paper_id stringlengths 9 15 | title stringlengths 0 95.9k | authors listlengths 0 639 | abstract stringlengths 0 62k | latex listlengths 0 268 | bibtex listlengths 0 7 |
|---|---|---|---|---|---|
astro-ph0001001 | Statistics of Turbulence from Spectral-Line Data Cubes | [
{
"author": "Alex Lazarian"
}
] | Emission in spectral lines can provide unique information on interstellar turbulence. Doppler shifts due to supersonic motions contain information on turbulent velocity field which is otherwise difficult to measure. However, the problem of separation of velocity and density fluctuations is far from being trivial. Using... | [
{
"name": "procl.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n%\t\t\tprocl.tex\t\t\t%\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n\n\\documentstyle[procl]{article}\n\n\\input{psfig.sty}\n\n% A useful Journal macro\n\\def\\Journal#1#2#3#4{(#1) {#2} {\\bf #3}, #4... | [
{
"name": "astro-ph0001001.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\\bibitem{} Adler, D. S. \\& Roberts, W. W. Jr. \\Journal{1992}{\\ApJ}{384}{95}\n\\bibitem{} Armstrong, J.M., Rickett, B.J., \\& Spangler, S.R.\n\\Journal{1995}{\\ApJ}{443}{209}\n\\bibitem{} Brand, P. \\& Wouterloot, J.G.A. ... |
astro-ph0001002 | On the inverse Compton scattering model of radio pulsars | [
{
"author": "G. J. Qiao$^{1,2}$"
},
{
"author": "R. X. Xu$^{1,2}$"
},
{
"author": "J. F. Liu$^{1,2}$"
},
{
"author": "J. L. Han$^{1,3}$"
},
{
"author": "B. Zhang$^{1,2}$"
}
] | Some characteristics of the inverse Compton scattering (ICS) model are reviewed. At least the following properties of radio pulsars can be reproduced in the model: core or central emission beam, one or two hollow emission cones, different emission heights of these components, diverse pulse profiles at various frequenci... | [
{
"name": "qHK.tex",
"string": "\\documentstyle[11pt,newpasp,twoside]{article}\n\\pagestyle{myheadings}\n\\markboth{{\\it Qiao et. al.}}{{\\it ICS model of Pulsars}}\n\\begin{document}\n\n\\title{On the inverse Compton scattering model of radio pulsars}\n\n\\author{G. J. Qiao$^{1,2}$,\n R. X. Xu$^{1,... | [
{
"name": "astro-ph0001002.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem{} Beskin, V.S., Gurevich, A.V., Istomin, Y.N., 1988,\n Ap\\&SS, 146, 205\n\n\\bibitem{} Liu, J.F., Qiao, G.J., Xu, R.X., 1999,\n Chin. Phys. Lett., 16, 541\n\n\\bibitem{} Lyne A.G., Manchester R.N., 1988,\n ... |
astro-ph0001003 | Dark Halo and Disk Galaxy Scaling Laws in Hierarchical Universes | [
{
"author": "Julio F. Navarro\\altaffilmark{1}"
}
] | % We use cosmological N-body/gasdynamical simulations that include star formation and feedback to examine the proposal that scaling laws between the total luminosity, rotation speed, and angular momentum of disk galaxies reflect analogous correlations between the structural parameters of their surrounding dark matter h... | [
{
"name": "tfemapj.tex",
"string": "\\documentstyle[emulateapj]{article}\n\\singlespace\n%\\tighten\n%\\eqsecnum\n%\n% Macros\n%\n%\\newcommand{\\etal}{{et Pl.} \\thinspace}\n\\newcommand{\\etal}{{et al.~}}\n\\newcommand{\\eg}{{e.g.,} \\thinspace}\n\\newcommand{\\ie}{{i.e.,} \\thinspace}\n\\newcommand{\\Ms... | [
{
"name": "astro-ph0001003.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[]{} Barnes, J., Efstathiou, G., 1987, \\apj, 319, 575\n%\n\\bibitem[]{} Cole, S.M., Arag\\'on-Salamanca, A., Frenk, C.S., Navarro, J.F., \\& Zepf,\nS.E.\\ 1994, \\mnras, 271, 781\n%\n\\bibitem[]{} Cole S., \\& Lace... |
astro-ph0001004 | Theory of the Interaction of Planetary Nebulae with the Interstellar Medium | [
{
"author": "Ruth Dgani"
}
] | "The theory of the interaction of planetary nebulae with the interstellar medium is important for th(...TRUNCATED) | [{"name":"dgani.tex","string":"\\documentstyle[11pt,newpasp,twoside]{article}\n\\markboth{ Ruth Dgan(...TRUNCATED) | [] |
astro-ph0001005 | [] | [] | [] | ||
astro-ph0001006 | On the Clustering of GRBs on the Sky | [
{
"author": "Shiv K. Sethi$^1$"
},
{
"author": "S. G. Bhargavi$^2$"
},
{
"author": "and Jochen Greiner$^3$"
}
] | "The two-point correlation of the 4th (current) BATSE catalog (2494 objects) is calculated. It is sh(...TRUNCATED) | [{"name":"GP46.tex","string":"\\documentstyle[epsfig]{aipproc}\n\n\\begin{document}\n\n\\title{On th(...TRUNCATED) | [{"name":"astro-ph0001006.extracted_bib","string":"\\bibitem{greiner}Greiner, J. , {\\tt http://www.(...TRUNCATED) |
astro-ph0001007 | Wide Field CCD Surface Photometry of the Giant Elliptical Galaxy NGC 4472 in the Virgo Cluster | [{"author":"Eunhyeuk Kim"},{"author":"$^1$ Myung Gyoon Lee"},{"author":"$^1$Department of Astronomy"(...TRUNCATED) | "We present deep wide field ($16'.4 \\times 16'.4$ ) Washington $CT_1$ CCD surface photometry of the(...TRUNCATED) | [{"name":"Kim_m49surf.tex","string":"% mnsample.tex\n%% Author: Eunhyeuk Kim, Myung Gyoon Lee and Do(...TRUNCATED) | [{"name":"astro-ph0001007.extracted_bib","string":"\\begin{thebibliography}{}\n\\bibitem[Barsony 198(...TRUNCATED) |
astro-ph0001008 | [] | "\\noindent{In 1997 the first optical afterglow of a cosmic Gamma-Ray Burst was discovered, and subs(...TRUNCATED) | [{"name":"astro-ph0001008.tex","string":"\\NeedsTeXFormat{LaTeX2e}\n\\documentclass[twoside]{article(...TRUNCATED) | [] | |
astro-ph0001009 | THE NATURE OF ULTRA-LUMINOUS COMPACT\\ X-RAY SOURCES IN NEARBY SPIRAL GALAXIES | [{"author":"Kazuo {\\sc Makishima}"},{"author":"Aya {\\sc Kubota}"},{"author":"Tsunefumi {\\sc Mizun(...TRUNCATED) | "Studies were made of {ASCA} spectra of seven ultra-luminous compact X-ray sources (ULXs) in nearby (...TRUNCATED) | [{"name":"ms.tex","string":"\\documentstyle[12pt,aasms4,psfig]{article}\n%\\documentstyle[12pt,aasms(...TRUNCATED) | [{"name":"astro-ph0001009.extracted_bib","string":"\\begin{thebibliography}{}\n\\setlength{\\itemsep(...TRUNCATED) |
astro-ph0001010 | Feedback Processes in the Early Universe | [{"author":"A. Ferrara\\inst{1}"},{"author":"B. Ciardi\\inst{2}"},{"author":"S. Marri\\inst{3}"},{"a(...TRUNCATED) | "Feedback effects due to massive stars and supernovae in the first objects are shown to strongly reg(...TRUNCATED) | [{"name":"esa99.tex","string":"%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%(...TRUNCATED) | [{"name":"astro-ph0001010.extracted_bib","string":"\\begin{thebibliography}{}\n\n\\bibitem[\\protect(...TRUNCATED) |
End of preview. Expand in Data Studio
Hyperion: Scientific LaTeX Corpus
This dataset constitutes the Internal Scientific Corpus for the Hyperion Project of Synthetix Institute. It contains LaTeX source documents used for high-fidelity relational extraction and internal benchmarking of the Epistemic Manifold.
Dataset Details
- Total Documents: ~1,192,727 (Internal Base)
- Status: Private
- Access: Restricted to Synthetix Institute authorized personnel.
- Primary Use: Training the private sector of the Epistemic Manifold and validating domain-divergence strategies.
Dataset Structure
The schema mirrors the public corpus to ensure pipeline compatibility:
| Column | Type | Description |
|---|---|---|
latex |
string |
The full LaTeX source of the document. |
paper_id |
string |
Unique identifier. |
Usage (Internal Only)
Authorized users can access this dataset via the internal HF connection:
from datasets import load_dataset
import os
# Ensure HF_TOKEN is set in environment
ds = load_dataset(
"synthetix-institute/latex-data",
split="train",
streaming=True,
use_auth_token=True
)
for row in ds:
# Process internal data
pass
Maintenance
This dataset is maintained by the Synthetix Institute. For questions regarding the Hyperion Discovery Engine or the Epistemic Manifold, please refer to the project documentation.
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