J/A+A/658/A109      The SkyMapper DR3 SSOs                     (Sergeyev+, 2022)

Multifilter photometry of Solar System objects from the SkyMapper Southern Survey. Sergeyev A.V., Carry B., Onken C.A., Devillepoix H.A.R., Wolf C., Chang S.W. <Astron. Astrophys. 658, A109 (2022)> =2022A&A...658A.109S 2022A&A...658A.109S (SIMBAD/NED BibCode)
ADC_Keywords: Solar system ; Minor planets ; Comets ; Ephemerides ; Photometry ; Colors Keywords: minor planets, asteroids: general - catalogs Abstract: The populations of small bodies of the Solar System (asteroids, comets, and Kuiper Belt objects) are used to constrain the origin and evolution of the Solar System. Their orbital distribution and composition distribution are both required to track the dynamical pathway from their formation regions to their current locations. We aim to increase the sample of Solar System objects (SSOs) that have multifilter photometry and compositional taxonomy. Methods. We searched for moving objects in the SkyMapper Southern Survey. We used the predicted SSO positions to extract photometry and astrometry from the SkyMapper frames. We then applied a suite of filters to clean the catalog from false-positive detections. We finally used the near-simultaneous photometry to assign a taxonomic class to objects. We release a catalog of 880,528 individual observations, consisting of 205515 known and unique SSOs. The catalog completeness is estimated to be about 97% down to V=18mag and the purity is higher than 95% for known SSOs. The near-simultaneous photometry provides either three, two, or a single color that we use to classify 117356 SSOs with a scheme consistent with the widely used Bus-DeMeo taxonomy. The present catalog contributes significantly to the sample of asteroids with known surface properties (about 40% of main-belt asteroids down to an absolute magnitude of 16). We will release more observations of SSOs with future SkyMapper data releases. Description: There are four catalogs. 1. Taxonomy table contains the estimated taxonomy and orbital elements of asteroids (skm-taxo.dat. 2. The object table contains a single entry per SSO, with its average colors (skm-cobs.dat). 3. The color table contains all the measured SSO colors (skmcolor.dat). 4. The detection table contains 880528 observations of 205515 Solar System objects (asteroids, KBO, and comets) (skm-obs.dat). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file skm-taxo.dat 511 120566 Taxonomy table contains the estimated taxonomy and orbital elements of asteroids skm-cobs.dat 70 664349 Object table contains a single entry per SSO, with its average colors skmcolor.dat 65 388098 Color table contains all the measured SSO colors skm-obs.dat 190 880528 Detection table contains 880528 observations of 205515 Solar System objects (asteroids, KBO, and comets); updated version -------------------------------------------------------------------------------- Byte-by-byte Description of file: skm-taxo.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 7 I6 --- Number ? SSO IAU number 9- 24 A16 --- Name SSO IAU designation name 26- 44 A19 --- DynClass SSO dynamic class 46- 52 F7.4 mag u-v ? u-v color magnitude values 54- 59 F6.4 mag u-g ? u-g color magnitude values 61- 66 F6.4 mag u-r ? u-r color magnitude values 68- 73 F6.4 mag u-i ? u-i color magnitude values 75- 80 F6.4 mag u-z ? u-z color magnitude values 82- 87 F6.4 mag v-g ? v-g color magnitude values 89- 94 F6.4 mag v-r ? v-r color magnitude values 96-101 F6.4 mag v-i ? v-i color magnitude values 103-108 F6.4 mag v-z ? v-z color magnitude values 110-116 F7.4 mag g-r ? g-r color magnitude values 118-124 F7.4 mag g-i ? g-i color magnitude values 126-132 F7.4 mag i-z ? i-z color magnitude values 134-140 F7.4 mag g-z ? g-z color magnitude