most citedComparing PyMorph and SDSS photometry. I. Background sky and model fitting effects

29 citations · 57 across the 2 of their papers we have counts for

collaborators

5 papers

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.IM2018

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

D. S. Aguado, Romina Ahumada, Andres Almeida +230

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…

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.GA201728 cited

Stellar mass functions and implications for a variable IMF

M. Bernardi, R. K. Sheth, J. -L. Fischer +6

Spatially resolved kinematics of nearby galaxies has shown that the ratio of dynamical- to stellar population-based estimates of the mass of a galaxy () correlat…

astro-ph.GA201729 cited

Comparing PyMorph and SDSS photometry. I. Background sky and model fitting effects

J. -L. Fischer, M. Bernardi, A. Meert

A number of recent estimates of the total luminosities of galaxies in the SDSS are significantly larger than those reported by the SDSS pipeline. This is because of a combination o…