paper_id stringlengths 9 15 | title stringlengths 0 62.4k | authors listlengths 0 986 | abstract stringlengths 0 30.5k | latex listlengths 0 222 | bibtex listlengths 0 3 |
|---|---|---|---|---|---|
astro-ph0002001 | QSO Absorption Line Constraints on Intragroup High--Velocity Clouds | [
{
"author": "Jane~C.~Charlton\\altaffilmark{1}"
},
{
"author": "Christopher~W.~Churchill"
},
{
"author": "and Jane~R.~Rigby"
}
] | We show that the number statistics of moderate redshift {\MgII} and Lyman limit absorbers may rule out the hypothesis that high velocity clouds are infalling intragroup material. | [
{
"name": "astro-ph0002001.tex",
"string": "\\documentstyle[emulateapj,rotate,times]{article}\n%\\documentstyle[11pt,rotate,aaspp4]{article}\n%\\documentstyle[12pt,aasms4]{article}\n \n% this is the modification \n \n%-----------------------------------------------------------------------------\n%\n% perso... | [
{
"name": "astro-ph0002001.extracted_bib",
"string": "\\begin{thebibliography}{XXX}\n\n\\bibitem[Bergeron \\& Boiss\\'e 1991]{bb91}\nBergeron, J., \\& Boiss\\'e, P. 1991, A\\&A, 243, 344\n\n\\bibitem[Bergeron \\etal 1992]{bergeron92}\nBergeron, J., Cristiani, S., \\& Shaver, P. A. 1992, A\\&A, 257, 417\n\n\... |
astro-ph0002002 | Point source models for the gravitational lens B1608+656: Indeterminacy in the prediction of the Hubble constant | [
{
"author": "Gabriela Surpi and Roger Blandford"
}
] | We apply elliptical isothermal mass models to reproduce the point source properties, i.e. image positions, flux density ratios and time delay ratios, of the quadruple lens B1608+656. A wide set of suitable solutions is found, showing that models that only fit the properties of point sources are under-constrained and ca... | [
{
"name": "gsurpi.tex",
"string": "\\documentstyle[11pt,paspconf,epsf]{article}\n\n\\begin{document}\n\\title{Point source models for the gravitational lens B1608+656:\nIndeterminacy in the prediction of the Hubble constant}\n\n\\author{Gabriela Surpi and Roger Blandford}\n\\affil{California Institute of Te... | [] |
astro-ph0002003 | Compact Stellar Systems in the Fornax Cluster: Super-massive Star Clusters or Extremely Compact Dwarf Galaxies? | [
{
"author": "M. J. Drinkwater$^{1}$"
},
{
"author": "J. B. Jones$^{2}$"
},
{
"author": "M. D. Gregg$^{3}$"
},
{
"author": "S. Phillipps$^{4}$"
}
] | and % | [
{
"name": "fss4.tex",
"string": "%\n% LaTeX template file for\n% Publications of the Astronomical Society of Australia.\n% Version 2.4 - 28 April 1997\n%\n%\\documentstyle[12pt,psfig]{article}\n\\documentstyle[11pt,psfig]{article}\n%\n% Baselineskip may be altered if desired.\n%\n\\baselineskip=2em\n%\n% A ... | [] |
astro-ph0002004 | Extracting Energy from a Black Hole through Its Disk | [
{
"author": "Li-Xin Li"
}
] | When some magnetic field lines connect a Kerr black hole with a disk rotating around it, energy and angular momentum are transferred between them. If the black hole rotates faster than the disk, $ca/GM_H>0.36$ for a thin Keplerian disk, then energy and angular momentum are extracted from the black hole and transferred ... | [
{
"name": "bh_disk.tex",
"string": "% bh_disk.tex for ApJ Letters\n\n\\documentstyle[12pt,aaspp4]{article}\n\\begin{document}\n\n\\title{Extracting Energy from a Black Hole through Its Disk}\n\n\\author{Li-Xin Li}\n\\affil{Princeton University Observatory, Princeton, NJ 08544--1001, USA}\n\\affil{E-mail: lx... | [] |
astro-ph0002005 | A Comparison of Ultraviolet, Optical, and X-Ray Imagery of Selected Fields in the Cygnus Loop | [
{
"author": "\\sc Charles W.\\ Danforth\\altaffilmark{1}"
},
{
"author": "Robert H.\\ Cornett\\altaffilmark{2}"
},
{
"author": "N. A. Levenson\\altaffilmark{1}"
},
{
"author": "William P.\\ Blair\\altaffilmark{1}"
},
{
"author": "Theodore P.\\ Stecher\\altaffilmark{3}"
}
] | During the Astro-1 and Astro-2 Space Shuttle missions in 1990 and 1995, far ultraviolet (FUV) images of five 40\arcmin\ diameter fields around the rim of the Cygnus Loop supernova remnant were observed with the Ultraviolet Imaging Telescope (UIT). These fields sampled a broad range of conditions including both radiativ... | [
{
"name": "psfig.tex",
