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Data Sets and Information
• collection: Catalina Sky Survey Bundle: Raw Data Collection
  Raw Data files for Catalina Sky Survey
• collection: data collection for the "SEVEN COLOR ASTEROID SURVEY" bundle
  This is the data collection for the gbo.ast.7-color-survey bundle. The Seven-color Asteroid Survey (SCAS) consists of photometry in seven filters from 0.9 to 2.3 microns, of a total of 126 asteroids of types S, K, and M.
• collection: data collection for the "VILAS ASTEROID SPECTRA" bundle
  This is the data collection for the gbo.ast.vilas.spectra bundle. This data set contains 81 published spectra of asteroids obtained by Faith Vilas during the years 1982 - 1992.
• collection: Small Bodies Occultations V3.0
  This data set is intended to include all reported timings of observed asteroid, planet, and planetary satellite occultation events made by observers from around the world. Included are occultation axes derived from those timings, and (wherever possible) volume-equivalent diameters derived from fitting to shape models. This version is complete through to May 2019, with observations up until Sept 2019.
• collection: Asteroid (101955) Bennu Radar Shape Model V1.1
  We present the three-dimensional shape of near-Earth asteroid (101955) Bennu (provisional designation 1999 RQ36) based on radar images and optical lightcurves (Nolan et al., 2013). Bennu was observed both in 1999 at its discovery apparition, and in 2005 using the 12.6-cm radar at the Arecibo Observatory and the 3.5-cm radar at the Goldstone tracking station. Data obtained in both apparitions were used to construct a shape model of this object. Observations were also obtained at many other wavelengths to characterize this object, some of which were used to further constrain the shape modeling (Clark et al., 2011; Hergenrother et al., 2013; Krugly et al., 1999).
• collection: McDonald Observatory Column Density Observations of 19P/Borrelly (PDS4 Format)
  This data set includes the raw column densities of several gas species observed in the spectra of comet Borrelly, as a function of position in the coma. All measurements were made with the 2.7-m Harlan J Smith Telescope at McDonald Observatory. During the 1981 and 1987-1988 apparitions, the data were obtained with the Intensified Dissector Scanner (IDS), and during the 1994 apparition, the data were obtained with the Large Cassegrain Spectrograph (LCS). These data were migrated from the PDS3 dataset EAR-C-IDS/LCS-3-RDR-BORRELLY-MCDNLD-V1.0.
• collection: data collection for the "NESVORNY HCM ASTEROID FAMILIES" bundle
  This is the data collection for the ast.nesvorny.families bundle. This data set contains asteroid dynamical family memberships for 122 families calculated from synthetic proper elements, including high-inclination families. These families were calculated by David Nesvorny (Nesvorny et al. 2015) using his code based on the Hierarchical Clustering Method (HCM) described in Zappala et al. (1990, 1994). The input synthetic proper elements for 384,337 numbered asteroids were calculated by Knezevic and Milani.
• collection: Zappala et al. (1995) Asteroid Dynamical Families V1.0
  Dynamical family classification of asteroids by Zappala et al., based on the hierarchical clustering method
• collection: data collection for the "KHARKIV ASTEROID MAGNITUDE-PHASE RELATIONS" bundle
  This is the data collection for the compil.ast.magnitude-phase bundle. A database of asteroid magnitude-phase relations compiled at the Institute of Astronomy of Kharkiv Kharazin University by Shevchenko et al., including observations from 1978 through 2008. Mainly the observations were performed at the Institute of Astronomy (Kharkiv, Ukraine) and at the Astrophysics Institute (Dushanbe, Tadjikistan). For most asteroids the magnitude-phase relations were obtained down to phase angles less than 1 deg. For some asteroids the magnitudes are presented in three (UBV) or four (BVRI) standard spectral bands.
• collection: Small Main-Belt Asteroid Spectroscopic Survey (SMASS) V1.0
  The Small Main-Belt Asteroid Spectroscopic Survey (SMASS) was a wide wavelength-coverage visible spectroscopic survey of asteroids carried out primarily at the Michagan-Dartmouth-MIT (McGraw Hill) Observatory on Kitt Peak beginning in 1990. This data set covers the observations for the years 1990-1994 and includes spectra of 316 asteroids. The data have been published in Xu et al. (1995), Icarus 115, 1-35, 1995.
• collection: data collection for the "LEBOFSKY ET AL. 3-MICRON ASTEROID DATA " bundle
  This is the data collection for the gbo.ast.lebofsky-etal.3-micron-spectra bundle. 3-micron spectrophotometric data on asteroids collected from several papers by Lebofsky, Jones, and Feierberg and their collaborators, published 1980-1990.
