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| DES J021822.52-043035.8 , the SIMBAD biblio (5 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST01:40:23 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2013AJ....145...47M | 15 | D | 1 | 27 | 36 | Nebular attenuation in Hα-selected star-forming galaxies at z = 0.8 from the NewHα survey. | MOMCHEVA I.G., LEE J.C., LY C., et al. | ||
2015AJ....149...79D 
|
16 | D | 1 | 298 | 36 | The relationship between stellar mass, gas metallicity, and star formation rate for Hα-selected galaxies at z ≈ 0.8 from the NewHα survey. | DE LOS REYES M.A., LY C., LEE J.C., et al. | ||
| 2020MNRAS.496.3636G | 2330 | A | X C | 56 | 4 | ~ | Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability. | GUO H., BURKE C.J., LIU X., et al. | |
|
2021Sci...373..789B
|
17 | D | 1 | 344 | 46 | A characteristic optical variability time scale in astrophysical accretion disks. | BURKE C.J., SHEN Y., BLAES O., et al. | ||
| 2024ApJ...975..160R | 108 | D | X | 3 | 120 | ~ | How Long Will the Quasar UV/Optical Flickering Be Damped? II. The Observational Test. | REN G., ZHOU S., SUN M., et al. |
