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| VDES J0454-4448 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST18:28:20 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2015MNRAS.454.3952R | 762 | T K A | D | S X C | 17 | 1 | 42 |
DES J0454-4448: discovery of the first luminous z ≥ 6 quasar from the Dark Energy Survey. |
REED S.L., McMAHON R.G., BANERJI M., et al. |
|
2016ApJ...819...24W |
16 | D | 1 | 796 | 79 | A survey of luminous high-redshift quasars with SDSS and WISE. I. Target selection and optical spectroscopy. | WANG F., WU X.-B., FAN X., et al. | ||
| 2016MNRAS.460.1270D | 45 | X | 1 | 47 | 645 | The Dark Energy Survey: more than dark energy - an overview. | DARK ENERGY SURVEY COLLABORATION, ABBOTT T., ABDALLA F.B., et al. | ||
|
2016ApJS..227...11B |
16 | D | 1 | 173 | 283 | The Pan-STARRS1 distant z > 5.6 quasar survey: more than 100 quasars within the first Gyr of the Universe. | BANADOS E., VENEMANS B.P., DECARLI R., et al. | ||
| 2017MNRAS.468.4702R | 416 | D | S X C | 9 | 13 | 94 | Eight new luminous z ≥ 6 quasars discovered via SED model fitting of VISTA, WISE and Dark Energy Survey Year 1 observations. | REED S.L., McMAHON R.G., MARTINI P., et al. | |
| 2018ApJ...854...97D | 221 | D | X | 6 | 50 | 209 | An ALMA [C II] survey of 27 quasars at z > 5.94. | DECARLI R., WALTER F., VENEMANS B.P., et al. | |
| 2018ApJ...864...53E | 42 | X | 1 | 49 | 104 | The opacity of the intergalactic medium measured along quasar sightlines at z ∼ 6. | EILERS A.-C., DAVIES F.B. and HENNAWI J.F. | ||
| 2018MNRAS.479.1055B | 98 | D | F | 2 | 60 | 137 | New constraints on Lyman-α opacity with a sample of 62 quasars at z > 5.7. | BOSMAN S.E.I., FAN X., JIANG L., et al. | |
| 2018ApJ...866..159V | 16 | D | 2 | 98 | 72 | Dust emission in an accretion-rate-limited sample of z >= 6 quasars. | VENEMANS B.P., DECARLI R., WALTER F., et al. | ||
| 2018ApJ...867..153C | 16 | D | 2 | 54 | 13 | No evidence for millimeter continuum source overdensities in the environments of z >= 6 quasars. | CHAMPAGNE J.B., DECARLI R., CASEY C.M., et al. | ||
| 2019ApJ...882...77C | 16 | D | 1 | 73 | 40 | Heavy element absorption systems at 5.0 < z < 6.8: metal-poor neutral gas and a diminishing signature of highly ionized circumgalactic matter. | COOPER T.J., SIMCOE R.A., COOKSEY K.L., et al. | ||
|
2019A&A...630A..59B |
17 | D | 2 | 51 | 69 | Widespread QSO-driven outflows in the early Universe. | BISCHETTI M., MAIOLINO R., CARNIANI S., et al. | ||
|
2019A&A...631A..78S |
16 | D | 2 | 27 | ~ | A spectral stacking analysis to search for faint outflow signatures in z ∼ 6 quasars. | STANLEY F., JOLLY J.B., KONIG S., et al. | ||
|
2020MNRAS.494..789R |
16 | D | 1 | 489 | 25 | The near and mid-infrared photometric properties of known redshift z >= 5 quasars. | ROSS N.P. and CROSS N.J.G. | ||
| 2020A&A...637A..84P | 17 | D | 1 | 32 | 48 | The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies. | PENSABENE A., CARNIANI S., PERNA M., et al. | ||
| 2021MNRAS.503.2349D | 17 | D | 1 | 39 | 20 | Infrared emission of z ∼ 6 galaxies: AGN imprints. | DI MASCIA F., GALLERANI S., BEHRENS C., et al. | ||
| 2021MNRAS.506.3946D | 17 | D | 1 | 41 | 13 | The dust attenuation law in z ∼ 6 quasars. | DI MASCIA F., GALLERANI S., FERRARA A., et al. | ||
| 2021A&A...654A..79G | 18 | D | 2 | 3 | 3 | Quasar clustering at redshift 6. | GREINER J., BOLMER J., YATES R.M., et al. | ||
|
2021A&A...656A.137G |
17 | D | 1 | 493 | 12 | Low frequency radio properties of the z > 5 quasar population. | GLOUDEMANS A.J., DUNCAN K.J., ROTTGERING H.J.A., et al. | ||
| 2024MNRAS.528..499L | 18 | D | 1 | 192 | ~ | [C II] 158 μm emission as an indicator of galaxy star formation rate. | LIANG L., FELDMANN R., MURRAY N., et al. | ||
| 2024MNRAS.530..870B | 18 | D | 2 | 15 | ~ | Quasar Island - three new z ∼ 6 quasars, including a lensed candidate, identified with contrastive learning. | BYRNE X., MEYER R.A., FARINA E.P., et al. |