• collection: Catalina Sky Survey Bundle: Partially Processed Data Collection
  Partially Processed Data files for Catalina Sky Survey
• collection: data collection for the "TRANS-NEPTUNIAN OBJECT LIGHTCURVES" bundle
  This is the data collection for the compil.tno-centaur.lightcurves bundle. This data set includes a collection of published lightcurves of trans-Neptunian objects published through December 2002. The collection includes lightcurves of 18 TNOs.
• collection: Whiteley NEO Photometry V1.0
  This data set includes the ECAS system (Eight Color Asteroid Survey) photometry and taxonomic types of 77 Near Earth Objects published by R.J. Whiteley in his thesis (Whiteley, 2001. A compositional and dynamical survey of the near-earth asteroids. Ph.D. thesis, University of Hawaii), [WHITELEY2001] The ECAS system is established in Zellner et al. 1985, Icarus 61, 355-416 [ZELLNERETAL1985]. The original ECAS survey is available in PDS as data set EAR-A-2CP-3-RDR-ECAS-V3.0. The data presented here are new measurements based on the ECAS system.
• collection: data collection for the "POLARIMETRY OF ASTEROID ITOKAWA" bundle
  This is the data collection for the gbo.ast-itokawa.torino.polarimetry bundle. This data set contains the polarimetry of asteroid 25143 Itokawa published in Cellino et al. (2005). The observations were made from June 26 through July 3, 2004 with the Torino photopolarimeter at the 2.15 m telescope of the El Leoncito Observatory in Argentina. The degree of linear polarization was measured in five filters (Johnson-Cousins UBVRI).
• collection: data_tricam collection for the "NEAR EARTH ASTEROID TRACKING" bundle
  This is the data_tricam collection for the gbo.ast.neat.survey bundle. The Near-Earth Asteroid Tracking (NEAT) project began as a collaborative effort with the United States Air Force (USAF) in December 1995. It concentrated on the discovery and observations of near-Earth asteroids and comets, collectively called near-Earth objects (NEOs). NEAT ended its observations in April 2007. Throughout its history, NEAT utilized three 1m class telescopes - two on the Hawaiian island of Maui and the 1.2m Oschin Schmidt telescope at Palomar Observatory near San Diego, CA. Three unique cameras were developed and used throughout the program. These data are intended to be usable for photometric analysis of the various objects within the NEAT data. Most nights included calibration data, and the lists of photometric standard calibration fields.
• collection: data collection for the "TRIAD RADIOMETRIC DIAMETERS AND ALBEDOS " bundle
  This is the data collection for the compil.ast.triad.radiometry bundle. This data set reproduces the Tucson Revised Index of Asteroid Data (TRIAD) radiometric asteroid diameters and albedos tabulated in Morrison and Zellner (1979). Albedos and diameters for 195 asteroids are included.
• collection: data collection for the "UBV MEAN ASTEROID COLORS" bundle
  This is the data collection for the compil.ast.ubv-photometry bundle. This data set is a compilation of mean U-B and B-V color indices of asteroids, collected from the published literature and from the unpublished Lowell Observatory UBV Asteroid Survey.
• collection: data collection for the "METEOROID ORBITS" bundle
  This is the data collection for the meteoroid.steel.orbits bundle. This data set contains meteoroid orbits from photographic, TV system, and radar meteoroid surveys collected from the International Astronomical Union Meteor Data Center (IAU MDC) by Duncan Steel and reviewed and discussed in Steel (1996). The data cover the time period 1940-1983.
• collection: data collection for the "WISNIEWSKI ASTEROID ABSOLUTE MAGNITUDES " bundle
  This is the data collection for the gbo.ast.wisniewski.magnitudes bundle. Photometric observations of 125 asteroids, including absolute magnitudes, reported in Wisniewski et al. 1997.
• collection: McDonald Observatory Faint Comet Spectro-Photometric Survey (PDS4 Format)
  This study presents spectral data from 152 observations of 17 comets obtained using an Intensified Dissector Scanner spectrograph at the McDonald Observatory. A full description of these data and the reduction process, along with Haser model production rates can be found in Cochran et al. (1992). These data were migrated from the PDS3 dataset EAR-C-MCDIDS-3-RDR-MCDNLD-V1.0.
• collection: Visual Imaging and Photometry of (29981) 1999 TD10 V2.0
  The outer solar system object (29981) 1999 TD10 was observed in the R band in September 2001, and in B, V, R, and I in October 2002. We derive B-V=0.80+/-0.05mag, V-R=0.48+/-0.05mag, and R-I=0.44+/-0.05mag. Combining our data with the data from Rousselot et. al. 2003, we derive a synodic period of 15.382+/-0.001hr in agreement with the period from Rousselot et. al. 2003. Our observations show no evidence of a coma.
