H. P. Laboratory

发表

Reflection and refraction of (magneto-)acoustic waves at the magnetic canopy: further evidences from multi-height seismic data

Bangalore, India., Usa, 2013, 1308.5777.

The Ultra-fast Outflow of the Quasar PG 1211+143 as Viewed by Time-averaged Chandra Grating Spectroscopy

Bangalore, India., Cambridge, 2017, 1712.07118.

DARWIN – a next-generation liquid xenon observatory for dark matter and neutrino physics

Tokyo, Ny, The State University of New York, 2021, Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).

Effects of Weak Surface Fields on the Density Profiles and Adsorption of a Confined Fluid Near Bulk Criticality

UK., U. Bristol, A. Maciołek, 2003, cond-mat/0306028.

Sub-Arcsecond Imaging of 3C123:108-GHz Continuum Observations of the Radio Hotspots

H. P. Laboratory, L. W. L. M. H. Mpe, 1999, astro-ph/9912092.

Mass measurements of As, Se, and Br nuclei, and their implication on the proton-neutron interaction strength toward the N=Z line

Edinburgh, Israel, Canada., 2020, Physical Review C.

A. M. Guler, Napoli, Bonn, 2020, 2002.08722.

Analysis of Neutral B-Meson Decays into Two Muons.

Ny, Santiago de Compostela, Edinburgh, 2021, Physical review letters.

Measurement of the $B^0_s\to\mu^+\mu^-$ decay properties and search for the $B^0\to\mu^+\mu^-$ and $B^0_s\to\mu^+\mu^-\gamma$ decays

Santiago de Compostela, Edinburgh, Cambridge, 2021, 2108.09283.

Observation of the decay B-s(0) -> phi pi(+)pi(-) and evidence for B-0 -> phi pi(+)pi(-)

Ny, Santiago de Compostela, Edinburgh, 2016, 1610.05187.

CONSTRAINING INTRACLUSTER GAS MODELS WITH AMiBA13

Astrophysics, National Taiwan Normal University, Center for Computational Sciences, 2010, 1009.1943.

Galaxy and mass assembly (GAMA): The consistency of GAMA and WISE derived mass-to-light ratios

Liverpool John Moores University, Astronomy, International Centre for Radio Astronomy Research, 2017, 1709.08316.