TOI-530b: A giant planet transiting an M dwarf detected by TESS

@inproceedings{Gan2021TOI530bAG,
  title={TOI-530b: A giant planet transiting an M dwarf detected by TESS},
  author={Tianjun Gan and Zitao Lin and Sharon Xuesong Wang and Shude Mao and Pascal Fouqu'e and Keivan G. Stassun and Steven A. Giacalone and Akihiko Fukui and Felipe Murgas and David R. Ciardi and Steve B. Howell and Karen A. Collins and Avi Shporer and Luc Arnold and Thomas Barclay and David Charbonneau and Jessie L. Christiansen and Ian J. M. Crossfield and Courtney D. Dressing and Ashley Elliott and Emma Esparza-Borges and Phil Evans and Crystal L. Gnilka and Erica J. Gonzales and Andrew W. Howard and Keisuke Isogai and Kiyoe Kawauchi and Seiya Kurita and Beibei Liu and John H. Livingston and Rachel A. Matson and Norio Narita and Enric Pall{\'e} and Hannu Parviainen and Benjamin V. Rackham and D. R. Rodriguez and Mark E. Rose and Alexander Rudat and Joshua E. Schlieder and Nicholas J. Scott and Michael Vezie and George R. Ricker and Roland K. Vanderspek and David W. Latham and Sara Seager and Joshua N. Winn and Jon M. Jenkins},
  year={2021}
}
We report the discovery of TOI-530b, a transiting giant planet around an M0.5V dwarf, delivered by the Transiting Exoplanet Survey Satellite (TESS). The host star is located at a distance of 147.7 ± 0.6 pc with a radius of R∗ = 0.54 ± 0.03 R and a mass of M∗ = 0.53 ± 0.02 M . We verify the planetary nature of the transit signals by combining ground-based multi-wavelength photometry, high resolution spectroscopy from SPIRou as well as high-angular-resolution imaging. With V = 15.4 mag, TOI530b… 

References

SHOWING 1-6 OF 6 REFERENCES
SPIRou: A NIR Spectropolarimeter/High-Precision Velocimeter for the CFHT
SPIRou is a near-infrared (nIR) spectropolarimeter / velocimeter for the Canada-France-Hawaii Telescope (CFHT), that will focus on two forefront science topics, (i) the quest for habitable Earth-like
Doppler Tomography
I review the method of Doppler tomography which is widely used to understand the complex emission line profile variations displayed by accreting binary stars. Doppler tomography uses the information