Baryonic Ecosystem IN Galaxies (BEINGMgII) Article Swipe
Saurya Das
,
Ravi Joshi
,
Ram Prasad Chaudhary
,
Michele Fumagalli
,
Matteo Fossati
,
Céline Péroux
,
Luis C. Ho
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202452494
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202452494
We search for the galaxies associated with the intervening Mg II absorbers over a redshift range of 0.4 ≤ z ≤ 1 using imaging data from DESI Legacy Imaging Surveys and measure the redshift based on the direct detection of nebular emission in the background quasar spectra from the SDSS survey. We find 270 Mg II absorbers associated with strong O [ II ] or O [ III ] and H β nebular emissions, at a 2.5 σ level. Among them, for 213 Mg II absorbers, we detect an absorber host galaxy at impact parameters of 4 ≤ ρ ≤ 16 kpc, including three absorbers associated with a galaxy pair, with a best-fit galaxy spectral energy distribution model based on multi-passband photometric data from DESI Legacy Imaging surveys, supplemented with the infrared VISTA and unWISE imaging surveys. The detection rate of the Mg II absorber host with strong O [ II ] nebular emission in the finite SDSS fibre of a 2–3 arcsec diameter increases from 0.2% to ∼3% with an increasing equivalent width from 0.3 Å to ∼3.5 Å, which remains near-constant across the probed redshift range. The associated Mg II host galaxies exhibit a wide range of stellar mass from 7.94 ≤ log(M ⋆ /M ⊙ )≤11.11, with an average star formation rate (SFR) of 5.81 M ⊙ yr −1 . The Mg II absorber hosts selected based on O [ II ] nebular emission mostly exhibit active star-forming systems including 13.4% starburst systems, but 10.2% with a suppressed SFR. The near-constant absorption strength at low-impact parameters suggests a high gas covering fraction. We find that the Mg II equivalent width ( W 2796 ) positively correlates with the SFR and specific SFR, likely indicating their wind origin. The average velocity offset between the host and the absorber suggests that the Mg II gas is bound within the dark matter halo.
Related Topics
Concepts
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/202452494
- OA Status
- hybrid
- Cited By
- 2
- References
- 74
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4407168179
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
-
https://openalex.org/W4407168179Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.1051/0004-6361/202452494Digital Object Identifier
- Title
-
Baryonic Ecosystem IN Galaxies (BEINGMgII)Work title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2025Year of publication
- Publication date
-
2025-02-05Full publication date if available
- Authors
-
Saurya Das, Ravi Joshi, Ram Prasad Chaudhary, Michele Fumagalli, Matteo Fossati, Céline Péroux, Luis C. HoList of authors in order
- Landing page
-
https://doi.org/10.1051/0004-6361/202452494Publisher landing page
- Open access
-
YesWhether a free full text is available
- OA status
-
hybridOpen access status per OpenAlex
- OA URL
-
https://doi.org/10.1051/0004-6361/202452494Direct OA link when available
- Concepts
-
Physics, Astrophysics, Galaxy, Baryon, Galaxy group, Astronomy, Luminous infrared galaxyTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
2Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 2Per-year citation counts (last 5 years)
- References (count)
-
74Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
Full payload
| id | https://openalex.org/W4407168179 |
|---|---|
| doi | https://doi.org/10.1051/0004-6361/202452494 |
| ids.doi | https://doi.org/10.1051/0004-6361/202452494 |
| ids.openalex | https://openalex.org/W4407168179 |
| fwci | 6.55731427 |
| type | article |
| title | Baryonic Ecosystem IN Galaxies (BEINGMgII) |