values 142-148 F7.4 mag r-i ? r-i color magnitude values 150-156 F7.4 mag r-z ? r-z color magnitude values 158-163 F6.4 mag e_u-v ? u-v color uncertainties 165-170 F6.4 mag e_u-g ? u-g color uncertainties 172-177 F6.4 mag e_u-r ? u-r color uncertainties 179-184 F6.4 mag e_u-i ? u-i color uncertainties 186-191 F6.4 mag e_u-z ? u-z color uncertainties 193-198 F6.4 mag e_v-g ? v-g color uncertainties 200-205 F6.4 mag e_v-r ? v-r color uncertainties 207-212 F6.4 mag e_v-i ? v-i color uncertainties 214-219 F6.4 mag e_v-z ? v-z color uncertainties 221-226 F6.4 mag e_g-r ? g-r color uncertainties 228-233 F6.4 mag e_g-i ? g-i color uncertainties 235-240 F6.4 mag e_i-z ? i-z color uncertainties 242-247 F6.4 mag e_g-z ? g-z color uncertainties 249-254 F6.4 mag e_r-i ? r-i color uncertainties 256-261 F6.4 mag e_r-z ? r-z color uncertainties 263-269 F7.4 d Du-v ? u-v time values between observations 271-277 F7.4 d Du-g ? u-g time values between observations 279-285 F7.4 d Du-r ? u-r time values between observations 287-293 F7.4 d Du-i ? u-i time values between observations 295-301 F7.4 d Du-z ? u-z time values between observations 303-309 F7.4 d Dv-g ? v-g time values between observations 311-317 F7.4 d Dv-r ? v-r time values between observations 319-325 F7.4 d Dv-i ? v-i time values between observations 327-333 F7.4 d Dv-z ? v-z time values between observations 335-341 F7.4 d Dg-r ? g-r time values between observations 343-349 F7.4 d Dg-i ? g-i time values between observations 351-357 F7.4 d Di-z ? i-z time values between observations 359-365 F7.4 d Dg-z ? g-z time values between observations 367-373 F7.4 d Dr-i ? r-i time values between observations 375-381 F7.4 d Dr-z ? r-z time values between observations 383-388 F6.3 --- pC ? Probability of C complex 390-394 F5.3 --- pS ? Probability of S complex 396-400 F5.3 --- pB ? Probability of B complex 402-407 F6.3 --- pL ? Probability of L complex 409-413 F5.3 --- pD ? Probability of D complex 415-419 F5.3 --- pK ? Probability of K complex 421-425 F5.3 --- pX ? Probability of X complex 427-431 F5.3 --- pQ ? Probability of Q complex 433-437 F5.3 --- pV ? Probability of V complex 439-443 F5.3 --- pA ? Probability of A complex 445-449 F5.3 --- pU ? Probability of Unknown complex 457 A1 --- complex The most probably complex 463-467 F5.3 --- pcomplex ? Probability value of the complex 475-476 A2 --- complex1 First the most probably complex 484-485 A2 --- complex2 Second the most probably complex 492-496 F5.3 --- pcomplex1 ? Probability of first the most probably complex 502-507 F6.3 --- pcomplex2 ? Probability of second the most probably complex 511 I1 --- nc ? The taxonomy priority number based on used colors -------------------------------------------------------------------------------- Byte-by-byte Description of file: skm-cobs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 7 I6 --- Number ? SSO IAU number 9- 24 A16 --- Name SSO IAU designation name 26- 39 F14.6 d JD Average epoch of observation 43- 45 A3 --- Color Name of color (e.g., "u-v", "g-r", etc. ) 47- 53 F7.4 mag color Magnitude value of the color 55- 60 F6.4 mag e_color Uncertainty on the color measurments 62- 70 F9.6 d dMJD Time difference between color measurements -------------------------------------------------------------------------------- Byte-by-byte Description of file: skmcolor.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 7 A6 --- Number SSO IAU number 9- 24 A16 --- Name SSO IAU designation name 28- 30 A3 --- Color Name of color (e.g., "u-v", "g-r", etc. ) 32- 38 F7.4 mag wcolor Weighted value of the color 40- 45 F6.4 mag e_wcolor ?=- Weighted uncertainty of the color measurements 47- 48 I2 --- N Number of color measurements, 0 - computed 50- 55 F6.4 mag e_color Uncertainty on the color measurments 57- 65 F9.6 d dMJD ?