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!DOCTYPE html>html langen>  head>    meta charsetutf-8>    title>The Open Journal of Astrophysics/title>    link relcanonical hrefhttps://astro.theoj.org/>    base href/>    meta nameviewport contentwidthdevice-width, initial-scale1>    link relicon typeimage/x-icon hrefhttps://assets.scholasticahq.com/assets/favicon-575713edd1dc0dd5811bbc1b7893cf299318af3d22bc8e863eae37a7d61f7ebb.ico />        link relstylesheet hrefhttps://assets.scholasticahq.com/dist/journal-website/styles.5cf596c2a2a7c185.css>    meta itempropname contentThe Open Journal of Astrophysics />  meta namedescription contentThe Open Journal of Astrophysics is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology. />  meta itempropdescription contentThe Open Journal of Astrophysics is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology. />meta nametwitter:title contentThe Open Journal of Astrophysics />meta nametwitter:card contentsummary_large_image />meta nametwitter:site content@scholasticahq />  meta nametwitter:description contentThe Open Journal of Astrophysics is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology. />meta propertyog:title contentThe Open Journal of Astrophysics />  meta propertyog:description contentThe Open Journal of Astrophysics is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology. />  /head>  body>    app-root>/app-root>      script src/dist/journal-website/runtime.cf12a5a8bfba626f.js typemodule>/script>  script src/dist/journal-website/polyfills.5ab77736377a452c.js typemodule>/script>  script src/dist/journal-website/scripts.a5bcfbbd114efdfd.js defer>/script>  script src/dist/journal-website/main.e243ffba8f599b0f.js typemodule>/script>  /body>  script>    window.JOURNAL  {id:1436,name:The Open Journal of Astrophysics,description:\u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e, which is published by Maynooth Academic Publishing,  is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology.\n\nPapers can be submitted for publication free of charge, are refereed free of charge and are published (online only) free of charge.\n\nWe apply a simple criterion to decide whether a paper is on a suitable topic for this journal, namely that if it is suitable for the \u003ca href\//arxiv.org/archive/astro-ph/Astrophysics\\u003eastro-ph section\u003c/a\u003e of the arXiv then it is suitable for \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e. For further instructions, including a breakdown of the arXiv sections, see the \u003cem\u003eFor Authors\u003c/em\u003e tab.\n\n\u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e is a member of the \u003ca href\https://freejournals.org/\\u003eFree Journal Network\u003c/a\u003e.\n\n\u003cstrong\u003eAcknowledgments\u003c/strong\u003e. We are extremely grateful to Arfon Smith, Chris Lintott, Adam Becker, Robert Simpson, Stuart Lynn and Mark Rohloff for help developing the prototype of the site and for their ongoing support of the project.  We also acknowledge generous financial support from the \u003ca href\https://www.moore.org/\\u003eGordon and Betty Moore Foundation\u003c/a\u003e.,short_description:The Open Journal of Astrophysics is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology.,editorial_board:The members of the Editorial Board are listed below, together with their institutional affiliation and areas of expertise:\n\n\u003cstrong\u003ePeter Coles*\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, National University of Ireland Maynooth, Ireland\u003c/em\u003e). Cosmology, astrophysics, statistics and methodology. \n\n*Managing Editor\n\n\u003cstrong\u003eThierry Appourchaux\u003c/strong\u003e (\u003cem\u003eCNRS, Institut dAstrophysique Spatiale, Orsay, France\u003c/em\u003e). Space instrumentation, astroseismology, helioseismology, statistics and methodology.\n\n\u003cstrong\u003eEmory (Ted) Bunn\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, University of Richmond, USA\u003c/em\u003e). Relativity, cosmology. \n\n\u003cstrong\u003eWalter Dehnen\u003c/strong\u003e (\u003cem\u003eAstronomisches Rechen-Institut, University of Heidelberg, Germany\u003c/em\u003e). Stellar dynamics, galaxy dynamics, galaxies, bars, Milky-Way dynamics, Gaia, numerical methods, N-body techniques, smooth particle hydrodynamics (SPH).\n\n\u003cstrong\u003ePhilipp Edelmann\u003c/strong\u003e (\u003cem\u003eLos Alamos National Laboratory, New Mexico, USA\u003c/em\u003e). Stellar astrophysics, hydrodynamics, high-performance computing, supernovae, internal waves, stellar evolution, numerical methods.\n\n\u003cstrong\u003ePedro Ferreira\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, University of Oxford, UK\u003c/em\u003e). Large-scale structure, general relativity, cosmic microwave background, early universe, cosmology.