| biblio.issue | |
| biblio.volume | 695 |
| biblio.last_page | A207 |
| biblio.first_page | A207 |
| topics[0].id | https://openalex.org/T10026 |
| topics[0].field.id | https://openalex.org/fields/31 |
| topics[0].field.display_name | Physics and Astronomy |
| topics[0].score | 0.9944999814033508 |
| topics[0].domain.id | https://openalex.org/domains/3 |
| topics[0].domain.display_name | Physical Sciences |
| topics[0].subfield.id | https://openalex.org/subfields/3103 |
| topics[0].subfield.display_name | Astronomy and Astrophysics |
| topics[0].display_name | Galaxies: Formation, Evolution, Phenomena |
| topics[1].id | https://openalex.org/T12917 |
| topics[1].field.id | https://openalex.org/fields/31 |
| topics[1].field.display_name | Physics and Astronomy |
| topics[1].score | 0.9918000102043152 |
| topics[1].domain.id | https://openalex.org/domains/3 |
| topics[1].domain.display_name | Physical Sciences |
| topics[1].subfield.id | https://openalex.org/subfields/3105 |
| topics[1].subfield.display_name | Instrumentation |
| topics[1].display_name | Astronomy and Astrophysical Research |
| topics[2].id | https://openalex.org/T10402 |
| topics[2].field.id | https://openalex.org/fields/22 |
| topics[2].field.display_name | Engineering |
| topics[2].score | 0.9286999702453613 |
| topics[2].domain.id | https://openalex.org/domains/3 |
| topics[2].domain.display_name | Physical Sciences |
| topics[2].subfield.id | https://openalex.org/subfields/2204 |
| topics[2].subfield.display_name | Biomedical Engineering |
| topics[2].display_name | Phase Equilibria and Thermodynamics |
| is_xpac | False |
| apc_list | |
| apc_paid | |
| concepts[0].id | https://openalex.org/C121332964 |
| concepts[0].level | 0 |
| concepts[0].score | 0.9418319463729858 |
| concepts[0].wikidata | https://www.wikidata.org/wiki/Q413 |
| concepts[0].display_name | Physics |
| concepts[1].id | https://openalex.org/C44870925 |
| concepts[1].level | 1 |
| concepts[1].score | 0.7108608484268188 |
| concepts[1].wikidata | https://www.wikidata.org/wiki/Q37547 |
| concepts[1].display_name | Astrophysics |
| concepts[2].id | https://openalex.org/C98444146 |
| concepts[2].level | 2 |
| concepts[2].score | 0.6431552767753601 |
| concepts[2].wikidata | https://www.wikidata.org/wiki/Q318 |
| concepts[2].display_name | Galaxy |
| concepts[3].id | https://openalex.org/C154153549 |
| concepts[3].level | 2 |
| concepts[3].score | 0.5301010608673096 |
| concepts[3].wikidata | https://www.wikidata.org/wiki/Q159731 |
| concepts[3].display_name | Baryon |
| concepts[4].id | https://openalex.org/C160147972 |
| concepts[4].level | 4 |
| concepts[4].score | 0.5167931318283081 |
| concepts[4].wikidata | https://www.wikidata.org/wiki/Q204107 |
| concepts[4].display_name | Galaxy group |
| concepts[5].id | https://openalex.org/C1276947 |
| concepts[5].level | 1 |
| concepts[5].score | 0.4571395516395569 |
| concepts[5].wikidata | https://www.wikidata.org/wiki/Q333 |
| concepts[5].display_name | Astronomy |
| concepts[6].id | https://openalex.org/C89108925 |
| concepts[6].level | 3 |
| concepts[6].score | 0.4472613036632538 |
| concepts[6].wikidata | https://www.wikidata.org/wiki/Q1565388 |
| concepts[6].display_name | Luminous infrared galaxy |
| keywords[0].id | https://openalex.org/keywords/physics |
| keywords[0].score | 0.9418319463729858 |
| keywords[0].display_name | Physics |
| keywords[1].id | https://openalex.org/keywords/astrophysics |
| keywords[1].score | 0.7108608484268188 |
| keywords[1].display_name | Astrophysics |
| keywords[2].id | https://openalex.org/keywords/galaxy |
| keywords[2].score | 0.6431552767753601 |
| keywords[2].display_name | Galaxy |
| keywords[3].id | https://openalex.org/keywords/baryon |
