JWST/MIRI imaging of ESO 428-G14
JWST/MIRI imaging of ESO 428-G14
Supplementary data for Haidar et al. 2024: (title: Dust beyond the torus: Revealing the mid-infrared heart of local Seyfert ESO 428-G14 with JWST/MIRI) arxiv: 2404.16100, link: https://arxiv.org/abs/2404.16100 Authors: Houda Haidar, David J. Rosario, Almudena Alonso-Herrero, Miguel Pereira-Santaella, Ismael García-Bernete, Stephanie Campbell, Sebastian F. Hönig, Cristina Ramos Almeida, Erin Hicks, Daniel Delaney, Richard Davies, Claudio Ricci, Chris M. Harrison, Mason Leist, Enrique Lopez-Rodriguez, Santiago Garcia-Burillo, Lulu Zhang, Chris Packham, Poshak Gandhi, Anelise Audibert, Enrica Bellocchi, Peter Boorman, Andrew Bunker, Françoise Combes, Tanio Diaz Santos, Fergus R. Donnan, Omaira Gonzalez Martin, Laura Hermosa Muñoz, Matthaios Charidis, Alvaro Labiano, Nancy A. Levenson, Daniel May, Dimitra Rigopoulou, Alberto Rodriguez Ardila, T. Taro Shimizu, Marko Stalevski, Martin Ward
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).0 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Average influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Average impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Average
Citations provided by BIP!Popularity provided by BIP!