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Related papers: Lightcurves of 32 Large Transneptunian Objects

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We present the first-ever measurements of the surface colors and rotational properties of a recently discovered distant object in an unusual orbit 2016 ND21. In 2017, this object was close to its perihelion, which allowed us to observe it…

Earth and Planetary Astrophysics · Physics 2019-12-18 Tetiana Hromakina , Sergey Velichko , Irina Belskaya , Yurij Krugly , Aleksandr Sergeev

To study the population properties of small, remote objects beyond Neptune's orbit in the outer solar system, of kilometer size or smaller, serendipitous occultation search is so far the only way. For hectometer-sized Trans-Neptunian…

Earth and Planetary Astrophysics · Physics 2015-06-12 Hsiang-Kuang Chang , Chih-Yuan Liu , Kuan-Ting Chen

We present HAWK-I J-band light curves of five late-type T dwarfs (T6.5-T7.5) with a typical duration of four hours, and investigate the evidence for quasi-periodic photometric variability on intra-night timescales. Our photometry reaches…

Solar and Stellar Astrophysics · Physics 2017-03-06 S. P. Littlefair , B. Burningham , Ch. Helling

A correlation between astrophysical high-energy neutrinos and blazars has been suggested by various authors. In particular, a likely association between IceCube events and intermediate and high-energy peaked BL Lac objects has led to a…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Simona Paiano , Renato Falomo , Aldo Treves , Paolo Padovani , Paolo Giommi , Riccardo Scarpa , Susanna Bisogni , Ester Marini

We present new time-resolved photometric observations of the bright trans-Neptunian object (20000) Varuna and use them to study the rotation period, shape, and color. In observations from 2001 February and April, we find a best-fit…

Astrophysics · Physics 2009-11-07 David C. Jewitt , Scott S. Sheppard

Homogeneous observations and careful analysis of transit light curves can lead to the identification of transit timing variations (TTVs). TrES-2 is one of few exoplanets, which offer the matchless possibility to combine long-term…

We present a first systematic time series study of a sample of blazars observed by the Transiting Exoplanet Survey Satellite $\textit{TESS}$ spacecraft. By cross matching the positions of the sources in the TESS observations with those from…

High Energy Astrophysical Phenomena · Physics 2022-11-23 Vivek Reddy Pininti , Gopal Bhatta , Sagarika Paul , Aman Kumar , Aayushi Rajgor , Rahul Barnwal , Sarvesh Gharat

We have observed 1999 RZ253 with the Hubble Space Telescope at seven separate epochs and have fit an orbit to the observed relative positions of this binary. Two orbital solutions have been identified that differ primarily in the…

Astrophysics · Physics 2009-11-10 K. S. Noll , D. C. Stephens , W. M. Grundy , I. Griffin

I calculate the physical properties of 32 transiting extrasolar planet and brown dwarf systems from existing photometric observations and measured spectroscopic parameters. The systems studied include fifteen observed by CoRoT, ten by…

Earth and Planetary Astrophysics · Physics 2015-05-28 John Southworth

Continuing previous work on the identification and characterization of periodic and non-periodic variations in long and almost uninterrupted high cadence light curves of cataclysmic variables observed by the TESS mission, the results on 23…

Solar and Stellar Astrophysics · Physics 2023-08-31 Albert Bruch

The increasing number of objects orbiting the Earth justifies the great attention and interest in the observation, spacecraft protection and collision avoidance. These studies involve different disturbances and resonances in the orbital…

Space Physics · Physics 2012-10-31 J. C. Sampaio , E. Wnuk , R. Vilhena de Moraes , S. S. Fernandes

Planetary-mass objects and brown dwarfs at the transition ($\rm{T}_{eff}\sim1300$\,K) from relatively red L dwarfs to bluer mid-T dwarfs show enhanced spectrophotometric variability. Multi-epoch observations support atmospheric…

Earth and Planetary Astrophysics · Physics 2024-05-21 Michael K. Plummer , Ji Wang , Étienne Artigau , René Doyon , Genaro Suárez

The detached transneptunian objects (TNOs) are those with semimajor axes beyond the 2:1 resonance with Neptune, which are neither resonant nor scattering. Using the detached sample from the OSSOS telescopic survey, we produce the first…

Earth and Planetary Astrophysics · Physics 2023-11-01 Matthew Beaudoin , Brett Gladman , Yukun Huang , Michele Bannister , J. J. Kavelaars , Jean-Marc Petit , Kathryn Volk

The evolution of the luminosity of nova shells in the century following the nova outburst is studied for the lines H-alpha, H-beta, and [O III]. About 1200 flux measurements from 96 objects have been collected from the literature, from…

Astrophysics · Physics 2007-05-23 Ronald A. Downes , Hilmar W. Duerbeck , Catherine E. Delahodde

Neptune has brightened by more than 10% during the past several decades. We report on the analysis of published Johnson-Cousins B and V magnitudes dating back to 1954 along with new U, B, V, R, Rc, I and Ic photometry that we recorded…

Earth and Planetary Astrophysics · Physics 2016-04-05 Richard W. Schmude , Ronald E. Baker , Jim Fox , Bruce A. Krobusek , Hristo Pavlov , Anthony Mallama

We present new near-IR observations of 76 Class I/flat-spectrum objects in the nearby (d < 320 pc) Perseus, Taurus, Chamaeleon I and II, rho Ophiuchi, and Serpens dark clouds. These observations are part of a larger systematic infrared…

Astrophysics · Physics 2015-06-24 Karl E. Haisch , Thomas P. Greene , Mary Barsony , Steven W. Stahler

The Canada-France Ecliptic Plane Survey discovered four trans-Neptunian objects with semi-major axes near the 5:1 resonance, revealing a large and previously undetected intrinsic population. Three of these objects are currently resonant…

Earth and Planetary Astrophysics · Physics 2015-06-03 R. E. Pike , J. J. Kavelaars , J. M. Petit , B. J. Gladman , M. Alexandersen , K. Volk , C. J. Shankman

In the past decade, several rapidly-evolving transients have been discovered whose timescales and luminosities are not easily explained by traditional supernovae (SN) models. The sample size of these objects has remained small due, at least…

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