\n\n\u003cstrong\u003eEmmanuel Frion\u003c/strong\u003e (\u003cem\u003eDepartment of Physics \u0026 Astronomy, University of Western Ontario, Canada\u003c/em\u003e). Cosmology, tests of gravity, primordial magnetic fields, dark energy, Bayesian inference, bouncing cosmology, theoretical astrophysics and cosmology, cosmic inflation, quantum cosmology\n\n\u003cstrong\u003eAndrew Jaffe\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, Imperial College, London, UK\u003c/em\u003e). Astrophysics, statistics and methodology, cosmology.\n\n\u003cstrong\u003eHarley Katz\u003c/strong\u003e (\u003cem\u003eDepartment of Astronomy and Astrophysics, University of Chicago, USA\u003c/em\u003e).  Galaxy formation and evolution, numerical simulations\n\n\u003cstrong\u003eLucyna Kedziora-Chudczer\u003c/strong\u003e (\u003cem\u003eSchool of Physics, University of New South Wales, Sydney, Australia\u003c/em\u003e).  Active galactic nuclei, polarimetry, atmospheres of planets, exoplanets, solar system planets.\n\n\u003cstrong\u003eJulien Larena\u003c/strong\u003e (\u003cem\u003eLaboratoire Univers et Particules de Montpellier, Université de Montpellier, France\u003c/em\u003e). Cosmology, gravitation, lensing, large-scale structure, general relativity.\n\n\u003cstrong\u003eManuela Magliocchetti\u003c/strong\u003e (\u003cem\u003eNational Institute of Astrophysics, Rome, Italy\u003c/em\u003e).  Cosmology, galaxies, active galactic nuclei (AGN).\n\n\u003cstrong\u003eSean McGee\u003c/strong\u003e (\u003cem\u003eDepartment of Physics \u0026 Astronomy, University of Birmingham, UK\u003c/em\u003e). Galaxy formation, galaxy clusters, galaxy surveys.\n\n\u003cstrong\u003eFoteini Oikonomou\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, Norwegian University of Science \u0026 Technology, Norway\u003c/em\u003e.) High-energy astrophysics, ultra-high-energy cosmic rays, high-energy neutrinos, active galactic nuclei, high-energy gamma rays.\n\n\u003cstrong\u003eManolis Plionis\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, Aristotle University of Thessaloniki, Greece\u003c/em\u003e). Observational cosmology, extragalactic astrophysics, large-scale structure, active galactic nuclei.\n\n\u003cstrong\u003eAlkistis Pourtsidou\u003c/strong\u003e (\u003cem\u003eHiggs Centre \u0026 Institute for Astronomy, Edinburgh, UK\u003c/em\u003e). Cosmology, large-scale structure of the Universe, radio astronomy, galaxy surveys.\n\n\u003cstrong\u003eJustin Read\u003c/strong\u003e (\u003cem\u003eSchool of Mathematics and Physics, University of Surrey, UK\u003c/em\u003e). Dark matter, cosmology, galaxy formation and evolution, dwarf galaxies, milky way, galactic dynamics, galactic archaeology, computational modeling.\n\n\u003cstrong\u003eHanno Rein\u003c/strong\u003e (\u003cem\u003eDepartment of Physics and Environmental Sciences, University of Toronto at Scarborough, Canada\u003c/em\u003e).    Numerical methods, in particular N-body codes and integration methods for planetary systems, planet formation, stochastic processes, planet migration, celestial mechanics, and Saturns rings.\n\n\u003cstrong\u003eMartin Rey\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, University of Bath, UK\u003c/em\u003e.)  Galaxy formation and evolution, computational fluid dynamics, cosmology.\n\n\u003cstrong\u003eAleks Scholz\u003c/strong\u003e (\u003cem\u003eSchool of Physics \u0026 Astronomy, University of St Andrews, UK\u003c/em\u003e).  Exoplanets, brown dwarfs, protoplanetary disks, stellar evolution, star formation. \n\n\u003cstrong\u003eElena Sellentin\u003c/strong\u003e (\u003cem\u003eSterrewacht Leiden, Leiden University, The Netherlands\u003c/em\u003e). Applied Mathematics, Cosmology, Statistics, Statistical Inference.\n\n\u003cstrong\u003eHeloise Stevance\u003c/strong\u003e (\u003cem\u003eDepartment of Physics, University of Oxford, UK\u003c/em\u003e.) Transients, machine learning, sky surveys, supernovae.\n\n\u003cstrong\u003eElena Terlevich\u003c/strong\u003e (\u003cem\u003eInstituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico\u003c/em\u003e).  Stellar populations in galaxies, observational cosmology, violent star formation, element abundances, dynamics of stellar systems.\n\n\u003cstrong\u003eBingbing Wang\u003c/strong\u003e (\u003cem\u003eCenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, USA\u003c/em\u003e.) Particle astrophysics, MHD turbulence, cosmic rays acceleration, cosmic ray propagation in the Galaxy and heliosphere.,submission_guidelines:\u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e is an arXiv overlay journal. This means that, while we have a conventional Editorial Board and refereeing process, we apply this to papers on the \u003ca href\https://arXiv.org\\u003earXiv\u003c/a\u003e. The result of this is that the cost of running the journal is extremely low; we are therefore able to offer this service entirely free of charge both to authors and to readers.