Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results

Peter Vereš; Robert Jedicke; Alan Fitzsimmons; Larry Denneau; Mikael Granvik; Bryce Bolin; Serge Chastel; Richard J. Wainscoat; William S. Burgett; Kenneth C. Chambers; Heather Flewelling; Nick Kaiser; Eugen A. Magnier; Jeff S. Morgan; Paul A. Price; John L. Tonry; Christopher Waters

doi:10.1016/j.icarus.2015.08.007

Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results

Peter Vereš, Robert Jedicke, Alan Fitzsimmons, Larry Denneau, Mikael Granvik, Bryce Bolin, Serge Chastel, Richard J. Wainscoat, William S. Burgett, Kenneth C. Chambers, Heather Flewelling, Nick Kaiser, Eugen A. Magnier, Jeff S. Morgan, Paul A. Price, John L. Tonry, Christopher Waters

Research output: Contribution to journal › Article › peer-review

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Abstract

We present the results of a Monte Carlo technique to calculate the absolute magnitudes (H) and slope parameters (G) of about 240,000 asteroids observed by the Pan-STARRS1 telescope during the first 15 months of its 3-year all-sky survey mission. The system's exquisite photometry with photometric errors asteroids rotation period, amplitude and color to derive the most-likely H and G, but its major advantage is in estimating realistic statistical+systematic uncertainties and errors on each parameter. The method was confirmed by comparison with the well-established and accurate results for about 500 asteroids provided by Pravec et al. (2012) and then applied to determining H and G for the Pan-STARRS1 asteroids using both the Muinonen et al. (2010) and Bowell et al. (1989) phase functions. Our results confirm the bias in MPC photometry discovered by ( Jurić et al., 2002).

Original language	English
Pages (from-to)	34-47
Number of pages	14
Journal	Icarus
Volume	261
Early online date	13 Aug 2015
DOIs	https://doi.org/10.1016/j.icarus.2015.08.007
Publication status	Published - 15 Nov 2015

Bibliographical note

13 figures, 7 tables

Keywords

astro-ph.EP

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10.1016/j.icarus.2015.08.007

Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results.
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Alan Fitzsimmons
- A.Fitzsimmons@qub.ac.uk
- School of Mathematics and Physics - Professor
- Astrophysics Research Centre (ARC)
Person: Academic

Cite this

Vereš, P., Jedicke, R., Fitzsimmons, A., Denneau, L., Granvik, M., Bolin, B., Chastel, S., Wainscoat, R. J., Burgett, W. S., Chambers, K. C., Flewelling, H., Kaiser, N., Magnier, E. A., Morgan, J. S., Price, P. A., Tonry, J. L., & Waters, C. (2015). Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results. Icarus, 261, 34-47. https://doi.org/10.1016/j.icarus.2015.08.007

Vereš, Peter ; Jedicke, Robert ; Fitzsimmons, Alan ; Denneau, Larry ; Granvik, Mikael ; Bolin, Bryce ; Chastel, Serge ; Wainscoat, Richard J. ; Burgett, William S. ; Chambers, Kenneth C. ; Flewelling, Heather ; Kaiser, Nick ; Magnier, Eugen A. ; Morgan, Jeff S. ; Price, Paul A. ; Tonry, John L. ; Waters, Christopher. / Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results. In: Icarus. 2015 ; Vol. 261. pp. 34-47.

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title = "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results",

abstract = "We present the results of a Monte Carlo technique to calculate the absolute magnitudes (H) and slope parameters (G) of about 240,000 asteroids observed by the Pan-STARRS1 telescope during the first 15 months of its 3-year all-sky survey mission. The system's exquisite photometry with photometric errors asteroids rotation period, amplitude and color to derive the most-likely H and G, but its major advantage is in estimating realistic statistical+systematic uncertainties and errors on each parameter. The method was confirmed by comparison with the well-established and accurate results for about 500 asteroids provided by Pravec et al. (2012) and then applied to determining H and G for the Pan-STARRS1 asteroids using both the Muinonen et al. (2010) and Bowell et al. (1989) phase functions. Our results confirm the bias in MPC photometry discovered by ( Juri{\'c} et al., 2002).",

