This dataset describes a curated set of Wide-field Infrared Survey Explorer (WISE) observations of 4420 asteroids.

We analyzed 82,548 carefully curated observations of 4420 asteroids with Wide-field Infrared Survey Explorer (WISE) four-band data to produce estimates of diameters and infrared emissivities. We also used these diameter values in conjunction with absolute visual magnitudes to infer estimates of visible-band geometric albedos. We provide solutions to 131 asteroids not analyzed by the NEOWISE team and to 1778 asteroids not analyzed with four-band data by the NEOWISE team. Our process differs from the NEOWISE analysis in that it uses an accurate solar flux, integrates the flux with actual bandpass responses, obeys Kirchhoff’s law, and does not force emissivity values in all four bands to an arbitrary value of 0.9. We used a regularized model-fitting algorithm that yields improved fits to the data. Our results more closely match stellar-occultation diameter estimates than the NEOWISE results by a factor of ∼2. Using 24 high-quality stellar-occultation results as a benchmark, we found that the median error of four-infrared-band diameter estimates in a carefully curated data set is 9.3%. Our results also suggest the presence of a size-dependent bias in the NEOWISE diameter estimates, which may pollute estimates of asteroid size distributions and slightly inflate impact-hazard risk calculations. For more than 90% of asteroids in this sample, the primary source of error on the albedo estimate is the error in absolute visual magnitude.

This research has made use of the NASA/IPAC Infrared Science Archive, which is funded by the National Aeronautics and Space Administration and operated by the California Institute of Technology.

We selected a small, high-quality subset of the data from the WISE All-Sky Data Release. These data were obtained during the WISE full-cryogenic mission phase, from 7 January 2010 to 6 August 2010. This subset includes only observations of 4420 asteroids for which there are at least three high-quality observations in each one of the four WISE wavelength bands. We added ancillary data to each observation by querying the NASA JPL HORIZONS service. The data collection procedures are described in detail by N. Myhrvold, P. Pinchuk, J. L. Margot. Analysis of four-band WISE observations of asteroids. Planetary Science Journal, 3, 2022.

The data are provided as comma-separated values (CSV).

The field names, (types), [provenance], and descriptions are as follows:

• wavelength (str) [WISE]: WISE band (w1, w2, w3, or w4)  
• ras (float) [HORIZONS]: heliocentric distance in astronomical units
• rao (float) [HORIZONS]: geocentric distance in astronomical unit
• phase_ang (float) [HORIZONS]: phase angle in degrees
• name (str) [WISE]: asteroid number or provisional designation
• mjd (float) [WISE]: modified Julian date of the single-exposure covering the source
• m_flux (float) [WISE]: magnitude measured with profile-fitting photometry
• err (float) [WISE]: profile-fit photometric measurement uncertainty in mag units
• H (float) [HORIZONS]: absolute visual magnitude 
• G (float) [HORIZONS]: magnitude slope parameter
• data_filter_group (str) [authors]: internal description of data subset 
• dist_x (float) [WISE]: distance in arcsec between each moving object source and its potential match in the WISE All-Sky Single Exposure (L1b) Source Table
• nb (int) [WISE]: number of blend components used in each fit
• na (int) [WISE]: active deblend flag (=1 if actively deblended)
• sso_flg (int) [WISE]: known solar system object association flag (0=no association, >0=association)
• Epoch_ID (int) [authors]: zero-based index of cluster of observations (clusters were formed when consecutive observations were more than 30 days apart)