Galaxy morphology network: A convolutional neural network used to study morphology and quenching in∼ 100,000 sdss and∼ 20,000 candels galaxies

A Ghosh, CM Urry, Z Wang, K Schawinski… - The Astrophysical …, 2020 - iopscience.iop.org
We examine morphology-separated color–mass diagrams to study the quenching of star
formation in∼ 100,000 (z∼ 0) Sloan Digital Sky Survey (SDSS) and∼ 20,000 (z∼ 1) …

Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in∼ 100,000 SDSS and∼ 20,000 CANDELS Galaxies

A Ghosh, CM Urry, Z Wang, K Schawinski… - The Astrophysical …, 2020 - par.nsf.gov
We examine morphology-separated color–mass diagrams to study the quenching of star
formation in∼ 100,000 (z∼ 0) Sloan Digital Sky Survey (SDSS) and∼ 20,000 (z∼ 1) …

Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in SDSS and CANDELS Galaxies

A Ghosh, CM Urry, Z Wang, K Schawinski… - arXiv preprint arXiv …, 2020 - arxiv.org
We examine morphology-separated color-mass diagrams to study the quenching of star
formation in $\sim 100,000$($ z\sim0 $) Sloan Digital Sky Survey (SDSS) and $\sim …

[引用][C] Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in∼ 100,000 SDSS and∼ 20,000 CANDELS …

A Ghosh, CM Urry, Z Wang, K Schawinski… - The Astrophysical …, 2020 - cir.nii.ac.jp
Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and
Quenching in ∼100,000 SDSS and ∼20,000 CANDELS Galaxies | CiNii Research CiNii 国立 …

Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in∼ 100,000 SDSS and∼ 20,000 CANDELS Galaxies

A Ghosh, CM Urry, Z Wang… - The Astrophysical …, 2020 - ui.adsabs.harvard.edu
We examine morphology-separated color-mass diagrams to study the quenching of star
formation in∼ 100,000 (z∼ 0) Sloan Digital Sky Survey (SDSS) and∼ 20,000 (z∼ 1) …

Galaxy Morphology Network: A Convolutional Neural Network Used to Study Morphology and Quenching in∼ 100,000 SDSS and∼ 20,000 CANDELS Galaxies

A Ghosh, CM Urry, MC Powell, Z Wang… - Astrophysical …, 2020 - inis.iaea.org
[en] We examine morphology-separated color–mass diagrams to study the quenching of star
formation in∼ 100,000 (z∼ 0) Sloan Digital Sky Survey (SDSS) and∼ 20,000 (z∼ 1) …