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11 results on '"Eifler, T."'

1. A Deeper Look at DES Dwarf Galaxy Candidates: Grus i and Indus ii

Author

Cantu, Sarah A., primary, Pace, Andrew B., additional, Marshall, Jennifer, additional, Strigari, Louis E., additional, Crnojevic, Denija, additional, Simon, Joshua D., additional, Drlica-Wagner, A., additional, Bechtol, K., additional, Martínez-Vázquez, Clara E., additional, Santiago, B., additional, Amara, A., additional, Stringer, K. M., additional, Diehl, H. T., additional, Aguena, M., additional, Allam, S., additional, Avila, S., additional, Brooks, D., additional, Carnero Rosell, A., additional, Carrasco Kind, M., additional, Carretero, J., additional, Costanzi, M., additional, Da Costa, L. N., additional, De Vicente, J., additional, Desai, S., additional, Doel, P., additional, Eifler, T. F., additional, Everett, S., additional, Frieman, J., additional, García-Bellido, J., additional, Gaztanaga, E., additional, Gruen, D., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gutierrez, G., additional, Hinton, S. R., additional, Hollowood, D. L., additional, Honscheid, K., additional, James, D. J., additional, Kuehn, K., additional, Maia, M. A. G., additional, Menanteau, F., additional, Miquel, R., additional, Palmese, A., additional, Paz-Chinchón, F., additional, Plazas, A. A., additional, Sanchez, E., additional, Scarpine, V., additional, Schubnell, M., additional, Serrano, S., additional, Sevilla-Noarbe, I., additional, Smith, M., additional, Soares-Santos, M., additional, Suchyta, E., additional, Swanson, M. E. C., additional, Tarle, G., additional, Walker, A. R., additional, and Wilkinson, R. D., additional

Published
2021
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2. Constraints on the Physical Properties of GW190814 through Simulations Based on DECam Follow-up Observations by the Dark Energy Survey

Author

Morgan, R., primary, Soares-Santos, M., additional, Annis, J., additional, Herner, K., additional, Garcia, A., additional, Palmese, A., additional, Drlica-Wagner, A., additional, Kessler, R., additional, García-Bellido, J., additional, Bachmann, T. G., additional, Sherman, N., additional, Allam, S., additional, Bechtol, K., additional, Bom, C. R., additional, Brout, D., additional, Butler, R. E., additional, Butner, M., additional, Cartier, R., additional, Chen, H., additional, Conselice, C., additional, Cook, E., additional, Davis, T. M., additional, Doctor, Z., additional, Farr, B., additional, Figueiredo, A. L., additional, Finley, D. A., additional, Foley, R. J., additional, Galarza, J. Y., additional, Gill, M. S. S., additional, Gruendl, R. A., additional, Holz, D. E., additional, Kuropatkin, N., additional, Lidman, C., additional, Lin, H., additional, Malik, U., additional, Mann, A. W., additional, Marriner, J., additional, Marshall, J. L., additional, Martínez-Vázquez, C. E., additional, Meza, N., additional, Neilsen, E., additional, Nicolaou, C., additional, Olivares E., F., additional, Paz-Chinchón, F., additional, Points, S., additional, Quirola-Vásquez, J., additional, Rodriguez, O., additional, Sako, M., additional, Scolnic, D., additional, Smith, M., additional, Sobreira, F., additional, Tucker, D. L., additional, Vivas, A. K., additional, Wiesner, M., additional, Wood, M. L., additional, Yanny, B., additional, Zenteno, A., additional, Abbott, T. M. C., additional, Aguena, M., additional, Avila, S., additional, Bertin, E., additional, Bhargava, S., additional, Brooks, D., additional, Burke, D. L., additional, Rosell, A. Carnero, additional, Kind, M. Carrasco, additional, Carretero, J., additional, Costa, L. N. da, additional, Costanzi, M., additional, De Vicente, J., additional, Desai, S., additional, Diehl, H. T., additional, Doel, P., additional, Eifler, T. F., additional, Everett, S., additional, Flaugher, B., additional, Frieman, J., additional, Gaztanaga, E., additional, Gerdes, D. W., additional, Gruen, D., additional, Gschwend, J., additional, Gutierrez, G., additional, Hartley, W. G., additional, Hinton, S. R., additional, Hollowood, D. L., additional, Honscheid, K., additional, James, D. J., additional, Kuehn, K., additional, Lahav, O., additional, Lima, M., additional, Maia, M. A. G., additional, March, M., additional, Miquel, R., additional, Ogando, R. L. C., additional, Plazas, A. A., additional, Roodman, A., additional, Sanchez, E., additional, Scarpine, V., additional, Schubnell, M., additional, Serrano, S., additional, Sevilla-Noarbe, I., additional, Suchyta, E., additional, and Tarle, G., additional

Published
2020
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3. Steve: A Hierarchical Bayesian Model for Supernova Cosmology

Author

Hinton, S. R., primary, Davis, T. M., additional, Kim, A. G., additional, Brout, D., additional, D’Andrea, C. B., additional, Kessler, R., additional, Lasker, J., additional, Lidman, C., additional, Macaulay, E., additional, Möller, A., additional, Sako, M., additional, Scolnic, D., additional, Smith, M., additional, Wolf, R. C., additional, Childress, M., additional, Morganson, E., additional, Allam, S., additional, Annis, J., additional, Avila, S., additional, Bertin, E., additional, Brooks, D., additional, Burke, D. L., additional, Rosell, A. Carnero, additional, Kind, M. Carrasco, additional, Carretero, J., additional, Cunha, C. E., additional, Costa, L. N. da, additional, Davis, C., additional, Vicente, J. De, additional, DePoy, D. L., additional, Doel, P., additional, Eifler, T. F., additional, Flaugher, B., additional, Fosalba, P., additional, Frieman, J., additional, García-Bellido, J., additional, Gaztanaga, E., additional, Gerdes, D. W., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gutierrez, G., additional, Hartley, W. G., additional, Hollowood, D. L., additional, Honscheid, K., additional, Krause, E., additional, Kuehn, K., additional, Kuropatkin, N., additional, Lahav, O., additional, Lima, M., additional, Maia, M. A. G., additional, March, M., additional, Marshall, J. L., additional, Menanteau, F., additional, Miquel, R., additional, Ogando, R. L. C., additional, Plazas, A. A., additional, Sanchez, E., additional, Scarpine, V., additional, Schindler, R., additional, Schubnell, M., additional, Serrano, S., additional, Sevilla-Noarbe, I., additional, Soares-Santos, M., additional, Sobreira, F., additional, Suchyta, E., additional, Tarle, G., additional, Thomas, D., additional, Vikram, V., additional, and Zhang, Y., additional

Published
2019
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4. Mass Calibration of Optically Selected DES Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data

Author

Raghunathan, S., primary, Patil, S., additional, Baxter, E., additional, Benson, B. A., additional, Bleem, L. E., additional, Chou, T. L., additional, Crawford, T. M., additional, Holder, G. P., additional, McClintock, T., additional, Reichardt, C. L., additional, Rozo, E., additional, Varga, T. N., additional, Abbott, T. M. C., additional, Ade, P. A. R., additional, Allam, S., additional, Anderson, A. J., additional, Annis, J., additional, Austermann, J. E., additional, Avila, S., additional, Beall, J. A., additional, Bechtol, K., additional, Bender, A. N., additional, Bernstein, G., additional, Bertin, E., additional, Bianchini, F., additional, Brooks, D., additional, Burke, D. L., additional, Carlstrom, J. E., additional, Carretero, J., additional, Chang, C. L., additional, Chiang, H. C., additional, Cho, H-M., additional, Citron, R., additional, Crites, A. T., additional, Cunha, C. E., additional, Costa, L. N. da, additional, Davis, C., additional, Desai, S., additional, Diehl, H. T., additional, Dietrich, J. P., additional, Dobbs, M. A., additional, Doel, P., additional, Eifler, T. F., additional, Everett, W., additional, Evrard, A. E., additional, Flaugher, B., additional, Fosalba, P., additional, Frieman, J., additional, Gallicchio, J., additional, García-Bellido, J., additional, Gaztanaga, E., additional, George, E. M., additional, Gilbert, A., additional, Gruen, D., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gupta, N., additional, Gutierrez, G., additional, Haan, T. de, additional, Halverson, N. W., additional, Harrington, N., additional, Hartley, W. G., additional, Henning, J. W., additional, Hilton, G. C., additional, Hollowood, D. L., additional, Holzapfel, W. L., additional, Honscheid, K., additional, Hou, Z., additional, Hoyle, B., additional, Hrubes, J. D., additional, Huang, N., additional, Hubmayr, J., additional, Irwin, K. D., additional, James, D. J., additional, Jeltema, T., additional, Kim, A. G., additional, Kind, M. Carrasco, additional, Knox, L., additional, Kovacs, A., additional, Kuehn, K., additional, Kuropatkin, N., additional, Lee, A. T., additional, Li, T. S., additional, Lima, M., additional, Maia, M. A. G., additional, Marshall, J. L., additional, McMahon, J. J., additional, Melchior, P., additional, Menanteau, F., additional, Meyer, S. S., additional, Miller, C. J., additional, Miquel, R., additional, Mocanu, L., additional, Montgomery, J., additional, Nadolski, A., additional, Natoli, T., additional, Nibarger, J. P., additional, Novosad, V., additional, Padin, S., additional, Plazas, A. A., additional, Pryke, C., additional, Rapetti, D., additional, Romer, A. K., additional, Rosell, A. Carnero, additional, Ruhl, J. E., additional, Saliwanchik, B. R., additional, Sanchez, E., additional, Sayre, J. T., additional, Scarpine, V., additional, Schaffer, K. K., additional, Schubnell, M., additional, Serrano, S., additional, Sevilla-Noarbe, I., additional, Smecher, G., additional, Smith, R. C., additional, Soares-Santos, M., additional, Sobreira, F., additional, Stark, A. A., additional, Story, K. T., additional, Suchyta, E., additional, Swanson, M. E. C., additional, Tarle, G., additional, Thomas, D., additional, Tucker, C., additional, Vanderlinde, K., additional, Vicente, J. De, additional, Vieira, J. D., additional, Wang, G., additional, Whitehorn, N., additional, Wu, W. L. K., additional, and Zhang, Y., additional

Published
2019
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5. Chemical Abundance Analysis of Threeα-poor, Metal-poor Stars in the Ultrafaint Dwarf Galaxy Horologium I

Author

Nagasawa, D. Q., primary, Marshall, J. L., additional, Li, T. S., additional, Hansen, T. T., additional, Simon, J. D., additional, Bernstein, R. A., additional, Balbinot, E., additional, Drlica-Wagner, A., additional, Pace, A. B., additional, Strigari, L. E., additional, Pellegrino, C. M., additional, DePoy, D. L., additional, Suntzeff, N. B., additional, Bechtol, K., additional, Walker, A. R., additional, Abbott, T. M. C., additional, Abdalla, F. B., additional, Allam, S., additional, Annis, J., additional, Benoit-Lévy, A., additional, Bertin, E., additional, Brooks, D., additional, Rosell, A. Carnero, additional, Kind, M. Carrasco, additional, Carretero, J., additional, Cunha, C. E., additional, D’Andrea, C. B., additional, da Costa, L. N., additional, Davis, C., additional, Desai, S., additional, Doel, P., additional, Eifler, T. F., additional, Flaugher, B., additional, Fosalba, P., additional, Frieman, J., additional, García-Bellido, J., additional, Gaztanaga, E., additional, Gerdes, D. W., additional, Gruen, D., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gutierrez, G., additional, Hartley, W. G., additional, Honscheid, K., additional, James, D. J., additional, Jeltema, T., additional, Krause, E., additional, Kuehn, K., additional, Kuhlmann, S., additional, Kuropatkin, N., additional, March, M., additional, Miquel, R., additional, Nord, B., additional, Roodman, A., additional, Sanchez, E., additional, Santiago, B., additional, Scarpine, V., additional, Schindler, R., additional, Schubnell, M., additional, Sevilla-Noarbe, I., additional, Smith, M., additional, Smith, R. C., additional, Soares-Santos, M., additional, Sobreira, F., additional, Suchyta, E., additional, Tarle, G., additional, Thomas, D., additional, Tucker, D. L., additional, Wechsler, R. H., additional, Wolf, R. C., additional, and Yanny, B., additional

Published
2018
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6. Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993

Author

Palmese, A., primary, Hartley, W., additional, Tarsitano, F., additional, Conselice, C., additional, Lahav, O., additional, Allam, S., additional, Annis, J., additional, Lin, H., additional, Soares-Santos, M., additional, Tucker, D., additional, Brout, D., additional, Banerji, M., additional, Bechtol, K., additional, Diehl, H. T., additional, Fruchter, A., additional, García-Bellido, J., additional, Herner, K., additional, Levan, A. J., additional, Li, T. S., additional, Lidman, C., additional, Misra, K., additional, Sako, M., additional, Scolnic, D., additional, Smith, M., additional, Abbott, T. M. C., additional, Abdalla, F. B., additional, Benoit-Lévy, A., additional, Bertin, E., additional, Brooks, D., additional, Buckley-Geer, E., additional, Rosell, A. Carnero, additional, Kind, M. Carrasco, additional, Carretero, J., additional, Castander, F. J., additional, Cunha, C. E., additional, D’Andrea, C. B., additional, da Costa, L. N., additional, Davis, C., additional, DePoy, D. L., additional, Desai, S., additional, Dietrich, J. P., additional, Doel, P., additional, Drlica-Wagner, A., additional, Eifler, T. F., additional, Evrard, A. E., additional, Flaugher, B., additional, Fosalba, P., additional, Frieman, J., additional, Gaztanaga, E., additional, Gerdes, D. W., additional, Giannantonio, T., additional, Gruen, D., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gutierrez, G., additional, Honscheid, K., additional, Jain, B., additional, James, D. J., additional, Jeltema, T., additional, Johnson, M. W. G., additional, Johnson, M. D., additional, Krause, E., additional, Kron, R., additional, Kuehn, K., additional, Kuhlmann, S., additional, Kuropatkin, N., additional, Lima, M., additional, Maia, M. A. G., additional, March, M., additional, Marshall, J. L., additional, McMahon, R. G., additional, Menanteau, F., additional, Miller, C. J., additional, Miquel, R., additional, Neilsen, E., additional, Ogando, R. L. C., additional, Plazas, A. A., additional, Reil, K., additional, Romer, A. K., additional, Sanchez, E., additional, Schindler, R., additional, Smith, R. C., additional, Sobreira, F., additional, Suchyta, E., additional, Swanson, M. E. C., additional, Tarle, G., additional, Thomas, D., additional, Thomas, R. C., additional, Walker, A. R., additional, Weller, J., additional, Zhang, Y., additional, and Zuntz, J., additional

Published
2017
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7. 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

Author

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

Published
2017
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8. GALAXIES IN X-RAY SELECTED CLUSTERS AND GROUPS IN DARK ENERGY SURVEY DATA. I. STELLAR MASS GROWTH OF BRIGHT CENTRAL GALAXIES SINCEz∼ 1.2

Author

Zhang, Y., primary, Miller, C., additional, McKay, T., additional, Rooney, P., additional, Evrard, A. E., additional, Romer, A. K., additional, Perfecto, R., additional, Song, J., additional, Desai, S., additional, Mohr, J., additional, Wilcox, H., additional, Bermeo-Hernandez, A., additional, Jeltema, T., additional, Hollowood, D., additional, Bacon, D., additional, Capozzi, D., additional, Collins, C., additional, Das, R., additional, Gerdes, D., additional, Hennig, C., additional, Hilton, M., additional, Hoyle, B., additional, Kay, S., additional, Liddle, A., additional, Mann, R. G., additional, Mehrtens, N., additional, Nichol, R. C., additional, Papovich, C., additional, Sahlén, M., additional, Soares-Santos, M., additional, Stott, J., additional, Viana, P. T., additional, Abbott, T., additional, Abdalla, F. B., additional, Banerji, M., additional, Bauer, A. H., additional, Benoit-Lévy, A., additional, Bertin, E., additional, Brooks, D., additional, Buckley-Geer, E., additional, Burke, D. L., additional, Rosell, A. Carnero, additional, Castander, F. J., additional, Diehl, H. T., additional, Doel, P., additional, Cunha, C. E, additional, Eifler, T. F., additional, Neto, A. Fausti, additional, Fernandez, E., additional, Flaugher, B., additional, Fosalba, P., additional, Frieman, J., additional, Gaztanaga, E., additional, Gruen, D., additional, Gruendl, R. A., additional, Honscheid, K., additional, James, D., additional, Kuehn, K., additional, Kuropatkin, N., additional, Lahav, O., additional, Maia, M. A. G., additional, Makler, M., additional, Marshall, J. L., additional, Martini, Paul, additional, Miquel, R., additional, Ogando, R., additional, Plazas, A. A., additional, Roodman, A., additional, Rykoff, E. S., additional, Sako, M., additional, Sanchez, E., additional, Scarpine, V., additional, Schubnell, M., additional, Sevilla, I., additional, Smith, R. C., additional, Sobreira, F., additional, Suchyta, E., additional, Swanson, M. E. C., additional, Tarle, G., additional, Thaler, J., additional, Tucker, D., additional, Vikram, V., additional, and Costa, L. N. da, additional

Published
2016
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9. MODELING THE TRANSFER FUNCTION FOR THE DARK ENERGY SURVEY

Author

Chang, C., primary, Busha, M. T., additional, Wechsler, R. H., additional, Refregier, A., additional, Amara, A., additional, Rykoff, E., additional, Becker, M. R., additional, Bruderer, C., additional, Gamper, L., additional, Leistedt, B., additional, Peiris, H., additional, Abbott, T., additional, Abdalla, F. B., additional, Balbinot, E., additional, Banerji, M., additional, Bernstein, R. A., additional, Bertin, E., additional, Brooks, D., additional, Carnero, A., additional, Desai, S., additional, da Costa, L. N., additional, Cunha, C. E, additional, Eifler, T., additional, Evrard, A. E., additional, Fausti Neto, A., additional, Gerdes, D., additional, Gruen, D., additional, James, D., additional, Kuehn, K., additional, Maia, M. A. G., additional, Makler, M., additional, Ogando, R., additional, Plazas, A., additional, Sanchez, E., additional, Santiago, B., additional, Schubnell, M., additional, Sevilla-Noarbe, I., additional, Smith, C., additional, Soares-Santos, M., additional, Suchyta, E., additional, Swanson, M. E. C., additional, Tarle, G., additional, and Zuntz, J., additional

Published
2015
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10. Constraints on the Physical Properties of GW190814 through Simulations Based on DECam Follow-up Observations by the Dark Energy Survey

Author

G. Tarle, Alyssa Garcia, V. Scarpine, Samuel Hinton, Marcelle Soares-Santos, David J. Brooks, Z. Doctor, C. Lidman, Douglas L. Tucker, G. Gutierrez, N. Meza, B. Flaugher, Kyler Kuehn, A. Carnero Rosell, Alex Drlica-Wagner, D. L. Burke, Eric H. Neilsen, J. Carretero, U. Malik, Huanqing Chen, A. K. Vivas, C. Nicolaou, Tamara M. Davis, Jhon Yana Galarza, Enrique Gaztanaga, Michael Schubnell, M. Sako, David J. James, K. Honscheid, J. Gschwend, Antonella Palmese, D. L. Hollowood, S. Allam, Robert A. Gruendl, S. Serrano, Alfredo Zenteno, F. Paz-Chinchón, Richard Kessler, Sunayana Bhargava, Ryan J. Foley, Daniel Scolnic, Ken Herner, Marcos Lima, Andre Luiz Figueiredo, S. Desai, M. Smith, S. Avila, Jennifer L. Marshall, Peter Doel, T. F. Eifler, Edward R. Cook, Daniel Gruen, Daniel E. Holz, E. Suchyta, M. A. G. Maia, James Annis, Clecio R. Bom, H. T. Diehl, T. M. C. Abbott, Michel Aguena, R. E. Butler, M. Costanzi, Melissa Butner, J. P. Marriner, Josh Frieman, M. S. S. Gill, Mackenna L. Wood, M. Carrasco Kind, S. Everett, D. J. Brout, I. Sevilla-Noarbe, R. Cartier, E. J. Sanchez, D. W. Gerdes, C. J. Conselice, Huan Lin, Ben Farr, Ramon Miquel, N. Kuropatkin, C. E. Martínez-Vázquez, W. G. Hartley, L. N. da Costa, Brian Yanny, D. A. Finley, Nora Sherman, Sean D. Points, A. A. Plazas, J. De Vicente, Flavia Sobreira, M. March, M. Wiesner, Tristan Bachmann, R. L. C. Ogando, Juan Garcia-Bellido, E. Bertin, Andrew W. Mann, Ofer Lahav, Robert Morgan, A. Roodman, O. Rodriguez, Keith Bechtol, J. Quirola-Vásquez, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, National Science Foundation (US), National Aeronautics and Space Administration (US), Kavli Institute for Particle Astrophysics and Cosmology, Department of Energy (US), Higher Education Funding Council for England, Ministerio de Ciencia y Tecnología (España), University of Illinois, University of Chicago, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil), German Research Foundation, Ministerio de Economía y Competitividad (España), European Commission, University of California, University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (España), University of Edinburgh, University of Michigan, National Optical Astronomy Observatory (US), University of Nottingham, The Ohio State University, University of Pennsylvania, University of Sussex, Texas A&M University, Morgan, R., Soares-Santos, M., Annis, J., Herner, K., Garcia, A., Palmese, A., Drlica-Wagner, A., Kessler, R., Garcia-Bellido, J., Bachmann, T. G., Sherman, N., Allam, S., Bechtol, K., Bom, C. R., Brout, D., Butler, R. E., Butner, M., Cartier, R., Chen, H., Conselice, C., Cook, E., Davis, T. M., Doctor, Z., Farr, B., Figueiredo, A. L., Finley, D. A., Foley, R. J., Galarza, J. Y., Gill, M. S. S., Gruendl, R. A., Holz, D. E., Kuropatkin, N., Lidman, C., Lin, H., Malik, U., Mann, A. W., Marriner, J., Marshall, J. L., Martinez-Vazquez, C. E., Meza, N., Neilsen, E., Nicolaou, C., Olivares, F. E., Paz-Chinchon, F., Points, S., Quirola-Vasquez, J., Rodriguez, O., Sako, M., Scolnic, D., Smith, M., Sobreira, F., Tucker, D. L., Vivas, A. K., Wiesner, M., Wood, M. L., Yanny, B., Zenteno, A., Abbott, T. M. C., Aguena, M., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Rosell, A. C., Kind, M. C., Carretero, J., Costa, L. N. D., Costanzi, M., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Eifler, T. F., Everett, S., Flaugher, B., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Lima, M., Maia, M. A. G., March, M., Miquel, R., Ogando, R. L. C., Plazas, A. A., Roodman, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., and Tarle, G.

Subjects
Gravitational wave sources, Optical observation, Light curve classification, Astronomical simulations, 010504 meteorology & atmospheric sciences, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Kilonova, 7. Clean energy, 01 natural sciences, 0103 physical sciences, Binary star, Astrophysics::Solar and Stellar Astrophysics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Gravitational wave, Astronomy and Astrophysics, Light curve, Redshift, Galaxy, LIGO, Neutron star, 13. Climate action, Space and Planetary Science, Gravitational wave source, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

Full author list: R. Morgan, M. Soares-Santos, J. Annis, K. Herner, A. Garcia, A. Palmese, A. Drlica-Wagner, R. Kessler, J. García-Bellido, T. G. Bachmann, N. Sherman, S. Allam, K. Bechtol, C. R. Bom, D. Brout, R. E. Butler, M. Butner, R. Cartier, H. Chen, C. Conselice, E. Cook, T. M. Davis, Z. Doctor, B. Farr, A. L. Figueiredo, D. A. Finley, R. J. Foley, J. Y. Galarza, M. S. S. Gill, R. A. Gruendl, D. E. Holz, N. Kuropatkin, C. Lidman, H. Lin, U. Malik, A. W. Mann, J. Marriner, J. L. Marshall, C. E. Martínez-Vázquez N. Meza, E. Neilsen, C. Nicolaou, F. Olivares E., F. Paz-Chinchón, S. Points, J. Quirola-Vásquez, O. Rodriguez, M. Sako, D. Scolnic, M. Smith, F. Sobreira, D. L. Tucker, A. K. Vivas, M. Wiesner, M. L. Wood, B. Yanny, A. Zenteno, T. M. C. Abbott, M. Aguena, S. Avila, E. Bertin, S. Bhargava, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, L. N. da Costa, M. Costanzi, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, T. F. Eifler, S. Everett, B. Flaugher, J. Frieman, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, G. Gutierrez, W. G. Hartley, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, M. March, R. Miquel, R. L. C. Ogando, A. A. Plazas, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, E. Suchyta, and G. Tarle, On 2019 August 14, the LIGO and Virgo Collaborations detected gravitational waves from a black hole and a 2.6 solar mass compact object, possibly the first neutron star-black hole merger. In search of an optical counterpart, the Dark Energy Survey (DES) obtained deep imaging of the entire 90% confidence level localization area with Blanco/DECam 0, 1, 2, 3, 6, and 16 nights after the merger. Objects with varying brightness were detected by the DES Pipeline, and we systematically reduced the candidate counterparts through catalog matching, light-curve properties, host-galaxy photometric redshifts, Southern Astrophysical Research spectroscopic follow-up observations, and machine-learning-based photometric classification. All candidates were rejected as counterparts to the merger. To quantify the sensitivity of our search, we applied our selection criteria to full light-curve simulations of supernovae and kilonovae as they would appear in the DECam observations. Because the source class of the merger was uncertain, we utilized an agnostic, three-component kilonova model based on tidally disrupted neutron star (NS) ejecta properties to quantify our detection efficiency of a counterpart if the merger included an NS. We find that, if a kilonova occurred during this merger, configurations where the ejected matter is greater than 0.07 solar masses, has lanthanide abundance less than 10-8.56, and has a velocity between 0.18c and 0.21c are disfavored at the 2σ level. Furthermore, we estimate that our background reduction methods are capable of associating gravitational wave signals with a detected electromagnetic counterpart at the 4σ level in 95% of future follow-up observations., R. Morgan thanks the LSSTC Data Science Fellowship Program, which is funded by LSSTC, NSF Cybertraining Grant #1829740, the Brinson Foundation, and the Moore Foundation; his participation in the program has benefited this work. F. O.E. acknowledges support from the FONDECYT grant No. 1201223. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship Program under grant No. 1744555. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and AstroParticle Physics at The Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at UrbanaChampaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NFS’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. The UCSC team is supported in part by NASA grant NNG17PX03C, NSF grant AST-1815935, the Gordon & Betty Moore Foundation, the Heising-Simons Foundation, and by fellowships from the David and Lucile Packard Foundation to R.J.F. Based in part on observations at Cerro Tololo InterAmerican Observatory at NSFʼs NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, Inovação e Comunicações (MCTIC) da República Federativa do Brasil, the U.S. NSF’s NOIRLab, the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU). The DES data management system is supported by the National Science Foundation under grant Nos. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007- 2013), including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2). This paper has gone through internal review by the DES collaboration. This manuscript has been authored by the Fermi Research Alliance, LLC under Contract No. DE-AC02- 07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.

Published
2020
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11. Supernova Siblings: Assessing the Consistency of Properties of Type Ia Supernovae that Share the Same Parent Galaxies

Author

W. G. Hartley, V. Scarpine, N. E. Sommer, I. Sevilla-Noarbe, David J. Brooks, David J. James, G. Tarle, N. Kuropatkin, A. A. Plazas, Jennifer L. Marshall, Ramon Miquel, K. D. Eckert, Ryan J. Foley, T. N. Varga, L. N. da Costa, L. Kelsey, K. Kuehn, Karl Glazebrook, Lluís Galbany, C. Lidman, Samuel Hinton, Robert Morgan, Anais Möller, E. Bertin, E. Suchyta, Marcus Lima, G. Gutierrez, Edward Macaulay, P. Doel, Geraint F. Lewis, Alex Drlica-Wagner, M. Costanzi, J. Gschwend, D. J. Brout, Daniela Carollo, Salcedo Romero de Ávila, A. Massiah, T. F. Eifler, Tianjun Li, Michael Schubnell, P. Wiseman, J. Annis, Brodie Popovic, Joshua A. Frieman, T. M. C. Abbott, P. Fosalba, R. D. Wilkinson, M. Pursiainen, S. Everett, E. J. Sanchez, H. T. Diehl, K. Honscheid, M. Carrasco Kind, M. Sako, Robert C. Nichol, D. L. Hollowood, M. E. C. Swanson, B. Flaugher, S. Serrano, Richard Kessler, S. Desai, Enrique Gaztanaga, M. N. K. Smith, Mark Sullivan, Felipe Menanteau, K. Bechtol, Juan Garcia-Bellido, A. Carnero Rosell, A. R. Walker, J. De Vicente, Antonella Palmese, Daniel Gruen, D. L. Burke, M. A. G. Maia, Daniel Scolnic, B. P. Thomas, D. W. Gerdes, S. Allam, Robert A. Gruendl, B. E. Tucker, Michel Aguena, J. Carretero, R. Hounsell, Tamara M. Davis, F. Paz-Chinchón, Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), National Aeronautics and Space Administration (US), European Commission, European Research Council, Department of Energy (US), Ministerio de Economía y Competitividad (España), Generalitat de Catalunya, Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Scolnic, D., Smith, M., Massiah, A., Wiseman, P., Brout, D., Kessler, R., Davis, T. M., Foley, R. J., Galbany, L., Hinton, S. R., Hounsell, R., Kelsey, L., Lidman, C., Macaulay, E., Morgan, R., Nichol, R. C., Moller, A., Popovic, B., Sako, M., Sullivan, M., Thomas, B. P., Tucker, B. E., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bechtol, K., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. C., Carollo, D., Kind, M. C., Carretero, J., Costanzi Alunno Cerbolini, M., Da Costa, L. N., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Everett, S., Flaugher, B., Fosalba, P., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Glazebrook, K., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lewis, G. F., Li, T. S., Lima, M., Maia, M. A. G., Marshall, J. L., Menanteau, F., Miquel, R., Palmese, A., Paz-Chinchon, F., Plazas, A. A., Pursiainen, M., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sommer, N. E., Suchyta, E., Swanson, M. E. C., Tarle, G., Varga, T. N., Walker, A. R., and Wilkinson, R.

Subjects
Observational cosmology, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Type (model theory), 01 natural sciences, 7. Clean energy, Consistency (statistics), 0103 physical sciences, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Line (formation), Physics, Astronomy and Astrophysics, Light curve, Astrophysics - Astrophysics of Galaxies, Galaxy, Supernova, Distance modulus, 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Dark energy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

DES Collaboration: et al. arXiv:2002.00974v2, While many studies have shown a correlation between properties of the light curves of SNe Ia and properties of their host galaxies, it remains unclear what is driving these correlations. We introduce a new direct method to study these correlations by analyzing "parent" galaxies that host multiple SNe Ia "siblings." Here, we search the Dark Energy Survey SN sample, one of the largest samples of discovered SNe, and find eight galaxies that hosted two likely SNe Ia. Comparing the light-curve properties of these SNe and recovered distances from the light curves, we find no better agreement between properties of SNe in the same galaxy as any random pair of galaxies, with the exception of the SN light-curve stretch. We show at 2.8σ significance that at least one-half of the intrinsic scatter of SNe Ia distance modulus residuals is not from common host properties. We also discuss the robustness with which we could make this evaluation with LSST, which will find 100× more pairs of galaxies, and pave a new line of study on the consistency of SNe Ia in the same parent galaxies. Finally, we argue that it is unlikely that some of these SNe are actually single, lensed SN with multiple images., D.S. is supported by DOE grant DE-SC0010007, the David and Lucile Packard Foundation. D.S. and R.K. are supported in part by NASA under Contract No. NNG17PX03C issued through the WFIRST Science Investigation Teams Programme. D.B. and M.S. were supported by DOE grant DE-FOA0001358 and NSF grant AST-1517742. L.G. was funded by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 839090. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We are grateful for the support of the University of Chicago Research Computing Center for assistance with the calculations carried out in this work. R.F. is supported in part by NSF grants AST-1518052 and AST1815935, the Gordon & Betty Moore Foundation, the HeisingSimons Foundation, and by fellowships from the David and Lucile Packard Foundation, as well as the NASA contract above. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at UrbanaChampaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo InterAmerican Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under grant Nos. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015-71825, ESP2015-66861, FPA2015-68048, SEV2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2). We acknowledge support from EU/FP7-ERC grant No. 615929. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.

Published
2020
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