\n\n\u003cstrong\u003eIs my paper suitable?\u003c/strong\u003e We apply a simple criterion to decide whether a paper is on a suitable topic for this journal, namely that if - and only if - it  is suitable for the astro-ph section of the arXiv then it is suitable for  \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e. A breakdown of the areas covered by astro-ph is given \u003ca href\https://arxiv.org/archive/astro-ph/Astrophysics\\u003eon the arXiv\u003c/a\u003e but for reference here they are.\n\nThe astro-ph section of the arXiv is divided into six main areas:\n\u003col\u003e\n  \u003cli\u003e\u003cstrong\u003eastro-ph.GA\u003c/strong\u003e - \u003cem\u003eAstrophysics of Galaxies\u003c/em\u003e.\nPhenomena pertaining to galaxies or the Milky Way. Star clusters, HII regions and planetary nebulae, the interstellar medium, atomic and molecular clouds, dust. Stellar populations. Galactic structure, formation, dynamics. Galactic nuclei, bulges, disks, halo. Active Galactic Nuclei, supermassive black holes, quasars. Gravitational lens systems. The Milky Way and its contents\u003c/li\u003e\n  \u003cli\u003e\u003cstrong\u003eastro-ph.CO\u003c/strong\u003e - \u003cem\u003eCosmology and Nongalactic Astrophysics\u003c/em\u003e.\nPhenomenology of early universe, cosmic microwave background, cosmological parameters, primordial element abundances, extragalactic distance scale, large-scale structure of the universe. Groups, superclusters, voids, intergalactic medium. Particle astrophysics: dark energy, dark matter, baryogenesis, leptogenesis, inflationary models, reheating, monopoles, WIMPs, cosmic strings, primordial black holes, cosmological gravitational radiation\u003c/li\u003e\n  \u003cli\u003e\u003cstrong\u003eastro-ph.EP\u003c/strong\u003e - \u003cem\u003eEarth and Planetary Astrophysics\u003c/em\u003e.\nInterplanetary medium, planetary physics, planetary astrobiology, extrasolar planets, comets, asteroids, meteorites. Structure and formation of the solar system\u003c/li\u003e\n  \u003cli\u003e\u003cstrong\u003eastro-ph.HE\u003c/strong\u003e - \u003cem\u003eHigh Energy Astrophysical Phenomena\u003c/em\u003e.\nCosmic ray production, acceleration, propagation, detection. Gamma ray astronomy and bursts, X-rays, charged particles, supernovae and other explosive phenomena, stellar remnants and accretion systems, jets, microquasars, neutron stars, pulsars, black holes\u003c/li\u003e\n \t\u003cli\u003e\u003cstrong\u003eastro-ph.IM\u003c/strong\u003e - \u003cem\u003eInstrumentation and Methods for Astrophysics\u003c/em\u003e.\nDetector and telescope design, experiment proposals. Laboratory Astrophysics. Methods for data analysis, statistical methods. Software, database design\u003c/li\u003e\n \t\u003cli\u003e\u003cstrong\u003eastro-ph.SR\u003c/strong\u003e - \u003cem\u003eSolar and Stellar Astrophysics\u003c/em\u003e.\nWhite dwarfs, brown dwarfs, cataclysmic variables. Star formation and protostellar systems, stellar astrobiology, binary and multiple systems of stars, stellar evolution and structure, coronas. Central stars of planetary nebulae. Helioseismology, solar neutrinos, production and detection of gravitational radiation from stellar systems.\u003c/li\u003e\n\u003c/ol\u003e\n\nIf your paper fits into one or more of these areas then it may be considered for publication. For ease of reference \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e is divided into sections reflecting the above categories.\n\nPapers must be written in English.\n\nOnce submitted the Editors will enlist the help of suitably qualified referees to assess whether the paper meets the criteria of scientific quality, originality, relevance and comprehensibility needed to justify publication.\n\nWe may accept review articles on appropriate subjects if the Editorial Board considers  them a useful contribution to the literature.\n\n\u003cstrong\u003eSubmitting an Article\u003c/strong\u003e. To submit an article to the journal, you should first post it on the arXiv. When asked which licence you wish to use, you should select CC-BY. (If your article is already posted with a more restricted licence it is not a major problem, since you can give a different licence to the published version.) \n\nWe have a Latex style file which you can download \u003ca href\http://www.thphys.nuim.ie/staff/pcoles/openjournal.cls\\u003ehere\u003c/a\u003e.  Please note that source files for all our published papers are available on the arXiv so you can use any of these as a template if you dont know how to start.