| keywords[3].score | 0.5301010608673096 |
| keywords[3].display_name | Baryon |
| keywords[4].id | https://openalex.org/keywords/galaxy-group |
| keywords[4].score | 0.5167931318283081 |
| keywords[4].display_name | Galaxy group |
| keywords[5].id | https://openalex.org/keywords/astronomy |
| keywords[5].score | 0.4571395516395569 |
| keywords[5].display_name | Astronomy |
| keywords[6].id | https://openalex.org/keywords/luminous-infrared-galaxy |
| keywords[6].score | 0.4472613036632538 |
| keywords[6].display_name | Luminous infrared galaxy |
| language | en |
| locations[0].id | doi:10.1051/0004-6361/202452494 |
| locations[0].is_oa | True |
| locations[0].source.id | https://openalex.org/S205231332 |
| locations[0].source.issn | 0004-6361, 1432-0746 |
| locations[0].source.type | journal |
| locations[0].source.is_oa | False |
| locations[0].source.issn_l | 0004-6361 |
| locations[0].source.is_core | True |
| locations[0].source.is_in_doaj | False |
| locations[0].source.display_name | Astronomy and Astrophysics |
| locations[0].source.host_organization | https://openalex.org/P4310319748 |
| locations[0].source.host_organization_name | EDP Sciences |
| locations[0].source.host_organization_lineage | https://openalex.org/P4310319748 |
| locations[0].source.host_organization_lineage_names | EDP Sciences |
| locations[0].license | cc-by |
| locations[0].pdf_url | |
| locations[0].version | publishedVersion |
| locations[0].raw_type | journal-article |
| locations[0].license_id | https://openalex.org/licenses/cc-by |
| locations[0].is_accepted | True |
| locations[0].is_published | True |
| locations[0].raw_source_name | Astronomy & Astrophysics |
| locations[0].landing_page_url | https://doi.org/10.1051/0004-6361/202452494 |
| indexed_in | crossref |
| authorships[0].author.id | https://openalex.org/A5008954026 |
| authorships[0].author.orcid | https://orcid.org/0000-0003-1191-8469 |
| authorships[0].author.display_name | Saurya Das |
| authorships[0].author_position | first |
| authorships[0].raw_author_name | Sarbeswar Das |
| authorships[0].is_corresponding | False |
| authorships[1].author.id | https://openalex.org/A5065878827 |
| authorships[1].author.orcid | |
| authorships[1].author.display_name | Ravi Joshi |
| authorships[1].author_position | middle |
| authorships[1].raw_author_name | Ravi Joshi |
| authorships[1].is_corresponding | False |
| authorships[2].author.id | https://openalex.org/A5013338282 |
| authorships[2].author.orcid | https://orcid.org/0000-0002-1839-0727 |
| authorships[2].author.display_name | Ram Prasad Chaudhary |
| authorships[2].author_position | middle |
| authorships[2].raw_author_name | Reena Chaudhary |
| authorships[2].is_corresponding | False |
| authorships[3].author.id | https://openalex.org/A5010271324 |
| authorships[3].author.orcid | https://orcid.org/0000-0001-6676-3842 |
| authorships[3].author.display_name | Michele Fumagalli |
| authorships[3].author_position | middle |
| authorships[3].raw_author_name | Michele Fumagalli |
| authorships[3].is_corresponding | False |
| authorships[4].author.id | https://openalex.org/A5035893141 |
| authorships[4].author.orcid | https://orcid.org/0000-0002-9043-8764 |
| authorships[4].author.display_name | Matteo Fossati |
| authorships[4].author_position | middle |
| authorships[4].raw_author_name | Matteo Fossati |
| authorships[4].is_corresponding | False |
| authorships[5].author.id | https://openalex.org/A5073472347 |
| authorships[5].author.orcid | https://orcid.org/0000-0002-4288-599X |
| authorships[5].author.display_name | Céline Péroux |
| authorships[5].author_position | middle |
| authorships[5].raw_author_name | Celine Peroux |
| authorships[5].is_corresponding | False |
