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Related papers: Reanalyzing the visible colors of Centaurs and KBO…

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Quasars are variable on timescales from days to years in UV/optical, and generally appear bluer while they brighten. The physics behind the variations in fluxes and colors remains unclear. Using SDSS g and r band photometric monitoring data…

Astrophysics of Galaxies · Physics 2015-06-22 Yu-Han Sun , Jun-Xian Wang , Xiao-Yang Chen , Zhen-Ya Zheng

Colors and binarity provide important constraints on the Kuiper belt formation. The cold classical objects at radial distance r=42-47 au from the Sun are predominantly very red (spectral slope s>17%) and often exist as equal-size binaries…

Earth and Planetary Astrophysics · Physics 2022-03-02 David Nesvorny , David Vokrouhlicky , Wesley C. Fraser

This project is a massive near-infrared (NIR) search for variable stars in highly reddened and obscured open cluster (OC) fields projected on regions of the Galactic bulge and disk. The search is performed using photometric NIR data in the…

Photometric measurements are prone to systematic errors presenting a challenge to low-amplitude variability detection. In search for a general-purpose variability detection technique able to recover a broad range of variability types…

Most of the existing blind image Super-Resolution (SR) methods assume that the blur kernels are space-invariant. However, the blur involved in real applications are usually space-variant due to object motion, out-of-focus, etc., resulting…

Computer Vision and Pattern Recognition · Computer Science 2023-04-10 Xuhai Chen , Jiangning Zhang , Chao Xu , Yabiao Wang , Chengjie Wang , Yong Liu

The RGB complementary metal-oxidesemiconductor (CMOS) sensor works within the visible light spectrum. Therefore it is very sensitive to environmental light conditions. On the contrary, a long-wave infrared (LWIR) sensor operating in 8-14…

Computer Vision and Pattern Recognition · Computer Science 2022-06-09 Mohsen Vadidar , Ali Kariminezhad , Christian Mayr , Laurent Kloeker , Lutz Eckstein

Existing works examining Vision-Language Models (VLMs) for social biases predominantly focus on a limited set of documented bias associations, such as gender:profession or race:crime. This narrow scope often overlooks a vast range of…

Computation and Language · Computer Science 2024-10-07 Chahat Raj , Anjishnu Mukherjee , Aylin Caliskan , Antonios Anastasopoulos , Ziwei Zhu

In the present work we compare in detail some of the major theoretical libraries with observations, aiming at detecting weaknesses and strengths from the stellar population modelling point of view. We compared model predictions and…

Astrophysics · Physics 2009-11-13 Lucimara Martins , Paula Coelho

The rareness of blazars, combined with the previous history of relatively shallow, single-band surveys, has dramatically colored our perception of these objects. Despite a quarter-century of research, it is not at all clear whether current…

Lesion images are frequently taken in open-set settings. Because of this, the image data generated is extremely varied in nature.It is difficult for a convolutional neural network to find proper features and generalise well, as a result…

Computer Vision and Pattern Recognition · Computer Science 2021-10-14 Priyam Mehta

We present the observational results of multi-colour optical monitoring of eight red blazars from 2003 September to 2004 February. The aim of our monitoring is to investigate the spectral variability as well as the flux variations at short…

Astrophysics · Physics 2009-11-11 Minfeng Gu , C. -U. Lee , Soojong Pak , H. S. Yim , A. B. Fletcher

LINER nuclei, which are present in many nearby galactic bulges, may be the manifestation of low-rate or low-radiative-efficiency accretion onto supermassive central black holes. However, it has been unclear whether the compact UV nuclear…

Astrophysics · Physics 2009-11-10 Dan Maoz , Neil M. Nagar , Heino Falcke , Andrew S. Wilson

We present optical (BVRI) photometric measurements of a sample of 76 common proper motion wide separation main sequence binary pairs. The pairs are composed of a F-, G-, or K-type primary star and an M-type secondary. The sample is selected…

Solar and Stellar Astrophysics · Physics 2015-06-22 Ting Li , J. L. Marshall , Sebastien Lepine , Patrick Williams , Joy Chavez

We carried out a high time-resolution, multicolour optical observing campaign for eight $\gamma$-ray detected blazars during 2010-2020. We analyze flux variations, correlations between magnitudes and colours on different timescales.…

High Energy Astrophysical Phenomena · Physics 2023-02-15 X. Chang , T. F. Yi , D. R. Xiong , C. X. Liu , X. Yang , H. Z. Li , Y. L. Gong , W. W. Na , Y. Li , Z. H. Chen , J. P. Chen , L. S. Mao

Almost all of the $>600$ known Kuiper belt objects (KBOs) have been discovered within 50 AU of the Sun. One possible explanation for the observed lack of KBOs beyond 50 AU is that the distant Kuiper belt is dynamically very cold, and thus…

Astrophysics · Physics 2016-08-30 R. Lynne Allen , Gary Bernstein , Renu Malhotra

We present an update of the visible and near-infrared colour database of Minor Bodies in the Outer Solar System (MBOSSes), which now includes over 2000 measurement epochs of 555 objects, extracted from over 100 articles. The list is fairly…

Earth and Planetary Astrophysics · Physics 2015-06-11 O. R. Hainaut , H. Boehnhardt , S. Protopapa

We examine a large collection of low resolution near-infrared spectra of Kuiper belt objects and centaurs in an attempt to understand the presence of water ice in the Kuiper belt. We find that water ice on the surface of these objects…

Earth and Planetary Astrophysics · Physics 2015-06-04 M. E. Brown , E. L. Schaller , W. C. Fraser

Color serves as a fundamental dimension of human visual perception and a primary means of communicating about objects and scenes. As vision-language models (VLMs) become increasingly prevalent, understanding whether they name colors like…

Computer Vision and Pattern Recognition · Computer Science 2025-09-29 Alexandra Gomez-Villa , Pablo Hernández-Cámara , Muhammad Atif Butt , Valero Laparra , Jesus Malo , Javier Vazquez-Corral

Viscous unified dark matter models aim to describe the dark sector of the Universe, as the dark matter fluid itself gives rise to an accelerated expansion due to a negative bulk viscous pressure. However, in most studies, radiation is often…

General Relativity and Quantum Cosmology · Physics 2024-06-19 Guillermo Palma , Gabriel Gomez , Norman Cruz

Synthetic photometry is a great tool for studying globular clusters, especially for understanding the nature of their multiple populations. Our goal is to quantify the errors on synthetic photometry that are caused by uncertainties on…

Solar and Stellar Astrophysics · Physics 2018-09-19 F. Martins