pathfinder: A Semantic Framework for Literature Review and Knowledge Discovery in Astronomy
Paper โข 2408.01556 โข Published โข 3
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12473133 | 1607.01526 | Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case | The Fornax dwarf spheroidal galaxy is the most massive satellites of the Milky Way, claimed to be embedded in a huge dark matter halo, and the only among the Milky Way satellites hosting five globular clusters. Interestingly, their estimated masses, ages and positions seem hardly compatible with the presence of a signi... | [
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] | 1 | [
"10.1093/mnras/stw1647",
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] | [
"Arca-Sedda, M.",
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"Department of Physics, Sapienza, University of Rome, Piazzale Aldo Moro 5, I-00185 Rome, Italy",
"Department of Physics, Sapienza, University of Rome, Piazzale Aldo Moro 5, I-00185 Rome, Italy"
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5209849 | 1607.03009 | Impacts of fragmented accretion streams onto classical T Tauri stars: UV and X-ray emission lines | Context. The accretion process in classical T Tauri stars (CTTSs) can be studied through the analysis of some UV and X-ray emission lines which trace hot gas flows and act as diagnostics of the post-shock downfalling plasma. In the UV-band, where higher spectral resolution is available, these lines are characterized by... | [
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"line profiles",
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"10.1051/0004-6361/201628858",
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"Colombo, S.",
"Orlando, S.",
"Peres, G.",
"Argiroffi, C.",
"Reale, F."
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"INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy",
"INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy",
"INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy; Dipartimento di Fisica & Chimica,... | [
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12586989 | 1607.06240 | Hybrid entropy stable HLL-type Riemann solvers for hyperbolic conservation laws | It is known that HLL-type schemes are more dissipative than schemes based on characteristic decompositions. However, HLL-type methods offer greater flexibility to large systems of hyperbolic conservation laws because the eigenstructure of the flux Jacobian is not needed. We demonstrate in the present work that several ... | [
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] | 1 | [
"10.1016/j.jcp.2016.10.034",
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] | [
"Schmidtmann, Birte",
"Winters, Andrew R."
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"MathCCES, RWTH Aachen University, Schinkelstr. 2, 52062 Aachen, Germany",
"Mathematisches Institut, Universitรคt zu Kรถln, Weyertal 86-90, 50931 Kรถln, Germany"
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168897 | 1607.07246 | Dynamics of Saturnโs great storm of 2010-2011 from Cassini ISS and RPWS | Saturnโs quasi-periodic planet-encircling storms are the largest convecting cumulus outbursts in the Solar System. The last eruption was in 1990 (Sรกnchez-Lavega, A. [1994]. Chaos 4, 341-353). A new eruption started in December 2010 and presented the first-ever opportunity to observe such episodic storms from a spacecra... | [
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"Astrophysics - Earth and Planetary Astrophysics"
] | 18 | [
"10.1016/j.icarus.2012.12.013",
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"Fischer, Georg",
"Ingersoll, Andrew P.",
"Kurth, William S.",
"Muro, Gabriel D.",
"Porco, Carolyn C.",
"West, Robert A."
] | [
"Department of Atmospheric and Planetary Sciences, Hampton University, Hampton, VA 23668, USA; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA",
"Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA",
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12408831 | 1607.07888 | Observed Variability at 1 and 4 ฮผm in the Y0 Brown Dwarf WISEP J173835.52+273258.9 | We have monitored photometrically the Y0 brown dwarf WISEP J173835.52+273258.9 (W1738) at both near- and mid-infrared wavelengths. This โฒ1 Gyr old 400 K dwarf is at a distance of 8 pc and has a mass around 5 M <SUB>Jupiter</SUB>. We observed W1738 using two near-infrared filters at ฮป โ 1 ฮผm, Y and J, on Gemini Observat... | [
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... | 7.153717 | 12.541796 | 2016-07-01 | 31 | 2016ApJ...830..141L | [
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] | 10 | [
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"Fortney, J. J.",
"Gelino, C. R.",
"Gizis, J. E.",
"Kirkpatrick, J. D.",
"Mace, G. N."
