Massive young clusters in the Milky Way and the Scutum Complex
The last decade has brought the discovery of a large number of massive (M > 10000 M?) young open clusters in the Milky Way, which had previously not been...
The main goal of the MASTER-Net project is to produce a unique fast sky survey with all sky observed over a single night down to a limiting magnitude of 21...
MaxiMask: A new tool to identify contaminants in astronomical images using convolutional neural networks.
We propose to use convolutional neural networks to detect contaminants in astronomical images. Once trained, our networks are able to detect various...
Measurement of a large scale flow with clusters of galaxies
Peculiar velocities of galaxies, derived using distance estimators, are plagued with systematic effects and are unreliable beyond 100 Mpc/h. In Kashlinsky &...
Measuring a Galaxy: Morphology, Mass, Environment and Evolution
What can the shape and size of a galaxy tell us about how it has evolved across cosmic time? Which evolutionary mechanisms are important, or relevant, and which...
Measuring galaxy clustering in photometric redshift surveys
In this talk I will show how we can study cosmolgy in a photometric redshift galaxy survey, by means of the angular clustering of galaxies. Previously to fit...
Measuring the CMB Polarization with the Atacama Cosmology Telescope.
We have learned a great deal about the universe from measurements ofthe cosmic microwave background (CMB). Most of what we have learned so far has been based on...
MEGARA about to start operations at GTC: performance review and commissioning results
MEGARA is a powerful instrument for the GTC 10m telescope lead by University Complutense de Madrid (UCM, PI: Armando Gil de Paz) and developed by a Consortium...
Metallicity distribution of Galactic thin disk & halo using Cepheids & RR Lyrae
We present new results concerning the radial gradients (Fe, alpha, s- and r-process elements) across the Galactic thin disk. We use young (t<300 Myr, classical...