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1. From Stellar Death to Cosmic Revelations: Zooming in on Compact Objects, Relativistic Outflows and Supernova Remnants with AXIS

2. The Multiview Observatory for Solar Terrestrial Science (MOST)

3. Helio2024 Science White Paper: Solar and Heliospheric Magnetism in 5D

4. Cognitive and psychiatric symptom trajectories 2–3 years after hospital admission for COVID-19: a longitudinal, prospective cohort study in the UK

6. LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit

7. The multiview observatory for solar terrestrial science (MOST)

8. Discovery of a ~30-Year-Duration Post-Nova Pulsating Supersoft Source in the Large Magellanic Cloud

9. The binary evolution of SAX J1808.4-3658: Implications of an evolved donor star

10. The GOES-R EUVS Model for EUV Irradiance Variability

11. Multiorgan MRI findings after hospitalisation with COVID-19 in the UK (C-MORE): a prospective, multicentre, observational cohort study

12. Effects of sleep disturbance on dyspnoea and impaired lung function following hospital admission due to COVID-19 in the UK: a prospective multicentre cohort study

13. Revealing the Origin and Cosmic Evolution of Supermassive Black Holes

14. Maximally accreting supermassive stars: a fundamental limit imposed by hydrostatic equilibrium

15. Comprehensive models of novae at metallicity $Z = 0.02$ and $Z = 10^{-4}$

16. Determinants of recovery from post-COVID-19 dyspnoea: analysis of UK prospective cohorts of hospitalised COVID-19 patients and community-based controls

17. Excluding super-soft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud

18. Prevalence of physical frailty, including risk factors, up to 1 year after hospitalisation for COVID-19 in the UK: a multicentre, longitudinal cohort study

19. SARS-CoV-2-specific nasal IgA wanes 9 months after hospitalisation with COVID-19 and is not induced by subsequent vaccination

22. Balmer-Dominated Shocks Exclude Hot Progenitors for Many Type Ia Supernovae

23. Clinical characteristics with inflammation profiling of long COVID and association with 1-year recovery following hospitalisation in the UK: a prospective observational study

25. No hot and luminous progenitor for Tycho's supernova

26. On the Maximum Mass of Accreting Primordial Supermassive Stars

28. Hohlraum Reheating from Burning NIF Implosions

29. Coronal Dynamic Activities in the Declining Phase of a Solar Cycle

30. Soft X-ray irradiance measured by the Solar Aspect Monitor on the Solar Dynamic Observatory Extreme ultraviolet Variability Experiment

31. Modelling nova populations in galaxies

32. Cognitive and psychiatric symptom trajectories 2–3 years after hospital admission for COVID-19: a longitudinal, prospective cohort study in the UK

34. Where are all of the nebulae ionized by supersoft X-ray sources?

35. Population synthesis of accreting white dwarfs: II. X-ray and UV emission

36. Magnetism in a family of $S = 1$ square lattice antiferromagnets Ni$X_2$(pyz)$_2$ ($X = $ Cl, Br, I, NCS; pyz = pyrazine)

37. Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESA

38. Mechanisms and Observations of Coronal Dimming for the 2010 August 7 Event

39. Upper limits on the luminosity of the progenitor of type Ia supernova SN2014J

40. Emission line diagnostics to constrain high temperature populations in early-type galaxies

41. On-Orbit Degradation of Solar Instruments

42. Recent variability of the solar spectral irradiance and its impact on climate modelling

43. He II recombination lines as a test of the nature of SN Ia progenitors in elliptical galaxies

44. The Origin of the EUV Late Phase: A Case Study of the C8.8 Flare on 2010 May 5

45. Can We Trust Models for Adiabatic Mass Loss?

46. On The Formation of Double White Dwarfs: Reevaluating How We Parametrize the Common Envelope Phase

47. On the Formation of Double White Dwarfs through Stable Mass Transfer and a Common Envelope

48. The Formation of Low-Mass Double White Dwarfs through an Initial Phase of Stable Non-Conservative Mass Transfer

49. Formation of black-hole X-ray binaries in globular clusters

50. Finding the best proxies for the solar UV irradiance

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