The MBH–M∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam Images Article Swipe
Takumi S. Tanaka
,
J. D. Silverman
,
Xuheng Ding
,
K. Jahnkę
,
Benny Trakhtenbrot
,
Erini Lambrides
,
Masafusa Onoue
,
I.T Andika
,
A. Bongiorno
,
Andreas L. Faisst
,
Steven Gillman
,
Christopher C. Hayward
,
Michaela Hirschmann
,
Anton M. Koekemoer
,
Vasily Kokorev
,
Zhaoxuan Liu
,
G. Magdis
,
A. Renzini
,
Caitlin M. Casey
,
Caitlin M. Casey
,
Nicole E. Drakos
,
Maximilien Franco
,
G. Gozaliasl
,
Jeyhan S. Kartaltepe
,
Daizhong Liu
,
H. J. McCracken
,
Jason Rhodes
,
Brant Robertson
,
Sune Toft
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ad9d0a
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ad9d0a
Our knowledge of relations between supermassive black holes and their host galaxies at z ≳ 1 is still limited, even though being actively sought out to z ∼ 6. Here, we use the high resolution and sensitivity of JWST to measure the host galaxy properties for 107 X-ray-selected type-I active galactic nuclei (AGNs) at 0.68 < z < 2.5 with rest-frame optical/near-infrared imaging from COSMOS-Web and PRIMER. Black hole masses ( ) are available from previous spectroscopic campaigns. We extract the host galaxy components from four NIRCam broadband images and the Hubble Space Telescope/Advanced Camera for Surveys F814W image by applying a 2D image decomposition technique. We detect the host galaxy for ∼90% of the sample after subtracting the unresolved AGN emission. With host photometry free of AGN emission, we determine the stellar mass of the host galaxies to be through spectral energy distribution fitting and measure the evolution of the mass relation between SMBHs and their host galaxies. Considering selection biases and measurement uncertainties, we find that the M BH / M * ratio evolves as thus remains essentially constant or exhibits mild evolution up to z ∼ 2.5. We also see an amount of scatter ( ), similar to the local relation and consistent with low- z studies, and a noncausal cosmic assembly history where mergers contribute to the statistical averaging toward the local relation is still feasible. We highlight improvements to come with larger samples from JWST and, particularly, Euclid, which will exceed the statistical power of current wide and deep surveys.
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Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ad9d0a
- OA Status
- gold
- Cited By
- 15
- References
- 166
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4406915130
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4406915130Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/ad9d0aDigital Object Identifier
- Title
-
The MBH–M∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam ImagesWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-01-28Full publication date if available
- Authors
-
Takumi S. Tanaka, J. D. Silverman, Xuheng Ding, K. Jahnkę, Benny Trakhtenbrot, Erini Lambrides, Masafusa Onoue, I.T Andika, A. Bongiorno, Andreas L. Faisst, Steven Gillman, Christopher C. Hayward, Michaela Hirschmann, Anton M. Koekemoer, Vasily Kokorev, Zhaoxuan Liu, G. Magdis, A. Renzini, Caitlin M. Casey, Caitlin M. Casey, Nicole E. Drakos, Maximilien Franco, G. Gozaliasl, Jeyhan S. Kartaltepe, Daizhong Liu, H. J. McCracken, Jason Rhodes, Brant Robertson, Sune ToftList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4357/ad9d0aPublisher landing page
- Open access
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YesWhether a free full text is available
- OA status
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goldOpen access status per OpenAlex
- OA URL
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https://doi.org/10.3847/1538-4357/ad9d0aDirect OA link when available
- Concepts
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Physics, Cosmos (plant), Relation (database), Astronomy, Decomposition, Astrophysics, Astrobiology, Art history, Database, Biology, Computer science, Ecology, ArtTop concepts (fields/topics) attached by OpenAlex
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15Total citation count in OpenAlex
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2025: 15Per-year citation counts (last 5 years)
