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Repository for extended dark matter object constraints (2025)
Journal Article
Croon, D., & Sevillano Muñoz, S. (2025). Repository for extended dark matter object constraints. The European Physical Journal C, 85(1), Article 8. https://doi.org/10.1140/epjc/s10052-024-13681-x

Extended dark matter objects (EDOs) are popular dark matter candidates that interact gravitationally with the Standard Model. These gravitational interactions can be used to constrain their allowed parameter space. However, EDOs can have different fo... Read More about Repository for extended dark matter object constraints.

Improved halo model calibrations for mixed dark matter models of ultralight axions (2025)
Journal Article
Dome, T., May, S., Laguë, A., Marsh, D. J., Johnston, S., Bose, S., Tocher, A., & Fialkov, A. (2025). Improved halo model calibrations for mixed dark matter models of ultralight axions. Monthly Notices of the Royal Astronomical Society, 537(1), 252-271. https://doi.org/10.1093/mnras/staf005

We study the implications of relaxing the requirement for ultralight axions to account for all dark matter in the Universe by examining mixed dark matter (MDM) cosmologies with axion fractions f ≤ 0.3 within the fuzzy dark matter window 10−25 eV ≤ m... Read More about Improved halo model calibrations for mixed dark matter models of ultralight axions.

Disparate effects of circumgalactic medium angular momentum in IllustrisTNG and SIMBA (2025)
Journal Article
Liu, K., Guo, H., Wang, S., Xu, D., Lu, S., Cui, W., & Davé, R. (2025). Disparate effects of circumgalactic medium angular momentum in IllustrisTNG and SIMBA. Astronomy & Astrophysics, 693, Article A48. https://doi.org/10.1051/0004-6361/202452248

In this study, we examine the role of the circumgalactic medium (CGM) angular momentum (jCGM) on star formation in galaxies, whose influence is currently not well understood. The analysis utilises central galaxies from two hydrodynamical simulations,... Read More about Disparate effects of circumgalactic medium angular momentum in IllustrisTNG and SIMBA.

Detection of Extended X-Ray Emission around the PeVatron Microquasar V4641 Sgr with XRISM (2025)
Journal Article
Suzuki, H., Tsuji, N., Kanemaru, Y., Shidatsu, M., Olivera-Nieto, L., Safi-Harb, S., Kimura, S. S., de la Fuente, E., Casanova, S., Mori, K., Wang, X., Kato, S., Tateishi, D., Uchiyama, H., Tanaka, T., Uchida, H., Inoue, S., Huang, D., Lemoine-Goumard, M., Miura, D., …Ueda, Y. (2025). Detection of Extended X-Ray Emission around the PeVatron Microquasar V4641 Sgr with XRISM. Astrophysical Journal Letters, 978(2), Article L20. https://doi.org/10.3847/2041-8213/ad9d11

A recent report on the detection of very-high-energy gamma rays from V4641 Sagittarii (V4641 Sgr) up to ≈0.8 PeV has made it the second confirmed “PeVatron” microquasar. Here we report on the observation of V4641 Sgr with X-Ray Imaging and Spectrosco... Read More about Detection of Extended X-Ray Emission around the PeVatron Microquasar V4641 Sgr with XRISM.

EDGE-INFERNO: Simulating Every Observable Star in Faint Dwarf Galaxies and Their Consequences for Resolved-star Photometric Surveys (2025)
Journal Article
Andersson, E. P., Rey, M. P., Pontzen, A., Cadiou, C., Agertz, O., Read, J. I., & Martin, N. F. (2025). EDGE-INFERNO: Simulating Every Observable Star in Faint Dwarf Galaxies and Their Consequences for Resolved-star Photometric Surveys. The Astrophysical Journal, 978(2), Article 129. https://doi.org/10.3847/1538-4357/ad99d6

Interpretation of data from faint dwarf galaxies is made challenging by observations limited to only the brightest stars. We present a major improvement to tackle this challenge by undertaking zoomed cosmological simulations that resolve the evolutio... Read More about EDGE-INFERNO: Simulating Every Observable Star in Faint Dwarf Galaxies and Their Consequences for Resolved-star Photometric Surveys.

