scenarios. A numerically stable and computationally efficient model of rigid-flex PCB robotics was permitted by using a combination of preexisting element types and a hyperelastic material model for the flexible hinges.
DOI: 10.17876/plate/dr.4/envelopes/208_112361
title: Digital object identifier (DOI) for the envelope 112361 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112362
title: Digital object identifier (DOI) for the envelope 112362 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112363
title: Digital object identifier (DOI) for the envelope 112363 in archive 208 from the APPLAUSE DR4
DOI: 10.48577/jpl.fexwtb
title: A retrieval of xCO2 from ground-based mid-infrared NDACC solar absorption spectra from Ny-Ålesund and comparison to TCCON

description: Two global networks of ground-based Fourier transform spec- trometers are measuring abundances of atmospheric trace gases that absorb in the near and mid infrared, Network for the Detec- tion of Atmospheric Composition Change (NDACC) and Total Carbon Column Observing Network (TCCON). The first lacks a CO2 product, therefore this study focuses on developing a CO2 retrieval method for NDACC from a new spectral window in the 4800 cm−1 region with a focus in applying it to Ny- Ålesund historical spectra. This region is covered by both TC- CON and NDACC, which is an advantage for collocated com- parisons where available. The results are compared with collo- cated TCCON measurements of column-averaged dry-air mole fractions of CO2 (denoted by xCO2) in Ny-Ålesund, Svalbard and only TCCON in Burgos, Philippines. We found that it is pos- sible to retrieve xCO2 from NDACC spectra. The comparison between the new retrieval to TCCON showed that the sensitivity of the new retrieval is high in the troposphere and lower in the upper stratosphere, similar to TCCON, and that the seasonality is well captured. We worked on determining an optimal retrieval setup covered in section 7.
DOI: 10.17876/plate/dr.4/envelopes/208_112364
title: Digital object identifier (DOI) for the envelope 112364 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112365
title: Digital object identifier (DOI) for the envelope 112365 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112366
title: Digital object identifier (DOI) for the envelope 112366 in archive 208 from the APPLAUSE DR4
DOI: 10.48577/jpl.gqjhyy
title: Reflected spectroscopy of small exoplanets III: probing the UV band to measure biosignature gasses

description: Direct-imaging observations of terrestrial exoplanets will enable characterizing their atmospheric compositions and assessing their habitability. Using Earth as a template, the key atmospheric signatures for the biosphere is O$_2$ and the photochemical product O$_3$, while this O$_2$-O$_3$ biosignature is not detectable in the visible wavelengths for most of the time after the emergence of oxygenic photosynthesis life (i.e., the Proterozoic Earth). Here we demonstrate spectroscopic observations in the ultraviolet wavelengths for detecting and characterizing O$_2$ and O$_3$ in terrestrial exoplanets like Proterozoic Earth, using a spectral retrieval framework developed for future exoplanet direct-imaging missions. For an O$_2$ mixing ratio 2--3 orders of magnitude less than the present-day Earth, and an O$_3$ mixing ratio of $10^{-7}-10^{-6}$, we find that O$_3$ can be detected and its mixing ratio can be measured precisely (to within $~1$ order of magnitude) with the addition of the ultraviolet ($0.25-0.4\ \mu$m) spectra to visible-wavelength spectroscopy. With a modest spectral resolution ($R=7$) in the ultraviolet, the O$_3$ detection is robust against other potential gases absorbing in the ultraviolet (e.g., H$_2$S and SO$_2$), as well as the short-wavelength cutoff between 0.2 and 0.25 $\mu$m. While the O$_3$ detection does not rely on the near-infrared spectra, extending the wavelength coverage to the near-infrared ($1-1.8\ \mu$m) would provide essential information to interpret the O$_3$ biosignature, including the mixing ratio of H$_2$O, the cloud pressure, as well as the determination that the atmosphere is N$_2$- rather than CO$_2$-dominated. Overall, this work indicates that the capabilities of ultraviolet spectroscopy are essential for characterizing Earth-like exoplanets, and reaffirms the importance of the near-infrared. The ultraviolet and near-infrared capabilities should thus be evaluated as critical components for the future missions aiming at imaging and characterizing terrestrial exoplanets, such as the Habitable World Observatory.
DOI: 10.17876/plate/dr.4/envelopes/208_112367
title: Digital object identifier (DOI) for the envelope 112367 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112368
title: Digital object identifier (DOI) for the envelope 112368 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112369
title: Digital object identifier (DOI) for the envelope 112369 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112370
title: Digital object identifier (DOI) for the envelope 112370 in archive 208 from the APPLAUSE DR4
DOI: 10.48577/jpl.u54qy9
title: Draft Genome sequencing of Naganishia species isolated from the polar environments

description: The draft genomes of five Naganishia strains were sequenced using MinION and annotated using Funannotate pipeline. Phylogenetic and pangenome analyses were performed to provide their genetic relationships, diversity, and potential functional capabilities. This approach will aid in understanding their potential to survive under microgravity and their resilience to extreme environments.
DOI: 10.17876/plate/dr.4/envelopes/208_112371
title: Digital object identifier (DOI) for the envelope 112371 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112372
title: Digital object identifier (DOI) for the envelope 112372 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112373
title: Digital object identifier (DOI) for the envelope 112373 in archive 208 from the APPLAUSE DR4
DOI: 10.48577/jpl.cewrte
title: Classification of planets and estimation of interior properties based on primary parameters

description: Classification is an essential method and has been developed and applied in astronomy for over onehundred years. However, the planet, still lack a universal classification method, mainly because thesample of the planet is too small to perform statistical analysis. Fortunately, nowadays, exoplanetssupply a large sample to support building a classification framework. In this study, we select 1M⊙systems as representative samples based on the exoplanet survey results. And use the numericalsimulation data to overcome the selecting effect in observation. In our analysis, planets are classifiedinto four main categories (giant, compact, puffy, terrestrial) with the mass divide line around 100M⊕. According to the evolution traces of all the planets, many relations are obtained. Giant planetsstrongly rely on low-density embryos, and compact planets are shown as the temporary category inthe formation of the giant planets, they should be the solid core of the giant planet. By analyzing themass-radius relation for the giant planets, a radius turning point is found at 3.9 MJ , which correspondsto the maximum size that cool giant planets can sustain. With the help of the interior model, we foundthat compact planets still hard to form an electron degeneracy core, but some of them are very close. Inthe low-mass region, using the structure model via the SMINT code, we discover two types of planetswith different gas envelope mass fractions fenv in ≥ 4.5g/cm3 region (≤3% and 10%) and one typein ≤ 4.5g/cm3 region (10-20%). Under the two-layers assumption, we calculate both maximum andminimum core radius fractions (CRF) for low mass region planets and the true planets from observationwith the hardCORE code. Obtain the pure-core structure boundary at 30 g/cm3 for dense planets inobservation, and the maximum CRF around 5.5 g/cm3 for non-dense planets in simulation. Besides,the 4 and 6 g/cm3 are the critical densities for a dense core and low-density component inside theplanets. Though there are still many details need to be settled, we build up a simple classificationframework for planets, and speculate on some interior properties of them. With the help of thisframework, we can easily find the potential evolution path and interior structure of a given planet.
DOI: 10.17876/plate/dr.4/envelopes/208_112374
title: Digital object identifier (DOI) for the envelope 112374 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112375
title: Digital object identifier (DOI) for the envelope 112375 in archive 208 from the APPLAUSE DR4
DOI: 10.17876/plate/dr.4/envelopes/208_112376
title: Digital object identifier (DOI) for the envelope 112376 in archive 208 from the APPLAUSE DR4