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166Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.host | 11, 43, 119, 147, 161, 174, 231 |
| abstract_inverted_index.low- | 341 |
| abstract_inverted_index.mass | 171, 225 |
| abstract_inverted_index.mild | 290 |
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| abstract_inverted_index.thus | 284 |
| abstract_inverted_index.wide | 385 |
| abstract_inverted_index.will | 378 |
| abstract_inverted_index.with | 60, 340, 369 |
| abstract_inverted_index.Black | 68 |
| abstract_inverted_index.F814W | 135 |
| abstract_inverted_index.Here, | 30 |
| abstract_inverted_index.SMBHs | 228 |
| abstract_inverted_index.Space | 130 |
| abstract_inverted_index.after | 154 |
| abstract_inverted_index.being | 22 |
| abstract_inverted_index.black | 7 |
| abstract_inverted_index.holes | 8 |
| abstract_inverted_index.image | 136, 141 |
| abstract_inverted_index.local | 336, 359 |
| abstract_inverted_index.power | 382 |
| abstract_inverted_index.ratio | 248 |
| abstract_inverted_index.still | 18, 362 |
| abstract_inverted_index.their | 10, 230 |
| abstract_inverted_index.where | 350 |
| abstract_inverted_index.which | 377 |
| abstract_inverted_index.(AGNs) | 53 |
| abstract_inverted_index.Camera | 132 |
| abstract_inverted_index.Hubble | 129 |
| abstract_inverted_index.NIRCam | 124 |
| abstract_inverted_index.active | 50 |
| abstract_inverted_index.amount | 301 |
| abstract_inverted_index.biases | 235 |
| abstract_inverted_index.cosmic | 347 |
| abstract_inverted_index.detect | 145 |
| abstract_inverted_index.energy | 216 |
| abstract_inverted_index.exceed | 379 |
| abstract_inverted_index.galaxy | 44, 120, 148 |
| abstract_inverted_index.images | 126 |
| abstract_inverted_index.larger | 370 |
| abstract_inverted_index.masses | 70 |
| abstract_inverted_index.nuclei | 52 |
| abstract_inverted_index.sample | 153 |
| abstract_inverted_index.sought | 24 |
| abstract_inverted_index.though | 21 |
| abstract_inverted_index.toward | 357 |
| abstract_inverted_index.type-I | 49 |
| abstract_inverted_index.∼90% | 150 |
| abstract_inverted_index.<mml:mi | 85 |
| abstract_inverted_index.Euclid, | 376 |
| abstract_inverted_index.PRIMER. | 67 |
| abstract_inverted_index.Surveys | 134 |
| abstract_inverted_index.between | 5, 227 |
| abstract_inverted_index.current | 384 |
| abstract_inverted_index.evolves | 249 |
| abstract_inverted_index.extract | 117 |
| abstract_inverted_index.fitting | 218 |
| abstract_inverted_index.history | 349 |
| abstract_inverted_index.imaging | 63 |
| abstract_inverted_index.measure | 41, 220 |
| abstract_inverted_index.mergers | 351 |
| abstract_inverted_index.remains | 285 |
| abstract_inverted_index.samples | 371 |
| abstract_inverted_index.scatter | 303 |
| abstract_inverted_index.similar | 333 |
| abstract_inverted_index.stellar | 170 |
| abstract_inverted_index.through | 214 |
| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.actively | 23 |
| abstract_inverted_index.applying | 138 |
| abstract_inverted_index.assembly | 348 |
| abstract_inverted_index.constant | 287 |
| abstract_inverted_index.exhibits | 289 |
| abstract_inverted_index.galactic | 51 |
| abstract_inverted_index.galaxies | 12, 175 |
| abstract_inverted_index.limited, | 19 |
| abstract_inverted_index.previous | 113 |
| abstract_inverted_index.relation | 226, 337, 360 |
| abstract_inverted_index.spectral | 215 |
| abstract_inverted_index.studies, | 343 |
| abstract_inverted_index.surveys. | 388 |
| abstract_inverted_index.<mml:math | 72, 178, 251, 305 |
| abstract_inverted_index.available | 111 |
| abstract_inverted_index.averaging | 356 |
| abstract_inverted_index.broadband | 125 |
| abstract_inverted_index.close=")" | 77, 183, 257 |
| abstract_inverted_index.determine | 168 |
| abstract_inverted_index.emission, | 166 |
| abstract_inverted_index.emission. | 159 |
| abstract_inverted_index.evolution | 222, 291 |
| abstract_inverted_index.feasible. | 363 |
| abstract_inverted_index.galaxies. | 232 |
| abstract_inverted_index.highlight | 365 |
| abstract_inverted_index.knowledge | 2 |
| abstract_inverted_index.noncausal | 346 |
| abstract_inverted_index.open="("> | 78, 184, 258 |
| abstract_inverted_index.relations | 4 |
