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The properties of the interstellar medium in dusty star-forming galaxies at z ∼ 2–4: the shape of the CO spectral line energy distributions (2024)
Journal Article
Taylor, D. J., Swinbank, A. M., Smail, I., Puglisi, A., Birkin, J. E., Dudzevičiūtė, U., Chen, C.-C., Ikarashi, S., Frias Castillo, M., Weiß, A., Li, Z., Chapman, S. C., Jansen, J., Jiménez-Andrade, E. F., Morabito, L. K., Murphy, E. J., Rybak, M., & van der Werf, P. P. (2025). The properties of the interstellar medium in dusty star-forming galaxies at z ∼ 2–4: the shape of the CO spectral line energy distributions. Monthly Notices of the Royal Astronomical Society, 536(2), 1149-1165. https://doi.org/10.1093/mnras/stae2642

The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies (2024)
Journal Article
Gillman, S., Smail, I., Gullberg, B., Swinbank, A. M., Vijayan, A. P., Lee, M., Brammer, G., Dudzevičiūtė, U., Greve, T. R., Almaini, O., Brinch, M., Chapman, S. C., Chen, C.-C., Ikarashi, S., Matsuda, Y., Wang, W.-H., Walter, F., & van der Werf, P. P. (2024). The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies. Astronomy & Astrophysics, 691, Article A299. https://doi.org/10.1051/0004-6361/202451006

We present an analysis of the JWST NIRCam and MIRI morphological and structural properties of 80 massive (log10(M*[M⊙]) = 11.2 ± 0.1) dusty star-forming galaxies at z = 2.7−0.7+1.2, identified as sub-millimetre galaxies (SMGs) by ALMA, which have bee... Read More about The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies.

Metal line emission around z < 1 galaxies (2024)
Journal Article
Dutta, R., Fumagalli, M., Fossati, M., Rafelski, M., Revalski, M., Arrigoni Battaia, F., D’Odorico, V., Péroux, C., Prichard, L. J., & Swinbank, A. M. (2024). Metal line emission around z < 1 galaxies. Astronomy & Astrophysics, 691, Article A236. https://doi.org/10.1051/0004-6361/202450733

We characterize, for the first time, the average extended emission in multiple lines ([O II], [O III], and Hβ) around a statistical sample of 560 galaxies at z ≈ 0.25 − 0.85. By stacking the Multi Unit Spectroscopic Explorer (MUSE) 3D data from two l... Read More about Metal line emission around z < 1 galaxies.

An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: an unbiased study of SMG environments measured with narrow-band imaging (2024)
Journal Article
Cornish, T. M., Wardlow, J., Wade, H., Sobral, D., Brandt, W. N., Cox, P., Dannerbauer, H., Decarli, R., Gullberg, B., Knudsen, K., Stott, J., Swinbank, M., Walter, F., & van der Werf, P. (2024). An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: an unbiased study of SMG environments measured with narrow-band imaging. Monthly Notices of the Royal Astronomical Society, 533(2), 2399-2419. https://doi.org/10.1093/mnras/stae1868

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

The Blue Multi Unit Spectroscopic Explorer (BlueMUSE) on the VLT: science drivers and overview of instrument design (2024)
Presentation / Conference Contribution
Richard, J., Giroud, R., Laurent, F., Krajnovic, D., Jeanneau, A., Bacon, R., Abreu, M., Adamo, A., Araujo, R., Bouché, N., Brinchmann, J., Cai, Z., Castro Rodriguez, N., Calcines, A., Chapuis, D., Claeyssens, A., Cortese, L., Daddi, E., Davison, C., Goodwin, M., …Zheng, J. (2024, June). The Blue Multi Unit Spectroscopic Explorer (BlueMUSE) on the VLT: science drivers and overview of instrument design. Presented at Ground-based and Airborne Instrumentation for Astronomy X, Yokohama, Japan

KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at z ∼ 1.3–2.6 (2024)
Journal Article
Birkin, J. E., Puglisi, A., Swinbank, A. M., Smail, I., An, F. X., Chapman, S. C., …van der Werf, P. (2024). KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at z ∼ 1.3–2.6. Monthly Notices of the Royal Astronomical Society, 531(1), 61-83. https://doi.org/10.1093/mnras/stae1089

We present spatially resolved kinematics of 27 ALMA-identified dust-obscured star-forming galaxies (DSFGs) at z ∼ 1.3–2.6, as traced by Hα emission using VLT/KMOS near-infrared integral field spectroscopy from the ‘KMOS-ALMA Observations of Submillim... Read More about KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at z ∼ 1.3–2.6.

An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies (2024)
Journal Article
Liao, C., Chen, C., Wang, W., Smail, I., Ao, Y., Chapman, S. C., …Zhao, Y. (2024). An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies. Astrophysical Journal, 961(2), Article 226. https://doi.org/10.3847/1538-4357/ad148c

We report the physical properties of the 18 brightest (S 870 μm = 12.4–19.2 mJy) and not strongly lensed 870 μm–selected dusty star-forming galaxies (DSFGs), also known as submillimeter galaxies (SMGs), in the COSMOS field. This sample is part of an... Read More about An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies.