Quasar Accretion Disk Sizes from Continuum Reverberation Mapping in the DES Standard-star Fields Article Swipe
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· 2020
· Open Access
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· DOI: https://doi.org/10.3847/1538-4365/ab5e7a
Measurements of the physical properties of accretion disks in active galactic nuclei are important for better understanding the growth and evolution of supermassive black holes. We present the accretion disk sizes of 22 quasars from continuum reverberation mapping with data from the Dark Energy Survey (DES) standard-star fields and the supernova C fields. We construct continuum light curves with the griz photometry that span five seasons of DES observations. These data sample the time variability of the quasars with a cadence as short as 1 day, which corresponds to a rest-frame cadence that is a factor of a few higher than most previous work. We derive time lags between bands with both JAVELIN and the interpolated cross-correlation function method and fit for accretion disk sizes using the JAVELIN thin-disk model. These new measurements include disks around black holes with masses as small as ∼10 7 M ⊙ , which have equivalent sizes at 2500 Å as small as ∼0.1 lt-day in the rest frame. We find that most objects have accretion disk sizes consistent with the prediction of the standard thin-disk model when we take disk variability into account. We have also simulated the expected yield of accretion disk measurements under various observational scenarios for the Large Synoptic Survey Telescope Deep Drilling Fields. We find that the number of disk measurements would increase significantly if the default cadence is changed from 3 days to 2 days or 1 day.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4365/ab5e7a
- https://iopscience.iop.org/article/10.3847/1538-4365/ab5e7a/pdf
- OA Status
- bronze
- Cited By
- 54
- References
- 73
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W2900305962
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W2900305962Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4365/ab5e7aDigital Object Identifier
- Title
-
Quasar Accretion Disk Sizes from Continuum Reverberation Mapping in the DES Standard-star FieldsWork title
- Type
-
articleOpenAlex work type
- Language
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enPrimary language
- Publication year
-
2020Year of publication
- Publication date
-
2020-01-01Full publication date if available
- Authors
-
Zhefu Yu, Paul Martini, T. M. Davis, R. A. Gruendl, J. K. Hoormann, C. S. Kochanek, C. Lidman, D. Mudd, B. M. Peterson, W. C. Wester, S. Allam, J. Annis, J. Asorey, S. Àvila, M. Banerji, E. Bertin, D. Brooks, E. Buckley‐Geer, Josh Calcino, A. Carnero Rosell, D. Carollo, M. Carrasco Kind, J. Carretero, C. E. Cunha, C. B. D’Andrea, L. N. da Costa, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, T. F. Eifler, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztañaga, Karl Glazebrook, D. Gruen, J. Gschwend, G. Gutiérrez, W. G. Hartley, S. R. Hinton, D. L. Hollowood, K. Honscheid, B. Hoyle, D. J. James, Alex Kim, E. Krause, K. Kuehn, N. Kuropatkin, Geraint F. Lewis, M. Lima, E. Macaulay, M. A. G. Maia, J. L. Marshall, F. Menanteau, R. Miquel, A. Möller, A. A. Plazas, A. K. Romer, E. Sánchez, V. Scarpine, M. Schubnell, S. Serrano, M. Smith, Rory Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, Elizabeth Swann, M. E. C. Swanson, G. Tarlé, B. Tucker, D. L. Tucker, V. VikramList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4365/ab5e7aPublisher landing page
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https://iopscience.iop.org/article/10.3847/1538-4365/ab5e7a/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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bronzeOpen access status per OpenAlex
- OA URL
-
https://iopscience.iop.org/article/10.3847/1538-4365/ab5e7a/pdfDirect OA link when available
- Concepts
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Physics, Astrophysics, Reverberation mapping, Quasar, Thin disk, Accretion (finance), Photometry (optics), Supermassive black hole, Astronomy, Active galactic nucleus, Thick disk, Cadence, Accretion disc, Rest frame, Galaxy, Redshift, Stars, Halo, AcousticsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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54Total citation count in OpenAlex
- Citations by year (recent)
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2025: 7, 2024: 12, 2023: 8, 2022: 10, 2021: 5Per-year citation counts (last 5 years)
- References (count)
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73Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.from | 35, 41, 231 |
| abstract_inverted_index.griz | 61 |
