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| HSCS J223947+020747 , the SIMBAD biblio (28 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST22:45:46 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018ApJ...869..150M | 17 | D | 1 | 111 | 151 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar luminosity function and contribution to cosmic reionization at z = 6. | MATSUOKA Y., STRAUSS M.A., KASHIKAWA N., et al. | ||
| 2018PASJ...70S..35M | 17 | D | 1 | 66 | 104 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8. | MATSUOKA Y., ONOUE M., KASHIKAWA N., et al. | ||
| 2019ApJ...880...77O | 713 | D | X C | 17 | 13 | 89 | Subaru high-z exploration of low-luminosity quasars (SHELLQs). VI. Black hole mass Measurements of six quasars at 6.1 <= z <= 6.7. | ONOUE M., KASHIKAWA N., MATSUOKA Y., et al. | |
|
2019MNRAS.490.2542P |
16 | D | 1 | 2245 | ~ | Unveiling the weak radio quasar population at z≥4. | PERGER K., FREY S., GABANYI K.E., et al. | ||
| 2019PASJ...71..111I | 1278 | D | X C | 31 | 16 | 53 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). VIII. A less biased view of the early co-evolution of black holes and host galaxies. | IZUMI T., ONOUE M., MATSUOKA Y., 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. | ||
| 2020ApJ...903...60I | 140 | D | X | 4 | 39 | 13 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity zone analysis for faint quasar spectra at z ∼ 6. | ISHIMOTO R., KASHIKAWA N., ONOUE M., et al. | |
| 2021ApJ...908..124L | 17 | D | 1 | 38 | 28 | Constraining the quasar radio-loud fraction at z ∼ 6 with deep radio observations. | LIU Y., WANG R., MOMJIAN E., et al. | ||
| 2021ApJ...908..235I | 85 | X | 2 | 7 | 11 | Subaru high-z exploration of low-luminosity quasars (SHELLQs). XII. Extended [C II] structure (merger or outflow) in a z = 6.72 Red quasar. | IZUMI T., ONOUE M., MATSUOKA Y., et al. | ||
| 2021ApJ...914...36I | 44 | X | 1 | 15 | 33 | Subaru high-z exploration of low-luminosity quasars (SHELLQs). XIII. Large-scale feedback and star formation in a low-luminosity quasar at z = 7.07 on the local black hole to host mass relation. | IZUMI T., MATSUOKA Y., FUJIMOTO S., et al. | ||
| 2021ApJ...914L..26F | 20 | D | 1 | 10 | 33 | Seeding supermassive black holes with self-interacting dark matter: a unified scenario with baryons. | FENG W.-X., YU H.-B. and ZHONG Y.-M. | ||
|
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. | ||
|
2022ApJS..259...20H |
17 | D | 1 | 1042 | 83 | GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. | HARIKANE Y., ONO Y., OUCHI M., et al. | ||
| 2022MNRAS.517.1264L | 102 | D | F | 2 | 94 | 3 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) - XV. Constraining the cosmic reionization at 5.5 < z < 7. | LU T.-Y., GOTO T., HASHIMOTO T., et al. | |
|
2022ApJ...941..106F |
17 | D | 1 | 120 | 26 | The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars. | FARINA E.P., SCHINDLER J.-T., WALTER F., et al. | ||
| 2023ApJ...953..180S | 1332 | A | X C | 30 | 16 | ~ | Detection of the Low-stellar-mass Host Galaxy of a z ∼ 6.25 Quasar with JWST. | STONE M.A., LYU J., RIEKE G.H., et al. | |
| 2023ApJ...954..164T | 17 | D | 1 | 106 | ~ | Modeling the Central Supermassive Black Hole Mass of Quasars via the LSTM Approach. | TABASI S.S., SALMANI R.V., KHALILIYAN P., et al. | ||
| 2024ApJ...960..112T | 134 | X F | 2 | 13 | ~ | Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at z ∼ 6 Estimated via Spectral Comparison with Low-z Quasars. | TAKAHASHI A., MATSUOKA Y., ONOUE M., 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. | ||
| 2024ApJ...964...90S | 1138 | D | X C | 25 | 12 | ~ | Undermassive Host Galaxies of Five z ∼ 6 Luminous Quasars Detected with JWST. | STONE M.A., LYU J., RIEKE G.H., et al. | |
| 2024MNRAS.530.4765B | 45 | X | 1 | 6 | ~ | Simulated host galaxy analogues of high-z quasars observed with JWST. | BERGER S., MARSHALL M.A., WYITHE J.S.B., et al. | ||
| 2024MNRAS.531.4584S | 18 | D | 1 | 22 | ~ | Diagnosing the massive-seed pathway to high-redshift black holes: statistics of the evolving black hole to host galaxy mass ratio. | SCOGGINS M.T. and HAIMAN Z. | ||
| 2025MNRAS.536.3177A | 19 | D | 1 | 93 | ~ | Deciphering the origins and growth of supermassive black holes. | AGGARWAL Y. | ||
| 2025A&A...693A.176B | 93 | C | 1 | 3 | ~ | JWST ERS Program Q3D: The pitfalls of virial black hole mass constraints shown for a z ∼ 3 quasar with an ultramassive host. | BERTEMES C., WYLEZALEK D., RUPKE D.S.N., et al. | ||
| 2025ApJ...979..183I | 19 | D | 1 | 73 | ~ | Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XXI. Candidate Red Quasars at z ≥ 6 from Near-infrared Photometry. | IWAMOTO R., MATSUOKA Y., IMANISHI M., et al. | ||
| 2025ApJ...981L..20L | 2361 | A | S X C | 49 | 4 | ~ | Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn. | LYU J., RIEKE G.H., STONE M., et al. | |
| 2025ApJ...981...19L | 47 | X | 1 | 23 | ~ | Tip of the Iceberg: Overmassive Black Holes at 4 < z < 7 Found by JWST Are Not Inconsistent with the Local ${{ \mathcal M }}_{\mathrm{BH}}-{{ \mathcal M }}_{\star }$ Relation. | LI J., SILVERMAN J.D., SHEN Y., et al. | ||
| 2025ApJ...983..165S | 47 | X | 1 | 33 | ~ | Evolution of the M∗-MBH Relation from z ∼ 6 to the Present Epoch. | SUN Y., RIEKE G.H., LYU J., et al. |