Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM)

Publication: Research - peer-reviewJournal article – Annual report year: 2012

Standard

Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM). / Marciniak, A.; Bartczak, P.; Santana-Ros, T.; Michałowski, T.; Borczyk, W.; Fagas, M.; Hirsch, R.; Kamiński, K.; Kryszczyńska, A.; Kwiatkowski, T.; Polińska, M.; Sobkowiak, K.; Stasik, M.; Antonini, P.; Behrend, R.; Bembrick, C.; Bernasconi, L.; Colas, F.; Coloma, J.; Crippa, R.; Manzini, F.; Esseiva, N.; Santacana, G.; Wucher, H.; Fauvaud, M.; Fauvaud, S.; Ferreira, Desiree Della Monica; Hein Bertelsen, R.P.; Higgins, D.; Kajava, J.J.E.; Michałowski, J.; Michałowski, M.J.; Paschke, A.; Poncy, R.; Roy, R.; Starczewski, S.; Velichko, F.; Zafar, T.

In: Astronomy & Astrophysics, Vol. 545, A131, 2012.

Publication: Research - peer-reviewJournal article – Annual report year: 2012

Harvard

Marciniak, A, Bartczak, P, Santana-Ros, T, Michałowski, T, Borczyk, W, Fagas, M, Hirsch, R, Kamiński, K, Kryszczyńska, A, Kwiatkowski, T, Polińska, M, Sobkowiak, K, Stasik, M, Antonini, P, Behrend, R, Bembrick, C, Bernasconi, L, Colas, F, Coloma, J, Crippa, R, Manzini, F, Esseiva, N, Santacana, G, Wucher, H, Fauvaud, M, Fauvaud, S, Ferreira, DDM, Hein Bertelsen, RP, Higgins, D, Kajava, JJE, Michałowski, J, Michałowski, MJ, Paschke, A, Poncy, R, Roy, R, Starczewski, S, Velichko, F & Zafar, T 2012, 'Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM)' Astronomy & Astrophysics, vol 545, A131., 10.1051/0004-6361/201219542

APA

Marciniak, A., Bartczak, P., Santana-Ros, T., Michałowski, T., Borczyk, W., Fagas, M., ... Zafar, T. (2012). Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM). Astronomy & Astrophysics, 545, [A131]. 10.1051/0004-6361/201219542

CBE

Marciniak A, Bartczak P, Santana-Ros T, Michałowski T, Borczyk W, Fagas M, Hirsch R, Kamiński K, Kryszczyńska A, Kwiatkowski T, Polińska M, Sobkowiak K, Stasik M, Antonini P, Behrend R, Bembrick C, Bernasconi L, Colas F, Coloma J, Crippa R, Manzini F, Esseiva N, Santacana G, Wucher H, Fauvaud M, Fauvaud S, Ferreira DDM, Hein Bertelsen RP, Higgins D, Kajava JJE, Michałowski J, Michałowski MJ, Paschke A, Poncy R, Roy R, Starczewski S, Velichko F, Zafar T. 2012. Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM). Astronomy & Astrophysics. 545. Available from: 10.1051/0004-6361/201219542

MLA

Vancouver

Marciniak A, Bartczak P, Santana-Ros T, Michałowski T, Borczyk W, Fagas M et al. Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM). Astronomy & Astrophysics. 2012;545. A131. Available from: 10.1051/0004-6361/201219542

Author

Marciniak, A.; Bartczak, P.; Santana-Ros, T.; Michałowski, T.; Borczyk, W.; Fagas, M.; Hirsch, R.; Kamiński, K.; Kryszczyńska, A.; Kwiatkowski, T.; Polińska, M.; Sobkowiak, K.; Stasik, M.; Antonini, P.; Behrend, R.; Bembrick, C.; Bernasconi, L.; Colas, F.; Coloma, J.; Crippa, R.; Manzini, F.; Esseiva, N.; Santacana, G.; Wucher, H.; Fauvaud, M.; Fauvaud, S.; Ferreira, Desiree Della Monica; Hein Bertelsen, R.P.; Higgins, D.; Kajava, J.J.E.; Michałowski, J.; Michałowski, M.J.; Paschke, A.; Poncy, R.; Roy, R.; Starczewski, S.; Velichko, F.; Zafar, T. / Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM).

In: Astronomy & Astrophysics, Vol. 545, A131, 2012.

Publication: Research - peer-reviewJournal article – Annual report year: 2012

Bibtex

@article{fc5ac324b82b40a0a1e831fd3d798a6c,
title = "Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM)",
keywords = "Photometry, Radar imaging, Stars, Asteroids",
publisher = "E D P Sciences",
author = "A. Marciniak and P. Bartczak and T. Santana-Ros and T. Michałowski and W. Borczyk and M. Fagas and R. Hirsch and K. Kamiński and A. Kryszczyńska and T. Kwiatkowski and M. Polińska and K. Sobkowiak and M. Stasik and P. Antonini and R. Behrend and C. Bembrick and L. Bernasconi and F. Colas and J. Coloma and R. Crippa and F. Manzini and N. Esseiva and G. Santacana and H. Wucher and M. Fauvaud and S. Fauvaud and Ferreira, {Desiree Della Monica} and {Hein Bertelsen}, R.P. and D. Higgins and J.J.E. Kajava and J. Michałowski and M.J. Michałowski and A. Paschke and R. Poncy and R. Roy and S. Starczewski and F. Velichko and T. Zafar",
year = "2012",
doi = "10.1051/0004-6361/201219542",
volume = "545",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",

}

RIS

TY - JOUR

T1 - Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM)

A1 - Marciniak,A.

A1 - Bartczak,P.

A1 - Santana-Ros,T.

A1 - Michałowski,T.

A1 - Borczyk,W.

A1 - Fagas,M.

A1 - Hirsch,R.

A1 - Kamiński,K.

A1 - Kryszczyńska,A.

A1 - Kwiatkowski,T.

A1 - Polińska,M.

A1 - Sobkowiak,K.

A1 - Stasik,M.

A1 - Antonini,P.

A1 - Behrend,R.

A1 - Bembrick,C.

A1 - Bernasconi,L.

A1 - Colas,F.

A1 - Coloma,J.

A1 - Crippa,R.

A1 - Manzini,F.

A1 - Esseiva,N.

A1 - Santacana,G.

A1 - Wucher,H.

A1 - Fauvaud,M.

A1 - Fauvaud,S.

A1 - Ferreira,Desiree Della Monica

A1 - Hein Bertelsen,R.P.

A1 - Higgins,D.

A1 - Kajava,J.J.E.

A1 - Michałowski,J.

A1 - Michałowski,M.J.

A1 - Paschke,A.

A1 - Poncy,R.

A1 - Roy,R.

A1 - Starczewski,S.

A1 - Velichko,F.

A1 - Zafar,T.

AU - Marciniak,A.

AU - Bartczak,P.

AU - Santana-Ros,T.

AU - Michałowski,T.

AU - Borczyk,W.

AU - Fagas,M.

AU - Hirsch,R.

AU - Kamiński,K.

AU - Kryszczyńska,A.

AU - Kwiatkowski,T.

AU - Polińska,M.

AU - Sobkowiak,K.

AU - Stasik,M.

AU - Antonini,P.

AU - Behrend,R.

AU - Bembrick,C.

AU - Bernasconi,L.

AU - Colas,F.

AU - Coloma,J.

AU - Crippa,R.

AU - Manzini,F.

AU - Esseiva,N.

AU - Santacana,G.

AU - Wucher,H.

AU - Fauvaud,M.

AU - Fauvaud,S.

AU - Ferreira,Desiree Della Monica

AU - Hein Bertelsen,R.P.

AU - Higgins,D.

AU - Kajava,J.J.E.

AU - Michałowski,J.

AU - Michałowski,M.J.

AU - Paschke,A.

AU - Poncy,R.

AU - Roy,R.

AU - Starczewski,S.

AU - Velichko,F.

AU - Zafar,T.

PB - E D P Sciences

PY - 2012

Y1 - 2012

N2 - Context. The shapes and spin states of asteroids observed with photometric techniques can be reconstructed using the lightcurve inversion method. The resultant models can then be confirmed or exploited further by other techniques, such as adaptive optics, radar, thermal infrared, stellar occultations, or space probe imaging. Aims. During our ongoing work to increase the set of asteroids with known spin and shape parameters, there appeared a need for displaying the model plane-of-sky orientations for specific epochs to compare models from different techniques. It would also be instructive to be able to track how the complex lightcurves are produced by various asteroid shapes. Methods. Basing our analysis on an extensive photometric observational dataset, we obtained eight asteroid models with the convex lightcurve inversion method. To enable comparison of the photometric models with those from other observing/modelling techniques, we created an on-line service where we allow the inversion models to be orientated interactively. Results. Our sample of objects is quite representative, containing both relatively fast and slow rotators with highly and lowly inclined spin axes. With this work, we increase the sample of asteroid spin and shape models based on disk-integrated photometry to over 200. Three of the shape models obtained here are confirmed by the stellar occultation data; this also allowed independent determinations of their sizes to be made. Conclusions. The ISAM service can be widely exploited for past and future asteroid observations with various, complementary techniques and for asteroid dimension determination. © 2012 ESO.

AB - Context. The shapes and spin states of asteroids observed with photometric techniques can be reconstructed using the lightcurve inversion method. The resultant models can then be confirmed or exploited further by other techniques, such as adaptive optics, radar, thermal infrared, stellar occultations, or space probe imaging. Aims. During our ongoing work to increase the set of asteroids with known spin and shape parameters, there appeared a need for displaying the model plane-of-sky orientations for specific epochs to compare models from different techniques. It would also be instructive to be able to track how the complex lightcurves are produced by various asteroid shapes. Methods. Basing our analysis on an extensive photometric observational dataset, we obtained eight asteroid models with the convex lightcurve inversion method. To enable comparison of the photometric models with those from other observing/modelling techniques, we created an on-line service where we allow the inversion models to be orientated interactively. Results. Our sample of objects is quite representative, containing both relatively fast and slow rotators with highly and lowly inclined spin axes. With this work, we increase the sample of asteroid spin and shape models based on disk-integrated photometry to over 200. Three of the shape models obtained here are confirmed by the stellar occultation data; this also allowed independent determinations of their sizes to be made. Conclusions. The ISAM service can be widely exploited for past and future asteroid observations with various, complementary techniques and for asteroid dimension determination. © 2012 ESO.

KW - Photometry

KW - Radar imaging

KW - Stars

KW - Asteroids

U2 - 10.1051/0004-6361/201219542

DO - 10.1051/0004-6361/201219542

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

VL - 545

ER -