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Small and Nearby NEOs Observed by NEOWISE During the First Three Years of Survey: Physical Properties.

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TLDR
In this article, the authors conducted a search of the first three years of the reactivated NEOWISE data, looking for near-Earth objects discovered by ground-based surveys that have previously unreported thermal infrared data.
Abstract
Automated asteroid detection routines set requirements on the number of detections, signal-to-noise ratio, and the linearity of the expected motion in order to balance completeness, reliability, and time delay after data acquisition when identifying moving object tracklets. However, when the full-frame data from a survey are archived, they can be searched later for asteroids that were below the initial detection thresholds. We have conducted such a search of the first three years of the reactivated NEOWISE data, looking for near-Earth objects discovered by ground-based surveys that have previously unreported thermal infrared data. Using these measurements, we can then perform thermal modeling to measure the diameters and albedos of these objects. We present new physical properties for 116 Near-Earth Objects found in this search.

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CMB-S4 Science Case, Reference Design, and Project Plan

Kevork N. Abazajian, +224 more
TL;DR: In this article, the authors present the science case, reference design, and project plan for the Stage-4 ground-based cosmic microwave background experiment CMB-S4, as well as the experimental data.
Journal ArticleDOI

Asteroid Diameters and Albedos from NEOWISE Reactivation Mission Years 4 and 5

TL;DR: The Near Earth Object Wide-field Infrared Survey Explorer (NEOWISE) spacecraft has been conducting a two-band thermal infrared survey to detect and characterize asteroids and comets since its reactivation in 2013 December as discussed by the authors.
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Thermophysical modeling of NEOWISE observations of DESTINY+ targets Phaethon and 2005 UD

TL;DR: In this paper, a Monte Carlo Markov Chain (MCMC) was used to explore the multi-dimensional parameter space of the fit of the model for two near-Earth asteroids, Phaethon and (155140) 2005 UD.
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The Debiased Compositional Distribution of MITHNEOS: Global Match between the Near-Earth and Main-belt Asteroid Populations, and Excess of D-type Near-Earth Objects

TL;DR: In this article , the authors reported 491 near-infrared spectroscopic measurements of 420 near-Earth objects (NEOs) collected on the NASA InfraRed Telescope Facility as part of the MIT-Hawaii NEO Spectroscopic Survey.
Journal ArticleDOI

ATM: An open-source tool for asteroid thermal modeling and its application to NEOWISE data

TL;DR: ATM as mentioned in this paper is a Python package designed to model asteroid flux measurements to estimate an asteroid's size, surface temperature distribution, and emissivity using Markov Chain Monte Carlo (MCMC).
References
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Journal ArticleDOI

A Thermal Model for Near-Earth Asteroids

Alan W. Harris
- 01 Feb 1998 - 
TL;DR: In this paper, a simple simple thermal model for estimating albedos and diameters of near-Earth asteroids was proposed as a default simple model for estimation albedo and diameter.
Journal ArticleDOI

Neowise observations of near-earth objects: preliminary results

TL;DR: In this article, the authors carried out a highly uniform survey of the near-Earth object (NEO) population at thermal infrared wavelengths ranging from 3 to 22 μm, allowing them to refine estimates of their numbers, sizes, and albedos.
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