2.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Center for Astrophysics Harvard & SmithsonianUS71 papers
- Space Telescope Science InstituteUS70 papers
- University of MichiganUS65 papers
- University of California, DavisUS55 papers
- University of ArizonaUS53 papers
- Max Planck Institute for Extraterrestrial PhysicsDE52 papers
- University of FloridaUS51 papers
- California Institute of TechnologyUS49 papers
- Jet Propulsion LaboratoryUS49 papers
- University of ChicagoUS46 papers
- Massachusetts Institute of TechnologyUS44 papers
- University of California, Santa CruzUS42 papers
17 papers · 1 filter
Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Ryan Brennan +37
The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (). We us…
Galaxy growth in a massive halo in the first billion years of cosmic history
D. P. Marrone, J. S. Spilker, C. C. Hayward +34
According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in reg…
Evidence for Merger-Driven Growth in Luminous, High-z, Obscured AGN in the CANDELS/COSMOS Field
J. L. Donley, J. Kartaltepe, D. Kocevski +27
While major mergers have long been proposed as a driver of both AGN activity and the M-sigma relation, studies of moderate to high redshift Seyfert-luminosity AGN hosts have found…
CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2
Dale D. Kocevski, Guillermo Barro, S. M. Faber +31
We examine the fraction of massive (), compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at . These cSFGs are likely…
Demographics of Star-forming Galaxies since . I. The Diagram in CANDELS
Jerome J. Fang, S. M. Faber, David C. Koo +41
This is the first in a series of papers examining the demographics of star-forming galaxies at in CANDELS. We study 9,100 galaxies from GOODS-S and UDS having published…
First Weak-lensing Results from "See Change": Quantifying Dark Matter in the Two Z>1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
M. James Jee, Jongwan Ko, Saul Perlmutter +4
We present a weak-lensing study of SPT-CLJ2040-4451 and IDCSJ1426+3508 at z=1.48 and 1.75, respectively. The two clusters were observed in our "See Change" program, a HST survey of…
Robust Emotion Recognition from Low Quality and Low Bit Rate Video: A Deep Learning Approach
Bowen Cheng, Zhangyang Wang, Zhaobin Zhang +5
Emotion recognition from facial expressions is tremendously useful, especially when coupled with smart devices and wireless multimedia applications. However, the inadequate network…
Anisotropic Mesh Adaptation for Finite Element Solution of Anisotropic Porous Medium Equation
Xianping Li
Anisotropic Porous Medium Equation (APME) is developed as an extension of the Porous Medium Equation (PME) for anisotropic porous media. A special analytical solution is derived fo…
The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22
David Rubin, Brian Hayden, Xiaosheng Huang +32
We present the discovery and measurements of a gravitationally lensed supernova (SN) behind the galaxy cluster MOO J1014+0038. Based on multi-band Hubble Space Telescope and Very L…
The AGN-Star Formation Connection: Future Prospects with JWST
Allison Kirkpatrick, Stacey Alberts, Alexandra Pope +12
The bulk of the stellar growth over cosmic time is dominated by IR luminous galaxies at cosmic noon (z=1-2), many of which harbor a hidden active galactic nucleus (AGN). We use sta…
The Ages of Passive Galaxies in a z=1.62 Protocluster
Donald B. Lee-Brown, Gregory H. Rudnick, Ivelina G. Momcheva +9
We present a study of the relation between galaxy stellar age and mass for 14 members of the protocluster IRC 0218, using multiband imaging and HST G102 and G141 grism spe…
Moving mesh finite element simulation for phase-field modeling of brittle fracture and convergence of newton's iteration
Fei Zhang, Weizhang Huang, Xianping Li +1
A moving mesh finite element method is studied for the numerical solution of a phase-field model for brittle fracture. The moving mesh partial differential equation approach is emp…
A controlled study of cold dust content in galaxies from
Allison Kirkpatrick, Alexandra Pope, Anna Sajina +12
At , the formation of new stars is dominated by dusty galaxies whose far-IR emission indicates they contain colder dust than local galaxies of a similar luminosity. We explo…
Arm and interarm abundance gradients in CALIFA spiral galaxies
L. Sánchez-Menguiano, S. F. Sánchez, I. Pérez +23
Spiral arms are the most singular features in disc galaxies. These structures can exhibit different patterns, namely grand design and flocculent arms, with easily distinguishable c…
Projection based advanced motion model for cubic mapping for 360-degree video
Li Li, Zhu Li, Madhukar Budagavi +1
This paper proposes a novel advanced motion model to handle the irregular motion for the cubic map projection of 360-degree video. Since the irregular motion is mainly caused by th…
Convolutional Neural Network-Based Block Up-sampling for Intra Frame Coding
Yue Li, Dong Liu, Houqiang Li +4
Inspired by the recent advances of image super-resolution using convolutional neural network (CNN), we propose a CNN-based block up-sampling scheme for intra frame coding. A block…
The X-ray and Mid-Infrared luminosities in Luminous Type 1 Quasars
Chien-Ting J. Chen, Ryan C. Hickox, Andrew D. Goulding +16
Several recent studies have reported different intrinsic correlations between the AGN mid-IR luminosity () and the rest-frame 2-10 keV luminosity () for luminous qu…