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[MFD95] Lensing G , the SIMBAD biblio (23 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST09:04:50 |
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 |
---|---|---|---|---|---|---|---|---|---|
1995ApJ...447L...5M | 5 | 7 | 155 | 1608+656 : a quadruple-lens system found in the CLASS gravitational lens survey. | MYERS S.T., FASSNACHT C.D., DJORGOVSKI S.G., et al. | ||||
1997ApJ...475..457I | 19 | 48 | A measurement of the cosmological constant using elliptical galaxies as strong gravitational lenses. | IM M., GRIFFITHS R.E. and RATNATUNGA K.U. | |||||
1998A&A...334L..33J | 24 | 35 | Lensing galaxies: light or dark? | JACKSON N., HELBIG P., BROWNE I., et al. | |||||
2003ApJ...587..143R | 62 | 134 | The evolution of a mass-selected sample of early-type field galaxies. | RUSIN D., KOCHANEK C.S., FALCO E.E., et al. | |||||
2003ApJ...595...29R | 45 | 130 | Self-similar models for the mass profiles of early-type lens galaxies. | RUSIN D., KOCHANEK C.S. and KEETON C.R. | |||||
2003MNRAS.344..924V | 34 | 54 | The Fundamental Plane and the evolution of the M/L ratio of early-type field galaxies up to z ∼ 1. | VAN DE VEN G., VAN DOKKUM P.G. and FRANX M. | |||||
2005ApJ...623L...5F | 42 | 66 | Stellar and total mass in early-type lensing galaxies. | FERRERAS I., SAHA P. and WILLIAMS L.L.R. | |||||
2005ApJ...625..633D | 23 | 13 | Chandra observations of the gravitational lenses B1600+434 and B1608+656. | DAI X. and KOCHANEK C.S. | |||||
2005ApJ...630..764C | 44 | 13 | Constraints on the velocity dispersion function of early-type galaxies from the statistics of strong gravitational lensing. | CHAE K.-H. | |||||
2006ApJ...642...30F | 2 | 12 | 59 | Mass along the line of sight to the gravitational lens B1608+656: galaxy groups and implications for H0. | FASSNACHT C.D., GAL R.R., LUBIN L.M., et al. | ||||
2006MNRAS.366...39S | 8 | 15 | The anatomy of a quadruply imaged gravitational lens system. | SUYU S.H. and BLANDFORD R.D. | |||||
2006ApJ...650L..17S | 1 | 24 | 51 | The Hubble time inferred from 10 time delay lenses. | SAHA P., COLES J., MACCIO A.V., et al. | ||||
2006ApJ...651..667F | 2 | 4 | 16 | Three gravitational lenses for the price of one: enhanced strong lensing through galaxy clustering. | FASSNACHT C.D., McKEAN J.P., KOOPMANS L.V.E., et al. | ||||
2007ApJ...660....1O | 1 | 46 | 156 | Gravitational lens time delays: a statistical assessment of lens model dependences and implications for the global Hubble constant. | OGURI M. | ||||
2008ApJ...681.1017F | 35 | 21 | The X-ray properties of moderate-redshift galaxy groups selected by association with gravitational lenses. | FASSNACHT C.D., KOCEVSKI D.D., AUGER M.W., et al. | |||||
2011ApJ...740...97L | 553 | D | X C | 14 | 27 | 23 | Resolving the baryon-fraction profile in lensing galaxies. | LEIER D., FERRERAS I., SAHA P., et al. | |
2012MNRAS.424..104L | 39 | X | 1 | 22 | 8 | Diagnostics of baryonic cooling in lensing galaxies. | LEIER D., FERRERAS I. and SAHA P. | ||
2012ApJ...755...31C | 15 | D | 1 | 313 | 26 | Testing the dark energy with gravitational lensing statistics. | CAO S., COVONE G. and ZHU Z.-H. | ||
2014MNRAS.437..600S | 173 | D | X | 5 | 40 | 30 | Hubble constant and dark energy inferred from free-form determined time delay distances. | SERENO M. and PARAFICZ D. | |
2015ApJS..219...29M | 16 | D | 1 | 10653 | 17 | A spectroscopic survey of the fields of 28 strong gravitational lenses. | MOMCHEVA I.G., WILLIAMS K.A., COOL R.J., et al. | ||
2019MNRAS.486.5046W | 17 | D | 1 | 3 | ~ | The Hubble-Lemaitre constant and sound horizon from low-redshift probes. | WOJTAK R. and AGNELLO A. | ||
2020PASP..132d4501T | 1 | 11 | ~ | Comparison of multi-class and binary classification machine learning models in identifying strong gravitational lenses. | TEIMOORINIA H., TOYONAGA R.D., FABBRO S., et al. | ||||
2020ApJ...897..127W | 145 | D | X | 4 | 14 | ~ | Cosmology-independent estimate of the Hubble constant and spatial curvature using time-delay lenses and quasars. | WEI J.-J. and MELIA F. |