HARDERSEN IRTF ASTEROID NIR REFLECTANCE SPECTRA V1.0

This dataset includes average near-infrared (NIR) reflectance spectra for 68 main-belt asteroids that were observed at the NASA Infrared Telescope Facility (IRTF), Mauna Kea, Hawaii, from April 2001 to January 2015. Raw NIR spectral data were obtained under mostly uniform instrumental conditions and include observations of the asteroids, extinction stars, and solar analog stars that were necessary for data reduction and production of the final average asteroid NIR reflectance spectra. SpecPR and Spextool were used during data reduction to produce the final spectra and both programs utilize similar functions that include sky background subtraction, telluric corrections, channel shifting, and averaging routines. The set of asteroids observed include a wide variety of taxonomic types and include V-, S-, M-, X-types that correspond to a wide variety of surface mineralogies, rock types, and potential meteorite analogs.

Data and Resources

This dataset has no data

Field Value
accessLevel public
accrualPeriodicity irregular
bureauCode {026:00}
catalog_@context https://project-open-data.cio.gov/v1.1/schema/catalog.jsonld
catalog_@id https://data.nasa.gov/data.json
catalog_conformsTo https://project-open-data.cio.gov/v1.1/schema
catalog_describedBy https://project-open-data.cio.gov/v1.1/schema/catalog.json
identifier urn:nasa:pds:context_pds3:data_set:data_set.ear-a-i0046-3-hardersenspec-v1.0
issued 2018-06-26
landingPage https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=EAR-A-I0046-3-HARDERSENSPEC-V1.0
modified 2020-01-29
programCode {026:005}
publisher National Aeronautics and Space Administration
references {https://pds.nasa.gov}
resource-type Dataset
source_datajson_identifier true
source_hash 5b21b8faaa03b0a128f12806cbba1968721ef0e9
source_schema_version 1.1
theme {"Earth Science"}
Groups
  • AmeriGEOSS
  • National Provider
  • North America
Tags
  • 10666-feldberg
  • 110-lydia
  • 1210-morosovia
  • 125-liberatrix
  • 129-antigone
  • 132-aethra
  • 135-hertha
  • 136-austria
  • 1459-magnya
  • 1461-jean-jacques
  • 16-psyche
  • 184-dejopeja
  • 201-penelope
  • 2011-veteraniya
  • 21-lutetia
  • 216-kleopatra
  • 2168-swope
  • 22-kalliope
  • 224-oceana
  • 250-bettina
  • 31414-rotarysusa
  • 325-heidelberga
  • 338-budrosa
  • 347-pariana
  • 369-aeria
  • 3715-stohl
  • 3782-celle
  • 382-dodona
  • 3849-incidentia
  • 3867-shiretoko
  • 413-edburga
  • 417-suevia
  • 418-alemannia
  • 441-bathilde
  • 497-iva
  • 504-cora
  • 516-amherstia
  • 5235-jean-loup
  • 55-pandora
  • 5560-amytis
  • 558-carmen
  • 5875-kuga
  • 69-hesperia
  • 6976-kanatsu
  • 71-niobe
  • 739-mandeville
  • 758-mancunia
  • 766-moguntia
  • 77-frigga
  • 785-zwetana
  • 796-sarita
  • 798-ruth
  • 8149-ruff
  • 857-glasenappia
  • 860-ursina
  • 872-holda
  • 9147-kourakuen
  • 931-whittemora
  • 9553-colas
  • 97-klotho
  • amerigeo
  • amerigeoss
  • asteroid
  • asteroid-15237
  • asteroid-17469
  • asteroid-19165
  • asteroid-29796
  • asteroid-30872
  • asteroid-32940
  • asteroid-5754
  • asteroid-6331
  • ckan
  • geo
  • geoss
  • national
  • north-america
  • support-archives
  • united-states
isopen False
license_id notspecified
license_title License not specified
maintainer Thomas Morgan
maintainer_email thomas.h.morgan@nasa.gov
metadata_created 2025-11-21T12:59:49.320580
metadata_modified 2025-11-21T12:59:49.320584
notes This dataset includes average near-infrared (NIR) reflectance spectra for 68 main-belt asteroids that were observed at the NASA Infrared Telescope Facility (IRTF), Mauna Kea, Hawaii, from April 2001 to January 2015. Raw NIR spectral data were obtained under mostly uniform instrumental conditions and include observations of the asteroids, extinction stars, and solar analog stars that were necessary for data reduction and production of the final average asteroid NIR reflectance spectra. SpecPR and Spextool were used during data reduction to produce the final spectra and both programs utilize similar functions that include sky background subtraction, telluric corrections, channel shifting, and averaging routines. The set of asteroids observed include a wide variety of taxonomic types and include V-, S-, M-, X-types that correspond to a wide variety of surface mineralogies, rock types, and potential meteorite analogs.
num_resources 0
num_tags 78
title HARDERSEN IRTF ASTEROID NIR REFLECTANCE SPECTRA V1.0