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Antenna subtraction for processes with identified particles at hadron colliders (2024)
Journal Article
Bonino, L., Gehrmann, T., Marcoli, M., Schürmann, R., & Stagnitto, G. (2024). Antenna subtraction for processes with identified particles at hadron colliders. Journal of High Energy Physics, 2024(8), Article 73. https://doi.org/10.1007/jhep08%282024%29073

Collider processes with identified hadrons in the final state are widely studied in view of determining details of the proton structure and of understanding hadronization. Their theory description requires the introduction of fragmentation functions,... Read More about Antenna subtraction for processes with identified particles at hadron colliders.

Indirect measurement of atomic magneto-optical rotation via Hilbert transform (2024)
Journal Article
Briscoe, J. D., Pizzey, D., Wrathmall, S. A., & Hughes, I. G. (2024). Indirect measurement of atomic magneto-optical rotation via Hilbert transform. Journal of Physics B: Atomic, Molecular and Optical Physics, 57(17), 175401. https://doi.org/10.1088/1361-6455/ad5e24

The Kramers–Kronig relations are a pivotal foundation of linear optics and atomic physics, embedding a physical connection between the real and imaginary components of any causal response function. A mathematically equivalent, but simpler, approach i... Read More about Indirect measurement of atomic magneto-optical rotation via Hilbert transform.

Tri-boson and WH production in the W + W + jj channel: predictions at full NLO accuracy and beyond (2024)
Journal Article
Denner, A., Pellen, M., Schönherr, M., & Schumann, S. (2024). Tri-boson and WH production in the W + W + jj channel: predictions at full NLO accuracy and beyond. Journal of High Energy Physics, 2024(8), Article 43. https://doi.org/10.1007/jhep08%282024%29043

In this work, we present the first full NLO predictions for the process pp → μ+νμe+νejj at the LHC in a typical tri-boson phase space. The NLO corrections reach 50% at the level of the fiducial cross section and have a very different hierarchy with r... Read More about Tri-boson and WH production in the W + W + jj channel: predictions at full NLO accuracy and beyond.

HARMONI at ELT: project status and instrument overview (2024)
Presentation / Conference Contribution
Thatte, N. A., Melotte, D., Neichel, B., Le Mignant, D., Rees, P., Clarke, F., Ferraro-Wood, V., Gonzalez, O., Jones, M., Álvarez Urueña, A., Vilaseca, H., Arribas Mocoroa, S., Caballero, J. A., Carracedo Carballal, G. J., Estrada Piqueras, A., Ferro, I., García García, M., Lamperti, I., Pereira Santaella, M., Perna, M., …York, A. (2024, June). HARMONI at ELT: project status and instrument overview. Paper presented at Ground-based and Airborne Instrumentation for Astronomy X, Yokohama, Japan

AGNFITTER-RX: Modeling the radio-to-X-ray spectral energy distributions of AGNs (2024)
Journal Article
Martínez-Ramírez, L. N., Rivera, G. C., Lusso, E., Bauer, F. E., Nardini, E., Buchner, J., Brown, M. J. I., Pineda, J. C. B., Temple, M. J., Banerji, M., Stalevski, M., & Hennawi, J. F. (2024). AGNFITTER-RX: Modeling the radio-to-X-ray spectral energy distributions of AGNs. Astronomy & Astrophysics, 688, Article A46. https://doi.org/10.1051/0004-6361/202449329

We present new advancements in the modeling of the spectral energy distributions (SEDs) of active galaxies by introducing the radio-to-X-ray fitting capabilities of the publicly available Bayesian code AGNFITTER. The new code release, called AGNFITTE... Read More about AGNFITTER-RX: Modeling the radio-to-X-ray spectral energy distributions of AGNs.

First measurements of energetic protons in Mega Amp Spherical Tokamak Upgrade (MAST-U). (2024)
Journal Article
Aboutaleb, A., Allan, S. Y., Boeglin, W. U., Cecconello, M., Jackson, A., McClements, K. G., & Parr, E. (2024). First measurements of energetic protons in Mega Amp Spherical Tokamak Upgrade (MAST-U). Review of Scientific Instruments, 95(8), Article 083522. https://doi.org/10.1063/5.0218380

First proton production rates from the d(d,p)t reaction in the Mega Amp Spherical Tokamak Upgrade (MAST-U) are measured. The data were taken during the MAST-U experimental campaign with an upgraded version of the proton detector (PD) previously used... Read More about First measurements of energetic protons in Mega Amp Spherical Tokamak Upgrade (MAST-U)..

Revisiting the Fundamental Metallicity Relation with Observation and Simulation (2024)
Journal Article
Ma, C., Wang, K., Wang, E., Peng, Y., Jiang, H., Yu, H., Jia, C., Chen, Z., Li, H., & Kong, X. (2024). Revisiting the Fundamental Metallicity Relation with Observation and Simulation. Astrophysical Journal Letters, 971(1), Article L14. https://doi.org/10.3847/2041-8213/ad675f

The gas-phase metallicity of galaxies is regulated by multiple astrophysical processes, which makes it a crucial diagnostic of galaxy formation and evolution. Beyond the fundamental mass–metallicity relation, a debate about the secondary galaxy prope... Read More about Revisiting the Fundamental Metallicity Relation with Observation and Simulation.

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 μ m and Data Release for the COSMOS Field (2024)
Journal Article
Gao, Z.-K., Lim, C.-F., Wang, W.-H., Chen, C.-C., Smail, I., Chapman, S. C., Zheng, X. Z., Shim, H., Kodama, T., Ao, Y., Chang, S.-Y., Clements, D. L., Dunlop, J. S., Ho, L. C., Hsu, Y.-H., Hwang, C.-Y., Hwang, H. S., Koprowski, M. P., Scott, D., Serjeant, S., …Urquhart, S. A. (2024). SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 μ m and Data Release for the COSMOS Field. The Astrophysical Journal, 971(1), 117. https://doi.org/10.3847/1538-4357/ad53c1

We present confusion-limited SCUBA-2 450 μm observations in the COSMOS-CANDELS region as part of the James Clerk Maxwell Telescope Large Program SCUBA-2 Ultra Deep Imaging EAO Survey. Our maps at 450 and 850 μm cover an area of 450 arcmin2. We achiev... Read More about SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 μ m and Data Release for the COSMOS Field.