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1. Planet Formation and Disk Chemistry: Dust and Gas Evolution during Planet Formation

2. Testing analytical methods to derive the cosmic-ray ionisation rate in cold regions via synthetic observations

3. A 3D physico-chemical model of a pre-stellar core. I. Environmental and structural impact on the distribution of CH$_3$OH and $c$-C$_3$H$_2$

4. Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models

5. Broadband spectroscopy of astrophysical ice analogues: II. Optical constants of CO and CO$_2$ ices in the terahertz and infrared ranges

7. Establishing the evolutionary timescales of the massive star formation process through chemistry

8. Reducing the complexity of chemical networks via interpretable autoencoders

9. Performance of the CMS Zero Degree Calorimeters in pPb collisions at the LHC

10. A novel framework to study the impact of binding energy distributions on the chemistry of dust grains

11. Modelling thermochemical processes in protoplanetary disks I: numerical methods

12. Broadband spectroscopy of astrophysical ice analogs. I. Direct measurement of complex refractive index of CO ice using terahertz time-domain spectroscopy

13. The challenges of modelling microphysics: ambipolar diffusion, chemistry, and cosmic rays in MHD shocks

14. Low-Volume Metastases in Apparent Early-Stage Endometrial Cancer: Prevalence, Clinical Significance, and Future Perspectives

15. Low-Volume Metastases in Cervical Cancer: Does Size Matter?

16. SUrgical Access and Pattern of Recurrence of Endometrial Cancer: The SUPeR Study, a Multicenter Retrospective Observational Study

17. Fertility outcomes in stage I ovarian immature teratomas

18. The paradigm shift in advanced ovarian cancer: Outcomes of extensive primary cytoreductive surgery. A single-center retrospective analysis

19. Effect of COVID-19 pandemic lockdowns on planned cancer surgery for 15 tumour types in 61 countries: an international, prospective, cohort study

20. Modeling the role of electron attachment rates on column density ratios for CnH-/CnH (n=4,6,8) in dense molecular clouds

21. A detailed framework to incorporate dust in hydrodynamical simulations

22. The formation of the primitive star SDSS J102915+172927: effect of the dust mass and the grain-size distribution

23. Photoevaporation of protoplanetary discs with PLUTO+PRIZMO: I. Lower X-ray–driven mass-loss rates due to enhanced cooling.

24. How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

25. Effects of turbulence and rotation on protostar formation as a precursor to seed black holes

26. Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation

27. The formation of massive primordial stars in the presence of moderate UV backgrounds

28. A UV flux constraint on the formation of direct collapse black holes

29. Dark-matter halo mergers as a fertile environment for low-mass Population III star formation

30. An assessment of climate change impacts on oases in northern Africa

31. Outcome of patients with stage I immature teratoma after surveillance or adjuvant chemotherapy

32. KROME - a package to embed chemistry in astrophysical simulations

33. Primordial star formation: relative impact of H2 three-body rates and initial conditions

34. CH+ depletion by atomic hydrogen: accuracy of new rates in photo-dominated and self-shielded environments

35. Impact of an accurate modeling of primordial chemistry in high resolution studies

36. Mutagenic and genotoxic effects induced by PM0.5 of different Italian towns in human cells and bacteria: The MAPEC_LIFE study

37. Chemical complexity in astrophysical simulations: optimization and reduction techniques

38. Carbon Cations and Silicon Atoms in the ISM: modeling their charge exchange reaction

39. Electron-attachment rates for carbon-rich molecules in protoplanetary atmospheres: the role of chemical differences

40. Electron attachment rates for PAH anions in the ISM and dark molecular clouds: dependence on their chemical properties

41. Complexity reduction of astrochemical networks

42. Formation and Evolution of the Dust in Galaxies. III. The Disk of the Milky Way

43. Formation and Evolution of the Dust in Galaxies. II. The Solar Neighbourhood

44. Formation and Evolution of the Dust in Galaxies. I. The Condensation Efficiencies

45. MaNN: Multiple Artificial Neural Networks for modelling the Interstellar Medium

46. ROBO: a Model and a Code for the Study of the Interstellar Medium

47. Genomic instability analysis in DNA from Papanicolaou test provides proof-of-principle early diagnosis of high-grade serous ovarian cancer

48. Radical Hysterectomy in Early-Stage Cervical Cancer: Abandoning the One-Fits-All Concept

49. The Risk of Recurrence in Endometrial Cancer Patients with Low-Volume Metastasis in the Sentinel Lymph Nodes: A Retrospective Multi-Institutional Study

50. Long-COVID in Italy: a country perspective

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