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[CL2003] PKS 0439-433 1 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST08:20:13 |
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 |
---|---|---|---|---|---|---|---|---|---|
2001ApJ...560...92C | 10 | 22 | Mg II absorber number density at z≃0.05: implications for ΩDLA evolution. | CHURCHILL C.W. | |||||
2003A&A...399..857K | 44 | 118 | A deep search for 21-cm absorption in high redshift damped Lyman-α systems. | KANEKAR N. and CHENGALUR J.N. | |||||
2003A&A...412..707R | 829 | 11 | A catalogue of absorption-line systems in QSO spectra. | RYABINKOV A.I., KAMINKER A.D. and VARSHALOVICH D.A. | |||||
2003ApJ...597..706C | 1 | 25 | 106 | The nature of damped Lyα absorbing galaxies at z ≤ 1: a photometric redshift survey of damped Lyα absorbers. | CHEN H.-W. and LANZETTA K.M. | ||||
2004MNRAS.352.1291P | 36 | 15 | Classical and MgII-selected damped Lyman α absorbers: impact on ΩHI at z < 1.7. | PEROUX C., DEHARVENG J.-M., LE BRUN V., et al. | |||||
2005ApJ...620..703C | 3 | 11 | 127 | Abundance profiles and kinematics of damped Lyα absorbing galaxies at z < 0.65(1,)(2,). | CHEN H.-W., KENNICUTT R.C.Jr and RAUCH M. | ||||
2005MNRAS.356.1509C | 44 | 34 | Spin temperatures and covering factors for HI 21-cm absorption in damped Lyman α systems. | CURRAN S.J., MURPHY M.T., PIHLSTROEM Y.M., et al. | |||||
2005MNRAS.364.1467Z | 1 | 36 | 185 | Reconciling the local galaxy population with damped Lyman α cross-sections and metal abundances. | ZWAAN M.A., VAN DER HULST J.M., BRIGGS F.H., et al. | ||||
2006MNRAS.371..356C | 39 | 25 | The detectability of HI 21-cm absorption in damped Lyman α systems. | CURRAN S.J. and WEBB J.K. | |||||
2007MNRAS.379.1409Z | 15 | D | 1 | 17 | 12 | The host galaxies of strong CaII quasar absorption systems at z < 0.5. | ZYCH B.J., MURPHY M.T., PETTINI M., et al. | ||
2009A&A...505..385A | 15 | D | 1 | 99836 | 35 | The large quasar reference frame (LQRF). An optical representation of the ICRS. | ANDREI A.H., SOUCHAY J., ZACHARIAS N., et al. |