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
Characterization of HD 206893 B from Near- to Thermal-infrared
Tiffany Meshkat
; Peter Gao; Eve J. Lee; Dimitri Mawet; Elodie Choquet; Marie Ygouf; Rahul Patel; Garreth Ruane; Jason Wang; Nicole Wallack; Olivier Absil; Charles Beichman
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 62
An Observational Signature of Sub-equipartition Magnetic Fields in the Spectra of Black Hole Binaries
John Wallace; Asaf Pe’er
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 63
The Blue Supergiant Progenitor of the Supernova Imposter AT 2019krl
Jennifer E. Andrews; Jacob E. Jencson; Schuyler D. Van Dyk; Nathan Smith; Jack M. M. Neustadt; David J. Sand; K. Kreckel; C. S. Kochanek; S. Valenti; Jay Strader; M. C. Bersten; Guillermo A. Blanc; K. Azalee Bostroem; Thomas G. Brink; Eric Emsellem; Alexei V. Filippenko; Gastón Folatelli; Mansi M. Kasliwal; Frank J. Masci; Rebecca McElroy; Dan Milisavljevic; Francesco Santoro; Tamás Szalai
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 63
Alfvénicity-related Long Recovery Phases of Geomagnetic Storms: A Space Weather Perspective
Daniele Telloni; Raffaella D’Amicis; Roberto Bruno; Denise Perrone; Luca Sorriso-Valvo; Anil N. Raghav; Komal Choraghe
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 64
The AGORA High-resolution Galaxy Simulations Comparison Project. III. Cosmological Zoom-in Simulation of a Milky Way–mass Halo
Santi Roca-Fàbrega; Ji-hoon Kim; Loic Hausammann; Kentaro Nagamine; Alessandro Lupi; Johnny W. Powell; Ikkoh Shimizu; Daniel Ceverino; Joel R. Primack; Thomas R. Quinn; Yves Revaz; Héctor Velázquez; Tom Abel; Michael Buehlmann; Avishai Dekel; Bili Dong; Oliver Hahn; Cameron Hummels; Ki-won Kim; Britton D. Smith; Clayton Strawn; Romain Teyssier; Matthew J. Turk
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 64
Characteristics of Interplanetary Discontinuities in the Inner Heliosphere Revealed by Parker Solar Probe
Y. Y. Liu; H. S. Fu; J. B. Cao; C. M. Liu; Z. Wang; Z. Z. Guo; Y. Xu; S. D. Bale; J. C. Kasper
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 65
A New Broadening Technique of the Numerically Unresolved Solar Transition Region and Its Effect on the Spectroscopic Synthesis Using Coronal Approximation
Haruhisa Iijima; Shinsuke Imada
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 65
Brightness Fluctuation Spectra of Sun-like Stars. I. The Mid-frequency Continuum
Timothy M. Brown; Rafael A. García; Savita Mathur; Travis S. Metcalfe; Ângela R. G. Santos
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 66
An Improved and Physically Motivated Scheme for Matching Galaxies with Dark Matter Halos
Stephanie Tonnesen; Jeremiah P. Ostriker
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 66
Three-dimensional Reconstruction of Weak-lensing Mass Maps with a Sparsity Prior. I. Cluster Detection
Xiangchong Li; Naoki Yoshida; Masamune Oguri; Shiro Ikeda; Wentao Luo
<jats:title>Abstract</jats:title> <jats:p>We propose a novel method to reconstruct high-resolution three-dimensional mass maps using data from photometric weak-lensing surveys. We apply an adaptive LASSO algorithm to perform a sparsity-based reconstruction on the assumption that the underlying cosmic density field is represented by a sum of Navarro–Frenk–White halos. We generate realistic mock galaxy shear catalogs by considering the shear distortions from isolated halos for the configurations matched to the Subaru Hyper Suprime-Cam Survey with its photometric redshift estimates. We show that the adaptive method significantly reduces line-of-sight smearing that is caused by the correlation between the lensing kernels at different redshifts. Lensing clusters with lower mass limits of 10<jats:sup>14.0</jats:sup> h<jats:sup>−1</jats:sup> <jats:italic> M</jats:italic> <jats:sub>⊙</jats:sub>, 10<jats:sup>14.7 </jats:sup>h<jats:sup>−1</jats:sup> <jats:italic> M</jats:italic> <jats:sub>⊙</jats:sub>, 10<jats:sup>15.0</jats:sup> h<jats:sup>−1</jats:sup> <jats:italic> M</jats:italic> <jats:sub>⊙</jats:sub> can be detected with 1.5<jats:italic>σ</jats:italic> confidence at the low (<jats:italic>z</jats:italic> < 0.3), median (0.3 ≤ <jats:italic>z</jats:italic> < 0.6), and high (0.6 ≤ <jats:italic>z</jats:italic> < 0.85) redshifts, respectively, with an average false detection rate of 0.022 deg<jats:sup>−2</jats:sup>. The estimated redshifts of the detected clusters are systematically lower than the true values by Δ<jats:italic>z</jats:italic> ∼ 0.03 for halos at <jats:italic>z</jats:italic> ≤ 0.4, but the relative redshift bias is below 0.5% for clusters at 0.4 < <jats:italic>z</jats:italic> ≤ 0.85. The standard deviation of the redshift estimation is 0.092. Our method enables direct three-dimensional cluster detection with accurate redshift estimates.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 67