Astronomical Observatory of Capodimonte

Recent papers from Astronomical Observatory of Capodimonte

1. Euclid Data Release 1 (DR1). Near-infrared processing and data products2026
2. Euclid Data Release 1 (DR1). Persistence in NISP detectors2026
3. Euclid: Data Release 1 (DR1) - First NISP emission-line maps: Methodology, validation, and applications to galaxy evolution2026
4. Euclid data release 1 (DR1) - SIR spectroscopic calibration2026
5. Euclid Data Release 1 (DR1). The PHZ processing function for the physical properties of galaxies2026
6. Euclid Data Release 1 (DR1). NIR astrometric calibration2026
7. Euclid Data Release 1 (DR1). Colouring Euclid with external ground-based imaging data2026
8. Euclid Data Release 1 (DR1) - NISP-P point-spread function modelling pipelines2026
9. Euclid Data Release 1 (DR1). An overview of the Science Ground Segment architecture and operations2026
10. Euclid Data Release 1 (DR1) Euclid photometric masks2026
11. Euclid Data Release 1 (DR1): Spacecraft performance in the L2 environment2026
12. Euclid Data Release 1 (DR1). Multi-band photometry validation on COSMOS extragalactic sources2026
13. Euclid Quick Data Release (Q1). Refining the strong lens sample with Space Warps crowd-sourced science2026
14. Reconciling the Fundamental Plane of Early-Type Galaxies with hydrodynamical simulations: The case of IllustrisTNG100-1Monthly Notices of the Royal Astronomical Society · 2026
15. JWST’s Dusty Blue BOAT - GRB 221009AMonthly Notices of the Royal Astronomical Society · 2026
16. A Study on the geoeffective event of 11 April 20222026
17. Hydrogen-line Emission in Accreting Low-mass Objects. I. Spectral Analysis of Shock-origin Narrow ComponentThe Astronomical Journal · 2026
18. JUICE-JANUS observations of Earth in preparation for the JANUS investigation of Jupiter's atmosphereAnnales Geophysicae · 2026
19. The First Multi-Messenger Nova: External Shocks, TeV Photons, and Neutrinos in the Next Eruption of T CrBMonthly Notices of the Royal Astronomical Society · 2026
20. Assessing transitional pulsar candidates through a quantitative estimation of their light-curve similarityRAS Techniques and Instruments · 2026