<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:media="http://search.yahoo.com/mrss/" xmlns:atom="http://www.w3.org/2005/Atom">
  <channel>
    <title>The Open Journal of Astrophysics</title>
    <link>https://astro.theoj.org/</link>
    <description>The Open Journal of Astrophysics is an arXiv overlay journal providing open access to peer-reviewed research in astrophysics and cosmology.</description>
    <language>en</language>
    <atom:link href="https://astro.theoj.org/feed" rel="self" type="application/rss+xml"/>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/170057/medium/deugenio.jpg?1788942387"/>
      <title>A Dusty Quenching-Candidate AGN host at $z = 5.7$: massive quiescent galaxies may quench already during the dust-obscured phase</title>
      <pubDate>Wed, 09 Sep 2026 03:25:00 -0500</pubDate>
      <description>RUBIES-EGS-9809, a dust-reddened galaxy with a dominant point-source component, suggests that AGN feedback may influence its host., indicating that massive galaxies can host evolved stellar populations during their dust-obscured phase.</description>
      <guid>https://doi.org/10.33232/001c.170057</guid>
      <link>https://astro.theoj.org/article/170057-a-dusty-quenching-candidate-agn-host-at-z-5-7-massive-quiescent-galaxies-may-quench-already-during-the-dust-obscured-phase</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169866/medium/lazarev.jpg?1788767569"/>
      <title>Dependences of radio pulsar parameters on the kick velocity</title>
      <pubDate>Mon, 07 Sep 2026 02:51:00 -0500</pubDate>
      <description>This study analyzes the velocity kick of neutron stars, finding that 23% belong to the low-velocity mode. Differences in magnetic field distribution emerge, but no significant bimodality in physical parameters.</description>
      <guid>https://doi.org/10.33232/001c.169866</guid>
      <link>https://astro.theoj.org/article/169866-dependences-of-radio-pulsar-parameters-on-the-kick-velocity</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169865/medium/deming.jpg?1788766713"/>
      <title>The Third Option: Color Phase Curves to Characterize the Atmospheres of Temperate Rocky Exoplanets</title>
      <pubDate>Mon, 07 Sep 2026 02:37:00 -0500</pubDate>
      <description>The study proposes using color phase curves to detect and characterize the atmospheres of rocky exoplanets, including non-transiting ones, by observing their longitudinal heat transfer.</description>
      <guid>https://doi.org/10.33232/001c.169865</guid>
      <link>https://astro.theoj.org/article/169865-the-third-option-color-phase-curves-to-characterize-the-atmospheres-of-temperate-rocky-exoplanets</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169864/medium/dattathri.jpg?1788765786"/>
      <title>Not all cores are equal: Phase-space origins of dynamical friction, stalling and buoyancy</title>
      <pubDate>Mon, 07 Sep 2026 02:22:00 -0500</pubDate>
      <description>How the distribution function of a galaxy, not just its central density gradient, influences the efficiency and direction of dynamical friction, affecting the movement of massive objects within it.</description>
      <guid>https://doi.org/10.33232/001c.169864</guid>
      <link>https://astro.theoj.org/article/169864-not-all-cores-are-equal-phase-space-origins-of-dynamical-friction-stalling-and-buoyancy</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169445/medium/koposov.jpg?1788440536"/>
      <title>CORRECTION - DESI Data Release 1: Stellar Catalogue</title>
      <pubDate>Thu, 03 Sep 2026 07:55:00 -0500</pubDate>
      <description>The paper "DESI Data Release 1: Stellar Catalogue" by Koposov et al. contained a Figure that was incorrect. This has now been corrected.</description>
      <guid>https://doi.org/10.33232/001c.169445</guid>
      <link>https://astro.theoj.org/article/169445-correction-desi-data-release-1-stellar-catalogue</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169444/medium/berton.jpg?1788420738"/>
      <title>How similar are narrow-line Seyfert 1 galaxies and high-z type 1 AGN?</title>
      <pubDate>Thu, 03 Sep 2026 02:28:00 -0500</pubDate>
      <description>The study reviews the properties of local narrow-line Seyfert 1 galaxies and compares them with high-redshift active galactic nuclei, aiding understanding of early black hole evolution.</description>
      <guid>https://doi.org/10.33232/001c.169444</guid>
      <link>https://astro.theoj.org/article/169444-how-similar-are-narrow-line-seyfert-1-galaxies-and-high-z-type-1-agn</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169299/medium/fores_toribio_2.jpg?1788332601"/>
      <title>The neighboring stars of N6946-BH1 and the observational characteristics of failed supernovae</title>
      <pubDate>Wed, 02 Sep 2026 02:01:00 -0500</pubDate>
      <description>The study re-analyzes images of potential failed supernova N6946-BH1, finding four unrelated near-infrared neighbors. It also compares the luminosity of failed supernova remnants to stellar merger remnants, noting significant differences.</description>
      <guid>https://doi.org/10.33232/001c.169299</guid>
      <link>https://astro.theoj.org/article/169299-the-neighboring-stars-of-n6946-bh1-and-the-observational-characteristics-of-failed-supernovae</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169213/medium/tucker_scat.jpg?1788248106"/>
      <title>SCAT Data Release 1: 1812 optical spectra of 1331 transients</title>
      <pubDate>Tue, 01 Sep 2026 02:34:00 -0500</pubDate>
      <description>The first data release of the Spectroscopic Classification of Astronomical Transients survey includes 1812 spectra of 1331 transients, offering valuable insights for photometric/light curve classification pipelines.</description>
      <guid>https://doi.org/10.33232/001c.169213</guid>
      <link>https://astro.theoj.org/article/169213-scat-data-release-1-1812-optical-spectra-of-1331-transients</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/169008/medium/royer_magrathea.jpg?1788159252"/>
      <title>Modeling Carbon-Based Planets with MAGRATHEA</title>
      <pubDate>Mon, 31 Aug 2026 01:50:00 -0500</pubDate>
      <description>A modification of the planetary interior solver MAGRATHEA to include Carbon-based mantles to enable it to understand more fully the range of possible planet structures.</description>
      <guid>https://doi.org/10.33232/001c.169008</guid>
      <link>https://astro.theoj.org/article/169008-modeling-carbon-based-planets-with-magrathea</link>
    </item>
    <item>
      <media:content type="image/jpeg" url="https://s3.amazonaws.com/production.scholastica/article/168763/medium/simon.jpg?1787900007"/>
      <title>The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models</title>
      <pubDate>Fri, 28 Aug 2026 01:52:00 -0500</pubDate>
      <description>The study explores the impact of non-Gaussian line spread function (LSF) profiles on stellar kinematics recovery. A method was developed to reduce bias in dispersion, with a Python implementation available.</description>
      <guid>https://doi.org/10.33232/001c.168763</guid>
      <link>https://astro.theoj.org/article/168763-the-impact-of-non-gaussian-line-spread-functions-on-stellar-kinematic-recovery-consequences-for-dynamical-models</link>
    </item>
  </channel>
</rss>
