The Near-Earth Object Wide-field Infrared Survey Explorer at IPAC

The NEOWISE 2015 Data Release
March 26, 2015

Access the Database and Image data via IRSA Read the Explanatory Supplement
Top Ten List of things you should know about the NEOWISE Release Products
NEOWISE 2015 Release sky coverage
NEOWISE Project website NEOWISE mission description paper
Contact the WISE/NEOWISE Help Desk
Frequently asked questions (FAQ)

The NEOWISE 2015 Data Release contains the 3.4 and 4.6 μm (W1 and W2) Single-exposure images and extracted source information that were acquired between December 13, 2013 and December 13, 2014 UTC, the first year of survey operations of the Near-Earth Object Wide-field Infrared Survey Explorer Reactivation Mission (NEOWISE; Mainzer et al. 2014, ApJ, 792, 30).

NEOWISE utilizes the Wide-Field Infrared Explorer (WISE; Wright et al. 2010, AJ, 140, 1868) spacecraft that surveyed the entire sky in 2010 with a cryogenically cooled 40 cm telescope and four 1kx1k mid-infrared array detectors. WISE continued to survey for four months following the exhaustion of its solid hydrogen cryogen in September 2010 using its two short wavelength bands. After completing a survey of the inner main asteroid belt and a second coverage of the inertial sky, WISE was placed into hibernation in February 2011.

The WISE spacecraft was brought out of hibernation in September 2013 and renamed NEOWISE with a mission to detect and characterize asteroids and comets, and to learn more about the population of near-Earth objects that could pose an impact hazard to the Earth. The spacecraft was returned to zenith pointing which enabled the telescope and focal plane to passively cool down to approximately 73 K. Survey operations were resumed on December 13, 2013 UTC with the W1 and W2 detectors operating at sensitivities near those of the original cryogenic survey. The first solar system moving object tracklet candidates were reported to the IAU Minor Planet Center on December 26, and tracklet deliveries continue to be made three times per week. As of mid-March, 2015, NEOWISE has made over 215,000 confirmed infrared measurements of nearly 12,000 solar system objects.

The NEOWISE 2015 Data Release data products include:

NEOWISE scanned the inertial sky nearly two complete times during the first year of survey operations, with each sky pass separated by approximately six months. Twelve independent exposures are acquired at each point on the sky near the ecliptic plane during each survey epoch, and the number of samples increases towards the ecliptic poles. As illustrated in Figure 1, the NEOWISE 2015 Release contains 24 independent observations near the ecliptic plane, increasing to over 5300 observations very close to the ecliptic poles.

The NEOWISE 2015 Release Single-exposure data products are time-domain resources for extracting thermal flux and position measurements for NEOWISE moving object detections, as well as a precovery archive for solar system objects discovered after the NEOWISE observations. The NEOWISE products are also an archive for studying flux variability and proper motion of galactic and extragalactic objects. When combined from the Single-exposure data from the original WISE mission, the NEOWISE images and source detection database provide an archive that spans a four year baseline with four or five separate epochs of observation.

The NEOWISE Reactivation Mission is funded by the NASA Planetary Science Division. Planetary science research using NEOWISE data is eligible for proposals to the NASA ROSES Solar System Workings and Planetary Data Archiving, Restoration and Tools Programs. Astrophysics reasearch using NEOWISE data is eligible for proposals to the NASA ROSES Astrophysics Data Analysis Program.

Figure 1 - NEOWISE Year 1 Depth-of-Coverage. Ecliptic Aitoff projection sky map showing the average number of individual Single-exposures within 12´ × 12´ spatial bins that are included in the NEOWISE 2015 data release. Colors encode different frame depths-of-coverage as specified by the legend on the bottom. Approximately 10% of the sky bounded by ecliptic longitude ranges 107.5°<λ<126.1° and 281.4°<λ<299.2° was not observed during the first coverage epoch because of a safe hold event.

Please use this acknowledgement in any published material that makes use of NEOWISE data products:

"This publication makes use of data products from the Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE), which is a project of the Jet Propulsion Laboratory/California Institute of Technology. NEOWISE is funded by the National Aeronautics and Space Administration."

Last update - 2015 April 2