2020

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• Observing the stellar halo of Andromeda in cosmological simulations: the Auriga2PAndAS pipeline

        Thomas G. F. et al., arXiv: 2009.00010

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• The hidden past of M92: Detection and characterization of a newly formed 17° long stellar stream using the Canada-France Imaging Survey

          Thomas G. F. et al., In press (ApJ; arXiv: 2009.04487)

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• The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way

        Arentsen A. et al. (including Thomas G. F.),  arXiv:2006.08641

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• The Pristine Dwarf-Galaxy survey -- III. Revealing the nature of the Milky Way globular cluster Sagittarius II

        Longeard, N. et al. (including Thomas G. F.),  arXiv:2005.05976

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• Globular clusters in the Sagittarius stream. Revising members and candidates with Gaia DR2

        Bellazzini, M. et al. (including Thomas G. F.),  2020, A&A, 636A, 107

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• The Pristine Survey - VIII. The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime  

        Youakim K. et al. (including Thomas G. F.),  2020, MNRAS, 492, 4986

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• The Pristine survey - IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars    

        Venn K. et al. (including Thomas G. F.),  2020, MNRAS, 492, 3241

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• A Panoramic Landscape of the Sagittarius Stream in Gaia DR2 Revealed with the STREAMFINDER Spyglass    

        Ibata R., Bellazzini M., Thomas G. F., et al.,  2020, ApJ, 891L, 19

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• Detection of Strong Epicyclic Density Spikes in the GD-1 Stellar Stream: An Absence of Evidence for the Influence of Dark Matter Subhalos?    
  Ibata R., Thomas, G. F., et al.,  2020, ApJ, 891, 161

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• The Pristine survey - X. A large population of low-metallicity stars permeates the Galactic disc  
  Sestito F. et al. (including Thomas G. F.),  2020, MNRAS, 497L, 7

 

• The Pristine Inner Galaxy Survey (PIGS) I: tracing the kinematics of metal-poor stars in the Galactic bulge    

        Arentsen A. et al. (including Thomas G. F.),  2020, MNRAS, 491L, 11

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