Exploring the crowded central region of ten Galactic globular clusters using EMCCDs Variable star searches and new discoveries (2016)
Journal Article
Figuera Jaimes, R., Bramich, D., Skottfelt, J., Kains, N., Jørgensen, U., Horne, K., Dominik, M., Alsubai, K., Bozza, V., Calchi Novati, S., Ciceri, S., D’Ago, G., Galianni, P., Gu, S.-H., Harpsøe, K., Haugbølle, T., Hinse, T., Hundertmark, M., Juncher, D., Korhonen, H., …MiNDSTEp Consortium, T. (2016). Exploring the crowded central region of ten Galactic globular clusters using EMCCDs Variable star searches and new discoveries. Astronomy & Astrophysics, 588, Article A128. https://doi.org/10.1051/0004-6361/201527641

Aims. We aim to obtain time-series photometry of the very crowded central regions of Galactic globular clusters; to obtain better angular resolution thanhas been previously achieved with conventional CCDs on ground-based telescopes; and to complete,... Read More about Exploring the crowded central region of ten Galactic globular clusters using EMCCDs Variable star searches and new discoveries.

A WISE view of novae - I. The data (2014)
Journal Article
(2014). A WISE view of novae - I. The data. Monthly Notices of the Royal Astronomical Society, 1683 - 1697. https://doi.org/10.1093/mnras/stu1467

We present the results of data-mining the Wide-field Infrared Survey Explorer (WISE) archive for data on classical and recurrent novae. We find that the detections are consistent with dust emission, line emission, emission by a stellar photosphere, o... Read More about A WISE view of novae - I. The data.

The evolution of massive stars and their spectra I. A non-rotating 60 Msun star from the zero-age main sequence to the pre-supernova stage (2014)
Journal Article
(2014). The evolution of massive stars and their spectra I. A non-rotating 60 Msun star from the zero-age main sequence to the pre-supernova stage. Astronomy & Astrophysics,

For the first time, the interior and spectroscopic evolution of a massive star is analyzed from the zero-age main sequence (ZAMS) to the pre-supernova (SN) stage. For this purpose, we combined stellar evolution models using the Geneva code and atmosp... Read More about The evolution of massive stars and their spectra I. A non-rotating 60 Msun star from the zero-age main sequence to the pre-supernova stage.