2MASS J13503888-2512167 , the SIMBAD biblio

2MASS J13503888-2512167 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST22:53:35


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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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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.

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