Research

Artist depiction of exoplanet K2-18 b. Credits: NASA, ESA, CSA, Joseph Olmsted (STScI)

Current Research

To be updated

Previous Research

During my bachelor’s studies at the Faculty of Mathematics and Physics, Charles University, I joined the newly created Exoplanetary group at the Astronomical Institute of the Czech Academy of Sciences under the supervision of Dr. Petr Kabáth. There I spent a considerable amount of time conducting spectroscopic observation using the Ondřejov Echelle Spectrograph (OES) mounted on the 2-meter Perek telescope at the Astronomical Institute of the Czech Academy of Sciences.

Our group focused on follow-up observations of Kepler/K2 exoplanetary candidates. The published research covered the initial results and findings from the observations and radial-velocity measurements of the targets, making ground for the follow-up observations of TESS mission candidates. I actively participated in observations and data reduction. We used IRAF software (Image Reduction and Analysis Facility, ancient software also known as hell on Earth) for spectra reduction and radial velocity measurements.

To explain it more details; we were taking the spectra of stars, which were pre-selected by the Kepler Space Telescope as a potential host stars for exoplanets. After basic image reduction we processed an echelle spectrum to get a 1D spectrum of the host star. From a time series of many spectra we were able to measure the radial velocity shifts of the spectra. If an RV shift occurred we studied whether it could be caused by the Doppler effect. This would be caused by the exoplanet and star orbiting a common center of gravity.

List of Publications

You can find publications also at ResearchGate of in Scopus. You can also look for my ORCiD number 0009-0009-0516-4972 .

Research Papers

  • Kabáth P., Skarka M., Sabotta S., Guenther E., Jones D., Klocová T., Šubjak J., Žák J., Špoková M., Blažek M., Dvořáková J., Dupkala D. (2020): Ondřejov Echelle Spectrograph, Ground Based Support Facility for Exoplanet Missions. PASP 132 1009, 035002
    DOI: 10.1088/1538-3873/ab6752
  • Sabotta S., Kabáth P., Korth J., Guenther E., Dupkala D., Grziwa S., Klocová T., Skarka M. (2019): Lack of close-in, massive planets of main-sequence A-type stars from Kepler. MNRAS 489 2, 2069-2078
    DOI: 10.1093/mnras/stz2232
  • Skarka M., Kabáth P., Paunzen E., Fedurco M., Budaj J., Dupkala D., Krtička J., Hatzes A., Pribulla T., Parimucha Š., Mikulášek Z., Guenther E., Sabotta S., Blažek M., Dvořáková J., Hambálek L., Klocová T., Kollár V., Kundra E., Šlechta M., Vaňko M. (2019): HD 99458: First time ever Ap-type star as a δ Scuti pulsator in a short period eclipsing binary? MNRAS 487 3, 4230-4237
    DOI: 10.1093/mnras/stz1478
  • Gajdoš P., Vaňko M., Pribulla T., Dupkala D., Šubjak J., Skarka M., Kabáth P., Hambálek Ľ., Parimucha Š. (2019): Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410. MNRAS 484 3, 4352-4359
    DOI: 10.1093/mnras/stz305

Final Theses

  • Dupkala D. (2023): Outreach of an Exoplanet Research and the PLATO Space Mission in the Czech Republic. Prague. Master’s thesis. Charles University, Faculty of Mathematics and Physics. Supervised by Drozd Z.
    –> Thesis Final Text & Defense Slides
  • Dupkala D. (2019): High resolution spectroscopy of exoplanets — tool for characterization. Ondřejov. Bachelor’s thesis. Charles University, Faculty of
    Mathematics and Physics. Supervised by Kabath P.
    –> Thesis Final Version & Defense Slides
  • Dupkala D. (2018): Characterization of exoplanetary candidates from
    mission K2 — measurements of radial velocities.
    Ondřejov. Student Faculty
    Grant summary, Charles University, Faculty of Mathematics and Physics.
    Supervised by Kabath P., Skarka M.
    –> Grant Summary Text

Other Publications