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 released in March 2012. 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 and 'tumbling' asteroids.

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.

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.

Dataset Description:

This dataset comprises handwritten digit images ranging from 0 to 9, captured in the Kegalle region. Each image is manually written, representing a unique numeric digit. The dataset is intended for tasks such as image recognition, machine learning model training, and deep learning applications.

Features:

Image Files: High-resolution images of handwritten digits (0-9). Labels: Numeric labels corresponding to each handwritten digit image.

Data Specifications:

Image Format: JPEG/PNG Image Resolution: 28x28 pixels

Potential Applications:

Handwritten digit recognition Neural network and machine learning model training Computer vision tasks

Usage Recommendations:

Researchers, data scientists, and machine learning enthusiasts can utilize this dataset for training and testing machine learning models, particularly in the field of image classification and recognition.

Acknowledgment:

We acknowledge the contributors and data collectors from the Kegalle region for their valuable efforts in creating this dataset.

This data set contains the Magellan the FMAP, a full-resolution (75 meters/pixel) global mosaic, produced by the U.S. Geological Survey from Magellan F-BIDR data. The complete dataset consists of 340 quadrangles in Sinusoidal equal-area projection. Quadrangles extend approximately 12 degrees in latitude, except for those between 84 and 90 degrees North and South. Quadrangles near the equator extend 12 degrees in longitude longitudinal extent is increased to maintain a roughly constant number of samples.

This PDS data set represents a compilation of published diameters, optical albedos, near-infrared albedos, and beaming parameters for minor planets detected by NEOWISE during the fully cryogenic, 3-band cryo, post-cryo and NEOWISE-Reactivation Year 1 operations. It contains data covering near-Earth asteroids, Main Belt asteroids, active Main Belt objects, Hildas, Jupiter Trojans, Centaurs, and Jovian and Saturnian irregular satellites. Methodology for physical property determination is described in the referenced articles.

The Near Infrared Mapping Spectrometer (NIMS) on the Galileo spacecraft took unique data of Comet Shoemaker-Levy/9's impact with Jupiter. A preliminary analysis of this data is presented in this submission to the Planetary Data System (PDS). It consists of nine small tables with detached labels and documentation.

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 Paleoceanography. The data include parameters of paleoceanography with a geographic location of Central Pacific Ocean. The time period coverage is from 144000 to 0 in calendar years before present (BP). See metadata information for parameter and study location details. Please cite this study when using the data.

The NEAR Mathilde Radio Science Data Set is a time-ordered collection of raw and partially processed data collected during the NEAR flyby of minor planet 253 Mathilde.

ydwen/synthesized-data-0 dataset hosted on Hugging Face and contributed by the HF Datasets community

ALOS PALSAR Level 1.0

the current is 1.81mA

Dataset

This dataset was created by ShafieeAmir

Contents

Global trade data of 0 under 071331, 071331 global trade data, trade data of 0 from 80+ Countries.

Global trade data of 0 under 35079000, 35079000 global trade data, trade data of 0 from 80+ Countries.

A dataset contain full information of papers published from volume 0 to 12 of conference on neural information processing systems (NIPS).

MMSD2.0: Towards a Reliable Multi-modal Sarcasm Detection System

This is a copy of the dataset uploaded on Hugging Face for easy access. The original data comes from this work, which is an improvement upon a previous study.

  Usage

from typing import TypedDict, cast

import pytorch_lightning as pl from datasets import Dataset, load_dataset from torch import Tensor from torch.utils.data import DataLoader from transformers import CLIPProcessor

class… See the full description on the dataset page: https://huggingface.co/datasets/coderchen01/MMSD2.0.

tanhuajie2001/RoboBrain2.0-ERQA-Train-Data-Subset dataset hosted on Hugging Face and contributed by the HF Datasets community

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.

Version 10 is the current version of the data set. Older versions will no longer be available and are superseded by Version 10. 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.