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61 Publications


2020 | Journal Article | IST-REx-ID: 11529 | OA
J. J. Matthee et al., “The nature of CR7 revealed with MUSE: A young starburst powering extended Ly α emission at z = 6.6,” Monthly Notices of the Royal Astronomical Society, vol. 498, no. 2. Oxford University Press, pp. 3043–3059, 2020.
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2020 | Journal Article | IST-REx-ID: 11533 | OA
S. Santos et al., “The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs,” Monthly Notices of the Royal Astronomical Society, vol. 493, no. 1. Oxford University Press, pp. 141–160, 2020.
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2020 | Journal Article | IST-REx-ID: 11534 | OA
J. J. Matthee et al., “Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 ,” Monthly Notices of the Royal Astronomical Society, vol. 492, no. 2. Oxford University Press, pp. 1778–1790, 2020.
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2020 | Journal Article | IST-REx-ID: 11531 | OA
M. V. Maseda et al., “Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-α emitters,” Monthly Notices of the Royal Astronomical Society, vol. 493, no. 4. Oxford University Press, pp. 5120–5130, 2020.
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2020 | Journal Article | IST-REx-ID: 11530 | OA
J. S. den Brok et al., “Probing the AGN unification model at redshift z ∼ 3 with MUSE observations of giant Lyα nebulae,” Monthly Notices of the Royal Astronomical Society, vol. 495, no. 2. Oxford University Press, pp. 1874–1887, 2020.
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2020 | Journal Article | IST-REx-ID: 11539 | OA
J. Calhau et al., “The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population,” Monthly Notices of the Royal Astronomical Society, vol. 493, no. 3. Oxford University Press, pp. 3341–3362, 2020.
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2020 | Journal Article | IST-REx-ID: 13465 | OA
M. Renzo, R. J. Farmer, S. Justham, S. E. de Mink, Y. L. L. Götberg, and P. Marchant, “Sensitivity of the lower edge of the pair-instability black hole mass gap to the treatment of time-dependent convection,” Monthly Notices of the Royal Astronomical Society, vol. 493, no. 3. Oxford University Press, pp. 4333–4341, 2020.
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2020 | Journal Article | IST-REx-ID: 15220 | OA
I. Caiazzo and J. Heyl, “Polarization of accreting X-ray pulsars. I. A new model,” Monthly Notices of the Royal Astronomical Society, vol. 501, no. 1. Oxford University Press, pp. 109–128, 2020.
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2020 | Journal Article | IST-REx-ID: 15221 | OA
I. Caiazzo and J. Heyl, “Polarization of accreting X-ray pulsars – II. Hercules X-1,” Monthly Notices of the Royal Astronomical Society, vol. 501, no. 1. Oxford University Press, pp. 129–136, 2020.
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2019 | Journal Article | IST-REx-ID: 11535 | OA
A. A. Khostovan et al., “The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities,” Monthly Notices of the Royal Astronomical Society, vol. 489, no. 1. Oxford University Press, pp. 555–573, 2019.
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2019 | Journal Article | IST-REx-ID: 11541 | OA
D. Sobral et al., “On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components,” Monthly Notices of the Royal Astronomical Society, vol. 482, no. 2. Oxford University Press, pp. 2422–2441, 2019.
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2019 | Journal Article | IST-REx-ID: 11540 | OA
J. J. Matthee and J. Schaye, “The origin of scatter in the star formation rate–stellar mass relation,” Monthly Notices of the Royal Astronomical Society, vol. 484, no. 1. Oxford University Press, pp. 915–932, 2019.
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2019 | Journal Article | IST-REx-ID: 11615 | OA
M. Hon et al., “A search for red giant solar-like oscillations in all Kepler data,” Monthly Notices of the Royal Astronomical Society, vol. 485, no. 4. Oxford University Press, pp. 5616–5630, 2019.
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2018 | Journal Article | IST-REx-ID: 11549
A. A. Khostovan et al., “The clustering of H β + [O III] and [O II] emitters since z ∼ 5: Dependencies with line luminosity and stellar mass,” Monthly Notices of the Royal Astronomical Society, vol. 478, no. 3. Oxford University Press, pp. 2999–3015, 2018.
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2018 | Journal Article | IST-REx-ID: 11557 | OA
D. Sobral et al., “The nature of luminous Ly α emitters at z ∼ 2–3: Maximal dust-poor starbursts and highly ionizing AGN,” Monthly Notices of the Royal Astronomical Society, vol. 477, no. 2. Oxford University Press, pp. 2817–2840, 2018.
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2018 | Journal Article | IST-REx-ID: 11558 | OA
D. Sobral et al., “Slicing COSMOS with SC4K: The evolution of typical Ly α emitters and the Ly α escape fraction from z ∼ 2 to 6,” Monthly Notices of the Royal Astronomical Society, vol. 476, no. 4. Oxford University Press, pp. 4725–4752, 2018.
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2018 | Journal Article | IST-REx-ID: 11555 | OA
S. Carniani et al., “Kiloparsec-scale gaseous clumps and star formation at z = 5–7,” Monthly Notices of the Royal Astronomical Society, vol. 478, no. 1. Oxford University Press, pp. 1170–1184, 2018.
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2018 | Journal Article | IST-REx-ID: 11620 | OA
Van Eylen V, Dai F, Mathur S, Gandolfi D, Albrecht S, Fridlund M, García RA, Guenther E, Hjorth M, Justesen AB, Livingston J, Lund MN, Pérez Hernández F, Prieto-Arranz J, Regulo C, Bugnet LA, Everett ME, Hirano T, Nespral D, Nowak G, Palle E, Silva Aguirre V, Trifonov T, Winn JN, Barragán O, Beck PG, Chaplin WJ, Cochran WD, Csizmadia S, Deeg H, Endl M, Heeren P, Grziwa S, Hatzes AP, Hidalgo D, Korth J, Mathis S, Montañes Rodriguez P, Narita N, Patzold M, Persson CM, Rodler F, Smith AMS. 2018. HD 89345: A bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2. Monthly Notices of the Royal Astronomical Society. 478(4), 4866–4880.
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2018 | Journal Article | IST-REx-ID: 13474 | OA
N. Smith, Y. L. L. Götberg, and S. E. de Mink, “Extreme isolation of WN3/O3 stars and implications for their evolutionary origin as the elusive stripped binaries,” Monthly Notices of the Royal Astronomical Society, vol. 475, no. 1. Oxford University Press, pp. 772–782, 2018.
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2018 | Journal Article | IST-REx-ID: 15236 | OA
C. Ng et al., “PSR J1755−2550: A young radio pulsar with a massive, compact companion,” Monthly Notices of the Royal Astronomical Society, vol. 476, no. 4. Oxford University Press, pp. 4315–4326, 2018.
[Preprint] View | DOI | Download Preprint (ext.) | arXiv
 

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