] | [
"Gemini Observatory, Northern Operations Center, 670 N. A'ohoku Place, Hilo, HI 96720, USA",
"The University of Toledo, 2801 West Bancroft Street, Mailstop 111, Toledo, OH 43606, USA",
"The University of Toledo, 2801 West Bancroft Street, Mailstop 111, Toledo, OH 43606, USA",
"The University of Toledo, 2801 W... | [
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12518466 | 1607.08820 | "Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio (...TRUNCATED) | "Our understanding of the universe relies mostly on electromagnetism. As photons are the messengers,(...TRUNCATED) | [-0.00632535619661212,0.011160125955939293,0.012271640822291374,0.01770714297890663,0.00273381313309(...TRUNCATED) | 6.522832 | 3.614386 | 2016-07-01 | 28 | 2017AdSpR..59..736B | ["unknown origin","pulsar observations","Radio astronomy","OLFAR","observations","low frequencies","(...TRUNCATED) | ["Photons","Radio astronomy","Satellites","Pulsars","Magnetars","Fast radio bursts","Astrophysics - (...TRUNCATED) | 6 | [
"10.1016/j.asr.2016.10.018",
"10.48550/arXiv.1607.08820"
] | [
"Bentum, Mark J.",
"Bonetti, Luca",
"Spallicci, Alessandro D. A. M."
] | ["Universiteit van Twente, Faculteit van Elektrotechniek, Wiskunde en Informatica, Telecommunication(...TRUNCATED) | ["2017ApJ...842...23Y","2017CQGra..34u5006S","2017FoPh...47..769A","2017PhLB..764..203B","2017PhLB..(...TRUNCATED) | ["1933PhRv...44..855H","1934PhRv...46.1087B","1934RSPSA.144..425B","1936AnP...418..398E","1936ZPhy..(...TRUNCATED) |
12406228 | 1607.06710 | "Setting the volatile composition of (exo)planet-building material. Does chemical evolution in disk (...TRUNCATED) | "Context. The atmospheres of extrasolar planets are thought to be built largely through accretion of(...TRUNCATED) | [0.008736980147659779,0.01737302727997303,0.059953976422548294,0.0015250288415700197,-0.003882751800(...TRUNCATED) | 10.068603 | 13.044076 | 2016-07-01 | 146 | 2016A&A...595A..83E | ["SUB>2</SUB","interstellar ice abundances","grain surfaces","CO","initial abundances","ices","atomi(...TRUNCATED) | ["astrochemistry","planets and satellites: formation","protoplanetary disks","planets and satellites(...TRUNCATED) | 12 | [
"10.1051/0004-6361/201628509",
"10.48550/arXiv.1607.06710"
] | [
"Eistrup, Christian",
"Walsh, Catherine",
"van Dishoeck, Ewine F."
