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相关论文: Synthetic tracking using ZTF Long Dwell Datasets

200 篇论文

We introduce PointOdyssey, a large-scale synthetic dataset, and data generation framework, for the training and evaluation of long-term fine-grained tracking algorithms. Our goal is to advance the state-of-the-art by placing emphasis on…

计算机视觉与模式识别 · 计算机科学 2023-07-28 Yang Zheng , Adam W. Harley , Bokui Shen , Gordon Wetzstein , Leonidas J. Guibas

The discovery of two interstellar objects passing through the Solar System, 1I/`Oumuamua and 2I/Borisov, implies that a galactic population exists with a spatial number density of order $\sim0.1$ au$^{-3}$. The forthcoming Rubin Observatory…

地球与行星天体物理 · 物理学 2023-10-27 Dušan Marčeta , Darryl Z. Seligman

We present an automated and probabilistic method to make prediscovery detections of near-Earth asteroids (NEAs) in archival survey images, with the goal of reducing orbital uncertainty immediately after discovery. We refit Minor Planet…

地球与行星天体物理 · 物理学 2025-10-10 Sage Li , Alex Geringer-Sameth , Nathan Golovich

We have obtained extensive photometric observations of the polluted white dwarf WD 1145+017 which has been reported to be transited by at least one, and perhaps several, large asteroids (or, planetesimals) with dust emission. We have…

地球与行星天体物理 · 物理学 2016-03-23 S. Rappaport , B. L. Gary , T. Kaye , A. Vanderburg , B. Croll , P. Benni , J. Foote

AM CVn systems are ultra-compact, helium-rich, accreting binaries with degenerate or semi-degenerate donors. We report the discovery of five new eclipsing AM CVn systems with orbital periods of 61.5, 55.5, 53.3, 37.4, and 35.4 minutes.…

By selecting astrometric and photometric data from the Sloan Digital Sky Survey (SDSS), the L{\'e}pine & Shara Proper Motion North Catalog (LSPM-North), the Two Micron All Sky Survey (2MASS), and the USNO-B1.0 catalog, we use a succession…

太阳与恒星天体物理 · 物理学 2015-06-04 Conor Sayres , John P. Subasavage , P. Bergeron , P. Dufour , James R. A. Davenport , Yusra AlSayyad , Benjamin M. Tofflemire

The Palomar Transient Factory (PTF) is a fully-automated, wide-field survey aimed at a systematic exploration of the optical transient sky. The transient survey is performed using a new 8.1 square degree camera installed on the 48-inch…

The SiTian project, with its vast field of view, will become an ideal platform for asteroid scientific research. In this study, we develop a pipeline to analyze the photometry of asteroids and derive their periods from the data collected by…

地球与行星天体物理 · 物理学 2025-04-03 Zhaoxing Liu , Jian Gao , Hongrui Gu , Yang Huang , Shaoming Hu , Hu Zou , Keyu Xing , Hao Huang , Zehao Zhang

Cometary activity in main-belt asteroids probes the ice content of these objects and provides clues to the history of volatiles in the inner solar system. We search the Palomar Transient Factory (PTF) survey to derive upper limits on the…

Drone-camera based human activity recognition (HAR) has received significant attention from the computer vision research community in the past few years. A robust and efficient HAR system has a pivotal role in fields like video…

计算机视觉与模式识别 · 计算机科学 2022-11-11 Santosh Kumar Yadav , Esha Pahwa , Achleshwar Luthra , Kamlesh Tiwari , Hari Mohan Pandey , Peter Corcoran

The Subaru Deep Field (SDF) project is a program of Subaru Observatory to carry out a deep galaxy survey over a blank field as large as 34'x27'. The program consists of very deep multi-band optical imaging, near infrared imaging for smaller…

In this work, we present the analysis of 976 814 FGKM dwarf and sub-giant stars in the TESS Full Frame Images (FFIs) of the Southern ecliptic hemisphere. We present a new pipeline, DIAmante, developed to extract optimized, multi-sector…

地球与行星天体物理 · 物理学 2020-08-25 M. Montalto , L. Borsato , V. Granata , G. Lacedelli , L. Malavolta , E. E. Manthopoulou , D. Nardiello , V. Nascimbeni , G. Piotto

The intra-night trajectories of asteroids can be approximated by straight lines, and so are their intra-night detections. Therefore, the Hough transform, a line detecting algorithm, can be used to connect the line-up detections to find…

Circumbinary disk occultation (CBO) systems, in which a misaligned circumbinary disk periodically obscures the central binary, provide unique probes of disk structure and dynamics. However, fewer than ten candidates with measured orbital…

太阳与恒星天体物理 · 物理学 2026-01-26 Zhecheng Hu , Wei Zhu , Shuming Wang , Sharon Xuesong Wang

The rotation period of a star is an important quantity that provides insight into its structure and state. For stars with surface features like starspots, their periods can be inferred from brightness variations as these features move…

太阳与恒星天体物理 · 物理学 2025-05-16 Soichiro Hattori , Ruth Angus , Daniel Foreman-Mackey , Yuxi , Lu , Isabel Colman

We present the spectroscopic redshift catalog from a wide-field survey of the fields of 28 galaxy-mass strong gravitational lenses. We discuss the acquisition and reduction of the survey data, collected over 40 nights of 6.5m MMT and…

宇宙学与河外天体物理 · 物理学 2015-08-26 Ivelina Momcheva , Kurtis A. Williams , Richard J. Cool , Charles R. Keeton , Ann I. Zabludoff

Over these years, Correlation Filter-based Trackers (CFTs) have aroused increasing interests in the field of visual object tracking, and have achieved extremely compelling results in different competitions and benchmarks. In this paper, our…

计算机视觉与模式识别 · 计算机科学 2015-09-21 Zhe Chen , Zhibin Hong , Dacheng Tao

This paper addresses the problem of detecting high-redshift clustering in deep photometric surveys. We have used photometric redshifts to select different samples of galaxies in the HDF, in order to study their clustering properties within…

天体物理学 · 物理学 2007-05-23 J. M. Miralles , R. Pello

We describe the fast transient classification algorithm in the center of the kilonova (KN) science module currently implemented in the Fink broker and report classification results based on simulated catalogs and real data from the ZTF…

天体物理仪器与方法 · 物理学 2023-10-06 B. Biswas , E. E. O. Ishida , J. Peloton , A. Moller , M. V. Pruzhinskaya , R. S. de Souza , D. Muthukrishna

Small planets are common around late-M dwarfs and can be detected through highly precise photometry by the transit method. Planets orbiting nearby stars are particularly important as they are often the best-suited for future follow-up…