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1. A Cautionary Tale of LyC Escape Fraction Estimates from High Redshift Galaxies

2. Upper limits on the escape fraction of ionizing radiation from galaxies at $2\lesssim z < 6$

3. IGM Transmission Bias for $z$ $\geq$ 2.9 Lyman Continuum Detected Galaxies

4. Outside the Lyman-break box: detecting Lyman continuum emitters at $3.5<z<5.1$ with CLAUDS

5. The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5

6. The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Ly$\alpha$ nebulae associated with a bright $z\approx 3.23$ quasar pair

7. The MUSE Ultra Deep Field (MUDF). V. Characterizing the Mass-Metallicity Relation for Low-mass Galaxies at z ∼ 1-2

9. The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging

10. Metal line emission from galaxy haloes at z ≈ 1

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14. The Muse Ultra deep field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5

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18. Outside the Lyman-break box: detecting Lyman continuum emitters at 3.5 &lt; z &lt; 5.1 with CLAUDS

19. cautionary tale of Ly C escape fraction estimates from high-redshift galaxies.

20. Outside the Lyman-break box: detecting Lyman continuum emitters at $3.5

21. Upper limits on the escape fraction of ionizing radiation from galaxies at 2 ≲ z < 6.

22. The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair

23. The evolution of early-type galaxies

24. The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 &lt; z &lt; 1.5

25. The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair

26. Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39

27. Outside the Lyman-break box: detecting Lyman continuum emitters at 3.5 < z < 5.1 with CLAUDS.

28. Orientation and Switching Properties of Advanced Metal Particle Recording Media

29. The KMOS GTO Cluster Program:Absorption Line Spectroscopy of Cluster Galaxies at z similar to 1.5

30. The KMOS GTO Cluster Program : Absorption Line Spectroscopy of Cluster Galaxies at z similar to 1.5

31. Determination of anisotropy fields in recording media.

38. Interactions between neurogranin and calmodulin in vivo.

39. The prooncoprotein EWS binds calmodulin and is phosphorylated by protein kinase C through an IQ domain.

45. Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 atz= 1.39

46. The MUSE Ultra Deep Field (MUDF) - I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair

47. The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5

48. Early prediction of end-stage kidney disease using electronic health record data: a machine learning approach with a 2-year horizon.

49. Convalescent plasma-mediated resolution of COVID-19 in a patient with humoral immunodeficiency.

50. Inhibition of the lymphocyte metabolic switch by the oxidative burst of human neutrophils.

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