Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF

  • Authors: Soichiro Hattori, Ruth Angus, Daniel Foreman-Mackey, Yuxi (Lucy) Lu, Isabel Colman

Soichiro Hattori et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 7.

A source (TIC 219795667) where we measured a TESS period that is half of what was measured from ZTF. We can see that the second TESS periodogram peak at 43 days corresponds to the same period as that measured from ZTF.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse