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1. The International Pulsar Timing Array: First data release

2. First Data Release of the COSMOS Ly α Mapping and Tomography Observations: 3D Ly α Forest Tomography at 2.05 < z < 2.55

3. High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array

4. From spin noise to systematics: stochastic processes in the first International Pulsar Timing Array data release

5. LOFAR discovery of a quiet emission mode in PSR B0823+26

6. Self-induced dust traps: overcoming planet formation barriers

7. Erratum: Self-induced dust traps: overcoming planet formation barriers

8. Wide-band, low-frequency pulse profiles of 100 radio pulsars with LOFAR

9. A Unified Framework for Producing CAI Melting, Wark-Lovering Rims and Bowl-Shaped CAIs

10. A LOFAR census of millisecond pulsars

11. ALMA images of discs: are all gaps carved by planets?

12. Limits on Fast Radio Bursts at 145 MHz with ARTEMIS, a real-time software backend

13. The accumulation and trapping of grains at planet gaps: effects of grain growth and fragmentation

14. The Morphological Transformation of Red-Sequence Galaxies in the Distant Cluster XMMU J1229+0151

15. Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5

16. The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z=1

17. The ATLAS 3D project - XI. Dense molecular gas properties of CO-luminous early-type galaxies

18. An icy Kuiper-Belt around the young solar-type star HD 181327

19. Planet gaps in the dust layer of 3D protoplanetary disks. II. Observability with ALMA

20. Optical-mechanical operation of the F2T2 Filter: a tunable filter designed to search for First Light

21. 3D SPH simulations of grain growth in protoplanetary disks

22. Gap Formation in the Dust Layer of 3D Protoplanetary Disks

23. The effect of a planet on the dust distribution in a 3D protoplanetary disk

24. Planet gaps in the dust layer of 3D proto-planetary disks: Observability with ALMA

25. The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe

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