| abstract_inverted_index.selection | 234 |
| abstract_inverted_index.<mml:mrow> | 79, 81, 84, 91, 94, 185, 187, 190, 196, 199, 255, 259, 266, 269, 272, 276, 309, 312, 319, 322, 326 |
| abstract_inverted_index.<mml:msub> | 80, 90, 186, 195, 308 |
| abstract_inverted_index.<mml:msup> | 254 |
| abstract_inverted_index.COSMOS-Web | 65 |
| abstract_inverted_index.campaigns. | 115 |
| abstract_inverted_index.components | 121 |
| abstract_inverted_index.consistent | 339 |
| abstract_inverted_index.contribute | 352 |
| abstract_inverted_index.photometry | 162 |
| abstract_inverted_index.properties | 45 |
| abstract_inverted_index.resolution | 35 |
| abstract_inverted_index.rest-frame | 61 |
| abstract_inverted_index.technique. | 143 |
| abstract_inverted_index.unresolved | 157 |
| abstract_inverted_index.</mml:math> | 108, 213, 283, 331 |
| abstract_inverted_index.</mml:mrow> | 83, 87, 93, 96, 98, 189, 192, 198, 201, 203, 263, 265, 271, 275, 279, 281, 311, 314, 321, 325, 329 |
| abstract_inverted_index.</mml:msub> | 88, 97, 193, 202, 315 |
| abstract_inverted_index.</mml:msup> | 282 |
| abstract_inverted_index.<mml:mspace | 102, 105, 206, 210 |
| abstract_inverted_index.Considering | 233 |
| abstract_inverted_index.essentially | 286 |
| abstract_inverted_index.measurement | 237 |
| abstract_inverted_index.sensitivity | 37 |
| abstract_inverted_index.statistical | 355, 381 |
| abstract_inverted_index.subtracting | 155 |
| abstract_inverted_index.<mml:mfenced | 76, 182, 256 |
| abstract_inverted_index.distribution | 217 |
| abstract_inverted_index.improvements | 366 |
| abstract_inverted_index.supermassive | 6 |
| abstract_inverted_index.<mml:msubsup> | 268, 318 |
| abstract_inverted_index.decomposition | 142 |
| abstract_inverted_index.particularly, | 375 |
| abstract_inverted_index.spectroscopic | 114 |
| abstract_inverted_index.</mml:mfenced> | 99, 204, 264 |
| abstract_inverted_index.</mml:msubsup> | 280, 330 |
| abstract_inverted_index.X-ray-selected | 48 |
| abstract_inverted_index.uncertainties, | 238 |
| abstract_inverted_index.width="-0.25em"/> | 103, 106, 207, 211 |
| abstract_inverted_index.<mml:mi>M</mml:mi> | 82, 92, 188, 197 |
| abstract_inverted_index.<mml:mi>z</mml:mi> | 262 |
| abstract_inverted_index.<mml:mn>0</mml:mn> | 320 |
| abstract_inverted_index.<mml:mn>1</mml:mn> | 260 |
| abstract_inverted_index.<mml:mn>8</mml:mn> | 270 |
| abstract_inverted_index.<mml:mo>*</mml:mo> | 191 |
| abstract_inverted_index.<mml:mo>+</mml:mo> | 261, 277, 327 |
| abstract_inverted_index.<mml:mo>/</mml:mo> | 89, 194 |
| abstract_inverted_index.<mml:mo>=</mml:mo> | 316 |
| abstract_inverted_index.Telescope/Advanced | 131 |
| abstract_inverted_index.overflow="scroll"> | 74, 180, 253, 307 |
| abstract_inverted_index.<mml:mi>μ</mml:mi> | 313 |
| abstract_inverted_index.<mml:mi>σ</mml:mi> | 310 |
| abstract_inverted_index.<mml:mi>log</mml:mi> | 75, 181 |
| abstract_inverted_index.<mml:mn>0.3</mml:mn> | 317 |
| abstract_inverted_index.<mml:mn>0.4</mml:mn> | 267 |
| abstract_inverted_index.<mml:mn>6.9</mml:mn> | 101 |
| abstract_inverted_index.<mml:mn>9.5</mml:mn> | 208 |
| abstract_inverted_index.<mml:mn>9.6</mml:mn> | 107 |
| abstract_inverted_index.<mml:mo>−</mml:mo> | 104, 209, 273, 323 |
| abstract_inverted_index.<mml:mo>∼</mml:mo> | 100, 205 |
| abstract_inverted_index.<mml:mo>⊙</mml:mo> | 95, 200 |
| abstract_inverted_index.<mml:mn>0.13</mml:mn> | 324 |
| abstract_inverted_index.<mml:mn>0.14</mml:mn> | 328 |
| abstract_inverted_index.<mml:mn>0.31</mml:mn> | 278 |
| abstract_inverted_index.<mml:mn>0.62</mml:mn> | 274 |
| abstract_inverted_index.<mml:mn>11.6</mml:mn> | 212 |
| abstract_inverted_index.optical/near-infrared | 62 |
| abstract_inverted_index.mathvariant="normal">BH</mml:mi> | 86 |
| abstract_inverted_index.xmlns:mml="http://www.w3.org/1998/Math/MathML" | 73, 179, 252, 306 |
| cited_by_percentile_year.max | 100 |
| cited_by_percentile_year.min | 99 |
| corresponding_author_ids | https://openalex.org/A5089406918 |
| countries_distinct_count | 1 |
| institutions_distinct_count | 29 |
| citation_normalized_percentile.value | 0.99590742 |
| citation_normalized_percentile.is_in_top_1_percent | True |
| citation_normalized_percentile.is_in_top_10_percent | True |