\n\nAlthough initial submissions can be made in any format acceptable to the arXiv, we prefer the final version to be typeset in this format and the process is therefore simplified if you use this at the outset.\n\nWhen the article has appeared on the arXiv, click on the \u003cem\u003eSubmit a manuscript\u003c/em\u003e button above and you will be taken through the very short submission process. If for some reason you have difficulty with the submission process, you can email an editor instead, who will be able to enter the paper into the system on your behalf.\n\nWe strongly encourage authors to submit in the manner described above (i.e. on the arXiv first). We can receive and review papers submitted directly to this platform but since the final version \u003cem\u003emust\u003c/em\u003e be on the arXiv in order to be published we feel it is far better to submit it there first in order to establish that it is on an appropriate topic for this journal.\n\n\u003cstrong\u003eThe Publication Process\u003c/strong\u003e. If your article is deemed  to be on a suitable topic for \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e, we will send it to referee(s) and then send you the comments of the referees. Once you have made any changes suggested by referees and/or editors, and the papers is accepted for publication we will add metadata (including the artice ID, acceptance date, etc) so that the accepted version can be posted to the arXiv. A Digital Object Identifier (DOI) will also be assigned and registered with CROSSREF for the purpose of citation tracking and bibliometric analysis. \n\nThe article will be added to the journal in the form of an overlay containing the abstract, author metadata, and the DOI, along  with a link to the arXiv entry.\n\nBecause we do not do copy-editing, we ask authors to take particular care with proofreading their articles before submitting their final version. We  do not offer an in-house copy-editing service but neither can we accept papers that are poorly written. If necessary, when a paper is rendered unacceptable by poor style we will refer authors to a third-party scientific copy-editing service, \u003ca href\http://www.scitext.com/\\u003eScitext Cambridge\u003c/a\u003e. Authors may wish to use this service before submission, to save time. The service is not free, but is \u003ca href\http://www.scitext.com/terms-and-prices/\\u003e relatively inexpensive\u003c/a\u003e and comes with the recommendation of the Managing Editor of \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e.\n\n\n\u003cstrong\u003eThe Editorial Process\u003c/strong\u003e. Articles will be evaluated exclusively with respect to our criteria of scientific quality, originality, relevance and comprehensibility.\n\nArticles submitted by our preferred route will already be in the public domain, since they will already have been posted to the arXiv. However, the information that they have been submitted to \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e will be not be disclosed to anyone other than those involved in the evaluation process and in the administration of the journal. This also applies to papers submitted directly to us.\n\nEditors may themselves submit papers to the journal, but if they do so, then all information about the processing of those papers will be hidden from their view and they will have no part in the decision process. \n\nEditors who have a significant conflict of interest connected with a paper will declare it to the other editors and will avoid participating in the decision process.\n\nWhen a paper is submitted it will be initially screened by the managing Editor and then assigned to an Editor who will engage the help of one or more referees in deciding on whether or not to accept the paper.\n\nWe expect Editors and Referees to carry out their duties fair-mindedly, diligently and without recourse to any form of inappropriate language.\n\n\u003cstrong\u003eResponsibilities of Authors\u003c/strong\u003e.  Authors should submit their own original work only. We will not accept papers submitted by individuals who are not in the author list of the paper.  Any results that are not due to the authors should be clearly cited. Copying or paraphrasing substantial parts of another paper without attribution is unacceptable, as is any other form of plagiarism. The arXiv submission process does an initial screen for plagiarism, and we will look very carefully at submissions that have triggered the arXiv filter.\n\nNo paper should be submitted to \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e that is already published elsewhere or is being considered for publication by another journal.