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1. Gaia Focused Product Release: Sources from Service Interface Function image analysis -- Half a million new sources in omega Centauri

2. Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars

3. Gaia Focused Product Release: Radial velocity time series of long-period variables

4. Recent Results from the SAFIR Project

5. Gaia Data Release 3: Summary of the content and survey properties

6. Gaia Data Release 3: Reflectance spectra of Solar System small bodies

7. Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way

8. Gaia Data Release 3: Pulsations in main sequence OBAF-type stars

9. Gaia Data Release 3: A Golden Sample of Astrophysical Parameters

10. Gaia Data Release 3: The extragalactic content

11. Gaia Data Release 3: Stellar multiplicity, a teaser for the hidden treasure

12. Gaia Data Release 3: Chemical cartography of the Milky Way

13. Gaia Early Data Release 3: The celestial reference frame (Gaia-CRF3)

14. Gaia Photometric Science Alerts

15. Gaia Early Data Release 3: The Galactic anticentre

16. Gaia Early Data Release 3: The astrometric solution

17. Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

18. Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry

19. Gaia Early Data Release 3: Structure and properties of the Magellanic Clouds

20. Gaia Early Data Release 3: Summary of the contents and survey properties

21. The CANDELS/SHARDS multi-wavelength catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission line fluxes and Star Formation Rates

22. Optically-faint massive Balmer Break Galaxies at z>3 in the CANDELS/GOODS fields

23. Gaia Data Release 2: Observational Hertzsprung-Russell diagrams

24. Gaia Data Release 2: The astrometric solution

25. SHARDS: Constraints on the dust attenuation law of star-forming galaxies at z~2

26. The spatial extent of Polycyclic Aromatic Hydrocarbons emission in the Herbig star HD 179218

27. SHARDS Frontier Fields: Physical properties of a low mass Lyman-alpha emitter at z=5.75

28. The dusty tori of nearby QSOs as constrained by high-resolution mid-IR observations

29. X-ray selected BALQSOs

30. The complex evolutionary paths of local infrared bright galaxies: a high angular resolution mid-infrared view

31. The nuclear and extended mid-infrared emission of Seyfert galaxies

32. Highly variable AGN from the XMM-Newton Slew Survey

33. The nuclear and integrated far-infrared emission of nearby Seyfert galaxies

34. Mid-infrared imaging- and spectro-polarimetric subarcsecond observations of NGC 1068

35. A mid-infrared spectroscopic atlas of local active galactic nuclei on sub-arcsecond resolution using GTC/CanariCam

36. A deep look at the nuclear region of UGC 5101 through high angular resolution mid-IR data with GTC/CanariCam

37. SHARDS: A global view of the star formation activity at z~0.84 and z~1.23

38. Pathways to quiescence: SHARDS view on the Star Formation Histories of massive quiescent galaxies at 1.0 < z < 1.5

39. The XMM-Newton serendipitous survey. VII. The third XMM-Newton serendipitous source catalogue

40. Resolving the AGN and host emission in the mid-infrared using a model-independent spectral decomposition

41. The nuclear and extended infrared emission of the Seyfert galaxy NGC 2992 and the interacting system Arp 245

42. An X-ray and UV flare from the galaxy XMMSL1 J061927.1-655311

43. A mid-infrared view of the inner parsecs of the Seyfert galaxy Mrk 1066 using CanariCam/GTC

44. The stellar initial mass function at 0.9<z<1.5

45. Nuclear 11.3$\mu$m PAH emission in local active galactic nuclei

46. Higher prevalence of X-ray selected AGN in intermediate age galaxies up to z~1

47. Uncovering the deeply embedded AGN activity in the nuclear regions of the interacting galaxy Arp299

48. Nuclear star formation activity and black hole accretion in nearby Seyfert galaxies

49. A high Eddington-ratio, true Seyfert 2 galaxy candidate: implications for broad-line-region models

50. The XMM-Newton Wide Angle Survey (XWAS)

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