• collection: Asteroid Lightcurve Database (LCDB) V4.0
  The asteroid lightcurve database (LCDB) is one of the more widely-used research tools for those doing research that compares and contrasts physical characteristics of asteroid spin axis rates, sizes, pole orientations, and/or taxonomic class - among others. The v4.0 release includes lightcurve photometry results for 34967 targets. Each object has one to several dozen detail records that contain results obtained by reviewing the literature.
• collection: Catalina Sky Survey Bundle: Derived Data Collection
  Derived Data files for Catalina Sky Survey
• collection: Small Planetary Satellite Colors V1.0
  This data set is intended to include published colors of small planetary satellites published up through December 2003. Small planetary satellites are defined as all those except the Moon, the Galilean satellites, Titan, and Triton.
• bundle: Visual Imaging and Photometry of (29981) 1999 TD10 V2.0
  The outer solar system object (29981) 1999 TD10 was observed in the R band in September 2001, and in B, V, R, and I in October 2002. We derive B-V=0.80+/-0.05mag, V-R=0.48+/-0.05mag, and R-I=0.44+/-0.05mag. Combining our data with the data from Rousselot et. al. 2003, we derive a synodic period of 15.382+/-0.001hr in agreement with the period from Rousselot et. al. 2003. Our observations show no evidence of a coma.
• bundle: WISNIEWSKI ASTEROID ABSOLUTE MAGNITUDES
  Photometric observations of 125 asteroids, including absolute magnitudes, reported in Wisniewski et al. 1997.
• bundle: Zappala et al. (1995) Asteroid Dynamical Families V1.0
  Dynamical family classification of asteroids by Zappala et al., based on the hierarchical clustering method
• bundle: SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC
  These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B].
• bundle: SPECTROSCOPY AND PHOTOMETRY OF JUPITER TROJANS
  This data set contains the results of the visible spectroscopic and photometric survey of Jupiter Trojans reported in Fornasier et al. 2004 and Fornasier et al. 2007. The survey was carried out in the years 2002-2005 at the 3.5 m New Technology Telescope of the European Southern Observatory at La Silla, Chile. Included are visible spectroscopy and BVRI photometry of 73 Jupiter Trojans.
• bundle: Gartrelle et al. IRTF Asteroid Spectra V1.0
  This data set is comprised of the VNIR (0.69-2.5 micron) spectra of twenty-five D-type asteroids from varying Solar System locations. The spectra were obtained from NASA/IRTF on Mauna Kea between 2016-2019 using the SpeX instrument in Low-Resolution Prism mode and the 0.8 x 15" slit. Guiding was performed using spillover light from the slit (GuideDog) for targets with apparent magnitude > 15.5. For targets fainter than magnitude 15.5, guiding was accomplished using the MORIS CCD imager.
• bundle: Asteroid (101955) Bennu Radar Shape Model V1.1
  We present the three-dimensional shape of near-Earth asteroid (101955) Bennu (provisional designation 1999 RQ36) based on radar images and optical lightcurves (Nolan et al., 2013). Bennu was observed both in 1999 at its discovery apparition, and in 2005 using the 12.6-cm radar at the Arecibo Observatory and the 3.5-cm radar at the Goldstone tracking station. Data obtained in both apparitions were used to construct a shape model of this object. Observations were also obtained at many other wavelengths to characterize this object, some of which were used to further constrain the shape modeling (Clark et al., 2011; Hergenrother et al., 2013; Krugly et al., 1999).
• bundle: OPTICAL CONSTANTS AND LAB SPECTRA OF WATER ICE
  Transmission spectra of amorphous and crystalline H2O-ice at temperatures from 20-150 K for a wavelength range from 1.11 to 2.63 microns. These spectra have not been continuum-corrected or had the infrared interference fringes removed. Optical constants (n and k values) were derived from these laboratory spectra and are included in the data set.
• bundle: REDDY NEAR-EARTH AND MARS-CROSSING ASTEROIDS
  This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 27 asteroids, 5 Mars-crossing and 22 near-Earth asteroids, observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2008.
• bundle: REDDY VESTA ROTATIONALLY RESOLVED NEAR-INFRARED SPECTRA
  This data set contains low-resolution near-infrared (~0.7-2.5 microns) spectra of main belt asteroid (4) Vesta observed with the SpeX instrument on NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i, and reported in Reddy et al. (2011). This data set archives reduced, calibrated spectra that were obtained as part of ground-based characterization of Vesta prior to the arrival of Dawn spacecraft. They have been used for detailed rotationally-resolved mineralogical/compositional analysis.