\n\nThose named as authors of a paper should have made a substantial contribution to the paper, or to a more general project of which the paper is a part, and anybody who has made such a contribution should be offered authorship.\n\nAuthors who discover important errors in their articles, whether published or under consideration for publication, should notify the journal promptly.\n\nA more complete statement of our Ethics policy can be found \u003ca href\https://astro.theoj.org/pages/390-ethics\\u003e here\u003ca\u003e.\n\n\u003cstrong\u003eOur Commitments.\u003c/strong\u003e \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e is committed to the permanent availability and preservation of  scholarly research and ensures accessibility by partnering with Maynooth Academic Publishing, which maintains its own digital archive.\n\nArticles in \u003cem\u003eThe Open Journal of Astrophysics\u003c/em\u003e are published under a Creative Commons CC-BY licence and will be free to read in perpetuity. 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effect,Galaxy clusters,Galaxy dark matter halos,Astronomy data analysis,Atacama Cosmology Telescope,Cosmology: large-scale structure of Universe,Galaxies: clusters: intracluster medium,software,generative AI,Sunyaev-Zeldovich effect,X-ray clusters,Dark Matter halos,Modified Gravity,Horndeski,angular bispectrum,cosmography,dipole anisotropy,cosmic acceleration,Large Scale Structure of the Universe,Systematics amelioration,J-PLUS,Peculiar velocities,Standard sirens,Large-scale structure,Hubbles constant,Stratlearn,physics.data-an (Physics - Data Analysis, Statistics and Probability),discreteness,covariance matrix,Primordial magnetic fields,Bouncing cosmology,Quantum cosmology,early Universe,scalar fields,magnetogenesis,dark energy,Quaia,lensing,cross-correlation,large-scale structure of the Universe,intergalactic medium,Astrid simulations,spectroscopy,redshift drift,cosmic expansion,cosmic reionization,shot noise,third-order statistics,stat.ME (Statistics - Methodology),Gaussian Random Fields,strong lensing,clusters of galaxies,MACS J0138.0-2155,MUSE,Sunyaev-Zeldovich Effect,Galaxy Clusters,supernovae,Type Ia Supernova,CMB lensing tomography,FSB,Filtered-Squared Bispectrum,Stage-III weak lensing surveys,cosmology observations,intrinsic aligments,Weak gravitational lensing,Cosmological parameters,Galaxy Cluster,Observational Cosmology,Subaru,weak lensing,astro-ph.EP (Physics - Earth and Planetary Astrophysics),astro-ph.SR (Physics - Solar and Stellar Astrophysics),physics.plasm-ph (Physics - Plasma Physics),physics.space-ph (Physics - Space Physics),Magnetohydrodynamics,Hall Effect,Non-Ideal MHD,Ariel,Exoplanets,Extra Solar Planets,Machine Learning,KEPLER,rubble-pile asteroids,planetesimals,Moon,co-orbital,quasi-satellite,planets and satellites: detection,Kuiper belt: general,methods: observational,galaxy merger,UNIONS,Feedback,Supernovae,SIMBA simulations,binary stars,Broad-Line Region,Accretion Disks,Quasars,Magnetic Fields,WIMPs,Dark Matter Halos,Galaxy modeling,Gaia,ultra-diffuse galaxies,dwarf galaxies,dark matter,Cloudy,hep-ph (High Energy Physics - Phenomenology),subhaloes,Stellar Streams,Milky Way,high-redshift galaxies,Lyman-AlphaEmitters,Lyman-Alpha Radiative Transfer,satellite galaxies,Vera C. Rubin Observatory,Lyman Continuum radiation,Attenuation-Free Model,Modified Newtonian Dynamics,MOND,Binary Stars,General Relativity,population III stars,Primordial Black Holes,Supermassive Black Holes,IllustrisTNG,Star formation,binary star systems,quiescent galaxies,downsizing,stellar streams,metallicity,globular clusters,Metallicity,nucleosynthesis,ultra-faint dwarf galaxies,Reticulum II,early universe,dust,Soltan argument,sulphur,star-forming galaxies,Dark Energy Spectroscopic Instrument,stellar reddening,galactic dust,galaxy halo,normalizing flow,Dynamical Friction,Gravitational Instability,Galaxy Dynamics,Galaxy Nuclei,Galaxy Dark Matter Halos,Dark matter distribution,Galaxy radii,Large-scale structure of the universe,star clusters,galaxy structure,SMUDGes,Dwarf Galaxies,Spectroscopy,Stellar Abundances,Local Group,first galaxies,barred galaxies,outflows,starburst,quasar,absorption line,galaxies - enrichment,galaxies - dwarf,semi-analytic models,star formation quenching,Galaxy: structure,Galaxy: abundances,galaxies: structure,galaxies: abundances,velocity dispersions,M104,extragalactic distances,Instrumentation: detectors,Methods: data analysis,Techniques: image processing,Techniques: photometric,Galaxies: halos,LIGHTS survey,point spread function,Large Binocular Telescope,LISA,gravitational waves,low surface brigntness galaxies,galaxy properties,SMUDGes Survey,Magellanic Stream,Satellite Galaxies,molecular clouds,Andromeda,gravitational collapse,virial theorem,Wasserstein Generative Adversarial Network (WGAN) model,Oxygen,ALMA,JWST,post-merger