This is a compilation of published rotational parameters derived from lightcurve data for asteroids, based on the Warner et al. (2009) Asteroid Lightcurve Database. This is the version as of February 16, 2016. In addition to reported rotational parameters by individual paper, there is a summary file with the values adopted by Harris, Warner, and Pravec as the most likely correct values for each asteroid. The data set also contains files listing known binary asteroids, asteroid spin axes, and 'tumbling' asteroids.

ALOS PALSAR Level 1.0

Version 11 is the current version of the data set. Older versions will no longer be available and are superseded by Version 11. The Orbiting Carbon Observatory is the first NASA missiondesigned to collect space-based measurements of atmospheric carbon dioxidewith the precision, resolution, and coverage needed to characterize theprocesses controlling its buildup in the atmosphere. The OCO-2 project uses the LEOStar-2 spacecraft that carries a single instrument. It incorporates three high-resolution spectrometers that make coincident measurements ofreflected sunlight in the near-infrared CO2 near 1.61 and 2.06 micrometers and inmolecular oxygen (O2) A-Band at 0.76 micrometers . Each band has 1016 spectralelements.This product contains pointing angles of the spacecraft for each orbit.It is generated using the following input data:+ APID 20 telemetry+ Orbit Boundary File.It is essential in generating the Geolocations of the science data.

The eight color asteroid survey provides reflectance spectra for minor planets using eight filter passbands. This dataset includes the primary data obtained for 589 minor planets, the mean values for each minor planet included in the survey, the principal component scores derived from the primary data, the response curves, effective wavelengths, and bandpasses for the filters, and the coordinates and values determined for standard stars defining the system.

This dataset includes the downsapled data from the single- and binary-star models grids used in POSYDON, as well as the trained classification and interpolation models.

Bunny-v1.0 Dataset Card

📖 Technical report | 🤗 Bunny-v1.0-3B | 🏠 Code | 🐰 Demo Bunny is a family of lightweight multimodal models. Bunny-v1.0-data is the training dataset for Bunny-v1.0 series, including Bunny-v1.0-3B.

  Pretrain

We use a high-quality coreset with less duplicates and more informative samples of LAION-2B built by this work. We randomly sample 2 million image-text pairs from the coreset and convert them to training format. The pretraining data and… See the full description on the dataset page: https://huggingface.co/datasets/BoyaWu10/Bunny-v1_0-data.

Delta Channel Depletion (DCD v1.0) is an extension of Delta Evapotranspiration of Applied Water (DETAWv2.0). Based on the estimation of Delta ground surface water balance by DETAW v2.0, DCD v1.0 simulates the daily channel depletions, including diversions, drainages and seepages, in the Sacramento-San Joaquin River Delta and distributes them on the Delta Simulation Model 2(DSM2) nodes. The package includes the model code, model inputs, technical reports, preliminary user’s manual, and necessary software to support the model.

This data set contains the monthly climatology (MC) data of the secondary forcing data for Phase 2 of the North American Land Data Assimilation System (NLDAS-2). The data are in 1/8th degree grid spacing. The temporal resolution is monthly, ranging from January to December. The NLDAS-2 monthly climatology data are the NLDAS-2 monthly data averaged over forty years (1981 - 2020). The file format is netCDF. The previous version of this dataset (NLDAS_MC 002) was a 30-year average and was stored in GRIB file format.A brief description about the NLDAS-2 hourly and monthly secondary forcing data can be found from the NLDAS_FORB0125_H_2.0 and NLDAS_FORB0125_M_2.0 landing pages.Details about the generation of the NLDAS-2 forcing datasets can be found in Xia et al. (2012).For more information, please see the README Document.

The Juno MWR RDR data set will ultimately include all calibrated MWR science data for the entire Juno mission. This volume will contain only those data obtained through the cruise phase of the Juno mission, when this phase of the mission is completed. The objective for these data is to provide calibration for the MWR instrument; however, it is anticipated that they may someday be useful for astrophysics. This volume consists of calibrated data records, each of which contains all instrumental data required for further processing. The RDR records have a one-to-one correspondence with the EDR records.