] | ["Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands","Leiden Obse(...TRUNCATED) | ["2017A&A...599A.101V","2017A&A...599A.113M","2017A&A...601A..36B","2017A&A...603A.123H","2017A&A...(...TRUNCATED) | ["1972GeCoA..36..597G","1977Ap&SS..51..153W","1982A&A...114..245T","1983ApJ...267..603P","1993MNRAS.(...TRUNCATED) |
2774767 | 1607.08619 | The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey | "Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical fiber-bundle integral-fie(...TRUNCATED) | [-0.018747791647911072,0.03372214362025261,0.015452002175152302,-0.010926260612905025,-0.02956658229(...TRUNCATED) | 11.558285 | 6.853098 | 2016-07-01 | 359 | 2016AJ....152...83L | ["Sloan Digital Sky Survey","MaNGA","individual dithered observations","SDSS-IV Data Release","centr(...TRUNCATED) | ["methods: data analysis","surveys","techniques: imaging spectroscopy","Astrophysics - Instrumentati(...TRUNCATED) | 32 | [
"10.3847/0004-6256/152/4/83",
"10.48550/arXiv.1607.08619"
] | ["Law, David R.","Cherinka, Brian","Yan, Renbin","Andrews, Brett H.","Bershady, Matthew A.","Bizyaev(...TRUNCATED) | ["Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA","Center for As(...TRUNCATED) | ["2016AJ....152..197Y","2016MNRAS.463.2513B","2017AJ....154...28B","2017ApJ...837...32L","2017ApJ...(...TRUNCATED) | ["1969PASP...81..527W","1982PASP...94..715F","1986PASP...98..609H","1996PASP..108..277O","1998ApJ...(...TRUNCATED) |
12585901 | 1607.08157 | Dark matter directional detection: comparison of the track direction determination | "Several directional techniques have been proposed for a directional detection of Dark matter, among(...TRUNCATED) | [0.011932607740163803,0.024745754897594452,0.01089667808264494,0.027581609785556793,-0.0341079644858(...TRUNCATED) | 7.520985 | -2.487568 | 2016-07-01 | 10 | 2017JCAP...01..027C | ["initial direction","different detector materials","crystal detectors","nuclear emulsion plates","W(...TRUNCATED) | ["Astrophysics - Instrumentation and Methods for Astrophysics","Physics - Instrumentation and Detect(...TRUNCATED) | 3 | [
"10.1088/1475-7516/2017/01/027",
"10.48550/arXiv.1607.08157"
] | [
"Couturier, C.",
"Zopounidis, J. P.",
"Sauzet, N.",
"Naraghi, F.",
"Santos, D."
] | ["LPSC, CNRS/IN2P3, UJF, INP, Avenue des Martyrs, 38000, Grenoble, France","LPSC, CNRS/IN2P3, UJF, I(...TRUNCATED) | ["2016arXiv160708765C","2017JInst..12P0009B","2017PhRvD..96h3011O","2020PhRvD.102g5036B","2020PhRvD.(...TRUNCATED) | ["1985PhRvD..31.3059G","1988PhRvD..37.1353S","2003PhLB..571..132S","2010NIMPB.268.1818Z","2012EAS...(...TRUNCATED) |
12509827 | 1607.01847 | Oscillating chiral tensor spectrum from axionic inflation | "We study axionic inflation with a modulated potential and examine if the primordial tensor power sp(...TRUNCATED) | [0.018994921818375587,0.023814870044589043,-0.02079528011381626,-0.005090570542961359,-0.01004440523(...TRUNCATED) | 10.62901 | -1.476708 | 2016-07-01 | 42 | 2016PhRvD..94d4062O | ["chiral gravitational waves","axion phenomenologies","BBO","single-field axion monodromy inflation"(...TRUNCATED) | ["Astrophysics - Cosmology and Nongalactic Astrophysics","General Relativity and Quantum Cosmology",(...TRUNCATED) | 6 | [
"10.1103/PhysRevD.94.044062",
"10.48550/arXiv.1607.01847"
] | [
"Obata, Ippei",
"Soda, Jiro"
] | ["Department of Physics, Kyoto University, Kyoto 606-8502, Japan","Department of Physics, Kobe Unive(...TRUNCATED) | ["2016JCAP...12..031G","2016JHEP...12..137A","2017JCAP...06..050O","2017JCAP...08..005G","2017JHEP..(...TRUNCATED) | ["1990PhRvL..65.3233F","1998PhRvD..57.7089C","2000PhR...331..283M","2001PhRvL..87v1103S","2005IJMPD.(...TRUNCATED) |
This dataset is associated with the Pathfinder app (https://pfdr.app, paper at https://arxiv.org/abs/2408.01556) and is updated roughly monthly to keep pace with new literature in astrophysics and cosmology.