=- Time difference between color measurements -------------------------------------------------------------------------------- Byte-by-byte Description of file: skm-obs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 I10 --- Source Source unique identifier 12- 25 I14 --- Frame Image unique identifier 27- 40 F14.6 d JD Julian Date of observation 47 A1 --- Filter Filter name (u,v,g,r,i,z) 54- 56 I3 s Exptime Exposure time 58- 67 F10.6 deg RAdeg Right Ascension (J2000) 69- 78 F10.6 deg DEdeg Declination (J2000) 80- 86 F7.4 mag psfmag PSF magnitude 92- 97 F6.4 mag e_psfmag PSF magnitude uncertainty 101-107 F7.4 mag petromag ?=- Petrosian magnitude 114-120 F7.4 mag e_petromag ?=- Petrosian magnitude uncertainty 123-128 A6 --- Number SSO IAU number 130-145 A16 --- Name SSO IAU designation name 147-165 A19 --- DynClass SSO dynamical class 167-175 F9.4 arcsec/h RArate RA cos(DEC) rate of motion 178-185 F8.3 arcsec/h DErate DEC rate of motion 187-190 F4.1 mag Vmag Predicted visual magnitude -------------------------------------------------------------------------------- Acknowledgements: This research has been conducted within the NEOROCKS project, which has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 870403. CAO was supported by the Australian Research Council (ARC) through Discovery Project DP190100252. SWC acknowledges support from the National Research Foundation of Korea (NRF) grant, No.2020R1A2C3011091, funded by the Korea government (MSIT). We thank J. Berthier, F. Spoto, M. Mahlke for discussions related to the present article. The national facility capability for SkyMapper has been funded through ARC LIEF grant LE130100104 from the Australian Research Council, awarded to the University of Sydney, the Australian National University, Swinburne University of Technology, the University of Queensland, the University of Western Australia, the University of Melbourne, Curtin University of Technology, Monash University and the Australian Astronomical Observatory. SkyMapper is owned and operated by The Australian National University's Research School of Astronomy and Astrophysics. The survey data were processed and provided by the SkyMapper Team at ANU. The SkyMapper node of the All-Sky Virtual Observatory (ASVO) is hosted at the National Computational Infrastructure (NCI). Development and support of the SkyMapper node of the ASVO has been funded in part by Astronomy Australia Limited (AAL) and the Australian Government through the Commonwealth's Education Investment Fund (EIF) and National Collaborative Research Infrastructure Strategy (NCRIS), particularly the National eResearch Collaboration Tools and Resources (NeCTAR) and the Australian National Data Service Projects (ANDS). The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation. This research made use of the cross-match service provided by CDS, Strasbourg (Pineau et al., 2017A&A...597A..89P 2017A&A...597A..89P), the IMCCE's skybot and Skybot3D VO tools (Berthier et al., 2006ASPC..351..367B 2006ASPC..351..367B, 2016MNRAS.458.3394B 2016MNRAS.458.3394B), the JPL Horizons system (Giorgini et al., 1996DPS....28.2504G 1996DPS....28.2504G ), the SVO Filter Profile Service (http://svo2.cab.inta-csic.es/theory/ fps/) supported from the Spanish MINECO through grant AYA2017-84089 (Rodrigo et al., 2012, SVO Filter Profile Service Version 1.0, Tech. rep.), and TOPCAT/STILTS (Taylor, 2005ASPC..347...29T 2005ASPC..347...29T ). Thanks to the developpers. History: From Alexey Sergeyev, alexey.v.sergeyev(at)gmail.com 18-May-2022:Insert into VizieR 22-Feb-2023: Misprint in JD column for table skm-obs.dat corrected (third digit was "9" instead of "5")
(End) Patricia Vannier [CDS] 17-Jan-2022
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