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1
ExoMol molecular line lists XXX: a complete high-accuracy line list for water
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ExoMol molecular line lists XXX: a complete high-accuracy line list for water

Polyansky, Oleg L ; Kyuberis, Aleksandra A ; Zobov, Nikolai F ; Tennyson, Jonathan ; Yurchenko, Sergei N ; Lodi, Lorenzo

Monthly notices of the Royal Astronomical Society, 2018-10, Vol.480 (2), p.2597-2608 [Periódico revisado por pares]

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2
The ATLAS3D Project – XXX. Star formation histories and stellar population scaling relations of early-type galaxies
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The ATLAS3D Project – XXX. Star formation histories and stellar population scaling relations of early-type galaxies

McDermid, Richard M. ; Alatalo, Katherine ; Blitz, Leo ; Bournaud, Frédéric ; Bureau, Martin ; Cappellari, Michele ; Crocker, Alison F. ; Davies, Roger L. ; Davis, Timothy A. ; de Zeeuw, P. T. ; Duc, Pierre-Alain ; Emsellem, Eric ; Khochfar, Sadegh ; Krajnović, Davor ; Kuntschner, Harald ; Morganti, Raffaella ; Naab, Thorsten ; Oosterloo, Tom ; Sarzi, Marc ; Scott, Nicholas ; Serra, Paolo ; Weijmans, Anne-Marie ; Young, Lisa M.

Monthly notices of the Royal Astronomical Society, 2015-04, Vol.448 (4), p.3484-3513 [Periódico revisado por pares]

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3
Prospects for measuring cosmic microwave background spectral distortions in the presence of foregrounds
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Prospects for measuring cosmic microwave background spectral distortions in the presence of foregrounds

Abitbol, Maximilian H. ; Chluba, Jens ; Hill, J. Colin ; Johnson, Bradley R.

Monthly notices of the Royal Astronomical Society, 2017-10, Vol.471 (1), p.1126-1140 [Periódico revisado por pares]

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4
Trinity I: self-consistently modelling the dark matter halo–galaxy–supermassive black hole connection from z  = 0–10
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Trinity I: self-consistently modelling the dark matter halo–galaxy–supermassive black hole connection from z  = 0–10

Zhang (张昊文), Haowen ; Behroozi, Peter ; Volonteri, Marta ; Silk, Joseph ; Fan, Xiaohui ; Hopkins, Philip F ; Yang (杨锦怡), Jinyi ; Aird, James

Monthly notices of the Royal Astronomical Society, 2023-01, Vol.518 (2), p.2123-2163 [Periódico revisado por pares]

Oxford University Press (OUP): Policy P - Oxford Open Option A

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5
Tomographic measurement of the intergalactic gas pressure through galaxy–tSZ cross-correlations
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Tomographic measurement of the intergalactic gas pressure through galaxy–tSZ cross-correlations

Koukoufilippas, Nick ; Alonso, David ; Bilicki, Maciej ; Peacock, John A

Monthly notices of the Royal Astronomical Society, 2020-02, Vol.491 (4), p.5464-5480 [Periódico revisado por pares]

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6
The rate, luminosity function and time delay of non-Collapsar short GRBs
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The rate, luminosity function and time delay of non-Collapsar short GRBs

Wanderman, David ; Piran, Tsvi

Monthly notices of the Royal Astronomical Society, 2015-04, Vol.448 (4), p.3026-3037 [Periódico revisado por pares]

London: Oxford University Press

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7
Importance of intracluster scattering and relativistic corrections from tSZ effect with cosmic infrared background
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Importance of intracluster scattering and relativistic corrections from tSZ effect with cosmic infrared background

Acharya, Sandeep Kumar ; Chluba, Jens

Monthly notices of the Royal Astronomical Society, 2023-02, Vol.519 (2), p.2138-2154 [Periódico revisado por pares]

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8
Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies
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Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies

Adak, Debabrata ; Shaikh, Shabbir ; Sinha, Srijita ; Ghosh, Tuhin ; Boulanger, Francois ; Lagache, Guilaine ; Souradeep, Tarun ; Miville-Deschênes, Marc-Antoine

Monthly notices of the Royal Astronomical Society, 2024-06, Vol.531 (4), p.4876-4892 [Periódico revisado por pares]

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9
Batchelor, Saffman, and Kazantsev spectra in galactic small-scale dynamos
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Batchelor, Saffman, and Kazantsev spectra in galactic small-scale dynamos

Brandenburg, Axel ; Zhou, Hongzhe ; Sharma, Ramkishor

Monthly notices of the Royal Astronomical Society, 2023-01, Vol.518 (3), p.3312-3325 [Periódico revisado por pares]

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10
Can the observed E/B ratio for dust galactic foreground be explained by sub-Alfvénic turbulence?
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Can the observed E/B ratio for dust galactic foreground be explained by sub-Alfvénic turbulence?

Kandel, D ; Lazarian, A ; Pogosyan, D

Monthly notices of the Royal Astronomical Society. Letters, 2017-11, Vol.472 (1), p.L10-L14 [Periódico revisado por pares]

Oxford University Press

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