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    <loc>https://www.astrochemistryreport.com/articles/rosa-asteroid-precursor</loc>
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    <lastmod>2026-03-09</lastmod>
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      <image:title>Articles - Potential Precursors for Life Found in a Carbon-Rich Asteroid - Make it stand out</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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    <loc>https://www.astrochemistryreport.com/articles/kessler-ai-neural-network</loc>
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    <lastmod>2026-03-08</lastmod>
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      <image:title>Articles - Artificial Intelligence at the Service of Astrochemistry - Make it stand out</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/taniguchi-missing-middle</loc>
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    <lastmod>2026-02-16</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/9611b31f-2376-44ca-a4d8-077598966aab/Figure1_Yebes.jpg</image:loc>
      <image:title>Articles - Bridging the Mass Gap: Chemical Complexity from Low- to High-Mass Star Formation - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>Articles - Bridging the Mass Gap: Chemical Complexity from Low- to High-Mass Star Formation</image:title>
      <image:caption>Fig.2: Comparisons of molecular abundances with respect to HC3N for carbon-chain species (top), and complex organic molecules, H2CCO, and HNCO (bottom). Errors indicate the standard deviation. In the caption, “high” and “low” indicate the high and low temperature components. The dashed red lines mark the abundance ratios for the low-mass WCCC source L1527 Credit: Yoshida et al. 2019</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/fadul-com-protoplanetdisk</loc>
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    <lastmod>2026-02-15</lastmod>
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      <image:title>Articles - A Deep Search for Complex Organic Molecules Around the V883 Ori Protoplanetary Disk - Make it stand out</image:title>
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      <image:title>Articles - A Deep Search for Complex Organic Molecules Around the V883 Ori Protoplanetary Disk - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/jaziri-exoplanet-k219b</loc>
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    <lastmod>2026-01-31</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/c1acc2fd-64ac-4966-a59d-dd6f296ae04d/Fig1_K2-18b.jpeg</image:loc>
      <image:title>Articles - K2-18 b: A Carbon-Rich Planet with a Methane-Dominated Atmosphere - Make it stand out</image:title>
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      <image:title>Articles - K2-18 b: A Carbon-Rich Planet with a Methane-Dominated Atmosphere - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/alvarado-torres-alma</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/59b33c1c-7e40-4d45-b0bb-123814c4912d/Figure-DISKS-Website_thumb.jpg</image:loc>
      <image:title>Articles - How Hydrogen’s Twin Helps Uncover the Hidden Gas in Protoplanetary Disks - Make it stand out</image:title>
      <image:caption>Fig. 1. Top: Gas in young planet-forming disks, traced with CO molecules (obtained from MAPS Program, Oberg et al. 2021). Bottom: Dust in the same disks, seen in millimeter-wavelength light (obtained from DSHARP Programme, Andrews et al. 2018; Huang et al. 2020; MAPS Oberg et al. 2021).</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/bonfand-gorai-isolated-star</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/693c0d1b-1e9c-458d-808b-86514e96c3f6/Gorai_et_al_Fig1.png</image:loc>
      <image:title>Articles - A Lonely Massive Star Reveals Secrets of Stellar Chemistry</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/missing-sulfur-reservoir-taillard</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/b729d7db-eea3-4745-b8bd-0a55bbaad558/sulfur_vibing.png</image:loc>
      <image:title>Articles - Predicting the Missing Sulfur Reservoir with Synthetic Observations and Laboratory Experiments - Make it stand out</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/alvarado-torres-hso</loc>
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    <lastmod>2026-01-26</lastmod>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/steffer-new-insights-into-formaldehyde-formation</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:title>Articles - Unraveling Cosmic Chemistry: New Insights into Formaldehyde Formation - Make it stand out</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/discovery-alma-imf-bonfand</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/cb0eca1d-566e-43a7-9bcf-0ffd682de14f/unnamed.png</image:loc>
      <image:title>Articles - Hidden Nurseries of Stars Unveiled Thanks to a Sweet-Smelling Cosmic Clue - Make it stand out</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/104a378f-dde2-42e8-9ee0-16d8796c3412/fig2.png</image:loc>
      <image:title>Articles - Hidden Nurseries of Stars Unveiled Thanks to a Sweet-Smelling Cosmic Clue - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/shopeicesjwst</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:title>Articles - Unlocking Secrets in Ice with The James Webb Space Telescope - Make it stand out</image:title>
      <image:caption>Figure 1: An illustration of a dust grain in space. On these dust grains, molecules form via various interstellar mechanisms.</image:caption>
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  </url>
  <url>
    <loc>https://www.astrochemistryreport.com/articles/christiansonmifsud</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/aa50922a-9823-4b9f-ba0d-0cb489ac4996/christiansondiagram.png</image:loc>
      <image:title>Articles - Unveiling the Origins of Sulfur in Comets - Make it stand out</image:title>
      <image:caption>Figure 1: A top-view schematic diagram of the ICA experimental setup, showing how ions hit the ice surfaces at a 36° angle while an infrared beam passes straight through the ice to analyze the results.</image:caption>
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  </url>
  <url>
    <loc>https://www.astrochemistryreport.com/articles/scibelli</loc>