A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys (2025)
Journal Article
Maus, M., Lai, Y., Noriega, H., Ramirez-Solano, S., Aviles, A., Chen, S., Fromenteau, S., Gil-Marín, H., Howlett, C., Vargas-Magaña, M., White, M., Zarrouk, P., Aguilar, J., Ahlen, S., Alves, O., Brieden, S., Brooks, D., Burtin, E., Claybaugh, T., Cole, S., …Zou, H. (2025). A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys. Journal of Cosmology and Astroparticle Physics, 2025(1), https://doi.org/10.1088/1475-7516/2025/01/134

In preparation for the next generation of galaxy redshift surveys, and in particular the year-one data release from the Dark Energy Spectroscopic Instrument (DESI), we investigate the consistency of a variety of effective field theory models that des... Read More about A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys.

Hunting for a charged Higgs boson pair in proton-proton collisions (2025)
Journal Article
Arroyo-Ureña, M. A., Rosado-Navarro, S., Salazar, H., & Herrera-Chacón, E. A. (2025). Hunting for a charged Higgs boson pair in proton-proton collisions. Physical Review D, 111(1), Article 015023. https://doi.org/10.1103/PhysRevD.111.015023

We explore the production and possible detection of a charged scalar Higgs pair H-H+ decaying into the final state μνμcb in proton-proton collisions at the LHC and its next step, the high luminosity LHC (HL-LHC). The charged scalars are predicted wit... Read More about Hunting for a charged Higgs boson pair in proton-proton collisions.

Symbolic regression for beyond the standard model physics (2025)
Journal Article
Abdussalam, S., Abel, S., & Romão, M. C. (2025). Symbolic regression for beyond the standard model physics. Physical Review D, 111(1), Article 015022. https://doi.org/10.1103/PhysRevD.111.015022

We propose symbolic regression as a powerful tool for the numerical studies of proposed models of physics beyond the Standard Model. In this paper we demonstrate the efficacy of the method on a benchmark model, namely the constrained minimal supersym... Read More about Symbolic regression for beyond the standard model physics.

Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024 (2025)
Journal Article
Chaussidon, E., de Mattia, A., Yèche, C., Aguilar, J., Ahlen, S., Brooks, D., Claybaugh, T., Cole, S., de la Macorra, A., Doel, P., Fanning, K., Gaztañaga, E., Gontcho, S. G. A., Howlett, C., Kisner, T., Lambert, A., Le Guillou, L., Manera, M., Meisner, A., Miquel, R., …Zou, H. (2025). Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024. Journal of Cosmology and Astroparticle Physics, 2025(1), Article 135. https://doi.org/10.1088/1475-7516/2025/01/135

The next generation of spectroscopic surveys is expected to achieve an unprecedented level of accuracy in the measurement of cosmological parameters. To avoid confirmation bias and thereby improve the reliability of these results, blinding procedures... Read More about Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024.

Investigating changing-look active galactic nuclei with long-term optical and X-ray observations (2025)
Journal Article
Jana, A., Ricci, C., Temple, M. J., Chang, H. K., Shablovinskaya, E., Trakhtenbrot, B., Diaz, Y., Ilic, D., Nandi, P., & Koss, M. (2025). Investigating changing-look active galactic nuclei with long-term optical and X-ray observations. Astronomy & Astrophysics, 693, Article A35. https://doi.org/10.1051/0004-6361/202451058

Context. Broad emission lines in the UV/optical spectra of changing-look active galactic nuclei (CLAGNs) appear and disappear on timescales of months to decades. Aims. We investigate how changing-look (CL) transitions depend on several active galacti... Read More about Investigating changing-look active galactic nuclei with long-term optical and X-ray observations.