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1. Snowmass 2021 CMB-S4 White Paper

2. New Ideas in Baryogenesis: A Snowmass White Paper

3. Snowmass White Paper: Effective Field Theories in Cosmology

4. Snowmass2021 Cosmic Frontier White Paper: Ultraheavy particle dark matter

5. Snowmass2021 CMB-HD White Paper

6. Voyage 2050 science white paper

7. Astro2020 White Paper: A Direct Measure of Cosmic Acceleration

8. Astro2020 Project White Paper: The Cosmic Accelerometer

9. Light Sterile Neutrinos: A White Paper

10. The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

11. A White Paper on keV sterile neutrino Dark Matter

12. EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade

13. Snowmass White Paper: Effective Field Theories for Dark Matter Phenomenology

14. White Paper on Light Sterile Neutrino Searches and Related Phenomenology

15. Searching for solar KDAR with DUNE

16. Galaxy shape statistics in the effective field theory

17. Effective field theory analysis of composite higgsino-like and wino-like thermal relic dark matter

18. The Target-selection Pipeline for the Dark Energy Spectroscopic Instrument

19. Axion Dark Matter

20. The first Hubble diagram and cosmological constraints using superluminous supernovae

21. New sensitivity curves for gravitational-wave signals from cosmological phase transitions

22. KiDS-1000 cosmology: Cosmic shear constraints and comparison between two point statistics

23. The Atacama Cosmology Telescope: Probing the baryon content of SDSS DR15 galaxies with the thermal and kinematic Sunyaev-Zel’dovich effects

24. The clustering of DESI-like luminous red galaxies using photometric redshifts

25. BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data

26. Atacama Cosmology Telescope: component-separated maps of CMB temperature and the thermal Sunyaev-Zel’dovich effect

27. A fresh look at the gravitational-wave signal from cosmological phase transitions

28. LISA Sensitivity to Gravitational Waves from Sound Waves

29. The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign – I. Overview and classification of candidates selected by two techniques

30. Deep Multi-object Spectroscopy to Enhance Dark Energy Science from LSST

31. Measuring the Hubble Constant Near and Far in the Era of ELT's

32. The LOFAR Two-metre Sky Survey. II. First data release

33. The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched on

34. Wide-field Multi-object Spectroscopy to Enhance Dark Energy Science from LSST

35. Sky-averaged 21-cm signal extraction using multiple antennas with an SVD framework: the REACH case

36. A new method to measure galaxy bias by combining the density and weak lensing fields

37. Discovery of two gravitationally lensed quasars in the Dark Energy Survey

38. CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST

39. Planck 2018 results. IV. Diffuse component separation

40. Exploring cosmic origins with CORE: cosmological parameters

41. Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation

42. Exploring Cosmic Origins with CORE: Cluster Science

43. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey:On the measurement of growth rate using galaxy correlation functions

44. H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology

45. Relativistic distortions in the large-scale clustering of SDSS-III BOSS CMASS galaxies

46. The Hawking Energy in a Perturbed Friedmann-Lema\^{i}tre Universe

47. The Dark Energy Survey: more than dark energy – an overview

48. Planck intermediate results XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth

49. Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

50. Planck 2015 results: XIII. Cosmological parameters