galaxies,galaxy interactions,starburst galaxies,quasar absorption lines,circumgalactic medium,ultraviolet background,carbon IV absorption,Radial velocity,Chemical abundances,Survey,Stellar stream,Stellar halo,GAMA,Sloan Digital Sky Survey,Lyman-Alpha,Sunburst Arc,SMBHs,FLARES,Star Formation,turbulence,ISM: structure,star formation rate,Inverse Compton Emission,Cosmic Rays,Inverse Compton,CircumGalactic Medium,X-ray astronomy,Fermi-LAT,Gamma-Ray Astronomy,Galaxy Mergers,plasma turbulence,binaries: eclipsing,stars: neutron,stars: winds,X-rays: bursts,circumstellar matter,mass-loss,M31,Black Hole Formation,Neutrino Astrophysics,Supernova,photometry,astrophysical jets,numerical modelling,Cassiopeia A,SN 1572 (Tychos supernova),extinction,supernova remnants,Core-collapse supernovae,Near ultraviolet astronomy,Time domain astronomy,Transient sources,gamma-ray bursts,transients,ultra-long gamma-ray bursts,ULGRBs,Gamma-Ray Bursts,GRBs,AGN disks,Millisecond Pulsar,Redback pulsar,J0523.5-2529,Nuclear Transient,AT2020adpi,AGN variability,Tidal Disruption Event,(stars:) white dwarfs,(stars:) supernovae: general,(stars:) binaries: close,ISM: supernova remnants,(ISM:) planetary nebulae: general,maria,sub-mm observations,mock galaxy catalogues,astro-ph.GA(Physics - Galaxy Astrophysics),Python,galaxy surveys,blended images,satellites,thermal emission,millimetre waves,time domain astronomy,cosmic microwave background radiation,Euclid,UKIDSS,neural networks,Fermi Paradox,SETI,Forbush decrease,space weather,neutron monitor,fractal dimension,entropy measures,galaxies: high-redshift,cosmology: early universe,Hanbury Brown and Twiss,stellar astrophysics,intensity interferometry,stellar dynamics,Photometric Redshifts,Deep Learning,correlation functions,clustering,inference,technosignature,seti,AGB stars,White Dwarf stars,All Sky Automated Survey for SuperNovae,ASAS-SN,Variable Stars,AM CVn stars,Atacama Large Millimetre Array,Solar Physics,Kepler,stellar flares,protoplanetary disks,parallax,Gaia DR3,Symbiotic Stars,classical novae,stellar physics,LAMOST J2354,white dwarf,stars: jets,stars: AGB and post-AGB,binaries: close,stars: white dwarfs,planetary nebulae: general,supernova natal kicks,population synthesis,fine structure constant,Big Dippers,binaries,eclipsing,spectroscopic,heartbeat stars,TESS,Eclipses,Protoplanetary disks,Circumstellar disks,Dust composition,evolved stars,massive stars,stellar kinematics,Magellanic Clouds,Fokker-Planck equation,transport equation,energetic particles,Low-mass Stars,rotational evolution,math-ph (Mathematical Physics),math.MP (Mathematics - Mathematical Physics),radiative transfer,solar atmosphere,focused transport equation,Zeta Boötis,Eta Ophiuchi,Eccentricity,astrophysics,gravity,numerical simulations,stellar feedback,interstellar medium,astrophysics of galaxies,properties of galaxies,galaxy-halo connection,black hole seeds,Radio galaxies,X-ray galaxies,Chandra,XMM-Newton,Swift,ROSAT,Asymmetric Drift,LAMOST,Axions,Particle Physics,QCD Axions,topological defects,Baryonic Matter,Random Forest,Explainable Boosting Machine,IllustrisTNG100,JAX,power spectra,bayesian model selection,galactic disk,vertical structure,galaxy,milky way,bayesian methods,Bayesian model selection,harmonic mean estimator,normalizing flows,Bayesian evidence estimation,marginal likelihood estimation,bias,multipole expansion,Binaries: Eclipsing,Techniques: Photometric,Stars: individual:V717 And,binaries: spectroscopic,stars: emission-line,stars: black holes,spectroscopic binaries,stars,Black Hole,Numerical,Super Massive Stars,ENZO,black hole physics,tidal disruptions,partial tidal disruptions,galactic nuclei,semi-analytical methods,high-energy astrophysical phenomena,solar and stellar astrophysics,neutron stars,orbits,Brown Dwarfs,Eclipsing Binaries,Close Binaries,Magnetic Braking,camspec,likelihood,Carbon IV,Absorption Lines,Photoionization,QSO PG1522+101,chemically peculiar star,Population III,Population II,Stellar Nucleosynthesis,Type 1a SN,LAMOST J1010+2358,citizen science,Craters,lunar craters,Planetary Science,CMB,y-distortion,high redshift,MoM-Z14,Cosmic Microwave Background,Open Science,Data Curation,Reproducibility,raw data,data products,Data analysis,Planck,ACT,SPT,Cosmic MIcrowave Background,Mapmaking,Instrumentation and methods for astrophysics,cosmic shear surveys,Bayesian Methods,Neural Nets,galaxy redshift surveys,neural operators,chemistry solver,Grackle,baryon acoustic oscillations,galaxy alignments,CombineHarvesterFlow,Cosmic inflation,scalar field,inflation,Monte Carlo Sampling,E-Mode,B-mode,Power spectrum,quadratic bias,shape measurement statistics,Discovery Simulations,haloes,halo mass,halo concentration,primordial black holes,expansion history,big bang nucleosynthesis,microhalos,early