This data set is a compilation of published diameters, albedos, and densities for Transneptunian Objects (TNOs) and Centaurs. A total of 190 objects are listed, many with more than one entry. This version covers published values through 31 March 2016.

The data were created by transformation of vector cadastral component of SM 5 to raster file. In territories, where vector SM 5 has not been created yet, the cadastral and altimetry components were created by scanning of individual printing masters of planimetry and altimetry from the last issue of the State Map 1:5,000 - derived. The cadastral component does not contain parcel numbers.

This data set contains CODMAC level 3 data acquired by the Rosetta Orbiter ALICE UV Spectrometer during the second earth swing-by phase of the Rosetta mission, which occurred 2007-09-13 to 2007-12-13. In addition to the second swingby of the earth, this period includes the active payload checkout #6 (PC6). The observations made during the period covered by this data set are primarily designed to improve the calibration of the Alice instrument.

The O*NET Database contains hundreds of standardized and occupation-specific descriptors on almost 1,000 occupations covering the entire U.S. economy. The database, which is available to the public at no cost, is continually updated by a multi-method data collection program. Sources of data include: job incumbents, occupational experts, occupational analysts, employer job postings, and customer/professional association input.

Data content areas include:

• Worker Characteristics (e.g., Abilities, Interests, Work Styles)
• Worker Requirements (e.g., Education, Knowledge, Skills)
• Experience Requirements (e.g., On-the-Job Training, Work Experience)
• Occupational Requirements (e.g., Detailed Work Activities, Work Context)
• Occupation-Specific Information (e.g., Job Titles, Tasks, Technology Skills)

This archived Paleoclimatology Study is available from the NOAA National Centers for Environmental Information (NCEI), under the World Data Service (WDS) for Paleoclimatology. The associated NCEI study type is Ice Core. The data include parameters of climate forcing|ice cores with a geographic location of Antarctica. The time period coverage is from 11103 to 390 in calendar years before present (BP). See metadata information for parameter and study location details. Please cite this study when using the data.

The observations were made using a double CVF (circularly variable filter). The short wavelength portion of the CVF covered the octave from 0.8 to 1.6 microns with 3 percent resolution, while the long wavelength portion covered 1.5 to 2.6 microns with 5 percent resolution. There is some overlap in the spectral coverage between 1.5 and 1.6 microns, which is evident as a discontinuity in the wavelengths after the first 32 values, which were obtained with the short wavelength portion, while the remaining 20 values were obtained with the long wavelength portion.

This data set is intended to include published broadband colors of centaurs and Transneptunian Objects (TNOs) published through April 2009. It supersedes all versions of the TNO colors data set EAR-A-3-RDR-TNO-PHOT.

We present a data table giving basic physical and orbital parameters for known binary minor planets in the Solar System (and Pluto/Charon) based on published literature. For the purposes of this table, a binary minor planet is any mutually orbiting pair of minor planets in our Solar System, where a minor planet is any substantial body orbiting the Sun that is not a major planet, nor is bound to a major planet.

This data set is intended to include all published groundbased asteroid radar detections. The file is based on the collection of asteroid radar detections established by Steven J. Ostro and currently maintained by Lance A.M. Benner. The file includes disc-integrated radar properties extracted from the published papers.

The GPROF 6.0 Pentads data set contains 5-day (pentad) averages of the GPROF 6.0 Gridded Orbits. The GPROF(Goddard Profiling Algorithm) data set contains a suite of 9 products providing instantaneous, gridded values of precipitation totals for each granule of the SSM/I (Special Sensor Microwave/Imager) data over the roughly 14-year period July 1987 through the present. Even though there have been at least two satellites for the entire period, sampling is sufficiently sparse that the data are averaged for pentads, then the pentads are smoothed with a 1-2-3-2-1 time-weighting. The last two pentads are unevenly weighted since the last (or last two) pentads in the average are not yet available. Consequently, the last two pentads must be recomputed when the next pentad becomes available.The data set prepared for SAFARI cover the years 1999, 2000, and 2001.The main refereed citations for the data set are Kummerow et al. (1996)and Olson et al. (1999)

This data set contains albedos for 57 asteroids determined from diameters obtained from stellar occultations. These albedos are from Shevchenko and Tedesco (2006).