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52 Eclipsing Quadruple Star Candidates Discovered in TESS Full Frame Images

  • Authors: V. B. Kostov, B. P. Powell, S. A. Rappaport, T. Borkovits, R. Gagliano, M. Omohundro, T. L. Jacobs, M. H. Kristiansen, G. Torres, G. Handler, A. R. Schmitt, H. M. Schwengeler, T. Mitnyan, I. A. Terentev, D. M. LaCourse, A. Vanderburg, S. D. Alexandrov, C. M. da Silva, Marco Z. Di Fraia, Aline U. Fornear, M. Huten, D. Iannone, Julien S. de Lambilly, S. Lee, J. Orosz, R. Rodrigues, A. Tarr, W. Welsh

V. B. Kostov et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 17.

Upper panels: phase-folded TESS (red) and ASAS-SN data (green and blue, for the corresponding g and V bands) for quadruple candidate TIC 277316707. We measured orbital periods for the two EB components of PA = 1.475034 days (left, compared to 6.965 days as reported by L. W. IJspeert et al. 2021) and PB = 1.93217 days (right, consistent with L. W. IJspeert et al. 2021). Lower panels: 11 × 11 pixel-by-pixel lightcurves centered of the target for Sector 27. The red contours represent the ELEANOR aperture used to extract the lightcurve. We do not see a 6.965 day signal in the pixels surrounding the target.

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