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| SDSS J103516.20+142200.6 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:18:55 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
2014A&A...563A..54P |
15 | D | 1 | 168926 | 217 | The Sloan Digital Sky Survey quasar catalog: tenth data release. | PARIS I., PETITJEAN P., AUBOURG E., et al. | ||
|
2017A&A...597A..79P |
16 | D | 1 | 302147 | 367 | The Sloan Digital Sky Survey Quasar Catalog: Twelfth data release. | PARIS I., PETITJEAN P., ROSS N.P., et al. | ||
|
2018ApJS..235...11C |
16 | D | 2 | 190674 | 1 | The associated absorption features in quasar spectra of the Sloan Digital Sky Survey. I. Mg II absorption doublets. | CHEN Z.-F., HUANG W.-R., PANG T.-T., et al. | ||
|
2018A&A...613A..51P |
16 | D | 1 | 525784 | 350 | The Sloan Digital Sky Survey Quasar Catalog: Fourteenth data release. | PARIS I., PETITJEAN P., AUBOURG E., et al. | ||
| 2019Natur.573...83Z | 1180 | X | 29 | 7 | 15 | Fast inflows as the adjacent fuel of supermassive black hole accretion disks in quasars. | ZHOU H., SHI X., YUAN W., et al. | ||
|
2020ApJS..249...17R |
16 | D | 1 | 525797 | 112 | Spectral properties of quasars from Sloan Digital Sky Survey data release 14: the catalog. | RAKSHIT S., STALIN C.S. and KOTILAINEN J. | ||
|
2020ApJS..250....8L |
16 | D | 1 | 750061 | 219 | The Sloan Digital Sky Survey quasar catalog: Sixteenth Data Release. | LYKE B.W., HIGLEY A.N., McLANE J.N., et al. | ||
| 2021ApJ...916...86L | 209 | X | 5 | 11 | ~ | Feeding the accretion disk from the dusty torus in a reddened quasar. | LI G., SHI X., TIAN Q., et al. | ||
| 2022A&A...659A.103C | 43 | X | 1 | 10 | 1 | Detections of inflowing gas from narrow absorption lines at parsec scales. | CHEN Z.-F., GU M., HE Z., et al. | ||
| 2025ApJ...995..113S | 47 | X | 1 | 4 | ~ | Fast Inflowing Ionized Absorber Tracing the Gas Dynamics at Subparsec Scale around Mrk 3. | SHI F., GUAINAZZI M. and WANG Y. |