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| 2MASS J13503888-2512167 , the SIMBAD biblio (15 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST22:53:35 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2008A&A...491..465D | 40 | 48 | An unbiased measurement of the UV background and its evolution via the proximity effect in quasar spectra. | DALL'AGLIO A., WISOTZKI L. and WORSECK G. | |||||
|
2016MNRAS.456.3509K |
20 | 1 | Evidence of bimodal physical properties of intervening, optically thin C III absorbers at z ∼ 2.5. | KIM T.-S., CARSWELL R.F. and RANQUIST D. | |||||
|
2017MNRAS.465.2120C |
16 | D | 1 | 227 | 130 | Correcting C IV-based virial black hole masses. | COATMAN L., HEWETT P.C., BANERJI M., et al. | ||
|
2017AJ....154..114O |
16 | D | 2 | 298 | 26 | The second data release of the KODIAQ survey. | O'MEARA J.M., LEHNER N., HOWK J.C., et al. | ||
|
2019MNRAS.482.3458M |
16 | D | 1 | 472 | 60 | The UVES Spectral Quasar Absorption Database (SQUAD) data release 1: the first 10 million seconds. | MURPHY M.T., KACPRZAK G.G., SAVORGNAN G.A.D., et al. | ||
| 2019MNRAS.484.5028M | 16 | D | 3 | 11 | ~ | Physical conditions in high-z optically thin C III absorbers: origin of cloud sizes and associated correlations. | MOHAPATRA A., SRIANAND R., KHAIRE V., et al. | ||
|
2019MNRAS.488.4690C |
97 | D | C | 6 | 81 | ~ | Probing quasar winds using intrinsic narrow absorption lines. | CULLITON C., CHARLTON J., ERACLEOUS M., et al. | |
| 2019ApJ...887..205T | 16 | D | 1 | 47 | ~ | Thermal state of the intergalactic medium at z ∼ 2-4. | TELIKOVA K.N., SHTERNIN P.S. and BALASHEV S.A. | ||
|
2020ApJ...904...28C |
16 | D | 1 | 247 | 9 | Mg II absorbers in high-resolution quasar spectra. I. Voigt profile models. | CHURCHILL C.W., EVANS J.L., STEMOCK B., et al. | ||
| 2021MNRAS.501.5811K | 17 | D | 1 | 84 | 11 | The evolution of the low-density H I intergalactic medium from z = 3.6 to 0: data, transmitted flux, and H I column density,+,++. | KIM T.-S., WAKKER B.P., NASIR F., et al. | ||
|
2021MNRAS.506.4389G |
17 | D | 1 | 104 | 43 | A consistent and robust measurement of the thermal state of the IGM at 2 <= z <= 4 from a large sample of Ly α forest spectra: evidence for late and rapid He II reionization. | GAIKWAD P., SRIANAND R., HAEHNELT M.G., et al. | ||
|
2022MNRAS.509.1536M |
17 | D | 1 | 287 | ~ | Measurement of redshift-space two- and three-point correlation of Lyα absorbers at 1.7 < z < 3.5: implications on evolution of the physical properties of IGM. | MAITRA S., SRIANAND R. and GAIKWAD P. | ||
| 2022MNRAS.512.2389D | 17 | D | 1 | 143 | 10 | The evolution of the Si IV content in the Universe from the epoch of reionization to cosmic noon. | D'ODORICO V., FINLATOR K., CRISTIANI S., et al. | ||
| 2022ApJS..261...30M | 187 | D | X | 5 | 49 | 5 | The Intermediate-ionization Lines as Virial Broadening Estimators for Population A Quasars. | MARZIANI P., DEL OLMO A., NEGRETE C.A., et al. | |
|
2024A&A...691A..15D |
18 | D | 2 | 144 | ~ | Exploring the links between quasar winds and radio emission along the main sequence at high redshift. | DECONTO-MACHADO A., DEL OLMO A. and MARZIANI P. |