The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release. arxiv.org/abs/2403.16976

Forecast constraints on the baryonic feedback effect from the future kinetic Sunyaev-Zel'dovich effect detection. arxiv.org/abs/2401.03510

Comprehensive Constraints on Dark Radiation Injection After BBN. arxiv.org/abs/2312.13235

'SNe Ia twins for life' towards a precise determination of H$_{0}$. arxiv.org/abs/2312.10334

The origin of supermassive black holes at cosmic dawn. arxiv.org/abs/2310.06898

Frequency-Domain Distribution of Astrophysical Gravitational-Wave Backgrounds. arxiv.org/abs/2305.09372

Primordial black hole formation during the QCD phase transition: threshold, mass distribution and abundance. arxiv.org/abs/2303.07980

Prospects of the multi-channel photometric survey telescope in the cosmological application of Type Ia supernovae. arxiv.org/abs/2404.07246

Distributions and Collision Rates of ALP Stars in the Milky Way. arxiv.org/abs/2404.07908

Monge Amp\`ere gravity: from the large deviation principle to cosmological simulations through optimal transport. arxiv.org/abs/2404.07697

Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO. arxiv.org/abs/2404.07419

Primordial Intermediate and Supermassive Black Hole formation during the electron-positron annihilation epoch. arxiv.org/abs/2404.07332

Effects of dynamical friction on perturbations for evolving dark energy. arxiv.org/abs/2404.07313

An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyond. arxiv.org/abs/2404.07312

A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond. arxiv.org/abs/2404.07283

Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis. arxiv.org/abs/2404.07282

A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys. arxiv.org/abs/2404.07272

Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyond. arxiv.org/abs/2404.07269

Full Modeling and Parameter Compression Methods in configuration space for DESI 2024 and beyond. arxiv.org/abs/2404.07268

Hot New Early Dark Energy bridging cosmic gaps: Supercooled phase transition reconciles (stepped) dark radiation solutions to the Hubble tension with BBN. arxiv.org/abs/2404.07256