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1. Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields

2. Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometry

3. Euclid. III. The NISP Instrument

4. Euclid. I. Overview of the Euclid mission

5. Euclid. II. The VIS Instrument

6. Euclid preparation. XXIX. Water ice in spacecraft part I: The physics of ice formation and contamination

7. Euclid preparation. XVIII. The NISP photometric system

8. Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering

9. Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3

10. Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses

11. Testing the 10 spectrograph units for DESI: approach and results

12. MOSAIC on the ELT: high-multiplex spectroscopy to unravel the physics of stars and galaxies from the dark ages to the present-day

13. Euclid preparation: X. The Euclid photometric-redshift challenge

14. Euclid preparation: V. Predicted yield of redshift 7<z<9 quasars from the wide survey

15. Populations behind the source-subtracted cosmic infrared background anisotropies

16. The WIRCam Ultra Deep Survey (WUDS) I. Survey overview and UV luminosity functions at z~5 and z~6

17. High-redshift quasar selection from the CFHQSIR survey

18. Simulating Surveys for ELT-MOSAIC: Status of the MOSAIC Science Case after Phase A

19. The THESEUS space mission concept: science case, design and expected performances

20. CFHQSIR: a Y-band extension of the CFHTLS-Wide survey

21. The E-ELT Multi-Object Spectrograph: latest news from MOSAIC

22. Science Requirements and Trade-offs for the MOSAIC Instrument for the European ELT

23. MUSE observations of the lensing cluster Abell 1689

24. Emission line selected galaxies at $z=0.6-2$ in GOODS South: Stellar masses, SFRs, and large scale structure

25. The VIMOS Ultra Deep Survey: Ly$\alpha$ Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5

26. The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3

27. The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5<z<5.5 and the colour selection of high redshift galaxies

28. The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey

29. The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)

30. Science Case and Requirements for the MOSAIC Concept for a Multi-Object Spectrograph for the European Extremely Large Telescope

31. VIMOS Ultra-Deep Survey (VUDS): Witnessing the Assembly of a Massive Cluster at z~3.3

32. The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6

33. The VIMOS Ultra-Deep Survey (VUDS): fast increase of the fraction of strong Lyman alpha emitters from z=2 to z=6

34. Discovering extremely compact and metal-poor, star-forming dwarf galaxies out to z ~ 0.9 in the VIMOS Ultra-Deep Survey

35. Discovery of a rich proto-cluster at z=2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)

36. Spatially-resolved dust properties of the GRB 980425 host galaxy

37. Multi-Object Spectroscopy with the European ELT: Scientific synergies between EAGLE & EVE

38. Constraining the nature of the most distant Gamma-Ray Burst host galaxies

39. A complex multi-notch astronomical filter to suppress the bright infrared sky

40. Euclid Definition Study Report

41. A highly magnified supernova at z=1.703 behind the massive galaxy cluster Abell 1689

42. Evolution of the observed Ly-alpha luminosity function from z = 6.5 to z = 7.7: evidence for the epoch of reionization ?

43. Stellar metallicities beyond the Local Group: the potential of J-band spectroscopy with extremely large telescopes

44. Spectroscopic confirmation of a galaxy at redshift z=8.6

45. The bright end of the z ~ 7 UV Luminosity Function from a wide and deep HAWK-I survey

46. The circumstellar environment of the YSO TMR-1 and a revisit to the candidate very low-mass object TMR-1C

47. Science Requirements and Performances for EAGLE for the E-ELT

48. Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts

49. EAGLE multi-object AO concept study for the E-ELT

50. The physics of galaxy evolution with EAGLE

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