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The Interpolation Constraint in the RV Analysis of M Dwarfs Using Empirical Templates

  • Authors: Dhvani Doshi, Nicolas B. Cowan, Étienne Artigau, René Doyon, André M. Silva, Khaled Al Moulla, Yashar Hezaveh

Dhvani Doshi et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Top: an intrinsic stellar spectrum which is Doppler shifted and then convolved. Middle: the convolved spectrum is down-sampled to SPIRou’s resolution, but no photon noise is added, thus representing a noiseless observation. Here, each black point represents a SPIRou pixel. This synthetic observation is then upsampled using spline interpolation as a precursor to constructing the template. Bottom: discrepancies between the upsampled and convolved spectrum, indicating that the template will contain altered stellar features.

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