Outputs (12454)

Structural chirality and related properties in the periodic inorganic solids: Review and perspectives (2025)
Journal Article
Bousquet, E., Fava, M., Romestan, Z., Gómez-Ortiz, F., McCabe, . E. E., & Romero, A. H. (online). Structural chirality and related properties in the periodic inorganic solids: Review and perspectives. Journal of Physics: Condensed Matter, https://doi.org/10.1088/1361-648X/adb674

Chirality refers to the asymmetry of objects that cannot be superimposed on their mirror image. It is a concept that exists in various scientific fields and has profound consequences. Although these are perhaps most widely recognized within biology,... Read More about Structural chirality and related properties in the periodic inorganic solids: Review and perspectives.

Shear banding as a cause of nonmonotonic stress relaxation after flow cessation (2025)
Journal Article
Ward, V. K., & Fielding, S. M. (2025). Shear banding as a cause of nonmonotonic stress relaxation after flow cessation. Physical Review Materials, 9(2), Article L022601. https://doi.org/10.1103/PhysRevMaterials.9.L022601

Recent flow cessation experiments on soft materials have shown a counter-intuitive non-monotonic relaxation of the shear stress: following the switch-off of a steady imposed shear flow, the stress initially decays before later increasing again. By si... Read More about Shear banding as a cause of nonmonotonic stress relaxation after flow cessation.

Monster Radio Jet (>66 kpc) Observed in Quasar at z ∼​​​​​ 5 (2025)
Journal Article
Gloudemans, A. J., Sweijen, F., Morabito, L. K., Farina, E. P., Duncan, K. J., Harikane, Y., Röttgering, H. J. A., Saxena, A., & Schindler, J.-T. (2025). Monster Radio Jet (>66 kpc) Observed in Quasar at z ∼​​​​​ 5. Astrophysical Journal Letters, 980(1), Article L8. https://doi.org/10.3847/2041-8213/ad9609

We present the discovery of a large extended radio jet associated with the extremely radio-loud quasar J1601+3102 at z ∼​​​​​ 5 from subarcsecond resolution imaging at 144 MHz with the International LOFAR Telescope. These large radio lobes have been... Read More about Monster Radio Jet (>66 kpc) Observed in Quasar at z ∼​​​​​ 5.

Lipid bilayer fracture under uniaxial stretch † (2025)
Journal Article
Goodband, R. J., & Staykova, M. (in press). Lipid bilayer fracture under uniaxial stretch †. Soft Matter, https://doi.org/10.1039/d4sm01410c

Most studies on pore formation in lipid membranes focus on lipid vesicles under isotropic tension. These models however fail to replicate the anisotropic stresses encountered by living cells and the complex rheological properties of the cell membrane... Read More about Lipid bilayer fracture under uniaxial stretch †.

Strong-lensing Analysis of SPT-CL J2325−4111 and SPT-CL J0049−2440, Two Powerful Cosmic Telescopes ( R E > 40″) from the SPT Clusters Sample (2025)
Journal Article
Mahler, G., Sharon, K., Bayliss, M., Bleem, L. E., Brodwin, M., Floyd, B., Gassis, R., Gladders, M. D., Khullar, G., Remolina González, J. D., & Sarkar, A. (2025). Strong-lensing Analysis of SPT-CL J2325−4111 and SPT-CL J0049−2440, Two Powerful Cosmic Telescopes ( R E > 40″) from the SPT Clusters Sample. The Astrophysical Journal, 980(1), Article 48. https://doi.org/10.3847/1538-4357/ad9aa5

We report the results from a study of two massive (M500c > 6.0 × 1014 M⊙) strong-lensing clusters selected from the South Pole Telescope cluster survey for their large Einstein radius (RE > 40″), SPT-CL J2325−4111 and SPT-CL J0049−2440. Ground-based... Read More about Strong-lensing Analysis of SPT-CL J2325−4111 and SPT-CL J0049−2440, Two Powerful Cosmic Telescopes ( R E > 40″) from the SPT Clusters Sample.

WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation (2025)
Journal Article
Perron-Cormier, M., Deg, N., Spekkens, K., Richardson, M. L. A., Glowacki, M., Oman, K. A., Verheijen, M. A. W., Hank, N. A. N., Blyth, S., Dénes, H., Rhee, J., Elagali, A., Shen, A. X., Raja, W., Lee-Waddell, K., Cortese, L., Catinella, B., & Westmeier, T. (2025). WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation. Astronomical Journal, 169(2), Article 114. https://doi.org/10.3847/1538-3881/ada567

An avenue for understanding cosmological galaxy formation is to compare morphometric parameters in observations and simulations of galaxy assembly. In this second paper of the ASymba: Asymmetries of H i in SIMBA Galaxies series, we measure atomic gas... Read More about WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation.

The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20–214 μ m Imaging Atlas of Active Galactic Nuclei Using SOFIA (2025)
Journal Article
Fuller, L., Lopez-Rodriguez, E., García-Bernete, I., Ramos Almeida, C., Alonso-Herrero, A., Packham, C., Zhang, L., Leist, M., Levenson, N. A., Imanishi, M., Hoenig, S., Stalevski, M., Ricci, C., Hicks, E., Bellocchi, E., Combes, F., Davies, R., García Burillo, S., González Martín, O., Izumi, T., …Ward, M. (2025). The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20–214 μ m Imaging Atlas of Active Galactic Nuclei Using SOFIA. The Astrophysical Journal, 276(2), Article 64. https://doi.org/10.3847/1538-4365/ad9907

We present a 19.7–214 μm imaging atlas of local (4–181 Mpc; median 43 Mpc) active galactic nuclei (AGN) observed with FORCAST and HAWC+ on board the SOFIA telescope with angular resolutions ~3″–20″. This atlas comprises 22 Seyferts (17 Type 2 and fiv... Read More about The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20–214 μ m Imaging Atlas of Active Galactic Nuclei Using SOFIA.

A physical optics formulation of Bloch waves and its application to 4D STEM, 3D ED and inelastic scattering simulations (2025)
Journal Article
Mendis, B. (2025). A physical optics formulation of Bloch waves and its application to 4D STEM, 3D ED and inelastic scattering simulations. Acta Crystallographica Section A: Foundations and Advances, 81(2), https://doi.org/10.1107/s2053273325000142

Bloch waves are often used in dynamical diffraction calculations, such as simulating electron diffraction intensities for crystal structure refinement. However, this approach relies on matrix diagonalization and is therefore computationally expensive... Read More about A physical optics formulation of Bloch waves and its application to 4D STEM, 3D ED and inelastic scattering simulations.

A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST (2025)
Journal Article
Kalita, B. S., Yu, S.-Y., Silverman, J. D., Daddi, E., Ho, L. C., Faisst, A. L., Dessauges-Zavadsky, M., Puglisi, A., Birrer, S., Kashino, D., Ding, X., Kartaltepe, J. S., Liu, Z., Kakkad, D., Valentino, F., Ilbert, O., Magdis, G., Long, A. S., Jin, S., Koekemoer, A. M., & Massey, R. (2025). A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST. Astrophysical Journal Letters, 979(2), Article L44. https://doi.org/10.3847/2041-8213/ada958

Recent JWST observations have revealed the prevalence of spiral structures at z > 1. Unlike in the local Universe, the origin and the consequence of spirals at this epoch remain unexplored. We use public JWST/NIRCam data from the COSMOS-Web survey to... Read More about A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST.

Identifying Key Physical Properties of Simple Organic Drop Cast Films that give Visible to Ultraviolet Light Up‐Conversion (2025)
Journal Article
Lodola, F., Miranda‐Salinas, H., Kuila, S., Danos, A., & Monkman, A. P. (online). Identifying Key Physical Properties of Simple Organic Drop Cast Films that give Visible to Ultraviolet Light Up‐Conversion. ChemPhotoChem, Article e202400341. https://doi.org/10.1002/cptc.202400341

We demonstrate UV‐emitting films of 2,5‐diphenyloxazole (PPO) sensitised by 3,3′‐carbonylbis(7‐diethylaminocoumarin) (CBDAC), prepared by simple drop casting with rapid solvent evaporation, giving up‐converted emission even at low excitation intensit... Read More about Identifying Key Physical Properties of Simple Organic Drop Cast Films that give Visible to Ultraviolet Light Up‐Conversion.