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H. Kusakabe et al., “The MUSE eXtremely Deep Field: Individual detections of Ly;1 haloes around rest-frame UV-selected galaxies at z  2.9–4.4,” Astronomy &; Astrophysics, vol. 660. EDP Sciences, 2022.
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Y. Isobe et al., “EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M= 10<sup>4</sup>-10<sup>5</sup> and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae,” The Astrophysical Journal, vol. 925, no. 2. IOP Publishing, 2022.
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D. Sobral et al., “The LEGA-C of nature and nurture in stellar populations at z c 0.6–1.0: Dn4000 and H;4 reveal different assembly histories for quiescent galaxies in different environments,” The Astrophysical Journal, vol. 926, no. 2. IOP Publishing, 2022.
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A. Gebek and J. J. Matthee, “On the variation in stellar ;1-enhancements of star-forming galaxies in the EAGLE simulation,” The Astrophysical Journal, vol. 924, no. 2. IOP Publishing, 2022.
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J. C. Zinn et al., “The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in – and 0–8,” The Astrophysical Journal, vol. 926, no. 2. IOP Publishing, 2022.
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S. Mathur et al., “Detections of solar-like oscillations in dwarfs and subgiants with Kepler D short-cadence data,” Astronomy &; Astrophysics, vol. 657. EDP Sciences, 2022.
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L. A. Bugnet, “Hidden currents at the Sun’s surface,” Nature Astronomy, vol. 6. Springer Nature, pp. 631–632, 2022.
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H. Dhouib, S. Mathis, L. A. Bugnet, T. Van Reeth, and C. Aerts, “Detecting deep axisymmetric toroidal magnetic fields in stars: The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field,” Astronomy &; Astrophysics, vol. 661. EDP Sciences, 2022.
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Z. Keszthelyi et al., “The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities,” Monthly Notices of the Royal Astronomical Society, vol. 517, no. 2. Oxford University Press, pp. 2028–2055, 2022.
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M. Gull et al., “A panchromatic study of massive stars in the extremely metal-poor local group dwarf galaxy Leo A,” The Astrophysical Journal, vol. 941, no. 2. American Astronomical Society, 2022.
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J. M. J. Ong, L. A. Bugnet, and S. Basu, “Mode mixing and rotational splittings. I. Near-degeneracy effects revisited,” The Astrophysical Journal, vol. 940, no. 1. American Astronomical Society, 2022.
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S. S. Tsygankov et al., “The x-ray polarimetry view of the accreting pulsar Cen X-3,” The Astrophysical Journal Letters, vol. 941, no. 1. American Astronomical Society, 2022.
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V. Doroshenko et al., “Determination of X-ray pulsar geometry with IXPE polarimetry,” Nature Astronomy, vol. 6, no. 12. Springer Nature, pp. 1433–1443, 2022.
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I. Caiazzo, D. González-Caniulef, J. Heyl, and R. Fernández, “Probing magnetar emission mechanisms with X-ray spectropolarimetry,” Monthly Notices of the Royal Astronomical Society, vol. 514, no. 4. Oxford University Press, pp. 5024–5034, 2022.
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K. Rink, I. Caiazzo, and J. Heyl, “Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40,” Monthly Notices of the Royal Astronomical Society, vol. 517, no. 1. Oxford University Press, pp. 1389–1397, 2022.
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H. B. Richer et al., “When do stars go boom?,” The Astrophysical Journal Letters, vol. 931, no. 2. American Astronomical Society, 2022.
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S. Ginzburg, J. Fuller, A. Kawka, and I. Caiazzo, “Slow convection and fast rotation in crystallization-driven white dwarf dynamos,” Monthly Notices of the Royal Astronomical Society, vol. 514, no. 3. Oxford University Press, pp. 4111–4119, 2022.
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