"string": "% Psfig/TeX Release 1.2\n% dvips version\n%\n% All software, documentation, and related files in this distribution of\n% psfig/tex are Copyright 1987, 1988 Trevor J. Darrell\n%\n% Permission is granted for use and non-profit distribution of psfig/tex \n% providing that this... | [
{
"name": "astro-ph0002005.extracted_bib",
"string": "\\begin{thebibliography}{Danforth00}\n\\bibitem[Arendt, Dwek, \\& Leisawitz 1992]{Arendt92}\nArendt, R.G., Dwek, E., \\& Leisawitz, D. 1992, \\apj, 400, 562\n\\bibitem[Bedogni \\& Woodward (1990)]{Bedogni90}\nBedogni, R. \\& Woodward, P. R. 1990, \\aap, ... |
astro-ph0002006 | ULTRA HIGH ENERGY COSMIC RAYS: the theoretical challenge | [
{
"author": "A. V. Olinto\\thanksref{corr}"
}
] | "The origin of the highest-energy cosmic rays remains a mystery. The lack of a high energy cutoff in(...TRUNCATED) | [{"name":"physrepf.tex","string":"\\def\\la{\\hbox{{\\lower -2.5pt\\hbox{$<$}}\\hskip -8pt\\raise\n-(...TRUNCATED) | [{"name":"astro-ph0002006.extracted_bib","string":"\\begin{thebibliography}{9}\n\n\\bibitem{watson99(...TRUNCATED) |
astro-ph0002007 | [] | [{"name":"astro-ph0002007.tex","string":"\\documentstyle[12pt]{article}\n\\textheight 9in\n\\textwid(...TRUNCATED) | [{"name":"astro-ph0002007.extracted_bib","string":"\\begin{thebibliography}{99}\n\\bibitem{alcock} A(...TRUNCATED) | ||
astro-ph0002008 | "ISO-SWS spectroscopy of NGC 1068 \\footnote{Based on observations with ISO, an ESA project with ins(...TRUNCATED) | [{"author":"D.~Lutz\\footnote{Max-Planck-Institut f\\\"ur extraterrestrische Physik, Postfach 1603, (...TRUNCATED) | "We present ISO-SWS spectroscopy of NGC 1068 for the complete wavelength range 2.4 to 45$\\mu$m at r(...TRUNCATED) | [{"name":"obspaper.tex","string":"%\\documentstyle[12pt,aasms4]{article}\n\\documentstyle[11pt,aaspp(...TRUNCATED) | [{"name":"astro-ph0002008.extracted_bib","string":"\\begin{thebibliography}{}\n\\bibitem[Alexander e(...TRUNCATED) |
astro-ph0002009 | The giant radio galaxy 8C\,0821+695 and its environment | [{"author":"L. Lara\\inst{1}"},{"author":"K.-H. Mack\\inst{2,3}"},{"author":"M. Lacy\\inst{4}"},{"au(...TRUNCATED) | "We present new VLA and Effelsberg observations of the radio galaxy 8C\\,0821+695. We have obtained (...TRUNCATED) | [{"name":"lara.tex","string":"%----------------------------------------------%\n% REFERENCES \n%----(...TRUNCATED) | [{"name":"astro-ph0002009.extracted_bib","string":"\\begin{thebibliography}{}\n\n\\bibitem[1977]{baa(...TRUNCATED) |
astro-ph0002010 | RADIATION SPECTRA FROM \\ADVECTION-DOMINATED ACCRETION FLOWS \\IN A GLOBAL MAGNETIC FIELD | [
{
"author": "MOTOKI KINO$^{1}$"
},
{
"author": "OSAMU KABURAKI and NAOHIRO YAMAZAKI"
}
] | "We calculate the radiation spectra from advection-dominated accretion flows (ADAFs), taking into ac(...TRUNCATED) | [{"name":"ms.tex","string":" \n%--------------------------------------------------------------------(...TRUNCATED) | [] |
End of preview. Expand in Data Studio
Hyperion: Scientific LaTeX Corpus (Public)
This dataset constitutes the Public Scientific Corpus for the Hyperion Project at the Synthetix Institute. It contains high-fidelity LaTeX source text extracted from diverse scientific repositories, optimized for topological knowledge discovery and relational mapping.
Dataset Details
- Total Documents: ~1,318,468
- Average Document Length: Variable (approx. 32KB - 256KB)
- Primary Domain: Mathematics, Physics, and Chemistry.
- Goal: Provide the raw evidence layer for the Stage I.A Hyperion Pipeline (Anchor Detection and Morphism Extraction).
Dataset Structure
The dataset is provided in a flat format with the following schema:
| Column | Type | Description |
|---|---|---|
latex |
string |
The full LaTeX source of the document. |
paper_id |
string |
Unique identifier (arXiv ID or DOI equivalent). |
id |
string |
Internal UUID for the document. |
Usage
You can load this dataset directly using the Hugging Face datasets library:
from datasets import load_dataset
# Stream the dataset to avoid massive memory usage
ds = load_dataset("synthetix-institute/latex-data-pub", split="train", streaming=True)
# Fetch the first document
for row in ds:
print(row['paper_id'])
break
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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