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| Format: | Preprint |
| Published: |
2025
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| Online Access: | https://arxiv.org/abs/2504.16927 |
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| _version_ | 1866915483657175040 |
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| author | Ferreira, Feliphe S. Camargo, Julio I. B. Boufleur, Rodrigo Banda-Huarca, M. V. Pieres, Adriano Peixoto, Viviane F. Assafin, Marcelo Bernardinelli, P. H. Lin, H. W. Braga-Ribas, Felipe Gomes-Junior, Altair Vieira-Martins, Roberto da Costa, L. N. Abbott, T. M. C. Aguena, M. Allam, Sahar S. Alves, O. Annis, J. Bacon, D. Brooks, D. Burke, D. L. Rosell, A. Carneiro Carretero, J. Desai, S. Doel, P. Everett, S. Ferrero, I. Frieman, J. García-Bellido, J. Gatti, M. Gaztanaga, E. Giannini, G. Gruen, D. Gruendl, R. A. Herner, K. Hinton, S. R. Hollowood, D. L. Honscheid, K. James, D. J. Kuehn, K. Lee, S. Marshall, J. L. Mena-Fernández, J. Miquel, R. Myles, J. Palmese, A. Malagón, A. A. Plazas Pereira, M. E. S. Samuroff, S. Sanchez, E. Cid, D. Sanchez Servila-Noarbe, I. Smith, M. Suchyta, E. Swanson, M. E. C. Tarle, G. To, C. Tucker, D. L. de Vicente, J. Vikram, V. Walker, A. R. Weaverdyck, N. Collaboration, DES |
| author_facet | Ferreira, Feliphe S. Camargo, Julio I. B. Boufleur, Rodrigo Banda-Huarca, M. V. Pieres, Adriano Peixoto, Viviane F. Assafin, Marcelo Bernardinelli, P. H. Lin, H. W. Braga-Ribas, Felipe Gomes-Junior, Altair Vieira-Martins, Roberto da Costa, L. N. Abbott, T. M. C. Aguena, M. Allam, Sahar S. Alves, O. Annis, J. Bacon, D. Brooks, D. Burke, D. L. Rosell, A. Carneiro Carretero, J. Desai, S. Doel, P. Everett, S. Ferrero, I. Frieman, J. García-Bellido, J. Gatti, M. Gaztanaga, E. Giannini, G. Gruen, D. Gruendl, R. A. Herner, K. Hinton, S. R. Hollowood, D. L. Honscheid, K. James, D. J. Kuehn, K. Lee, S. Marshall, J. L. Mena-Fernández, J. Miquel, R. Myles, J. Palmese, A. Malagón, A. A. Plazas Pereira, M. E. S. Samuroff, S. Sanchez, E. Cid, D. Sanchez Servila-Noarbe, I. Smith, M. Suchyta, E. Swanson, M. E. C. Tarle, G. To, C. Tucker, D. L. de Vicente, J. Vikram, V. Walker, A. R. Weaverdyck, N. Collaboration, DES |
| contents | We identified known Trans-Neptunian Objects (TNOs) and Centaurs in the complete Dark Energy Survey (DES) year six catalog (DES Y6) through the Sky Body Tracker (SkyBoT) tool. We classified our dataset of 144 objects into a widely used 4-class taxonomic system of TNOs. No such previous classification was available in the literature for most of these objects. From absolute magnitudes and average albedos, an estimation of the diameters of all these objects is obtained. Correlations involving colours, orbital parameters, dynamical classes and sizes are also discussed. In particular, our largest reddest object has a diameter of $390^{+68}_{-53}$ km and our largest cold classical, $255^{+19}_{-17}$ km. Also, a weak correlation between colour and inclination is found within the population of resonant TNOs in addition to weak correlations between colour and phase slope in different bands. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2504_16927 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Year six photometric measurements of known Trans-Neptunian Objects and Centaurs by the Dark Energy Survey Ferreira, Feliphe S. Camargo, Julio I. B. Boufleur, Rodrigo Banda-Huarca, M. V. Pieres, Adriano Peixoto, Viviane F. Assafin, Marcelo Bernardinelli, P. H. Lin, H. W. Braga-Ribas, Felipe Gomes-Junior, Altair Vieira-Martins, Roberto da Costa, L. N. Abbott, T. M. C. Aguena, M. Allam, Sahar S. Alves, O. Annis, J. Bacon, D. Brooks, D. Burke, D. L. Rosell, A. Carneiro Carretero, J. Desai, S. Doel, P. Everett, S. Ferrero, I. Frieman, J. García-Bellido, J. Gatti, M. Gaztanaga, E. Giannini, G. Gruen, D. Gruendl, R. A. Herner, K. Hinton, S. R. Hollowood, D. L. Honscheid, K. James, D. J. Kuehn, K. Lee, S. Marshall, J. L. Mena-Fernández, J. Miquel, R. Myles, J. Palmese, A. Malagón, A. A. Plazas Pereira, M. E. S. Samuroff, S. Sanchez, E. Cid, D. Sanchez Servila-Noarbe, I. Smith, M. Suchyta, E. Swanson, M. E. C. Tarle, G. To, C. Tucker, D. L. de Vicente, J. Vikram, V. Walker, A. R. Weaverdyck, N. Collaboration, DES Earth and Planetary Astrophysics We identified known Trans-Neptunian Objects (TNOs) and Centaurs in the complete Dark Energy Survey (DES) year six catalog (DES Y6) through the Sky Body Tracker (SkyBoT) tool. We classified our dataset of 144 objects into a widely used 4-class taxonomic system of TNOs. No such previous classification was available in the literature for most of these objects. From absolute magnitudes and average albedos, an estimation of the diameters of all these objects is obtained. Correlations involving colours, orbital parameters, dynamical classes and sizes are also discussed. In particular, our largest reddest object has a diameter of $390^{+68}_{-53}$ km and our largest cold classical, $255^{+19}_{-17}$ km. Also, a weak correlation between colour and inclination is found within the population of resonant TNOs in addition to weak correlations between colour and phase slope in different bands. |
| title | Year six photometric measurements of known Trans-Neptunian Objects and Centaurs by the Dark Energy Survey |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2504.16927 |