| authorships[6].author.id | https://openalex.org/A5054184482 |
| authorships[6].author.orcid | https://orcid.org/0000-0001-6947-5846 |
| authorships[6].author.display_name | Luis C. Ho |
| authorships[6].author_position | last |
| authorships[6].raw_author_name | Luis C. Ho |
| authorships[6].is_corresponding | False |
| has_content.pdf | False |
| has_content.grobid_xml | False |
| is_paratext | False |
| open_access.is_oa | True |
| open_access.oa_url | https://doi.org/10.1051/0004-6361/202452494 |
| open_access.oa_status | hybrid |
| open_access.any_repository_has_fulltext | False |
| created_date | 2025-02-06T00:00:00 |
| display_name | Baryonic Ecosystem IN Galaxies (BEINGMgII) |
| has_fulltext | False |
| is_retracted | False |
| updated_date | 2025-11-06T03:46:38.306776 |
| primary_topic.id | https://openalex.org/T10026 |
| primary_topic.field.id | https://openalex.org/fields/31 |
| primary_topic.field.display_name | Physics and Astronomy |
| primary_topic.score | 0.9944999814033508 |
| primary_topic.domain.id | https://openalex.org/domains/3 |
| primary_topic.domain.display_name | Physical Sciences |
| primary_topic.subfield.id | https://openalex.org/subfields/3103 |
| primary_topic.subfield.display_name | Astronomy and Astrophysics |
| primary_topic.display_name | Galaxies: Formation, Evolution, Phenomena |
| related_works | https://openalex.org/W4404409304, https://openalex.org/W4394637313, https://openalex.org/W1968347830, https://openalex.org/W2790283293, https://openalex.org/W3098118266, https://openalex.org/W2997786057, https://openalex.org/W1516397246, https://openalex.org/W3103547080, https://openalex.org/W2072013985, https://openalex.org/W2616292853 |
| cited_by_count | 2 |
| counts_by_year[0].year | 2025 |
| counts_by_year[0].cited_by_count | 2 |
| locations_count | 1 |
| best_oa_location.id | doi:10.1051/0004-6361/202452494 |
| best_oa_location.is_oa | True |
| best_oa_location.source.id | https://openalex.org/S205231332 |
| best_oa_location.source.issn | 0004-6361, 1432-0746 |
| best_oa_location.source.type | journal |
| best_oa_location.source.is_oa | False |
| best_oa_location.source.issn_l | 0004-6361 |
| best_oa_location.source.is_core | True |
| best_oa_location.source.is_in_doaj | False |
| best_oa_location.source.display_name | Astronomy and Astrophysics |
| best_oa_location.source.host_organization | https://openalex.org/P4310319748 |
| best_oa_location.source.host_organization_name | EDP Sciences |
| best_oa_location.source.host_organization_lineage | https://openalex.org/P4310319748 |
| best_oa_location.source.host_organization_lineage_names | EDP Sciences |
| best_oa_location.license | cc-by |
| best_oa_location.pdf_url | |
| best_oa_location.version | publishedVersion |
| best_oa_location.raw_type | journal-article |
| best_oa_location.license_id | https://openalex.org/licenses/cc-by |
| best_oa_location.is_accepted | True |
| best_oa_location.is_published | True |
| best_oa_location.raw_source_name | Astronomy & Astrophysics |
| best_oa_location.landing_page_url | https://doi.org/10.1051/0004-6361/202452494 |
| primary_location.id | doi:10.1051/0004-6361/202452494 |
| primary_location.is_oa | True |
| primary_location.source.id | https://openalex.org/S205231332 |
| primary_location.source.issn | 0004-6361, 1432-0746 |
| primary_location.source.type | journal |
| primary_location.source.is_oa | False |
| primary_location.source.issn_l | 0004-6361 |
| primary_location.source.is_core | True |
| primary_location.source.is_in_doaj | False |
| primary_location.source.display_name | Astronomy and Astrophysics |
| primary_location.source.host_organization | https://openalex.org/P4310319748 |
| primary_location.source.host_organization_name | EDP Sciences |
| primary_location.source.host_organization_lineage | https://openalex.org/P4310319748 |
| primary_location.source.host_organization_lineage_names | EDP Sciences |
| primary_location.license | cc-by |
| primary_location.pdf_url | |
| primary_location.version | publishedVersion |
| primary_location.raw_type | journal-article |
| primary_location.license_id | https://openalex.org/licenses/cc-by |
| primary_location.is_accepted | True |
| primary_location.is_published | True |
| primary_location.raw_source_name | Astronomy & Astrophysics |
| primary_location.landing_page_url | https://doi.org/10.1051/0004-6361/202452494 |
| publication_date | 2025-02-05 |
| publication_year | 2025 |
| referenced_works | https://openalex.org/W3147728474, https://openalex.org/W4225875721, https://openalex.org/W4309332454, https://openalex.org/W2511520071, https://openalex.org/W2070885265, https://openalex.org/W2101307399, https://openalex.org/W1980997484, https://openalex.org/W2125473068, https://openalex.org/W1974174849, https://openalex.org/W2772961215, https://openalex.org/W2052072846, https://openalex.org/W2083680971, https://openalex.org/W2408859036, https://openalex.org/W4391944882, https://openalex.org/W3130063150, https://openalex.org/W2799047820, https://openalex.org/W3091321448, https://openalex.org/W2770624382, https://openalex.org/W4289632715, https://openalex.org/W2092194717, https://openalex.org/W2100538510, https://openalex.org/W2999395374, https://openalex.org/W3125651462, https://openalex.org/W4312180428, https://openalex.org/W4400933192, https://openalex.org/W4226199354, https://openalex.org/W4388669284, https://openalex.org/W4389373622, https://openalex.org/W3092500027, https://openalex.org/W3202449849, https://openalex.org/W2147344503, https://openalex.org/W1827363964, https://openalex.org/W2543127845, https://openalex.org/W2625005707, https://openalex.org/W2783340554, https://openalex.org/W1927643699, https://openalex.org/W2071190804, https://openalex.org/W2016189541, https://openalex.org/W2116466430, https://openalex.org/W2808342581, https://openalex.org/W2075532844, https://openalex.org/W1878631143, https://openalex.org/W2535541914, https://openalex.org/W2985498878, https://openalex.org/W1993194316, https://openalex.org/W3130202506, https://openalex.org/W2121083155, https://openalex.org/W2025612492, https://openalex.org/W4402543622, https://openalex.org/W1532082951, https://openalex.org/W3026745777, https://openalex.org/W2129067514, https://openalex.org/W2103731818, https://openalex.org/W1885962465, https://openalex.org/W2527653396, https://openalex.org/W2909115629, https://openalex.org/W3086108862, https://openalex.org/W4221164894, https://openalex.org/W2149078886, https://openalex.org/W4391463035, https://openalex.org/W1649074782, https://openalex.org/W2768362915, https://openalex.org/W4394007348, https://openalex.org/W2155630450, https://openalex.org/W2131906729, https://openalex.org/W2899969883, https://openalex.org/W2561281082, https://openalex.org/W4388515781, https://openalex.org/W2911747721, https://openalex.org/W3184364761, https://openalex.org/W2558282339, https://openalex.org/W2890363482, https://openalex.org/W2045894289, https://openalex.org/W2047517180 |
| referenced_works_count | 74 |
| abstract_inverted_index.( | 273 |
| abstract_inverted_index.) | 276 |
| abstract_inverted_index.. | 222 |
| abstract_inverted_index.1 | 21 |
| abstract_inverted_index.4 | 96 |
| abstract_inverted_index.H | 70 |
| abstract_inverted_index.M | 218 |
| abstract_inverted_index.O | 60, 65, 148, 231 |
| abstract_inverted_index.W | 274 |
| abstract_inverted_index.[ | 61, 66, 149, 232 |
| abstract_inverted_index.] | 63, 68, 151, 234 |
| abstract_inverted_index.a | 13, 75, 107, 111, 160, 195, 249, 260 |
