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1. Adaptive algorithms for low-latency cancellation of seismic Newtonian-noise at the Virgo gravitational-wave detector

2. Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors

3. A weighted multidetector extension to the 5-vector method for the search of continuous gravitational wave signals

4. Doppler orbital correction for the targeted search of known pulsars with the 5-vector method

5. Search for gravitational wave signals from known pulsars in LIGO-Virgo O3 data using the 5n-vector ensemble method

6. Design and implementation of a seismic Newtonian-noise cancellation system for the Virgo gravitational-wave detector

7. Quantum zero point electromagnetic energy difference between the superconducting and the normal phase in a HTc superconducting metal bulk sample

8. External environmental noise influences on Virgo during O3

10. A lower limit for Newtonian-noise models of the Einstein Telescope

11. Thermal noise-limited beam balance as prototype of the Archimedes vacuum weight experiment and B-L dark photon search

12. Design and implementation of a seismic Newtonian noise cancellation system for the Virgo gravitational-wave detector

13. Characterization of the seismic field at Virgo and improved estimates of Newtonian-noise suppression by recesses

14. Liquid actuated gravity experiments

15. Measurement and subtraction of Schumann resonances at gravitational-wave interferometers

16. Subtraction of correlated noise in global networks of gravitational-wave interferometers

17. Casimir energy for N superconducting cavities: a model for the YBCO (GdBCO) sample to be used in the Archimedes experiment

20. Characterizing the Sardinia candidate site for the Einstein Telescope

21. Mitigation of the effect of changes of atmospheric pressure on gravity detectors: preliminary results obtained with microphones at the Sos Enattos mine

22. Search for gravitational wave signals from known pulsars in LIGO-Virgo O3 data using the 5n -vector ensemble method

23. Towards weighing the condensation energy to ascertain the Archimedes force of vacuum

24. A quasi-complete mechanical model for a double torsion pendulum

25. Testing gravitational theories using Eccentric Eclipsing Detached Binaries

26. Design and implementation of a seismic Newtonian-noise cancellation system for the Virgo gravitational-wave detector

27. Measurement of gravitational and thermal effects in a liquid-actuated torsion pendulum

29. Array analysis of seismic noise at the Sos Enattos mine, the Italian candidate site for the Einstein Telescope

30. Quantum zero point electromagnetic energy difference between the superconducting and the normal phase in a high- Tc superconducting metal bulk sample

31. The 5n-vector ensemble method

33. Quantum zero point electromagnetic energy difference between the superconducting and the normal phase in a high- Tc superconducting metal bulk sample

36. Study of the cosmic muon rate nearby the Advanced Virgo detector at the end of the O3 run

37. Characterization of the seismic field at Virgo and improved estimates of Newtonian-noise suppression by recesses

38. Picoradiant tiltmeter and direct ground tilt measurements at the Sos Enattos site

39. External environmental noise influences on Virgo during O3

40. A hybrid modular control and acquisition system

42. The Hunt for Environmental Noise in Virgo during the Third Observing Run

43. Neural networks for blind-source separation of stromboli explosion quakes

44. A Seismological Study of the Sos Enattos Area—the Sardinia Candidate Site for the Einstein Telescope

45. Progress in a Vacuum Weight Search Experiment

46. Real-time digital control of optical interferometers by the mechanical-modulation technique

47. Fringe-counting technique used to lock a suspended interferometer

48. Liquid actuated gravity experiments

50. Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo

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