| abstract_inverted_index.have | 150, 170, 191 |
| abstract_inverted_index.into | 188 |
| abstract_inverted_index.lags | 108 |
| abstract_inverted_index.most | 102, 168 |
| abstract_inverted_index.rest | 163 |
| abstract_inverted_index.span | 64 |
| abstract_inverted_index.take | 185 |
| abstract_inverted_index.than | 101 |
| abstract_inverted_index.that | 63, 93, 167, 216 |
| abstract_inverted_index.time | 74, 107 |
| abstract_inverted_index.when | 183 |
| abstract_inverted_index.with | 39, 59, 79, 111, 139, 175 |
| abstract_inverted_index.(DES) | 46 |
| abstract_inverted_index.Large | 207 |
| abstract_inverted_index.These | 70, 131 |
| abstract_inverted_index.bands | 110 |
| abstract_inverted_index.black | 24, 137 |
| abstract_inverted_index.disks | 8, 135 |
| abstract_inverted_index.holes | 138 |
| abstract_inverted_index.light | 57 |
| abstract_inverted_index.model | 182 |
| abstract_inverted_index.short | 83 |
| abstract_inverted_index.sizes | 31, 125, 152, 173 |
| abstract_inverted_index.small | 142, 157 |
| abstract_inverted_index.under | 201 |
| abstract_inverted_index.using | 126 |
| abstract_inverted_index.which | 87, 149 |
| abstract_inverted_index.work. | 104 |
| abstract_inverted_index.would | 222 |
| abstract_inverted_index.yield | 196 |
| abstract_inverted_index.∼10 | 144 |
| abstract_inverted_index.Energy | 44 |
| abstract_inverted_index.Survey | 45, 209 |
| abstract_inverted_index.active | 10 |
| abstract_inverted_index.around | 136 |
| abstract_inverted_index.better | 16 |
| abstract_inverted_index.curves | 58 |
| abstract_inverted_index.derive | 106 |
| abstract_inverted_index.factor | 96 |
| abstract_inverted_index.fields | 48 |
| abstract_inverted_index.frame. | 164 |
| abstract_inverted_index.growth | 19 |
| abstract_inverted_index.higher | 100 |
| abstract_inverted_index.holes. | 25 |
| abstract_inverted_index.lt-day | 160 |
| abstract_inverted_index.masses | 140 |
| abstract_inverted_index.method | 119 |
| abstract_inverted_index.model. | 130 |
| abstract_inverted_index.nuclei | 12 |
| abstract_inverted_index.number | 218 |
| abstract_inverted_index.sample | 72 |
| abstract_inverted_index.∼0.1 | 159 |
| abstract_inverted_index.Fields. | 213 |
| abstract_inverted_index.JAVELIN | 113, 128 |
| abstract_inverted_index.between | 109 |
| abstract_inverted_index.cadence | 81, 92, 228 |
| abstract_inverted_index.changed | 230 |
| abstract_inverted_index.default | 227 |
| abstract_inverted_index.fields. | 53 |
| abstract_inverted_index.include | 134 |
| abstract_inverted_index.mapping | 38 |
| abstract_inverted_index.objects | 169 |
| abstract_inverted_index.present | 27 |
| abstract_inverted_index.quasars | 34, 78 |
| abstract_inverted_index.seasons | 66 |
| abstract_inverted_index.various | 202 |
| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.Drilling | 212 |
| abstract_inverted_index.Synoptic | 208 |
| abstract_inverted_index.account. | 189 |
| abstract_inverted_index.expected | 195 |
| abstract_inverted_index.function | 118 |
| abstract_inverted_index.galactic | 11 |
| abstract_inverted_index.increase | 223 |
| abstract_inverted_index.physical | 4 |
| abstract_inverted_index.previous | 103 |
| abstract_inverted_index.standard | 180 |
| abstract_inverted_index.Telescope | 210 |
| abstract_inverted_index.accretion | 7, 29, 123, 171, 198 |
| abstract_inverted_index.construct | 55 |
| abstract_inverted_index.continuum | 36, 56 |
| abstract_inverted_index.evolution | 21 |
| abstract_inverted_index.important | 14 |
| abstract_inverted_index.scenarios | 204 |
| abstract_inverted_index.simulated | 193 |
| abstract_inverted_index.supernova | 51 |
| abstract_inverted_index.thin-disk | 129, 181 |
| abstract_inverted_index.consistent | 174 |
| abstract_inverted_index.equivalent | 151 |
| abstract_inverted_index.photometry | 62 |
| abstract_inverted_index.prediction | 177 |
| abstract_inverted_index.properties | 5 |
| abstract_inverted_index.rest-frame | 91 |
| abstract_inverted_index.corresponds | 88 |
| abstract_inverted_index.variability | 75, 187 |
| abstract_inverted_index.Measurements | 1 |
| abstract_inverted_index.interpolated | 116 |
| abstract_inverted_index.measurements | 133, 200, 221 |
| abstract_inverted_index.supermassive | 23 |
| abstract_inverted_index.observational | 203 |
| abstract_inverted_index.observations. | 69 |
| abstract_inverted_index.reverberation | 37 |
| abstract_inverted_index.significantly | 224 |
| abstract_inverted_index.standard-star | 47 |
| abstract_inverted_index.understanding | 17 |
| abstract_inverted_index.cross-correlation | 117 |
| cited_by_percentile_year.max | 99 |
| cited_by_percentile_year.min | 97 |
| countries_distinct_count | 12 |
| institutions_distinct_count | 75 |
| citation_normalized_percentile.value | 0.94860743 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |