Astronomy and Astrophysics, 432, pp. 851-859, http://dx.doi.org./10.1051/0004-6361:20041053
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2005 (v1)Journal articleUploaded on: December 3, 2022
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2005 (v1)Journal article
Astrophysical Journal, 621, pp. 777-784, http://dx.doi.org./10.1086/427796
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2019 (v1)Journal article
We present a deep Blanco/DECam colour-magnitude diagram (CMD) for the large but very diffuse Milky Way satellite dwarf galaxy Crater II. The CMD shows only old stars with a clearly bifurcated subgiant branch (SGB) that feeds a narrow red giant branch. The horizontal branch (HB) shows many RR Lyrae and red HB stars. Comparing the CMD with [Fe/H]...
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2022 (v1)Journal article
Context. Classical Cepheids are the most popular distance indicators and tracers of young stellar populations. The key advantage is that they are bright and they can be easily identified in Local Group and Local Volume galaxies. Their evolutionary and pulsation properties depend on their chemical abundances. Aims: The main aim of this...
Uploaded on: December 3, 2022 -
2010 (v1)Journal article
Publications of the Astronomical Society of the Pacific, 122, pp. 651-661 (2010)
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2012 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
June 1, 2020 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
December 2018 (v1)Publication
The main aim of this experiment is to provide a complete census of old (t > 10 Gyr, RR Lyrae, type II Cepheids, red horizontal branch), intermediate age (red clump, Miras) and young (classical Cepheids) stellar tracers across the Galactic Bulge. To fully exploit the unique photometric quality of LSST images, we plan to perform a Shallow...
Uploaded on: December 3, 2022