| abstract_inverted_index.z | 19 |
| abstract_inverted_index./M | 206 |
| abstract_inverted_index.16 | 100 |
| abstract_inverted_index.II | 10, 55, 62, 84, 143, 150, 191, 225, 233, 270, 304 |
| abstract_inverted_index.Mg | 9, 54, 83, 142, 190, 224, 269, 303 |
| abstract_inverted_index.We | 0, 51, 265 |
| abstract_inverted_index.an | 88, 170, 210 |
| abstract_inverted_index.at | 74, 92, 256 |
| abstract_inverted_index.in | 42, 154 |
| abstract_inverted_index.is | 306 |
| abstract_inverted_index.of | 16, 39, 95, 140, 159, 198, 216 |
| abstract_inverted_index.on | 35, 119, 230 |
| abstract_inverted_index.or | 64 |
| abstract_inverted_index.to | 167, 177 |
| abstract_inverted_index.we | 86 |
| abstract_inverted_index.yr | 220 |
| abstract_inverted_index.Å | 176 |
| abstract_inverted_index.β | 71 |
| abstract_inverted_index.ρ | 98 |
| abstract_inverted_index.σ | 77 |
| abstract_inverted_index.0.3 | 175 |
| abstract_inverted_index.0.4 | 17 |
| abstract_inverted_index.2.5 | 76 |
| abstract_inverted_index.213 | 82 |
| abstract_inverted_index.270 | 53 |
| abstract_inverted_index.III | 67 |
| abstract_inverted_index.SFR | 281 |
| abstract_inverted_index.The | 137, 188, 223, 252, 290 |
| abstract_inverted_index.and | 30, 69, 133, 282, 297 |
| abstract_inverted_index.but | 246 |
| abstract_inverted_index.for | 2, 81 |
| abstract_inverted_index.gas | 262, 305 |
| abstract_inverted_index.the | 3, 7, 32, 36, 43, 48, 130, 141, 155, 184, 268, 280, 295, 298, 302, 309 |
| abstract_inverted_index.Å, | 179 |
| abstract_inverted_index.≤ | 18, 20, 97, 99, 203 |
| abstract_inverted_index.⊙ | 207, 219 |
| abstract_inverted_index.⋆ | 205 |
| abstract_inverted_index.0.2% | 166 |
| abstract_inverted_index.2796 | 275 |
| abstract_inverted_index.5.81 | 217 |
| abstract_inverted_index.7.94 | 202 |
| abstract_inverted_index.DESI | 26, 124 |
| abstract_inverted_index.SDSS | 49, 157 |
| abstract_inverted_index.SFR, | 284 |
| abstract_inverted_index.SFR. | 251 |
| abstract_inverted_index.dark | 310 |
| abstract_inverted_index.data | 24, 122 |
| abstract_inverted_index.find | 52, 266 |
| abstract_inverted_index.from | 25, 47, 123, 165, 174, 201 |
| abstract_inverted_index.high | 261 |
| abstract_inverted_index.host | 90, 145, 192, 296 |
| abstract_inverted_index.kpc, | 101 |
| abstract_inverted_index.mass | 200 |
| abstract_inverted_index.over | 12 |
| abstract_inverted_index.rate | 139, 214 |
| abstract_inverted_index.star | 212 |
| abstract_inverted_index.that | 267, 301 |
| abstract_inverted_index.wide | 196 |
| abstract_inverted_index.wind | 288 |
| abstract_inverted_index.with | 6, 58, 106, 110, 129, 146, 169, 209, 248, 279 |
| abstract_inverted_index.−1 | 221 |
| abstract_inverted_index.(SFR) | 215 |
| abstract_inverted_index.10.2% | 247 |
| abstract_inverted_index.13.4% | 243 |
| abstract_inverted_index.2–3 | 161 |
| abstract_inverted_index.Among | 79 |
| abstract_inverted_index.VISTA | 132 |
| abstract_inverted_index.based | 34, 118, 229 |
| abstract_inverted_index.bound | 307 |
| abstract_inverted_index.fibre | 158 |
| abstract_inverted_index.halo. | 312 |
| abstract_inverted_index.hosts | 227 |
| abstract_inverted_index.log(M | 204 |
| abstract_inverted_index.model | 117 |
| abstract_inverted_index.pair, | 109 |
| abstract_inverted_index.range | 15, 197 |
| abstract_inverted_index.their | 287 |
| abstract_inverted_index.them, | 80 |
| abstract_inverted_index.three | 103 |
| abstract_inverted_index.using | 22 |
| abstract_inverted_index.which | 180 |
| abstract_inverted_index.width | 173, 272 |
| abstract_inverted_index.∼3% | 168 |
| abstract_inverted_index.Legacy | 27, 125 |
| abstract_inverted_index.across | 183 |
| abstract_inverted_index.active | 239 |
