Data Set Information
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| DATA_SET_NAME |
2MASS ASTEROID AND COMET SURVEY V1.0
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| DATA_SET_ID |
EAR-A-I0054/I0055-5-2MASS-V1.0
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| NSSDC_DATA_SET_ID |
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| DATA_SET_TERSE_DESCRIPTION |
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| DATA_SET_DESCRIPTION |
Data Set Overview : The Two Micron All-Sky Survey (2MASS) carried out a survey of the entire sky at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns) during the years 1997-2001. The survey was conducted by two nearly identical telescopes and instruments, one at the Whipple Observatory on Mt. Hopkins, in Arizona, and one at the Cerro Tololo Interamerican Observatory on Cerro Tololo in Chile. A single data processing pipeline was used for the entire survey. Some of the sources detected in 2MASS were positionally associated with known solar system bodies. There were 15,964 associations with 12,219 asteroids, 46 associations with 39 known comets, 3 associations with 3 planets, and 14 associations with 10 planetary satellites. The 2MASS data on these sources, including J, H, and Ks magnitudes, are in the three data files of this data set. Data files also include the positional, orbital, and brightness data used to make the associations, flags indicating the quality and processing status of each entry, and internal designations allowing cross-reference of the sources to the 2MASS Point Source Catalog and Extended Source Catalog. Orbital elements used to predict the positions of the asteroids, comets, planets, and satellites is given in the data files in the form of p and q position vectors. Detection of unknown solar system bodies in the 2MASS data is technically possible, but has not been carried out for this data set. Further documentation of the 2MASS survey can be found at: Cutri, R.M., et al. 2004. Explanatory Supplement to the 2MASS All Sky Data Release. http://www.ipac.caltech.edu/2mass/releases/allsky/doc. Sykes, M.V., R.M. Cutri, J.W. Fowler, D.J. Tholen, M.F. Skrutskie, S. Price, and E.F. Tedesco 2000. The 2MASS asteroid and comet survey. Icarus 146, 161-175.
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| DATA_SET_RELEASE_DATE |
2005-06-16T00:00:00.000Z
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| START_TIME |
1997-06-07T12:00:00.000Z
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| STOP_TIME |
2001-02-15T12:00:00.000Z
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| MISSION_NAME |
SUPPORT ARCHIVES
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| MISSION_START_DATE |
2004-03-22T12:00:00.000Z
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| MISSION_STOP_DATE |
N/A (ongoing)
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| TARGET_NAME |
ASTEROID
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| TARGET_TYPE |
ASTEROID
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| INSTRUMENT_HOST_ID |
OBS055T6
OBS320T13
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| INSTRUMENT_NAME |
2MASS CAMERA - NORTH
2MASS CAMERA - SOUTH
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| INSTRUMENT_ID |
I0054
I0055
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| INSTRUMENT_TYPE |
IMAGER
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| NODE_NAME |
Small Bodies
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| ARCHIVE_STATUS |
SUPERSEDED
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| CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview : Because the association of asteroid positions and 2MASS sources is blind, there is always the chance of association with background astrophysical sources, particularly at low galactic latitudes. Stars near the galactic plane will tend to be reddened by foreground dust, giving rise to a redward spike in the (J-H) (H-Ks) color-color plot. Contamination from galactic stars in the 2MASS asteroid associations is shown by such a redward spike in the color-color plot of the asteroid associations. For further discussion of the contamination problem, see [SYKESETAL2002]: Sykes, M.V., R.M. Cutri, J.M. Fowler, B. Nelson, D.J. Tholen, M.F. Skrutskie, and S. Price, 2MASS observations of the solar system, in the Proceedings of Asteroids, Comets, Meteors (ACM 2002), Technical University Berlin, Berlin, Germany, pp. 484-484, 2002. The confidence level of the positional association of sources with solar system bodies and of the photometric and astrometric measurements is indicated by flags within the data tables. These flags are defined in the file flagdef.txt in the document directory of the data set.
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| CITATION_DESCRIPTION |
Sykes, M.V., Cutri, R,M., Skrutskie, M.F., Fowler, J.W., Tholen, D.J., Painter, P.E., Nelson, B., and Kirkpatrick, D.J., 2MASS Asteroid and Comet Survey V1.0. EAR-A-I0054/I0055-5-2MASS-V1.0. NASA Planetary Data System, 2005.
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| ABSTRACT_TEXT |
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.
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| PRODUCER_FULL_NAME |
CAROL NEESE
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| SEARCH/ACCESS DATA |
SBN PSI WEBSITE
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