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- IUP-CO2M-REB-TN-1000 – Requirements Justification Report for anthropogenic CO2 Monitoring Mission (CO2M)
- SRON-CO2M-TN-2018-01 – Multi-Angle Polarimeter Reference Spectra
- SRON-CSS-TN-2021-004 – Cloud Imager Requirement Analysis for the Copernicus CO2 Monitoring mission
- SRON-CSS-TN-2020-001 – Study on Spectral Sizing for CO2 Observations: Executive Summary
- SRON-CSS-TN-2020-002 – Study on Spectral Sizing for CO2 Observations: Final Report
- SRON-ESA-S5L2PP-ATBD-001 – Sentinel 5 L2 Prototype Processors Algorithm Theoretical Baseline Document: Methane Retrieval
- SRON-ESA-S5L2PP-ATBD-002 – Sentinel 5 L2 Prototype Processors Algorithm Theoretical Baseline Document: Carbon Monoxide Retrieval
- SRON-ESG-RP-2021-010 – RemoTAP Algorithm Theoretical Baseline Document
- SRON-ESG-TN-2021-003 – Satellite instruments for CH4 and CO2 hotspot detection
- SRON-TROPSC-TN-2011-002 – Instrument noise model for the Sentinel 5 SWIR bands
The temperature and metallicity distributions of the ICM: insights with TNG-Cluster for XRISM-like observations
01/04/2026 - High-Energy
The new era of high-resolution X-ray spectroscopy will significantly improve our understanding of the intracluster medium (ICM) by providing precise constraints on its underlying physical properties. However, spectral fitting requires reasonable assumptions on the thermal and chemical distributions of the gas. We use the output of TNG-Cluster, the newest addition to the IllustrisTNG suite of…
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Asymmetric Distribution of Fe-peak Elements in Cassiopeia A Revealed by XRISM
01/04/2026 - High-Energy
The elemental abundances of the Fe-peak elements (such as Cr, Mn, Fe, and Ni) and Ti are important for understanding the environment of explosive nuclear burning for the core-collapse supernovae (CCSNe). In particular, the supernova remnant Cassiopeia A (Cas A), which is well known for its asymmetric structure, contains three “Fe-rich blobs,” and the composition…
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A JWST Transit of a Jupiter Analog. I. Constraints on the Oblateness of Kepler-167 e
01/03/2026 - Exoplanets
In 2024 October, JWST observed a transit of Kepler-167 e, a Jupiter-analog planet on a 1000+ day orbit. These observations, recorded over a long baseline of nearly 60 hr, were designed to search for signatures of planetary oblateness and/or exomoons comparable to Ganymede. In this first in a series of studies analyzing these data, we…
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