Publications

Everything published, from NASA ADS. Titles link to the journal version or arXiv.

Entries
47
Citations
1494
Years
2011–2026

Of the 1494 citations, 106 are to the 18 group-led entries, 783 to 5 papers of large collaborations (author lists of 100 or more, among them the three Planck intermediate results), and 605 to the other 24 entries written with partners.

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6
2015
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2020
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2025
7

Group-ledOther entries

Group-led means a group member is first or last author.

Research line
Instrument or survey
Role

47 of 47 entries

Instruments are matched from each title and abstract, so a paper that only uses a Planck-selected sample is also listed under Planck. Download all entries as publications.bib; author lists are cut at ten.

Papers

33 entries

  1. 2026
    Discovery of a compact hub-filament system in G286.21 + 0.17 with JWST and ALMA: insights into protocluster formation and competitive accretionDewangan, Bhadari, Yadav, … Alina (9 of 20) et al.Monthly Notices of the Royal Astronomical Society, 552, stag1764 · arXiv:2605.14693 ·
  2. 2026
    B-FROST: B-Fields and star formation across scales with TRAO: CO abundances, dynamics, and relative orientations in the translucent high latitude cloud MBM12Vorster, Montillaud, Juvela, … Alina (7 of 17) et al.Astronomy and Astrophysics, 711, A157 · arXiv:2605.21101 ·
  3. 2026
    Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regionsOers, Ristorcelli, Ferrière, … Alina (6 of 7) et al.Astronomy and Astrophysics, 711, A97 · arXiv:2606.04713 ·
    1 cit.
  4. 2026
    Interstellar Filament Detection and Characterization: Methods and Implications for Studies of the Magnetized Interstellar MediumAlinaGalaxies, 14, 53 · arXiv:2606.31507 ·
  5. 2026
    MAJORS II: HCO+ and HCN abundances in W40Plume, Eden, Currie, … Alina (18 of 37) et al.Monthly Notices of the Royal Astronomical Society, 547, stag186 · arXiv:2601.19971 ·
  6. 2025
    Deep Learning for Position Angle Quantification Applied to Interstellar FilamentsUmetaliev, Alina, SalmenovaThe Astronomical Journal, 170, 207 · Our method achieves a validation mean squared error of 7.73, demonstrating improved accuracy over existing approaches.
    1 cit.
  7. 2025
    Magnetic Field of a Ring-like Molecular CloudAlina, Umirbayeva, Doi et al.The Astronomical Journal, 170, 152 · arXiv:2507.19281 · Our findings support a scenario where G111's morphology results from turbulent shock-driven compression, rather than simple gravitational contraction.
  8. 2025
    The dust polarisation and magnetic field structure in the centre of NGC253 with ALMABelfiori, Paladino, Hughes, … Alina (5 of 10) et al.Astronomy and Astrophysics, 697, A24 · arXiv:2503.03493 ·
    4 cit.
  9. 2024
    The Magnetic Field in Quiescent Star-forming Filament G16.96+0.27Gu, Liu, Shen, … Alina (22 of 23) et al.The Astrophysical Journal, 976, 249 · arXiv:2410.15913 ·
    6 cit.
  10. 2024
    On the Scarcity of Dense Cores (n > 105 cm−3) in High-latitude Planck Galactic Cold ClumpsXu, Wang, Liu, … Alina (24 of 37) et al.The Astrophysical Journal Letters, 963, L9 · arXiv:2401.14658 ·
    3 cit.
  11. 2023
    Nature of striation in 21 cm channel Maps: velocity causticsHu, Lazarian, Alina et al.Monthly Notices of the Royal Astronomical Society, 524, 2994 · arXiv:2306.10005 ·
    20 cit.
  12. 2023
    Performance of the polarization leakage correction in the PILOT dataBernard, Bernard, Roussel, … Alina (5 of 37) et al.Experimental Astronomy, 56, 197 · arXiv:2205.03668 ·
    1 cit.
  13. 2023
    Unveiling polarized emission from interstellar dust of the Large Magellanic Cloud with PlanckAlina, Bernard, Yuen et al.Monthly Notices of the Royal Astronomical Society, 518, 4466 · arXiv:2205.01275 · After foreground removal, the geometry of the plane-of-the-sky magnetic field tends to follow the structure of the atomic gas.
    6 cit.
  14. 2022
    Large-scale magnetic field in the Monoceros OB 1 east molecular cloudAlina, Montillaud, Hu et al.Astronomy and Astrophysics, 658, A90 · arXiv:2007.15344 · Our analysis reveals a shock region in the northern part right between two filamentary clouds that, in previous studies, were suggested to be involved in a collision.
    26 cit.
  15. 2021
    Dust polarization studies on MHD simulations of molecular clouds: comparison of methods for the relative-orientation analysisMicelotta, Juvela, Padoan, … Alina (5 of 6) et al.Astronomy and Astrophysics, 647, A121 · arXiv:1810.10014 ·
