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Integral field spectroscopy of massive young stellar objects in the N113 H II region in the Large Magellanic Cloud (2015)
Journal Article
Ward, J., Oliveira, J., Van Loon, J. T., & Sewiło, M. (2016). Integral field spectroscopy of massive young stellar objects in the N113 H II region in the Large Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 455(3), 2345 - 2362. https://doi.org/10.1093/mnras/stv2424

The Spitzer Surveying the Agents of Galaxy Evolution (SAGE) survey has allowed the identification and analysis of significant samples of Young Stellar Object (YSO) candidates in the Large Magellanic Cloud (LMC). However, the angular resolution of Spi... Read More about Integral field spectroscopy of massive young stellar objects in the N113 H II region in the Large Magellanic Cloud.

Characterising the Protostellar Population of the Magellanic Clouds with VLT/SINFONI (2015)
Journal Article
Ward, J., Oliveira, J., van Loon, J., & Sewilo, M. (2015). Characterising the Protostellar Population of the Magellanic Clouds with VLT/SINFONI. Proceedings of the International Astronomical Union, 11(S315), https://doi.org/10.1017/s1743921316008449

At distances of ~50 kpc and ~60 kpc for the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) respectively the Magellanic Clouds present us with a unique opportunity to study star formation in environments outside our own galaxy. Through... Read More about Characterising the Protostellar Population of the Magellanic Clouds with VLT/SINFONI.

Spitzer infrared spectrograph point source classification in the Small Magellanic Cloud (2015)
Journal Article
Ruffle, P. M., Kemper, F., Jones, O., Sloan, G., Kraemer, K., Woods, P. M., …Zijlstra, A. (2015). Spitzer infrared spectrograph point source classification in the Small Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 451(4), 3504 -3536. https://doi.org/10.1093/mnras/stv1106

The Magellanic Clouds are uniquely placed to study the stellar contribution to dust emission. Individual stars can be resolved in these systems even in the mid-infrared, and they are close enough to allow detection of infrared excess caused by dust.... Read More about Spitzer infrared spectrograph point source classification in the Small Magellanic Cloud.

Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC (2015)
Journal Article
Hony, S., Gouliermis, D., Galliano, F., Galametz, M., Cormier, D., Chen, C., …Wu, R. (2015). Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC. Monthly Notices of the Royal Astronomical Society, 448(2), 1847 - 1862. https://doi.org/10.1093/mnras/stv107

The rate at which interstellar gas is converted into stars, and its dependence on environment, is one of the pillars on which our understanding of the visible Universe is build. We present a comparison of the surface density of young stars (S?) and d... Read More about Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC.

ERRATUM: “THE HERSCHEL INVENTORY OF THE AGENTS OF GALAXY EVOLUTION (HERITAGE) IN THE MAGELLANIC CLOUDS, A HERSCHEL OPEN TIME KEY PROGRAM” (2013, AJ, 146, 62) (2015)
Journal Article
Meixner, M., Panuzzo, P., Roman-Duval, J., Engelbracht, C., Babler, B., Seale, J., …Whitney, B. (2015). ERRATUM: “THE HERSCHEL INVENTORY OF THE AGENTS OF GALAXY EVOLUTION (HERITAGE) IN THE MAGELLANIC CLOUDS, A HERSCHEL OPEN TIME KEY PROGRAM” (2013, AJ, 146, 62). Astronomical Journal, 149(2), Article 88. https://doi.org/10.1088/0004-6256/149/2/88

We provide a corrected Table 4 that lists the total galaxy fluxes for the HERTIAGE bands and corresponding Figure 19 which plots these fluxes in comparison to prior measurements These corrected fluxes differ by up to 41% to what we reported in the or... Read More about ERRATUM: “THE HERSCHEL INVENTORY OF THE AGENTS OF GALAXY EVOLUTION (HERITAGE) IN THE MAGELLANIC CLOUDS, A HERSCHEL OPEN TIME KEY PROGRAM” (2013, AJ, 146, 62).