The Catalog of Unidentified Cometary Emission lines Data Set Overview ================= This data set contains tables of unidentified spectral emission lines and other ancillary information in a variety of comet observations. All these originally unidentified lines have been taken from the reference papers without adding or removing lines or using selection criteria. Archive Package Overview ======================== The data are presented in single .csv files with definitions. Entries that could not be found are filled with the value 'UNK' (Unknown) to represent there is no data for that entry in the reference papers. The units between different data may change and the label will have the proper units for the entry. The following are the categories you will find in the data. Product Name: - Comet Name Product Description: - Unidentified Emission Lines Start and Stop time in format of YYYY-MM-DDThh:mm:ss - where: - • YYYY - Represents the year (0001 to 9999) • - Is a required delimiter between date fields • MM - Represents the month (01 to 12) • DD - Represents the day of month (01 to 28, 29, 30 or 31) • T - Is a required delimiter between date and time • hh - Represents the UTC hour (00 to 23) • : Is a required delimiter between time fields • mm - Represents the UTC minute (00 to 59) • ss - Represents UTC whole seconds (00 to 59) Target Name: comet designation Target Type: comet Author List, Facility: - literature Instrument: - literature Observing Bookmark, Product Processing Level: - Derived Science Search Facet: - Tabulated Product Wavelength Ranges: - Visible, Near Infrared, Ultraviolet Reference Code/Key: - Automated given code to facilitate reference searching. Place of observation, Instruments, Slit (arcsecond), Exposure time (second), Geocentric Distance (AU), Heliocentric Distance (AU), Spectrograph Resolving Power, Spectral Range in Angstrom (Å), Signal to Noise, List of Unidentified Emissions Lines in Angstrom (Å) Known Issues or Problems with the Data ====================================== The data for the given 12 comets have been taken from the papers in the different per-reviewed journals. Take into consideration that, the data are not homegenious due to various methods used for results in calculations by different authors.