activity
20172021
most citedDeep learning for galaxy surface brightness profile fitting

87 citations · 119 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202132 cited

SDSS-IV MaNGA: drivers of stellar metallicity in nearby galaxies

Justus Neumann, Daniel Thomas, Claudia Maraston +12

The distribution of stellar metallicities within and across galaxies is an excellent relic of the chemical evolution across cosmic time. We present a detailed analysis of spatially…

astro-ph.GA2018

SDSS-IV MaNGA PyMorph Photometric and Deep Learning Morphological Catalogs and implications for bulge properties and stellar angular momentum

J. -L. Fischer, H. Domínguez Sánchez, M. Bernardi

We describe the SDSS-IV MaNGA PyMorph Photometric (MPP-VAC) and MaNGA Deep Learning Morphology (MDLM-VAC) Value Added Catalogs. The MPP-VAC provides photometric parameters from Sér…

astro-ph.GA2018

Transfer learning for galaxy morphology from one survey to another

H. Domínguez Sánchez, M. Huertas-Company, M. Bernardi +56

Deep Learning (DL) algorithms for morphological classification of galaxies have proven very successful, mimicking (or even improving) visual classifications. However, these algorit…

astro-ph.GA2018

A simultaneous search for High- LAEs and LBGs in the SHARDS survey

P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón +15

We have undertaken a comprehensive search for both Lyman Alpha Emitters (LAEs) and Lyman Break Galaxies (LBGs) in the SHARDS Survey of the GOODS-N field. SHARDS is a deep imaging s…

astro-ph.GA2018

Star-forming galaxies at low-redshift in the SHARDS survey

A. Lumbreras-Calle, C. Muñoz-Tuñón, J. Méndez-Abreu +13

The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these p…

astro-ph.GA201787 cited

Deep learning for galaxy surface brightness profile fitting

D. Tuccillo, M. Huertas-Company, E. Decencière +3

Numerous ongoing and future large area surveys (e.g. DES, EUCLID, LSST, WFIRST), will increase by several orders of magnitude the volume of data that can be exploited for galaxy mo…