| abstract_inverted_index.arcsec | 162 |
| abstract_inverted_index.detect | 87 |
| abstract_inverted_index.direct | 37 |
| abstract_inverted_index.energy | 115 |
| abstract_inverted_index.finite | 156 |
| abstract_inverted_index.galaxy | 91, 108, 113 |
| abstract_inverted_index.impact | 93 |
| abstract_inverted_index.level. | 78 |
| abstract_inverted_index.likely | 285 |
| abstract_inverted_index.matter | 311 |
| abstract_inverted_index.mostly | 237 |
| abstract_inverted_index.offset | 293 |
| abstract_inverted_index.probed | 185 |
| abstract_inverted_index.quasar | 45 |
| abstract_inverted_index.range. | 187 |
| abstract_inverted_index.search | 1 |
| abstract_inverted_index.strong | 59, 147 |
| abstract_inverted_index.unWISE | 134 |
| abstract_inverted_index.within | 308 |
| abstract_inverted_index.∼3.5 | 178 |
| abstract_inverted_index.Imaging | 28, 126 |
| abstract_inverted_index.Surveys | 29 |
| abstract_inverted_index.average | 211, 291 |
| abstract_inverted_index.between | 294 |
| abstract_inverted_index.exhibit | 194, 238 |
| abstract_inverted_index.imaging | 23, 135 |
| abstract_inverted_index.measure | 31 |
| abstract_inverted_index.nebular | 40, 72, 152, 235 |
| abstract_inverted_index.origin. | 289 |
| abstract_inverted_index.remains | 181 |
| abstract_inverted_index.spectra | 46 |
| abstract_inverted_index.stellar | 199 |
| abstract_inverted_index.survey. | 50 |
| abstract_inverted_index.systems | 241 |
| abstract_inverted_index.absorber | 89, 144, 226, 299 |
| abstract_inverted_index.best-fit | 112 |
| abstract_inverted_index.covering | 263 |
| abstract_inverted_index.diameter | 163 |
| abstract_inverted_index.emission | 41, 153, 236 |
| abstract_inverted_index.galaxies | 4, 193 |
| abstract_inverted_index.infrared | 131 |
| abstract_inverted_index.redshift | 14, 33, 186 |
| abstract_inverted_index.selected | 228 |
| abstract_inverted_index.specific | 283 |
| abstract_inverted_index.spectral | 114 |
| abstract_inverted_index.strength | 255 |
| abstract_inverted_index.suggests | 259, 300 |
| abstract_inverted_index.surveys, | 127 |
| abstract_inverted_index.surveys. | 136 |
| abstract_inverted_index.systems, | 245 |
| abstract_inverted_index.velocity | 292 |
| abstract_inverted_index.absorbers | 11, 56, 104 |
| abstract_inverted_index.detection | 38, 138 |
| abstract_inverted_index.formation | 213 |
| abstract_inverted_index.fraction. | 264 |
| abstract_inverted_index.including | 102, 242 |
| abstract_inverted_index.increases | 164 |
| abstract_inverted_index.starburst | 244 |
| abstract_inverted_index.)≤11.11, | 208 |
| abstract_inverted_index.absorbers, | 85 |
| abstract_inverted_index.absorption | 254 |
| abstract_inverted_index.associated | 5, 57, 105, 189 |
| abstract_inverted_index.background | 44 |
| abstract_inverted_index.correlates | 278 |
| abstract_inverted_index.emissions, | 73 |
| abstract_inverted_index.equivalent | 172, 271 |
| abstract_inverted_index.increasing | 171 |
| abstract_inverted_index.indicating | 286 |
| abstract_inverted_index.low-impact | 257 |
| abstract_inverted_index.parameters | 94, 258 |
| abstract_inverted_index.positively | 277 |
| abstract_inverted_index.suppressed | 250 |
| abstract_inverted_index.intervening | 8 |
| abstract_inverted_index.photometric | 121 |
| abstract_inverted_index.distribution | 116 |
| abstract_inverted_index.star-forming | 240 |
| abstract_inverted_index.supplemented | 128 |
| abstract_inverted_index.near-constant | 182, 253 |
| abstract_inverted_index.multi-passband | 120 |
| cited_by_percentile_year.max | 97 |
| cited_by_percentile_year.min | 95 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 7 |
| citation_normalized_percentile.value | 0.90639634 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |