adsabs/AstroCLIMB huggingface dataset:
Paper: The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis, K. Dziadura, M. Baes, J. M. Castro Cerón, G. Gentile, J. Hjorth, L. K. Hunt, C. K. Jespersen, M. P. Koprowski, E. Le Floc'h, H. Miraghaei, A. Nicuesa Guelbenzu, D. Oszkiewicz, E. Palazzi, M. Polińska, J. Rasmussen, P. Schady, D. Watson
Figure caption: GMRT interferometric spectrum (black dots) at three different resolutions and the single-dish spectrum (red dots; Theureau et al. 1998). The velocity axis is with respect to the redshift z = 0.01326.
Paper: The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis, K. Dziadura, M. Baes, J. M. Castro Cerón, G. Gentile, J. Hjorth, L. K. Hunt, C. K. Jespersen, M. P. Koprowski, E. Le Floc'h, H. Miraghaei, A. Nicuesa Guelbenzu, D. Oszkiewicz, E. Palazzi, M. Polińska, J. Rasmussen, P. Schady, D. Watson
Figure caption: Profiles of the atomic gas mass derived from the H I maps shown in Figure 1 as a function of distance from the galaxy center (top) and the rotation curve from the velocity field of H I (bottom). For both panels the galaxy center is marked as the red dashed line. The points on the top panel for which uncertainties are not shown represent upper limits.
Paper: The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis, K. Dziadura, M. Baes, J. M. Castro Cerón, G. Gentile, J. Hjorth, L. K. Hunt, C. K. Jespersen, M. P. Koprowski, E. Le Floc'h, H. Miraghaei, A. Nicuesa Guelbenzu, D. Oszkiewicz, E. Palazzi, M. Polińska, J. Rasmussen, P. Schady, D. Watson
Figure caption: (Left) Color-scale images of moment 0 maps of the GRB 111005A host detected by GMRT with three different resolutions from top to bottom: 16.″8 × 12.″9, 7.″4 × 5.″7, and 4.″0 × 2.″8 (the beams are shown as gray dotted ellipses). (Right) Color-scale images of the 1.4 GHz continuum emission of the GRB 111005A host at three different resolutions: 29.″7 × 22.″5 (top), 8.″4 × 6.″5 (middle), and 4.″7 × 3.″2 (bottom; the beams are shown as gray dotted ellipses).
Paper: The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis, K. Dziadura, M. Baes, J. M. Castro Cerón, G. Gentile, J. Hjorth, L. K. Hunt, C. K. Jespersen, M. P. Koprowski, E. Le Floc'h, H. Miraghaei, A. Nicuesa Guelbenzu, D. Oszkiewicz, E. Palazzi, M. Polińska, J. Rasmussen, P. Schady, D. Watson
Figure caption: Positions of regions analyzed in CO in Michałowski et al. (2018b, dotted circles) on our H I contours with a resolution of 7.″4 × 5.″7. The radii are 13.″6, corresponding to the beam size of the CO observations. These apertures were used to calculate the properties shown in Table 1.
Paper: The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis, K. Dziadura, M. Baes, J. M. Castro Cerón, G. Gentile, J. Hjorth, L. K. Hunt, C. K. Jespersen, M. P. Koprowski, E. Le Floc'h, H. Miraghaei, A. Nicuesa Guelbenzu, D. Oszkiewicz, E. Palazzi, M. Polińska, J. Rasmussen, P. Schady, D. Watson
Figure caption: Rotation curves from the tilted-ring modeling at two different resolutions as a function of distance from the galaxy center.
Paper: The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis, K. Dziadura, M. Baes, J. M. Castro Cerón, G. Gentile, J. Hjorth, L. K. Hunt, C. K. Jespersen, M. P. Koprowski, E. Le Floc'h, H. Miraghaei, A. Nicuesa Guelbenzu, D. Oszkiewicz, E. Palazzi, M. Polińska, J. Rasmussen, P. Schady, D. Watson
Figure caption: (Left) H I line emission of the GRB 111005A host (black contours) detected by GMRT with three different resolutions from top to bottom: 16.″8 × 12.″9, 7.″4 × 5.″7, and 4.″0 × 2.″8 (the beams are shown as gray dotted ellipses). The contours start at 0.7, 0.04, and 0.03 Jy beam−1 km s−1 from top to bottom. The lowest contours correspond to column densities of 3.7, 1.1, and 3.0 × 1021 cm2. The background is the UV image from Michałowski et al. (2018a). (Right) H I first-moment maps, with respect to the redshift z = 0.01326. The position of GRB 111005A is marked by the red arrow. The image size is 2.′5 × 2.′5 corresponding to 40.5 kpc × 40.5 kpc.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: The systems presented in this work, sorted by the algorithms that identified them. Left: a breakdown of the galaxy cluster subset, showing how many systems were identified in redMaPPer, ACT, and SPTPol ECS searches. Center: all 247 systems presented in this work. RNA and BNA include both the RNA and BNA searches, TI are systems found serendipitously in tile inspections, and Clusters includes redMaPPer, ACT, and SPTPol ECS catalogs. Right: all 81 newly identified systems presented in this work.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: An example of an SL candidate shown in the Target Viewer. The left panel is a list of cutouts and characteristics, such as the R.A. and decl. On the right side of the viewer is the optical image as well as some of the controls for manipulating the viewer. One cutout is displayed at a time, with an adjustable size of about 2′ on a side. In addition, the Target Viewer can access DES object catalogs and encircle the identified objects (not shown). Each circle can display useful information about the object, including the OBJECTID, which provides reference to the object in the respective data release.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: The footprints of the DES and other cluster catalogs referenced in this work. The DES redMaPPer catalogs span the DES footprint, outlined in black in the center. Searches were also conducted based on galaxy cluster catalogs from the SPTPol-ECS and ACT, whose footprints are shown in blue and orange, respectively. The background dust map was obtained from Planck Data Release 2. The overlap between the DES and ACT cluster footprints is approximately 4770 square degrees, and the overlap between the SPT and DES footprints is approximately 1510 square degrees. The intersection of all three footprints is approximately 1470 square degrees.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: In the visual data-quality test, we first displayed the full tile of DES data, 0.72 deg on each side (left). Then we zoomed-in a factor of 50–100 (in area) at roughly a dozen places on each tile, looking for problems noticeable in a cutout roughly 5′ on a side. If we noticed a potential SL candidate we recorded its position. The right side is about one-fourth of our typical zoomed-in area, but at the scale that we viewed it.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: Typical flowchart for the BNA and RNA search algorithms. The box with the dotted outline is a single computer program. At the last step within the program, “Y” and “N” stand for “yes” and “no.” The K > 2 subset selection was done on three of four of these searches.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: The binned distribution of Einstein radius estimates for the lens candidates. The cluster’s subset, as defined in Figure 6, is shown separately, and accounts for nearly all systems with an Einstein radius above 10″.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: The rank of all systems presented in this work. The solid black line shows all systems, the dashed line shows the galaxy cluster’s subset, and the dotted line shows newly discovered systems. The mean (median) rank of all systems presented is 6.12 (6).
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: DESDM-calculated photometric redshifts for the sources and lenses. As explained in Section 2, the redshifts of the sources are subject to larger uncertainties and systematic errors.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: The footprint of the DES. This result is based on searches of the DES Y3/Y6 footprint, outlined in black. Note that the DES Y3 footprint included additional observations of the Y1 and SV fields, and the Y6 footprint included additional observations in all of those.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: Eighth and last page of SL systems with a rank of 3 or more. Each cutout image has the visual inspection ranking displayed in a red box in the lower right corner. All images are oriented with north being the top, and east to the left. Each cutout is dynamically sized to fit the SL system well within the cutout, with a minimum size of 30″ × 30″. A 10″ long scale bar is displayed in the lower left corner. New SL systems are outlined with a gold border, previously known systems with white.
Paper: The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
Authors: J. H. O'Donnell, R. D. Wilkinson, H. T. Diehl, C. Aros-Bunster, K. Bechtol, S. Birrer, E. J. Buckley-Geer, A. Carnero Rosell, M. Carrasco Kind, L. N. da Costa, S. J. Gonzalez Lozano, R. A. Gruendl, M. Hilton, H. Lin, K. A. Lindgren, J. Martin, A. Pieres, E. S. Rykoff, I. Sevilla-Noarbe, E. Sheldon, C. Sifón, D. L. Tucker, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, J. De Vicente, S. Desai, J. P. Dietrich, K. Eckert, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, J. Gschwend, M. S. S. Gill, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, T. Jeltema, K. Kuehn, O. Lahav, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, B. Nord, R. L. C. Ogando, F. Paz-Chinchón, M. E. S. Pereira, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C. To, T. N. Varga
Figure caption: First page of SL systems with a rank of 3 or more. Each cutout image has the visual inspection ranking displayed in a red box in the lower right corner. All images are oriented with north being the top, and east to the left. Each cutout is dynamically sized to fit the SL system well within the cutout, with a minimum size of 30″ × 30″. A 10″ long scale bar is displayed in the lower left corner. New SL systems are outlined with a gold border, previously known systems with white.