    7 cit.
  16. 2021
    ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of Extremely High-density Compact Structure of Prestellar Cores and Multiple Substructures WithinSahu, Liu, Liu, … Alina (10 of 41) et al.The Astrophysical Journal Letters, 907, L15 · arXiv:2012.08737 ·
    32 cit.
  17. 2019
    Multi-scale analysis of the Monoceros OB 1 star-forming region. I. The dense core populationMontillaud, Juvela, Vastel, … Alina (17 of 27) et al.Astronomy and Astrophysics, 631, L1 · arXiv:1909.03781 ·
    12 cit.
  18. 2019
    Multi-scale analysis of the Monoceros OB 1 star-forming region. II. Colliding filaments in the Monoceros OB1 molecular cloudMontillaud, Juvela, Vastel, … Alina (17 of 27) et al.Astronomy and Astrophysics, 631, A3 · arXiv:1909.06145 ·
    29 cit.
  19. 2019
    The geometry of the magnetic field in the central molecular zone measured by PILOTMangilli, Aumont, Bernard, … Alina (17 of 40) et al.Astronomy and Astrophysics, 630, A74 · arXiv:1901.06196 ·
    49 cit.
  20. 2019
    Magnetic Fields in the Infrared Dark Cloud G34.43+0.24Soam, Liu, Andersson, … Alina (34 of 43) et al.The Astrophysical Journal, 883, 95 · arXiv:1908.03624 ·
    55 cit.
  21. 2019
    SCOPE: SCUBA-2 Continuum Observations of Pre-protostellar Evolution - survey description and compact source catalogueEden, Liu, Kim, … Alina (62 of 163) et al.Monthly Notices of the Royal Astronomical Society, 485, 2895 · arXiv:1902.10180 ·
    43 cit.
  22. 2019
    Statistical analysis of the interplay between interstellar magnetic fields and filaments hosting Planck Galactic cold clumpsAlina, Ristorcelli, Montier et al.Monthly Notices of the Royal Astronomical Society, 485, 2825 · arXiv:1712.09325 · …we find that this trend is significant only for low-contrast filaments, whereas high-contrast filaments tend to be randomly orientated with respect to the background magnetic field.
    34 cit.
  23. 2018
    Dust spectrum and polarisation at 850 μm in the massive IRDC G035.39-00.33Juvela, Guillet, Liu, … Alina (6 of 21) et al.Astronomy and Astrophysics, 620, A26 · arXiv:1809.00864 ·
    27 cit.
  24. 2018
    The TOP-SCOPE Survey of PGCCs: PMO and SCUBA-2 Observations of 64 PGCCs in the Second Galactic QuadrantZhang, Liu, Yuan, … Alina (22 of 26) et al.The Astrophysical Journal Supplement Series, 236, 49 · arXiv:1805.03883 ·
    15 cit.
  25. 2018
    A Holistic Perspective on the Dynamics of G035.39-00.33: The Interplay between Gas and Magnetic FieldsLiu, Li, Juvela, … Alina (37 of 57) et al.The Astrophysical Journal, 859, 151 · arXiv:1803.09457 ·
    81 cit.
  26. 2018
    The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17Liu, Kim, Juvela, … Alina (51 of 156) et al.The Astrophysical Journal Supplement Series, 234, 28 · arXiv:1711.04382 ·
    65 cit.
  27. 2017
    The optical performance of the PILOT instrument from ground end-to-end testsMisawa, Bernard, Longval, … Alina (6 of 51) et al.Experimental Astronomy, 43, 211 ·
    3 cit.
  28. 2016
    Polarization measurement analysis. III. Analysis of the polarization angle dispersion function with high precision polarization dataAlina, Montier, Ristorcelli et al.Astronomy and Astrophysics, 595, A57 · arXiv:1608.07105 · We characterize for the first time the bias on the conventional estimator of the polarization angle dispersion function and show that it can be positive or negative depending on the true value.
    16 cit.
  29. 2015
    Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visiblePlanck Collaboration, Ade, Aghanim, … Alina (4 of 196) et al.Astronomy and Astrophysics, 576, A106 · arXiv:1405.0873 ·
    94 cit.
  30. 2015
    Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dustPlanck Collaboration, Ade, Aghanim, … Alina (4 of 203) et al.Astronomy and Astrophysics, 576, A104 · arXiv:1405.0871 ·
    438 cit.
  31. 2015
    Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulencePlanck Collaboration, Ade, Aghanim, … Alina (4 of 189) et al.Astronomy and Astrophysics, 576, A105 · arXiv:1405.0872 ·
    143 cit.
  32. 2015
    Polarization measurement analysis. II. Best estimators of polarization fraction and angleMontier, Plaszczynski, Levrier, … Alina (5 of 8) et al.Astronomy and Astrophysics, 574, A136 · arXiv:1407.0178 ·
    75 cit.
  33. 2015
    Polarization measurement analysis. I. Impact of the full covariance matrix on polarization fraction and angle measurementsMontier, Plaszczynski, Levrier, … Alina (5 of 7) et al.Astronomy and Astrophysics, 574, A135 · arXiv:1406.6536 ·
    57 cit.

Preprints

2 entries

  1. 2026
    Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effectsMakarova, Alina, Padoan et al.arXiv e-prints, arXiv:2608.00441 · arXiv:2608.00441 · In our simulation, we find that 80% of future massive stars are associated with clustered environments.
  2. 2022
    MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISMAlina, Shomanov, BaimukhametovaarXiv e-prints, arXiv:2205.00683 · arXiv:2205.00683 · We showed that neural network training might be performed efficiently on a relatively small training sample of only around 100 maps.
    6 cit.

Proceedings and talks

6 entries

  1. 2026
    Magnetic field structure of the LMC: Insights from Atomic gas data and foreground emission separationAlina, Bernard, Yuen et al.IAU Symposium, 20, 179 ·
  2. 2024
    Neural Networks Unveiling Filamentary Structures in the Interstellar Medium: A Multi-Wavelength Approach Integrating Data from Advanced TelescopesAlina, Umetaliev32nd General Assembly International Union (IAUGA 2024), 104 · We test our model on observational data from the Planck and Herschel space telescopes and show its reliability.
  3. 2024
    The Magnetic Field Structure of the Large Magellanic Cloud: Insights from Atomic Gas Data and Foreground Emission SeparationAlina, Bernard, Yuen et al.32nd General Assembly International Union (IAUGA 2024), 103 · This allowed us to remove the foreground emission and reveal the outer spiral density structures and central molecular regions of the LMC.
  4. 2023
    An overview of the PILOT balloon-borne experiment dust polarization dataAlina, Bernard, Roussel et al.EAS2023, European Astronomical Society Annual Meeting, 1537 ·
  5. 2020
    Statistics on the relative orientation between magnetic fields and filaments hosting Planck Galactic Cold ClumpsAlina, Ristorcelli, Montier, JuvelaIAU General Assembly, 104 · The relative orientation clearly shows a transition from parallel to no preferential and perpendicular alignment depending on the volume densities of both clumps and filaments.
  6. 2014
    Galactic dust polarization with Planck: methods and first resultsAlina40th COSPAR Scientific Assembly, 40, H0.2-0006-14 ·

Data and code

1 entries

  1. 2025
    Temirkul/ism-filaments-analysis: U-Net for Angle Identification of Filamentary Structures --- First ReleaseUmetaliev, Alina, SalmenovaZenodo ·
    1 cit.

Proposals

1 entries

  1. 2025
    Mass inflow structures in star formation from filaments to streamers: the unique field of Orion Molecular Cloud 3Juvela, Alina, Demyk et al.JWST Proposal. Cycle 4, 7433 ·

Theses

1 entries

  1. 2015
    Analysis of the interstellar dust polarized emission with the Planck Satellite Survey dataAlinaPh.D. Thesis ·

Stellar magnetism

3 entries. Spectropolarimetry of Sirius and Vega, before the move to interstellar magnetic fields.

  1. 2012
    Long-term magnetic field stability of VegaAlina, Petit, Lignières et al.Stellar Polarimetry: from Birth to Death, 1429, 82 · arXiv:1107.5639 · …showing that most recognizable features of the photospheric field of Vega are only weakly distorted by large-scale surface flows (differential rotation or meridional circulation).
    16 cit.
  2. 2011
    Weak magnetic fields of intermediate-mass starsPetit, Lignières, Wade, … Alina (5 of 7) et al.Astronomische Nachrichten, 332, 943 · arXiv:1109.6888 ·
    10 cit.
  3. 2011
    Detection of a weak surface magnetic field on Sirius A: are all tepid stars magnetic?Petit, Lignières, Aurière, … Alina (5 of 11) et al.Astronomy and Astrophysics, 532, L13 · arXiv:1106.5363 ·
    118 cit.

Source: NASA ADS, query author:"Alina, D", refreshed with scripts/fetch_publications.py. One-line results are quoted from the abstracts.