universe phase transitions,baryogenesis,cosmic inflation,Control Variates,Statistical methods,splashback,infall,SPTPol,Sunyaev-Zeldovich Effect,Therman Sunyaev-Zeldovich effect,South Pole Telescope,Three Hundred Project,protoclusters,cosmic horizons,relative speed,parallel transport,recession speed,mass reconstruction,Minkowski Functionals,mass mapping,cosmology and nongalactic astrophysics,peculiar velocities,graph networks,data analysis methods,galaxy-galaxy lensing,local universe,monopole,21cm Radiation,Cosmic Dawn,Dark Ages,proper motions,gravitational lens equation,hyperbolic umbilic,cumulant generating function,probability density function,one-point probability density function,two-point probability density function,weak gravitation lensing,Kilo-Degree Survey,KIDS,Angular Power Spectrum,Limber Approximation,Statistical Methods,Unified Dark Matter,Substructure,Haloes,Numerical Methods,Back-reaction,Einstein Toolkit,numerical relativity,Julia,two-point autocorrelation function,two-point cross-correlation function,Tomography,Dark Energy Science Collaboration,Schrodinger-Poisson system,Wave Mechanics,cosmic voids,void evolution,Mass Maps,Markov Chain Monte Carlo,Wavelets,Data Analysis,Instrumentation and Methods for Astrophysics,Power Spectrum,Masked Sky,ΛCDM,Tensions,Hubble Tension,Cepheid Distances,Cosmology and NonGalactic Astorphysics,Cosmology and NonGalactic Astrophysics,cosmic web,Cosmology: large-scale structure of the Universe,Galaxies: fundamental parameters,GPU,Stellar Populations,methods: N-body simulations,gas physics,cosmology:miscellaneous,cosmology: observations,large-scale structure of universe,distance scale,cosmology: theory,cosmology theory,galaxy groups,galaxy halos,fossil groups,cosmology - theory,analytical methods,Schrödinger–Poisson,cosmological density fields,wave mechanics,Low Surface Brightness Galaxies,galaxy haloes,n-body simulations,dark-matter,axion,cosmological parameter estimation,type1a supernovae,Rubin Observatory,statistical methodology,Marginalised Normal Regression,Regression,Curve Fitting,karhunen—loève expansion,Data methods,cosmology: miscellaneous,software: simulations,wavelet phase harmonics,dual AGN,minor merger,dwarf galaxy,X-ray observations,MAGNETICUM,Dwarf galaxies,Chemical evolution,Stellar abundances,High-redshift galaxies,Star formation history,field galaxy,star-formation,large-scale environment,TNG50,LMC,SMC,dynamical systems,cosmological models,anisotropic cosmology,bianchi i cosmology,spatial curvature,early-type galaxies,NGC 3640,Earth and Planetary Astrophysics,Ephemeris Matching,K2 mission,Extrasolar Planets,Kepler Space Telescope,Einstein ring,Gravitational Lensing,Strong Gravitational Lensing,erosita,galaxies: groups: general,galaxies: clusters: general,galaxies: clusters: intracluster medium,cosmology: large-scale structure,x-rays: galaxies: clusters,euclid consortium,galaxy clustering statistics,euclid,Exoplanet catalogs,Astronomy databases,Astrostatistics tools,Computational methods,dynamical evolution,mean motion resonance,Kepler satellite,Exoplanet Systems,Planetary System Architectures,exoplanet systems,exoplanet formation,exoplanet evolution,obliquity,beta Pictoris,Radio Transients,Astronomical Software,Sources,High-Energy Astrophysical Phenomena,radio sources,low mass galaxies,high-redshift,galaxy simulations,forward-modelling,surveys,hydrodynamical simulations,ASTRID simulations,quadruple images,supernova,galaxy astrophysics,tidal fields,cosmic large-scale structure,tidal torques,computational,stellar content,numerical,COSMOS,High-redshift,Simulations,Tully-Fisher Relation,Baryonic Tully-Fisher Relation,galaxies: formation,galaxies: evolution,intracluster medium,galaxies: halos,galaxies: dark matter,galaxies: kinematics and dynamics,Astrophysics - Astrophysics of Galaxies,Method - Statistics,Galaxy Astrophysics,Wide Binary Systems,Stellar Dynamics,Intracluster medium,LambdaCDM,Galaxy Haloes,Galaxy-Galaxy lensing,galaxy outflows,interstellar turbulence,CSWA13,statistics,galaxy shapes,galaxy mergers,gaussian mixture model,Schwarzschild metric,General relativity,warp drives,null energy condition,Galactic Structure,Globular clusters,Galaxy formation,Galaxy evolution,Star clusters,Globular Clusters,Pulsars,gravitation,WFI2033-4723,hep-th (High Energy Physics - Theory),Gauge Theory,Cosmic Inflation,High Energy Physics,Palatini Formalism,high energy astrophysical phenomena,instrumentation and methods for astrophysics,extragalactic astrophysics,multimessenger astrophysics,Ultra-High-Energy Cosmic Rays,angular cross-correlation,spherical harmonics,signal-to-noise ratio,Gamma-rays,BL Lac objects,SED,Spectral Energy Distribution,compact objects,Zwicky Transient Facility,black hole,neutron star,Solar and Stellar