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Consistent Dust and Gas Models for Protoplanetary Disks. III. Models for Selected Objects from the FP7 DIANA Project
DOI: 10.1088/1538-3873/aaf4e5 Bibcode: 2019PASP..131f4301W

Waters, L. B. F. M.; Pinte, C.; Woitke, P. +17 more

The European FP7 project DIANA has performed a coherent analysis of a large set of observational data of protoplanetary disks by means of thermo-chemical disk models. The collected data include extinction-corrected stellar UV and X-ray input spectra (as seen by the disk), photometric fluxes, low and high resolution spectra, interferometric data, e…

2019 Publications of the Astronomical Society of the Pacific
ISO IUE eHST 72
Multiband Galaxy Morphologies for CLASH: A Convolutional Neural Network Transferred from CANDELS
DOI: 10.1088/1538-3873/aaeeb4 Bibcode: 2019PASP..131j8002P

Demarco, R.; Huertas-Company, M.; Cabrera-Vives, G. +5 more

We present visual-like morphologies over 16 photometric bands, from ultraviolet to near-infrared, for 8412 galaxies in the Cluster Lensing And Supernova survey with Hubble (CLASH) obtained using a convolutional neural network (ConvNet) model. Our model follows the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS) main morphologica…

2019 Publications of the Astronomical Society of the Pacific
eHST 21
Ultraviolet Activity as Indicators of Small-scale Magnetic Fields in γ Cassiopeiae
DOI: 10.1088/1538-3873/aaf70b Bibcode: 2019PASP..131d4201S

Smith, Myron A.

The recorded activity of γ Cas (B0.5 IVe) in the ultraviolet is important to an understanding of the mechanism behind this prototypical Be star’s high-energy activity, especially its hard X-ray emissions. The analysis here focuses first on the phasing of ultraviolet and optical light curves from different epochs. The rotational interpretation of t…

2019 Publications of the Astronomical Society of the Pacific
IUE eHST 8