Impact of Systematic Modeling Uncertainties on Kilonova Property Estimation

Autor: D. Brethauer, D. Kasen, R. Margutti, R. Chornock

Publikováno v: The Astrophysical Journal, Vol 975, Iss 2, p 213 (2024)

The precise atomic structure and therefore the wavelength-dependent opacities of lanthanides are highly uncertain. This uncertainty introduces systematic errors in modeling transients like kilonovae and estimating key properties such as mass, charact

Externí odkaz: https://doaj.org/article/ff14d4c6f61349348b25123e2629cebf

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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

Autor: P. S. Cowperthwaite, E. Berger, V. A. Villar, B. D. Metzger, M. Nicholl, R. Chornock, P. K. Blanchard, W. Fong, R. Margutti, M. Soares-Santos, K. D. Alexander, S. Allam, J. Annis, D. Brout, D. A. Brown, R. E. Butler, H.-Y. Chen, H. T. Diehl, Z. Doctor, M. R. Drout, T. Eftekhari, B. Farr, D. A. Finley, R. J. Foley, J. A. Frieman, C. L. Fryer, J. García-Bellido, M. S. S. Gill, J. Guillochon, K. Herner, D. E. Holz, D. Kasen, R. Kessler, J. Marriner, T. Matheson, E. H. Neilsen, E. Quataert, A. Palmese, A. Rest, M. Sako, D. M. Scolnic, N. Smith, D. L. Tucker, P. K. G. Williams, E. Balbinot, J. L. Carlin, E. R. Cook, F. Durret, T. S. Li, P. A. A. Lopes, A. C. C. Lourenço, J. L. Marshall, G. E. Medina, J. Muir, R. R. Muñoz, M. Sauseda, D. J. Schlegel, L. F. Secco, A. K. Vivas, W. Wester, A. Zenteno, Y. Zhang, T. M. C. Abbott, M. Banerji, K. Bechtol, A. Benoit-Lévy, E. Bertin, E. Buckley-Geer, D. L. Burke, D. Capozzi, A. Carnero Rosell, M. Carrasco Kind, F. J. Castander, M. Crocce, C. E. Cunha, C. B. D’Andrea, L. N. da Costa, C. Davis, D. L. DePoy, S. Desai, J. P. Dietrich, A. Drlica-Wagner, T. F. Eifler, A. E. Evrard, E. Fernandez, B. Flaugher, P. Fosalba, E. Gaztanaga, D. W. Gerdes, T. Giannantonio, D. A. Goldstein, D. Gruen, R. A. Gruendl, G. Gutierrez, K. Honscheid, B. Jain, D. J. James, T. Jeltema, M. W. G. Johnson, M. D. Johnson, S. Kent, E. Krause, R. Kron, K. Kuehn, N. Nuropatkin, O. Lahav, M. Lima, H. Lin, M. A. G. Maia, M. March, P. Martini, R. G. McMahon, F. Menanteau, C. J. Miller, R. Miquel, J. J. Mohr, E. Neilsen, R. C. Nichol, R. L. C. Ogando, A. A. Plazas, N. Roe, A. K. Romer, A. Roodman, E. S. Rykoff, E. Sanchez, V. Scarpine, R. Schindler, M. Schubnell, I. Sevilla-Noarbe, M. Smith, R. C. Smith, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, R. C. Thomas, M. A. Troxel, V. Vikram, A. R. Walker, R. H. Wechsler, J. Weller, B. Yanny, J. Zuntz

Publikováno v: Astrophys.J.
Astrophys.J., 2017, 848 (2), pp.L17. 〈10.3847/2041-8213/aa8fc7〉
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 848 (2), pp.L17. ⟨10.3847/2041-8213/aa8fc7⟩
Astrophys.J., 2017, 848 (2), pp.L17. ⟨10.3847/2041-8213/aa8fc7⟩
NASA Astrophysics Data System
Cowperthwaite, P S, Berger, E, Villar, V A, Metzger, B D, Nicholl, M, Chornock, R, Blanchard, P K, Fong, W, Margutti, R, Soares-Santos, M, Alexander, K D, Allam, S, Annis, J, Brout, D, Brown, D A, Butler, R E, Chen, H-Y, Diehl, H T, Doctor, Z, Drout, M R, Eftekhari, T, Farr, B, Finley, D A, Foley, R J, Frieman, J A, Fryer, C L, García-Bellido, J, Gill, M S S, Guillochon, J, Herner, K, Holz, D E, Kasen, D, Kessler, R, Marriner, J, Matheson, T, E. H. Neilsen, J, Quataert, E, Palmese, A, Rest, A, Sako, M, Scolnic, D M, Smith, N, Tucker, D L, Williams, P K G, Balbinot, E, Carlin, J L, Cook, E R, Durret, F, Li, T S, Lopes, P A A, Lourenço, A C C, Marshall, J L, Medina, G E, Muir, J, Muñoz, R R, Sauseda, M, Schlegel, D J, Secco, L F, Vivas, A K, Wester, W, Zenteno, A, Zhang, Y, Abbott, T M C, Banerji, M, Bechtol, K, Benoit-Lévy, A, Bertin, E, Buckley-Geer, E, Burke, D L, Capozzi, D, Rosell, A C, Kind, M C, Castander, F J, Crocce, M, Cunha, C E, D'Andrea, C B, Costa, L N D, Davis, C, DePoy, D L, Desai, S, Dietrich, J P, Drlica-Wagner, A, Eifler, T F, Evrard, A E, Fernandez, E, Flaugher, B, Fosalba, P, Gaztanaga, E, Gerdes, D W, Giannantonio, T, Goldstein, D A, Gruen, D, Gruendl, R A, Gutierrez, G, Honscheid, K, Jain, B, James, D J, Jeltema, T, Johnson, M W G, Johnson, M D, Kent, S, Krause, E, Kron, R, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Lin, H, Maia, M A G, March, M, Martini, P, McMahon, R G, Menanteau, F, Miller, C J, Miquel, R, Mohr, J J, Neilsen, E, Nichol, R C, Ogando, R L C, Plazas, A A, Roe, N, Romer, A K, Roodman, A, Rykoff, E S, Sanchez, E, Scarpine, V, Schindler, R, Schubnell, M, Sevilla-Noarbe, I, Smith, M, Smith, R C, Sobreira, F, Suchyta, E, Swanson, M E C, Tarle, G, Thomas, D, Thomas, R C, Troxel, M A, Vikram, V, Walker, A R, Wechsler, R H, Weller, J, Yanny, B & Zuntz, J 2017, ' The electromagnetic counterpart of the binary neutron star merger LIGO/VIRGO GW170817. II. UV, optical, and near-IR light curves and comparison to kilonova models ', Astrophysical Journal Letters, vol. 848, no. 2 . https://doi.org/10.3847/2041-8213/aa8fc7

We present UV, optical, and NIR photometry of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo, the binary neutron star merger GW170817. Our data set extends from the discovery of the optical counterpart a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d0676037e50c0a51918a7cc2d26b651
https://hal.archives-ouvertes.fr/hal-01669860

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