Astrophysics,binary mass transfer,helium stars,Interstellar Medium,ISM,white dwarfs,stellar jets,High Energy Astrophysics,Statistics,Log-Normal Distribution,Keck spectroscopy,HII regions,UV and Optical spectroscopy,Balmer Jump,MEGATRON,galaxy spectra,Horndeski Gravity,modified gravity,Einstein-Boltzmann solver,inference in cosmology,Monte-Carlo Markov-chains,Bayesian evidence,supernova cosmology,MCMC,generative models,Cosmology and Extragalactic Astrophysics,Implicit Likelihood Inference,Inference,likelihood-based inference,atmospheric modelling,atmospheric seeing,interstellar matter,Ionisation,Jets,Supernovae remnants,High Energy Astrophysical Phenomena,core-collapse supernovae,baryonic physics,redshift surveys,Schrödinger-Poisson,baryon feedback,massive neutrinos,f(R) gravity,Large-scale Structure of the Universe,light cones,Large-Scale Structure of the Universe,Intracluster Medium,Astronomical Simulations,large-scale structure of Universe,cosmology:observations,galaxies-high-redshift,galaxies-clustering,galaxies-statistics,galaxies-environment,marked correlation function,lenticular galaxies,elliptical galaxies,irregular galaxies,spiral galaxies,methods: data analysis,luminosity function,ultracool dwarfs,cool stars,Stellar Spectroscopy,Statistical Inference,Data-driven Model,Support Vector Machines,Neural Networks,Light curves,Magnetars,Giant flares,AXIS,$\\gamma$ rays,X-rays,stellar mass loss,SN 2024ggi,methods: analytical,galaxy dynamics,structure of galaxies,cosmology: large-scale structure of Universe,cosmic dipole,Dark Matter Halo,Large Magellanic Cloud,Molecular Cloud Collisions,Central Molecular Zone,Milky Way Disk,n-body,solarsystem,planets,N-body Integrator,Computational Methods,Solar System,Planetary Dynamics,Numerical method,Computational Physics,neural network,astronomical image processing,galaxy image denoising,neutral hydrogen,HI gas,post-starburst galaxies,21cm observations,Neutron star,Astrophysics - High Energy Astrophysical Phenomena,stellar evolution,Neutron Stars,SKAO,stability,large scale structure of the universe,orbital dynamics,direct imaging,Fomalhaut,planetary dynamics,solar system formation,stellar flyby,rogue planet,Plasma Physics,MHD,plasma physics,PSF,coaddition of images,Image processing,astronomical imaging,primordial black hole,supermassive black hole,black hole seeding,simulation,microwave spectroscopy,external photoevaporation,observations,Publications,Bibliography,Astronomical Observatories,Digital Libraries,Physics and Society,Astronomy,Pulsar,Ionised Interstellar Medium,Solar Wind,TSAS,Ionosphere,Radio Astronomy,pulsars,binary pulsars,SKA,Galactic centre,Gravitational waves,Supermassive black holes,Pulsar Timing Array,Dense matter,Equation of State,pulsars: general,radiation mechanisms: general,plasmas,telescopes,Stars: neutron,ISM: general,Stars: black holes,Instrumentation: interferometers,pulsar timing arrays,statistical anaisotropy,gravitational wave background,Software,intracluster mediu,pressure profiles,x-ray variability,Milliquas,random fields,Gaussian fields,Non-Gaussian fields,Primordial Density Fluctuations,redshift,statistical bias,Redshift Drift,Black Hole Shadow,Test of the Equivalence Principle,red supergiants,mass loss,ultra-violet,Lyman continuum,roque 12,pleiades,eclipsing binary,brown dwarf,SDSS-C4 3028,sed,luminosity,k-correction,SiPM,Ultra-Fast Astronomy,Fast Readout,pulsar wind nebulae,stellar variability,brown dwarfs,stellar pulsation,SSTc2d J163134.1-240100,Stellar Evolution,Instrumentation and Methods for Astronomy,Coronal Mass Ejections,Edge Detection,STEREO SECCHI HI-1,Pair Instability,Supernova relics,Solar and Stellar Physics,Galactic Astrophysics,magnetohydrodynamics,Star Clusters,SpikeNet,spike bursts,solar,radio,NenuFAR,semantic segmentation,convolutional neural network,Accretion Disk,radiation transfer,galaxy quenching,stars (initial mass function),High-Energy Astrophysical Phenomena,STARFORGE,feedback processes,early galaxies,Young stellar objects,Infrared stars,molecular cloud cores,millimetre dust and gas emission,PGCC 120.69+2.66,activities,binary,ages,moving groups,Galex,Stars,(stars:) binaries (including multiple): close,supernovae: general,transients: supernovae,stars: mass-loss,stars: variables: general,binaries (including multiple): close,common envelope evolution,galaxies: clusters,galaxies: jets,stars: Population III – dark ages,first stars,stars: luminosity function,mass function,equation of state,cosine-100,information theory,marginalisation,nuisance parameters,observational systematics,Nested Sampling,MultiNest,Stellar accretion,Neural networks,stellar magnetic activity,differential rotation,V889 Her,spectropolarimetry,stellar mergers,cataclysmic variables,red 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