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Cited article:

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MeerKAT-derived H i kinematics and the baryonic Tully–Fisher relation in the X-ray luminous cluster Abell 3408

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Predicting HCN, HCO+, multitransition CO, and dust emission of star-forming galaxies

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MAGIC: MUSE gAlaxy Groups In COSMOS – A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr

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Astronomy & Astrophysics 683 A205 (2024)
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AMICO-COSMOS galaxy cluster and group catalogue up to z = 2: Sample properties and X-ray counterparts

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Tully-Fisher relation of late-type galaxies at 0.6 ≤ z ≤ 2.5

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Astrophysical systematics in kinematic lensing: Quantifying an intrinsic alignment analog

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iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. - III. Stellar metallicity drivers in MaNGA and TNG50

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Stellar angular momentum of disk galaxies at z  ≈  0.7 in the MAGIC survey

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The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies atz≃ 1

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Scaling relations of z ∼ 0.25–1.5 galaxies in various environments from the morpho-kinematics analysis of the MAGIC sample

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The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium

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MIGHTEE-H i: the baryonic Tully–Fisher relation over the last billion years

Anastasia A Ponomareva, Wanga Mulaudzi, Natasha Maddox, Bradley S Frank, Matt J Jarvis, Enrico M Di Teodoro, Marcin Glowacki, Renée C Kraan-Korteweg, Tom A Oosterloo, Elizabeth A K Adams, Hengxing Pan, Isabella Prandoni, Sambatriniaina H A Rajohnson, Francesco Sinigaglia, Nathan J Adams, Ian Heywood, Rebecca A A Bowler, Peter W Hatfield, Jordan D Collier and Srikrishna Sekhar
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