DOI,IST REx ID,Title of publication
10.1021/acsnano.5c05186,21524,Nanophotonic thermal management in X-ray tubes
10.21468/scipostphyscore.6.2.029,13277,Stochastic representation of the quantum quartic oscillator
10.1016/j.physletb.2023.137871,14753,Low-pT quarkonium polarization measurements: Challenges and opportunities
10.15479/at:ista:12491,12491,Ultrastructural characterization of natively preserved extracellular matrix by cryo-electron tomography
10.1051/0004-6361/202142302,11488,"The MUSE eXtremely Deep Field: Individual detections of Ly<i>α</i> haloes around rest-frame UV-selected galaxies at <i>z</i> ≃ 2.9–4.4"
10.1051/0004-6361/202142187,11490,Deciphering stellar metallicities in the early universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
10.1051/0004-6361/202141900,11497,Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
10.1093/mnras/stac801,11521,"(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background"
10.1007/s00023-022-01188-8,12232,Density of small singular values of the shifted real Ginibre ensemble
10.1021/acsapm.1c01108,21824,Role of material composition in photothermal actuation of DASA-based polymers
10.15479/at:ista:11879,11879,Modulation of auxin transport via ZF proteins adjust plant response to high ambient temperature
10.1051/0004-6361/202140876,11498,Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
10.1051/0004-6361/202039887,11500,The MUSE Extremely Deep Field: The cosmic web in emission at high redshift
10.1093/mnras/stab1218,11524,"The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ∼ 2 to z ∼ 6"
10.1007/jhep03(2021)079,15269,Aspects of quantum information in finite density field theory
10.1146/annurev-genet-071819-103748,10406,Dissecting organismal morphogenesis by bridging genetics and biophysics
10.1051/0004-6361/202038133,11501,The MUSE Hubble Ultra Deep Field Survey: XV. The mean rest-UV spectra of Lyα emitters at z > 3
10.1051/0004-6361/201937340,11503,The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution of the Lyα emitter fraction from z = 3 to z = 6
10.1051/0004-6361/201937339,11504,The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral properties of Lyman α haloes around star-forming galaxies at z > 3
10.1093/mnras/staa1347,11528,MUSEQuBES: Calibrating the redshifts of Lyα emitters using stacked circumgalactic medium absorption profiles