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PreprintCC BY 4.0arXiv

Detection of new Galactic Wolf-Rayet stars with SPHEREx

Abstract

We assess the potential for the NASA Explorer SPHEREx mission in adding to the Milky Way census of Wolf-Rayet (WR) stars by extracting 0.75--5micron spectrophotometry of 30 candidate WR stars previously identified using Gaia XP spectra. We confirm an additional Galactic 13 WR (8 WN and 5 WC) stars, identify 3 probable [WC]-type central stars of Planetary Nebulae, plus 2 He emission line sources. SPHEREx has the potential to detect additional relatively isolated WR stars on the far size of the Milky Way by combining Machine Learning techniques with a judicious choice of candidate selection criteria. Indeed SPHEREx is sufficiently sensitive to identify bright Magellanic Cloud Wolf-Rayet stars.

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BibTeX
@misc{crowther2026detection,
  title = {{Detection of new Galactic Wolf-Rayet stars with SPHEREx}},
  author = {Paul A. Crowther and Erin L. Smith},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.28640},
  eprint = {2609.28640},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.28640},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Detection of new Galactic Wolf-Rayet stars with SPHEREx
AU  - Paul A. Crowther
AU  - Erin L. Smith
PY  - 2026
DA  - 2026/09/23
PB  - arXiv
DO  - 10.48550/arxiv.2609.28640
UR  - https://arxiv.org/abs/2609.28640
AB  - We assess the potential for the NASA Explorer SPHEREx mission in adding to the Milky Way census of Wolf-Rayet (WR) stars by extracting 0.75--5micron spectrophotometry of 30 candidate WR stars previously identified using Gaia XP spectra. We confirm an additional Galactic 13 WR (8 WN and 5 WC) stars, identify 3 probable [WC]-type central stars of Planetary Nebulae, plus 2 He emission line sources. SPHEREx has the potential to detect additional relatively isolated WR stars on the far size of the Milky Way by combining Machine Learning techniques with a judicious choice of candidate selection criteria. Indeed SPHEREx is sufficiently sensitive to identify bright Magellanic Cloud Wolf-Rayet stars.
ER  -