Results 81 to 90 of about 9,418 (215)
Trans-Neptunian Objects Found in the First Four Years of the Dark Energy Survey [PDF]
We present a catalog of 316 trans-Neptunian bodies (TNOs) detected from the first four seasons (“Y4” data) of the Dark Energy Survey (DES). The survey covers a contiguous 5000 deg2 of the southern sky in the grizY optical/NIR filter set, with a typical ...
P. Bernardinelli +63 more
semanticscholar +1 more source
The DECam Ecliptic Exploration Project (DEEP). III. Survey Characterization and Simulation Methods
We present a detailed study of the observational biases of the DECam Ecliptic Exploration Project’s B1 data release and survey simulation software that enables direct statistical comparisons between models and our data.
Pedro H. Bernardinelli +26 more
doaj +1 more source
Vapor pressure is a relevant quantity that is necessary in order to improve the study of the atmosphere dynamics that take place within astrophysical scenarios.
C. Millán +4 more
semanticscholar +1 more source
Dynamically studying trans-Neptunian object (TNO) binaries allows us to measure masses and orbits. Most of the known objects appear to have only two components, except (47171) Lempo, which is the single known hierarchical triple system with three similar-
Maia A Nelsen +4 more
doaj +1 more source
Col-OSSOS: The Two Types of Kuiper Belt Surfaces
The Colors of the Outer Solar System Origins Survey (Col-OSSOS) has gathered a high-quality, near-simultaneous, and brightness-complete sample of ( g − r ) and ( r − J ) colors for 102 Kuiper Belt objects (KBOs) with ( u − g ) and ( r − z ) gathered for ...
Wesley C. Fraser +14 more
doaj +1 more source
Formation and Migration of Trans-Neptunian Objects [PDF]
Trans-Neptunian objects (TNOs) with diameter d>100 km moving now in not very eccentric orbits could be formed directly by the compression of large rarefied dust condensations (with semi-major axes a>30 AU), but not by the accretion of smaller solid planetesimals.
openaire +3 more sources
Logos-Zoe: A Contact Binary Triple System in the Trans-Neptunian Belt
The trans-Neptunian object (58534) 1997 CQ _29 (a.k.a. Logos) is a resolved wide binary in the dynamically Cold Classical population. With Hubble Space Telescope resolved observations where the primary Logos is well separated from its secondary Zoe it ...
Audrey Thirouin +5 more
doaj +1 more source
THE INCLINATIONS OF FAINT TRANS-NEPTUNIAN OBJECTS
Bernstein et al. found that the population of faint (R> 26) trans-Neptunian objects (TNOs) known at that time was dominated by "Classical" objects, which have low inclinations (i < 5°) and distances of 40-45 AU. Since those observations, the number of faint TNOs whose orbits are sufficiently well known to be classified as "Classical" or "Excited" has ...
D. E. Trilling +2 more
openaire +1 more source
Rotational Study of 5:3 and 7:4 Resonant Objects within the Main Classical Trans-Neptunian Belt
The 5:3 and 7:4 mean motion resonances of Neptune are at 42.3 and 43.7 au, respectively, and overlap with objects in the classical trans-Neptunian belt (Kuiper Belt).
Audrey Thirouin, Scott S. Sheppard
doaj +1 more source
FindPOTATOs: Minor Planet Observation Linking Software
For minor planet observations to be archived and used by the scientific community, observations of individual objects must be linked together into groups called tracklets.
C. R. Nugent +2 more
doaj +1 more source