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    <priority>0.5</priority>
    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/9b67463d-2193-43c6-bc1f-b43248b0f1cf/scibelligraphic2.jpeg</image:loc>
      <image:title>Articles - Hot off the disk: New detections of complex molecules in warm planet-forming disks - Make it stand out</image:title>
      <image:caption>Emissions of molecules studied by Booth et al. 2024 toward IRS 48. The bright emissions indicate the presence of that molecule in that region of space. This data was collected by ALMA, a radio telescope.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/yassin2024</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/a058cb8c-334e-461e-8e31-e4b76c862302/GJ1214b_GCM_Charnay2015.gif</image:loc>
      <image:title>Articles - Scientists Uncover Flaws in Common Models for Studying Exoplanet Atmospheres - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>Articles - Scientists Uncover Flaws in Common Models for Studying Exoplanet Atmospheres - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/stelmachchirality</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/78b83c6d-4c4e-40db-a613-519a2084ac94/handedness.jpg</image:loc>
      <image:title>Articles - Life’s Building Blocks Have a Handedness and a Cosmic Connection - Make it stand out</image:title>
      <image:caption>Figure 1. Above is a pair of molecules that are non-superimposable mirror images of one another. Pairs like this are called enantiomers. This molecule here is a generic amino acid where the R group represents some chemical group that is not already represented (-COOH, -NH2, -H).</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/aa6c66a0-4618-43d2-9074-ff5ae7d5556f/kamildiagram.jpg</image:loc>
      <image:title>Articles - Life’s Building Blocks Have a Handedness and a Cosmic Connection - Make it stand out</image:title>
      <image:caption>Figure 2. A modified diagram from Meierhenrich (2008) edited to show some other symmetry breaking hypotheses since the book’s publication. Since 2008, Globus et al. (2021) suggested that polarized muons could have led to enantioselective mutagenesis, which in turn could have allowed more favorable mutations to a lineage of proto-organisms or prebiotic chemistry that was using the “correct” chirality. The CISS effect, which has utilized a strong magnetic field and large, flat magnetite surfaces, has been able to produce strong biases. However, it remains to be seen if it can operate in an astrophysically or prebiotically relevant environment. In my own research, I am studying to see whether circularly polarized light could have indirectly influenced the chirality of amino acids and sugar alcohols by first biasing a chiral inorganic intermediate, namely, clinoenstatite.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/flint2023</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/98627e31-4dd3-43c3-8a30-b9669f38dcba/fig1flint.png</image:loc>
      <image:title>Articles - Galactic sandbox: From quartz clouds to lunar water generation - Make it stand out</image:title>
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      <image:title>Articles - Galactic sandbox: From quartz clouds to lunar water generation - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/rocha2023</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:title>Articles - Detections of Complex Molecules in Interstellar Ices - Make it stand out</image:title>
      <image:caption>Figure 1: Fits of JWST spectral data of high-mass protostar IRAS 23385 (top) and low-mass protostar IRAS 2A (bottom) to laboratory infrared data. Legend corresponds to the ice mixture used in the fits. Ice mixtures are representative of astronomical conditions of molecules on ice surfaces that have a varying degree of solid ices present. Credit: Rocha et al. 2023</image:caption>
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  <url>
    <loc>https://www.astrochemistryreport.com/articles/bonfandsalty</loc>
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    <lastmod>2026-01-26</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/2288d2d1-f056-4671-8477-d38f631db3a8/Figures_salt_detection.png</image:loc>
      <image:title>Articles - The environment of massive stars is salty! - Make it stand out</image:title>
      <image:caption>Figure 1: Example of the spectral data delivered by the ALMA telescope. This spectrum represents the chemical signature of the disk around the young massive star Orion Source I. It reveals all the molecular species responsible for the emission coming from the disk, seen as “spikes” in the spectrum at different frequencies, and of which the intensities are measured in units of “Jansky per beam” (power per unit area, unit frequency, and unit solid angle). In total, about 60 different transitions of KCl (in blue) and NaCl (in red) were identified, confirming their detection. Image credit: The Astrophysical Journal, Ginsburg, A., et al. (2019), ApJ, 872, 54.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/7eee0cc9-f1c5-4cab-8e1f-dd103f6c5d8d/envelope.png</image:loc>
      <image:title>Articles - The environment of massive stars is salty! - Make it stand out</image:title>
      <image:caption>Figure 2: 2D schematic view of a forming star, that accretes material from its surrounding spherical envelope, through its accretion disk.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/649b4c4df57a68563f3f3e90/19778ff3-6440-4c52-9413-a520806b65cc/Figures_salt_detection2.png</image:loc>
      <image:title>Articles - The environment of massive stars is salty! - Make it stand out</image:title>
      <image:caption>The blue ring shows the ALMA image of the salty disk surrounding the young massive star Orion Source I (Ginsburg, A., et al. 2019, ApJ, 872, 54). The narrow vertical extent of the salt emission indicates that NaCl is off the dust grains following their destruction, nearly immediately after being raised from the surface of the disk. The background image, taken from the Gemini Observatory, shows the Orion cloud, a region of explosive starbirth, located about 1500 light-years from Earth. Image credit: ALMA (NRAO/ESO/NAOJ); NRAO/AUI/NSF; Gemini Observatory/AURA.</image:caption>
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    <lastmod>2024-12-19</lastmod>
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