keywords = "astro-ph.EP",

author = "Peter Vere{\v s} and Robert Jedicke and Alan Fitzsimmons and Larry Denneau and Mikael Granvik and Bryce Bolin and Serge Chastel and Wainscoat, {Richard J.} and Burgett, {William S.} and Chambers, {Kenneth C.} and Heather Flewelling and Nick Kaiser and Magnier, {Eugen A.} and Morgan, {Jeff S.} and Price, {Paul A.} and Tonry, {John L.} and Christopher Waters",

note = "13 figures, 7 tables",

year = "2015",

month = nov,

day = "15",

doi = "10.1016/j.icarus.2015.08.007",

language = "English",

volume = "261",

pages = "34--47",

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Vereš, P, Jedicke, R, Fitzsimmons, A, Denneau, L, Granvik, M, Bolin, B, Chastel, S, Wainscoat, RJ, Burgett, WS, Chambers, KC, Flewelling, H, Kaiser, N, Magnier, EA, Morgan, JS, Price, PA, Tonry, JL & Waters, C 2015, 'Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results', Icarus, vol. 261, pp. 34-47. https://doi.org/10.1016/j.icarus.2015.08.007

Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results. / Vereš, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; Chastel, Serge; Wainscoat, Richard J.; Burgett, William S.; Chambers, Kenneth C.; Flewelling, Heather; Kaiser, Nick; Magnier, Eugen A.; Morgan, Jeff S.; Price, Paul A.; Tonry, John L.; Waters, Christopher.

In: Icarus, Vol. 261, 15.11.2015, p. 34-47.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results

AU - Vereš, Peter

AU - Jedicke, Robert

AU - Fitzsimmons, Alan

AU - Denneau, Larry

AU - Granvik, Mikael

AU - Bolin, Bryce

AU - Chastel, Serge

AU - Wainscoat, Richard J.

AU - Burgett, William S.

AU - Chambers, Kenneth C.

AU - Flewelling, Heather

AU - Kaiser, Nick

AU - Magnier, Eugen A.

AU - Morgan, Jeff S.

AU - Price, Paul A.

AU - Tonry, John L.

AU - Waters, Christopher

N1 - 13 figures, 7 tables

PY - 2015/11/15

Y1 - 2015/11/15

N2 - We present the results of a Monte Carlo technique to calculate the absolute magnitudes (H) and slope parameters (G) of about 240,000 asteroids observed by the Pan-STARRS1 telescope during the first 15 months of its 3-year all-sky survey mission. The system's exquisite photometry with photometric errors asteroids rotation period, amplitude and color to derive the most-likely H and G, but its major advantage is in estimating realistic statistical+systematic uncertainties and errors on each parameter. The method was confirmed by comparison with the well-established and accurate results for about 500 asteroids provided by Pravec et al. (2012) and then applied to determining H and G for the Pan-STARRS1 asteroids using both the Muinonen et al. (2010) and Bowell et al. (1989) phase functions. Our results confirm the bias in MPC photometry discovered by ( Jurić et al., 2002).

AB - We present the results of a Monte Carlo technique to calculate the absolute magnitudes (H) and slope parameters (G) of about 240,000 asteroids observed by the Pan-STARRS1 telescope during the first 15 months of its 3-year all-sky survey mission. The system's exquisite photometry with photometric errors asteroids rotation period, amplitude and color to derive the most-likely H and G, but its major advantage is in estimating realistic statistical+systematic uncertainties and errors on each parameter. The method was confirmed by comparison with the well-established and accurate results for about 500 asteroids provided by Pravec et al. (2012) and then applied to determining H and G for the Pan-STARRS1 asteroids using both the Muinonen et al. (2010) and Bowell et al. (1989) phase functions. Our results confirm the bias in MPC photometry discovered by ( Jurić et al., 2002).

KW - astro-ph.EP

U2 - 10.1016/j.icarus.2015.08.007

DO - 10.1016/j.icarus.2015.08.007

M3 - Article

VL - 261

SP - 34

EP - 47

JO - Icarus

JF - Icarus

SN - 0019-1035

ER -