Catálogo de publicaciones - revistas
Título de Acceso Abierto
The Astrophysical Journal (ApJ)
Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal is an open access journal devoted to recent developments, discoveries, and theories in astronomy and astrophysics. Publications in ApJ constitute significant new research that is directly relevant to astrophysical applications, whether based on observational results or on theoretical insights or modeling.Palabras clave – provistas por la editorial
astronomy; astrophysics
Disponibilidad
| Institución detectada | Período | Navegá | Descargá | Solicitá |
|---|---|---|---|---|
| No detectada | desde jul. 1995 / hasta dic. 2023 | IOPScience |
Información
Tipo de recurso:
revistas
ISSN impreso
0004-637X
ISSN electrónico
1538-4357
Editor responsable
American Astronomical Society (AAS)
Idiomas de la publicación
- inglés
País de edición
Reino Unido
Información sobre licencias CC
Cobertura temática
Tabla de contenidos
The Nuclear Star Cluster and Nuclear Stellar Disk of the Milky Way: Different Stellar Populations and Star Formation Histories
Francisco Nogueras-Lara
; Rainer Schödel; Nadine Neumayer
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 97
Electron Acceleration at Rippled Low-mach-number Shocks in High-beta Collisionless Cosmic Plasmas
Oleh Kobzar; Jacek Niemiec; Takanobu Amano; Masahiro Hoshino; Shuichi Matsukiyo; Yosuke Matsumoto; Martin Pohl
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 97
Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii
J. D. Remolina González; K. Sharon; G. Mahler; C. Fox; C. A. Garcia Diaz; K. Napier; L. E. Bleem; M. D. Gladders; N. Li; A. Niemiec
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 98
Connecting the Low to the High Corona: A Method to Isolate Transients in STEREO/COR1 Images
Nathalia Alzate; Huw Morgan; Nicholeen Viall; Angelos Vourlidas
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 98
Ultracool Dwarfs Observed with the Spitzer Infrared Spectrograph. I. An Accurate Look at the L-to-T Transition at ∼300 Myr from Optical Through Mid-infrared Spectrophotometry
Genaro Suárez; Stanimir Metchev; Sandy K. Leggett; Didier Saumon; Mark S. Marley
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 99
Mid-infrared Period–Luminosity Relations for Miras in the Large Magellanic Cloud
Patryk Iwanek; Igor Soszyński; Szymon Kozłowski
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 99
Detailed Abundances of Planet-hosting Open Clusters. The Praesepe (Beehive) Cluster*
George Vejar; Simon C. Schuler; Keivan G. Stassun
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 100
A New Reconstruction of the Sun’s Magnetic Field and Total Irradiance since 1700
Y.-M. Wang; J. L. Lean
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 100
The Ultraviolet Deep Imaging Survey of Galaxies in the Bootes Void. I. Catalog, Color–Magnitude Relations, and Star Formation
Divya Pandey; Kanak Saha; Ananta C. Pradhan
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 101
Generation of He i 1083 nm Images from SDO AIA Images by Deep Learning
Jihyeon Son; Junghun Cha; Yong-Jae Moon; Harim Lee; Eunsu Park; Gyungin Shin; Hyun-Jin Jeong
<jats:title>Abstract</jats:title> <jats:p>In this study, we generate He <jats:sc>i</jats:sc> 1083 nm images from Solar Dynamic Observatory (SDO)/Atmospheric Imaging Assembly (AIA) images using a novel deep learning method (pix2pixHD) based on conditional Generative Adversarial Networks (cGAN). He <jats:sc>i</jats:sc> 1083 nm images from National Solar Observatory (NSO)/Synoptic Optical Long-term Investigations of the Sun (SOLIS) are used as target data. We make three models: single-input SDO/AIA 19.3 nm image for Model I, single-input 30.4 nm image for Model II, and double-input (19.3 and 30.4 nm) images for Model III. We use data from 2010 October to 2015 July except for June and December for training and the remaining one for test. Major results of our study are as follows. First, the models successfully generate He <jats:sc>i</jats:sc> 1083 nm images with high correlations. Second, Model III shows better results than those with one input image in terms of metrics such as correlation coefficient (CC) and root mean square error (RMSE). CC and RMSE between real and synthetic ones for model III with 4 by 4 binnings are 0.88 and 9.49, respectively. Third, synthetic images show well observational features such as active regions, filaments, and coronal holes. This work is meaningful in that our model can produce He <jats:sc>i</jats:sc> 1083 nm images with higher cadence without data gaps, which would be useful for studying the time evolution of the chromosphere and transition region.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 101