The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab |Alam, Munazza K., L\\u00f3pez-Morales, Mercedes, et al. | AJ | 160-51 | 2020 | 2020AJ....160...51A | http://ui.adsabs.harvard.edu/#abs/2020AJ....160...51A
CARMENES detection of the Ca II infrared triplet and possible evidence of He I in the atmosphere of WASP-76b |Casasayas-Barris, N., Orell-Miquel, J., et al. | A&A | 654-163 | 2021 | 2021A&A...654A.163C | http://ui.adsabs.harvard.edu/#abs/2021A&A...654A.163C
H\\u03b1 and He I absorption in HAT-P-32 b observed with CARMENES. Detection of Roche lobe overflow and mass loss |Czesla, S., Lamp\\u00f3n, M., et al. | A&A | 657-6 | 2022 | 2022A&A...657A...6C | http://ui.adsabs.harvard.edu/#abs/2022A&A...657A...6C
HORuS transmission spectroscopy and revised planetary parameters of KELT-7 b |Tabernero, H. M., Zapatero Osorio, M. R., et al. | MNRAS | 515-1247 | 2022 | 2022MNRAS.515.1247T | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.1247T
Possible origin of the non-detection of metastable He I in the upper atmosphere of the hot Jupiter WASP-80b |Fossati, L., Pillitteri, I., et al. | A&A | 673-37 | 2023 | 2023A&A...673A..37F | http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..37F
The MUSCLES Extension for Atmospheric Transmission Spectroscopy: UV and X-Ray Host-star Observations for JWST ERS & GTO Targets |Behr, Patrick R., France, Kevin, et al. | AJ | 166-35 | 2023 | 2023AJ....166...35B | http://ui.adsabs.harvard.edu/#abs/2023AJ....166...35B
The elusive atmosphere of WASP-12 b. High-resolution transmission spectroscopy with CARMENES |Czesla, S., Lamp\\u00f3n, M., et al. | A&A | 683-A67 | 2024 | 2024A&A...683A..67C | http://ui.adsabs.harvard.edu/#abs/2024A&A...683A..67C
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Dr NORBERT SCHARTEL openParPSclosePar, 2020, 'ToO proposal on exoplanet atmospheres', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-5rmsizn
