@article{CamposPelisoliKamannetal.2018,
  author    = {Campos, Fabiola and Pelisoli, Ingrid Domingos and Kamann, Sebastian and Husser, T. -O. and Dreizler, S. and Bellini, A. and Robinson, E. L. and Nardiello, Domenico and Piotto, G. and Kepler, S. O. and Istrate, A. G. and Winget, D. E. and Montgomery, M. H. and Dotter, A.},
  title     = {Outliers},
  series = {Monthly notices of the Royal Astronomical Society},
  volume    = {481},
  journal   = {Monthly notices of the Royal Astronomical Society},
  number    = {4},
  publisher = {Oxford Univ. Press},
  address   = {Oxford},
  issn      = {0035-8711},
  doi       = {10.1093/mnras/sty2591},
  pages     = {4397 -- 4409},
  year      = {2018},
  abstract  = {We use Hubble Space Telescope multicolour photometry of the globular cluster 47 Tucanae to uncover a population of 24 objects with no previous classification that are outliers from the single-star model tracks in the colour-magnitude diagram and yet are likely cluster members. By comparing those sources with evolutionary models and X-ray source catalogues, we were able to show that the majority of those sources are likely binary systems that do not have any X-ray source detected nearby, most possibly formed by a white dwarf and a main-sequence star and a small number of possible double-degenerate systems.},
  language  = {en}
}
@article{GriggioBedinRaddietal.2022,
  author    = {Griggio, Massimo and Bedin, Luigi R. and Raddi, Roberto and Reindl, Nicole and Tomasella, Lina and Scalco, M. and Salaris, M. and Cassisi, S. and Ochner, P. and Ciroi, S. and Rosati, P. and Nardiello, Domenico and Anderson, J. and Libralato, Mattia and Bellini, A. and Vallenari, A. and Spina, L. and Pedani, M.},
  title     = {Astro-photometric study of M37 with Gaia and wide-field ugi-imaging},
  series = {Monthly notices of the Royal Astronomical Society},
  volume    = {515},
  journal   = {Monthly notices of the Royal Astronomical Society},
  number    = {2},
  publisher = {Oxford University Press},
  address   = {Oxford},
  issn      = {0035-8711},
  doi       = {10.1093/mnras/stac1920},
  pages     = {1841 -- 1853},
  year      = {2022},
  abstract  = {We present an astrometric and photometric wide-field study of the Galactic open star cluster M37 (NGC 2099). The studied field was observed with ground-based images covering a region of about four square degrees in the Sloan-like filters ugi. We exploited the Gaia catalogue to calibrate the geometric distortion of the large field mosaics, developing software routines that can be also applied to other wide-field instruments. The data are used to identify the hottest white dwarf (WD) member candidates of M37. Thanks to the Gaia EDR3 exquisite astrometry we identified seven such WD candidates, one of which, besides being a high-probability astrometric member, is the putative central star of a planetary nebula. To our knowledge, this is a unique object in an open cluster, and we have obtained follow-up low-resolution spectra that are used for a qualitative characterization of this young WD. Finally, we publicly release a three-colour atlas and a catalogue of the sources in the field of view, which represents a complement of existing material.},
  language  = {en}
}