Search Results
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Catalina Sky Survey Bundle: Raw Data Collection
Raw Data files for Catalina Sky Survey -
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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. -
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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. -
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Small Bodies Occultations V4.0
Inventory of the document collection for the Small Bodies Occultations Bundle V4.0. -
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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). -
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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. -
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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. -
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Zappala et al. (1995) Asteroid Dynamical Families V1.0
Dynamical family classification of asteroids by Zappala et al., based on the hierarchical clustering method -
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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. -
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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. -
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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. -
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Catalina Sky Survey Bundle: Partially Processed Data Collection
Partially Processed Data files for Catalina Sky Survey -
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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. -
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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. -
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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). -
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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. -
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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. -
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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. -
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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. -
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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. -
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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. -
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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. -
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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. -
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Catalina Sky Survey Bundle: Derived Data Collection
Derived Data files for Catalina Sky Survey -
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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. -
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Small Bodies Occultations V4.0
Inventory of the data collection for the Small Bodies Occultations Bundle V4.0. -
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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. -
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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. -
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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]). -
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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. -
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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. -
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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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data collection for the "SDSS-BASED ASTEROID TAXONOMY" bundle
This is the data collection for the ast.sdss-based-taxonomy bundle. The Sloan Digital Sky Survey Moving Object Catalog (SDSS-MOC) is a large data set that provides five-filter magnitudes and astrometric information for all moving objects identified in the SDSS images (Izevic et al., 2010). The photometric observations were classified by Carvano et al. (2010) into nine taxonomic classes: Vp, Op, Qp, Sp, Ap, Lp, Dp, Xp and Cp, which are related to the classes and complexes of Bus Taxonomy (Bus & Binzel, 2002b). This data set is contains the taxonomic classification of each SDSS detections and its compilation for each observed asteroid. -
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data collection for the "EIGHT COLOR ASTEROID SURVEY" bundle
This is the data collection for the gbo.ast.ecas.phot bundle. This data set contains the reflectance spectra and associated data of the Eight Color Asteroid Survey (ECAS), including results for 589 asteroids. -
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Asteroid Photometric Catalog V1.0
This collection contains the documents applicable to the Asteroid Photometric Catalog bundle. -
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data collection for the "ASTEROID RADAR" bundle
This is the data collection for the compil.ast.radar-properties bundle. 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. -
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Radar shape models of asteroids compiled by Lawrence V1.0
This data set contains three-dimensional shape models for asteroids observed by ground-based radar facilities. The data set contains shape models for the following asteroids: (2100) Ra-Shalom (4486) Mithra (4660) Nereus (10115) 1992 SK (29075) 1950 DA (Retrograde and Prograde models) (33342) 1998 WT24 (54509) YORP (66391) 1999 KW4 Alpha (primary) and Beta (secondary) (136617) 1994 CC Alpha (primary) (276049) 2002 CE26 Alpha (primary) (341843) 2008 EV5 -
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data collection for the "NEAR-INFRARED PHOTOMETRY OF ASTEROIDS FROM DENIS" bundle
This is the data collection for the gbo.ast.denis.ir-photometry bundle. The DENIS program (Deep European Near-Infrared southern sky Survey) was a ground-based survey of the southern sky with the aim of providing an extensive I,J,Ks photometric catalog of point and extended sources. It was carried out at the 1.0 meter ESO telescope at La Silla, Chile from late 1995 through the end of 1999. This data set contains the DENIS I,J,Ks photometry for 2000 known asteroids identified in the DENIS catalog. -
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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. -
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data collection for the "REDDY NEAR-EARTH AND MARS-CROSSING ASTEROIDS" bundle
This is the data collection for the ast_spectra_reddy_neos_marscrossers bundle. 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. -
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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. -
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data collection for the "SDSS MOVING OBJECT CATALOG" bundle
This is the data collection for the gbo.sdss-moc.phot bundle. 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. -
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ALMA Ceres Imaging and Spectrum V1.0
This archive package contains the calibrated imaging and spectral data, as well as the integrated photometric (lightcurve) data of Ceres at about 1 mm wavelength obtained from the Atacama Large Millimeter/submillimeter Array (ALMA) in October - November 2015, September 2017, and October 2017. The imaging data were collected with the ALMA 12-meter array in all three epochs with Ceres spatially resolved into about 10, 15, and 15 beams, respectively, and have an average frequency of 265 GHz. Each epoch covers one full rotation of Ceres. The lightcurve data of Ceres were derived from the 12-meter images plus the ALMA Compact Array (ACA) data (effective frequency 259.39 GHz) obtained in the October 2017 epoch. The spectral data cover a frequency range of 256.636 - 266.136 GHz. -
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Compilation of Comet Polarimetry from Published and Unpublished Sources
This collection presents comet polarimetry results collected and tabulated from both published literature and unpublished sources. -
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Small Bodies Radar Shape Models V1.0
This data set contains radar-based shape models for small solar system bodies, prepared by various authors. -
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Sawyer Asteroid Spectra V1.0
This data set contains 94 optical asteroid spectra obtained by Scott Sawyer as part of his Ph.D. dissertation at the University of Texas at Austin. Observational circumstances and processing level are also provided. -
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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. -
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TNO AND CENTAUR DIAMETERS, ALBEDOS, AND DENSITIES V1.0
This data set is a compilation of published diameters, albedos, and densities for Transneptunian Objects (TNOs) and Centaurs. A total of 194 objects are listed, many with more than one entry. This version covers published values through 31 March 2018. -
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data collection for the "TORINO ASTEROID POLARIMETRY" bundle
This is the data collection for the gbo.ast.torino.polarimetry bundle. This data set contains asteroid polarimetric observations made during 1995-2005 with the Torino photopolarimeter at the 2.15-m telescope at El Leoncito Observatory in Argentina. These observations are reported in Cellino et al. (2005). -
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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]).
Data Sets and Information