A fast method for quantifying observational selection effects in asteroid surveys

TL;DR: In this article, the authors presented a new four-dimensional model of the near-Earth objects population that describes debiased steady-state distributions of semimajor axis, eccentricity, inclination, and absolute magnitude H in the range 17.962 − 56 + 52 + 52 ( 802 − 42 + 48 × 10 3 ) NEOs with H.

TL;DR: In this article, the authors present a systematic search for optical counterparts to 13 GW triggers involving at least one neutron star during LIGO/Virgo's third observing run (O3).

TL;DR: The most recent models converged to a population of approximately 1000 NEAs larger than 1.5 km and up to approximately 109 NEAs with absolute magnitude H as discussed by the authors, which is the largest NEAs known to date.

TL;DR: In this paper , a series of operation simulations using the Rubin Observatory scheduler have been generated to explore the various options for tuning observing parameters and prioritizations, and the impact of various simulated LSST observing strategies on studying the solar system's small body reservoirs.

TL;DR: This chapter discusses Graphics, Image Processing, and Pattern Recognition, and the Reconstruction techniques used in this program, as well as some of the problems faced in implementing this program.

TL;DR: In this paper, a Johnson-glass system is proposed and its absolute calibration derived based on the Bell model atmosphere fluxes for Alpha Lyrae, and the homogenized colors of the standard stars are used to derive intrinsic colors for stars with spectral types between B7V and M6V, and G7III and MSIII.

TL;DR: The Asteroid Lightcurve Database (LCDB) as mentioned in this paper is a central database for asteroid lightcurve data, i.e., rotation rate and amplitude along with ancillary information such as diameter and albedo, taxonomic class, etc.