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相关论文: Zwicky Transient Facility Observations of Trojan A…

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The Zwicky Transit Factory (ZTF) is a powerful time domain survey facility with a large field of view. We apply the synthetic tracking technique to integrate a ZTF's long-dwell dataset, which consists of 133 nominal 30-second exposure…

天体物理仪器与方法 · 物理学 2020-04-29 Chengxing Zhai , Quanzhi Ye , Michael Shao , Russell Trahan , Navtej S. Saini , Janice Shen , Thomas A. Prince

A new asteroid rotation period survey have been carried out by using the Palomar Transient Factory (PTF). Twelve consecutive PTF fields, which covered an area of 87 deg$^2$ in the ecliptic plane, were observed in $R$ band with a cadence of…

Context: We use phase curves of small bodies to measure absolute magnitudes and, together with complementary theoretical and laboratory results, to understand their surfaces' micro and macroscopic properties. Although we can observe…

地球与行星天体物理 · 物理学 2022-11-09 A. Alvarez-Candal , S. Jiménez Corral , M. Colazo

Aims. The goal of this investigation is to determine the origin and surface composition of the asteroid (121514) 1999 UJ7, the only currently known L4 Martian Trojan asteroid. Methods. We have obtained visible reflectance spectra and…

地球与行星天体物理 · 物理学 2018-10-24 G. Borisov , A. A. Christou , F. Colas , S. Bagnulo , A. Cellino , A. Dell'Oro

In a search for eclipsing white dwarfs using the Zwicky Transient Facility lightcurves, we identified a deep eclipsing white dwarf with a dark, substellar companion. The lack of an infrared excess and an orbital period of 10 hours made this…

Most of the stars in the Universe are M spectral class dwarfs, which are known to be the source of bright and frequent stellar flares. In this paper, we propose new approaches to discover M-dwarf flares in ground-based photometric surveys.…

We study the Hawking radiation of 3D rotating hairy black holes. More concretely, we compute the transition probability of a bosonic and fermionic particle in such backgrounds. Thew, we show that the transition probability is independent of…

高能物理 - 理论 · 物理学 2015-10-28 A. Belhaj , M. Chabab , H. EL Moumni , K. Masmar , M. B. Sedra

Context. Trojan asteroids of Mars date from an early phase of solar system evolution. Based on a sample of <10 asteroids, MT distribution has been previously shown to be both asymmetric and inhomogeneous with population evolution dominated…

地球与行星天体物理 · 物理学 2025-05-28 Apostolos A. Christou , Nikos Georgakarakos , Matija Cuk , Aldo Dell'Oro , Andrew Marshall-Lee , Alice Humpage

Gaia provided the largest-ever catalogue of white dwarf stars. We use this catalogue, along with the third public data release of the Zwicky Transient Facility (ZTF), to identify new eclipsing white dwarf binaries. Our method exploits light…

太阳与恒星天体物理 · 物理学 2021-11-18 Pascal M. Keller , Elmé Breedt , Simon Hodgkin , Vasily Belokurov , James Wild , Ignacio García-Soriano , Jacob L. Wise

Collisional families offer a unique window into the interior composition of asteroid populations. Previous dynamical studies of the Jupiter Trojans have uncovered a handful of potential collisional families, two of which have been…

地球与行星天体物理 · 物理学 2022-12-19 Ian Wong , Michael E. Brown

The third observing run by LVC has brought the discovery of many compact binary coalescences. Following the detection of the first binary neutron star merger in this run (LIGO/Virgo S190425z), we performed a dedicated follow-up campaign…

The manifestation of surface spots on magnetic chemically peculiar (mCP) stars is most commonly explained by the atomic diffusion theory, which requires a calm stellar atmosphere and only moderate rotation. While very successful and well…

太阳与恒星天体物理 · 物理学 2024-06-11 B. Bauer-Fasching , K. Bernhard , E. Brändli , H. Burger , B. Eisele , S. Hümmerich , J. Neuhold , E. Paunzen , M. Piecka , S. Ratzenböck , M. Prišegen

The Trojan population consists of two swarms of asteroids following the same orbit as Jupiter and located at the L4 and L5 Lagrange points of the Jupiter-Sun system (leading and following Jupiter by 60 degrees). The asteroid 617 Patroclus…

We calculate the planet-star flux-density ratios as a function of wavelength from 0.5 microns to 25 microns for the transiting extrasolar giant planets TrES-1 and HD209458b and compare them with the recent Spitzer/IRAC-MIPS secondary…

天体物理学 · 物理学 2009-11-10 A. Burrows , I. Hubeny , D. Sudarsky

The Zwicky Transient Facility (ZTF) survey generates real-time alerts for optical transients, variables, and moving objects discovered in its wide-field survey. We describe the ZTF alert stream distribution and processing (filtering)…

Context: Large all-sky surveys provide us with a lot of photometric data that are sparse in time (typically few measurements per night) and can be potentially used for the determination of shapes and rotational states of asteroids. The…

地球与行星天体物理 · 物理学 2016-11-30 Helena Cibulková , Josef Ďurech , David Vokrouhlický , Mikko Kaasalainen , Dagmara A. Oszkiewicz

Asteroids with satellites are natural laboratories to constrain the formation and evolution of our solar system. The binary Trojan asteroid (624) Hektor is the only known Trojan asteroid to possess a small satellite. Based on W.M. Keck…

地球与行星天体物理 · 物理学 2014-03-03 F. Marchis , J. Durech , J. Castillo-Rogez , F. Vachier , M. Cuk , J. Berthier , M. H. Wong , P. Kalas , G. Duchene , M. A. van Dam , H. Hamanowa , M. Viikinkoski

The Zwicky Transient Facility (ZTF) is performing a three-day cadence survey of the visible Northern sky (~3$\pi$). The transient candidates found in this survey are announced via public alerts. As a supplementary product ZTF is also…

The optical, full-phase photometric variations of a short-period planet provide a unique view of the planet's atmospheric composition and dynamics. The number of planets with optical phase curve detections, however, is currently too small…

地球与行星天体物理 · 物理学 2017-08-16 Sarah Millholland , Gregory Laughlin

Phase-resolved spectroscopy of the newly discovered X-ray transient MAXI J0556-332 has revealed the presence of narrow emission lines in the Bowen region that most likely arise on the surface of the mass donor star in this low mass X-ray…