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Effect of Ephemeris on Pulsar Timing and Navigation Accuracy Based on X-ray Pulsar Navigation-I Data

open access: yesUniverse, 2022
Solar system ephemeris is very important for pulsar timing and navigation. In order to explore the effect of different precision ephemerides on X-ray pulsar timing and navigation, the differences between timing and navigation results with four JPL ...
Yongtao Deng, Shuanggen Jin
doaj   +1 more source

New Data on the Eclipsing Binary V1848 Ori and Improved Orbital and Light Curve Solutions

open access: yesOpen Astronomy, 2020
New observations of the eclipsing binary system V1848 Ori were carried out using the V filter resulting in a determination of new times of minima and new ephemeris were obtained.
Davoudi Fatemeh   +13 more
doaj   +1 more source

Original Research by Young Twinkle Students (ORBYTS): ephemeris refinement of transiting exoplanets [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
We report follow-up observations of transiting exoplanets that have either large uncertainties (>10 min) in their transit times or have not been observed for over 3 yr.
B. Edwards   +62 more
semanticscholar   +1 more source

An Efficient Fault Detection and Exclusion Method for Ephemeris Monitoring

open access: yesRemote Sensing, 2023
The ephemeris fault needs to be detected and mitigated in the ground-based augmentation system to provide precision approach for the aircraft. In the current fault detection and exclusion (FDE) method, the double-differenced carrier phase (DDCP ...
Yiping Jiang, Wang Li, Hengwei Zhang
doaj   +1 more source

TraMoS: V. Updated ephemeris and multi-epoch monitoring of the hot Jupiters WASP-18Ab, WASP-19b, and WASP-77Ab [PDF]

open access: yes, 2020
We present 22 new transit observations of the exoplanets WASP-18Ab, WASP-19b, and WASP-77Ab, from the Transit Monitoring in the South (TraMoS) project. We simultaneously model our newly collected transit light curves with archival photometry and radial ...
P. Cortés-Zuleta   +7 more
semanticscholar   +1 more source

Ephemeris of Mars [PDF]

open access: yesSymposium - International Astronomical Union, 1979
Newcomb's (1898) Tables of Mars with Ross's corrections have been used to compute its ephemeris in national ephemerides. Clemence (1949 and 1961) constructed a more precise theory of Mars and determined preliminary mean elements using a limited number of observations. Laubscher (1971) compared Clemence's theory with about 11000 observations by meridian
Hiroshi Nakai, Hiroshi Kinoshita
openaire   +2 more sources

Excluding Primordial Black Holes as Dark Matter Based on Solar System Ephemeris [PDF]

open access: yesResearch Notes of the AAS
Current cosmological constraints allow primordial black holes to constitute dark matter in the mass range of 1018–1022 g. I show that a major portion of this logarithmic window can be ruled-out based on the solar system ephemeris, given that the external
Abraham Loeb
semanticscholar   +1 more source

Time Ephemeris [PDF]

open access: yesHighlights of Astronomy, 1995
The location-independent part of TCB–TCG, the difference between the two new time scales adopted by the IAU (1992), was integrated numerically for three JPL planetary/lunar ephemerides; DE102, DE200, and DE245. The differences among these three integrations were mostly explained by the difference in the adopted constants of the ephemerides.
openaire   +1 more source

Astrometry of mutual approximations between natural satellites. Application to the Galilean moons [PDF]

open access: yes, 2016
Typically we can deliver astrometric positions of natural satellites with errors in the 50-150 mas range. Apparent distances from mutual phenomena, have much smaller errors, less than 10 mas. However, this method can only be applied during the equinox of
Assafin, M.   +5 more
core   +1 more source

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