• bundle: ASTEROID ABSOLUTE MAGNITUDES
  Absolute magnitudes and slopes, mostly IAU-adopted with exceptions noted, for all asteroids numbered as of the 2008 April 20 batch of Minor Planet Circulars.
• bundle: ASTEROID ALBEDOS
  This data set comprises a compilation of asteroid albedos for the convenience of the user. Most but not all of the albedos compiled here also appear in other PDS data sets.
• bundle: SDSS MOVING OBJECT CATALOG
  The Sloan Digital Sky Survey (SDSS) Moving Object Catalog 4th release lists astrometric and photometric data for moving objects detected in the SDSS. The catalog includes various identification parameters, SDSS astrometric measurements (five SDSS magnitudes and their errors), and orbital elements for previously cataloged asteroids. The data set also includes a list of the runs from which data are included, and filter response curves.
• bundle: 2MASS ASTEROID AND COMET SURVEY
  This data set includes J, H, and Ks magnitudes from the Two Micron All-Sky Survey (2MASS) for sources which were positionally associated with asteroids, comets, planets, and planetary satellites. This version includes the 2MASS Extended Mission.
• bundle: Fieber-Beyer IRTF Mainbelt Asteroid Spectra V2.0
  The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained by Sherry Fieber-Beyer.
• bundle: POLARIMETRY OF TRANSNEPTUNIAN OBJECTS AND CENTAURS
  The bundle contains a summary of polarimetric observations of Transneptunian objects (including Pluto-Charon system) and Centaurs published by March 19, 2013.
• bundle: Asteroid Polarimetric Database V2.0
  The Asteroid Polarimetric Database (APD) is a collection of asteroid polarimetry results compiled by D.F. Lupishko of Karazin Kharkiv National University, Ukraine. It is intended to include most asteroid polarimetry available through November 15, 2021.
• bundle: TNO AND CENTAUR COLORS
  This data set is intended to include published broadband colors of centaurs and Transneptunian Objects (TNOs) published through March 2014. It includes some comets with Centaur orbits. It supersedes all versions of the TNO colors data set EAR-A-3-RDR-TNO-PHOT.
• bundle: UBV MEAN ASTEROID COLORS
  This data set is a compilation of mean U-B and B-V color indices of asteroids, collected from the published literature and from the unpublished Lowell Observatory UBV Asteroid Survey.
• collection: data collection for the "POLARIMETRY OF TRANSNEPTUNIAN OBJECTS AND CENTAURS" bundle
  This is the data collection for the compil.tno-centaur.polarimetry bundle. The bundle contains a summary of polarimetric observations of Transneptunian objects (including Pluto-Charon system) and Centaurs published by March 19, 2013.
• collection: BINARY MINOR PLANETS V3.0
  The data set lists orbital and physical properties for well-observed or suspected binary/multiple minor planets including the Pluto system, compiled from the published literature as inspired by Richardson and Walsh (2006) and similar reviews (Merline et al., 2003; Noll, 2006; Pravec et al., 2006; Pravec and Harris, 2007; Descamps and Marchis, 2008; Noll et al., 2008; Walsh, 2009). In total 370 companions in 351 systems are included. Data are presented in three tables: one for orbital and physical properties; one for companion designations, discovery information, and reference codes for data values; and one giving full references for each reference code. This data set is complete for binary/multiple components reported through 31 March 2019.
• collection: Gaffey Meteorite Spectra V1.0
  This data set contains 166 laboratory spectra of 108 meteorite samples, as reported by M. J. Gaffey in Gaffey (1976) [GAFFEY1976]. This in turn was based on his PhD thesis work (Gaffey 1974 [GAFFEY1974]).
• collection: High Spectral Resolution Atlas of Comet 122P/deVico (PDS4 Format)
  This collection presents an atlas of 12,219 identified and 4,055 unidentified spectral lines from high resolution spectra of comet 122P/deVico. The spectra were obtained at the McDonald Observatory using the 2D Coude cross-dispersed echelle spectrograph (CS2) at the Coude f/32.5 focus of the 2.7m Harlan J. Smith telescope. These data were migrated from the PDS3 dataset EAR-C-CS2-5-RDR-DEVICO-ATLAS-V1.0.
• collection: data collection for the "SHAPE AND ROTATION OF (8567) 1996 HW1 " bundle
  This is the data collection for the gbo.ast-8567.radar.shape-model bundle. We present the three-dimensional shape and rotation state of near-Earth asteroid (8567) 1996 HW1 based on radar images and optical lightcurves (Magri et al., 2011). 1996 HW1 was observed in 2008 using the 12.6-cm radar at Arecibo Observatory. Optical lightcurves were obtained at several observatories and used to further constrain the shape modeling.
• collection: Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
  This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process.

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