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相关论文: Through a Lens Darkly: Evidence for Dusty Gravitat…

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Recent observations suggest appreciable star formation activity in early-type galaxies down to redshift $z\sim 0.5$. If so, there is likely to be dust in these galaxies. We consider the possibility that obscuration by dust can reconcile the…

天体物理学 · 物理学 2007-05-23 M. Fukugita , P. J. E. Peebles

Context. Observations of quasars shining through foreground galaxies, offer a way to probe the dust extinction curves of distant galaxies. Interesting objects for this study are found in strong gravitational lensing systems, where the…

天体物理学 · 物理学 2009-11-13 Linda Ostman , Ariel Goobar , Edvard Mortsell

We determine 37 differential extinctions in 23 gravitational lens galaxies over the range 0 < z_l < 1. Only 7 of the 23 systems have spectral differences consistent with no differential extinction. The median differential extinction for the…

天体物理学 · 物理学 2009-10-31 E. E. Falco , C. D. Impey , C. S. Kochanek , J. Lehar , B. A. McLeod , H-W. Rix , C. R. Keeton , J. A. Munoz , C. Y. Peng

Gravitational lensing directly measures mass density fluctuations along the lines of sight to very distant objects. No assumptions need to be made concerning bias, the ratio of fluctuations in galaxy density to mass density. Hence, lensing…

天体物理学 · 物理学 2007-05-23 Joachim Wambsganss , Renyue Cen , Jeremiah P. Ostriker

Gravitational lensing of a quasar by a spiral galaxy should often be accompanied by damped Lyman-alpha absorption and dust extinction due to the intervening gaseous disk. In nearly edge-on configurations, the surface mass density of the gas…

天体物理学 · 物理学 2009-10-30 Matthias Bartelmann , Abraham Loeb

Submillimeter (and in some cases millimeter) wavelength continuum measurements are presented for a sample of 40 active galactic nuclei (probably all quasars) lensed by foreground galaxies. The object of this study is to use the lensing…

天体物理学 · 物理学 2009-11-07 Richard Barvainis , Rob Ivison

In a recent paper, Hawkins (1997) argues on the basis of statistical studies of double-image gravitational lenses and lens candidates that a large population of dark lenses exists and that these outnumber galaxies with more normal…

We show that most gravitational lenses lie on the passively evolving fundamental plane for early-type galaxies. For burst star formation models (1 Gyr of star formation, then quiescence) in low Omega_0 cosmologies, the stellar populations…

天体物理学 · 物理学 2009-10-31 C. S. Kochanek , E. E. Falco , C. D. Impey , J. Lehar , B. A. McLeod , H. -W. Rix

We present near infrared observations of the red gravitational lens system MG0414+0534. Our images are of sufficient quality to allow photometry of all four QSO images and the lens galaxy. The observations show that the K-band brightnesses…

天体物理学 · 物理学 2009-10-30 B. A. McLeod , G. M. Bernstein , M. J. Rieke , D. W. Weedman

Unless properly corrected for, the existence of intergalactic dust will introduce a redshift dependent magnitude offset to standard candle sources. This would lead to overestimated luminosity distances compared to a dust-free universe and…

宇宙学与河外天体物理 · 物理学 2015-06-11 Joel Johansson , Edvard Mortsell

We investigate the luminosity and redshift dependence of the quasar continuum by means of composite spectrum using a large non-BAL radio-quiet quasar sample drawn from the Sloan Digital Sky Survey. Quasar continuum slopes in the UV-Opt band…

宇宙学与河外天体物理 · 物理学 2015-06-24 Xiaoyi Xie , Shiyin Shen , Zhengyi Shao , Jun Yin

The last decade has shown a considerable development of gravitational lensing for cosmology because it probes the amount and the nature of dark matter, and provides information on the density parameter $\Omega$, the cosmological constant…

天体物理学 · 物理学 2007-05-23 Y. Mellier , F. Bernardeau , L. van Waerbeke

Very deep imaging data of three optically luminous radio-loud quasars with redshifts between z=0.9 and z=1.36 are presented. The data are complete for galaxies down to R=26. There is no evidence for excess numbers of galaxies around the…

天体物理学 · 物理学 2007-05-23 J. W. Fried

The light we observe from distant astrophysical objects including supernovae and quasars allows us to determine large distances in terms of a cosmological model. Despite the success of the standard cosmological model in fitting the data,…

宇宙学与河外天体物理 · 物理学 2024-05-07 Angela L. H. Ng

The exploration of the redshift drift, a direct measurement of cosmological expansion, is expected to take several decades of observation with stable, sensitive instruments. We introduced a new method to probe cosmology which bypasses the…

宇宙学与河外天体物理 · 物理学 2023-08-16 Chengyi Wang , Krzysztof Bolejko , Geraint F. Lewis

As the Universe expands, the redshift of distant sources changes with time. Here we discuss gravitational lensing phenomena that are consequence of the redshift drift between lensed source, gravitational lens, and observer. When the source…

宇宙学与河外天体物理 · 物理学 2022-06-01 Giovanni Covone , Mauro Sereno

We report Hubble Space Telescope observations of 6 gravitational lenses with the Advanced Camera for Surveys. We measured the flux ratios between the lensed images in 6 filters from 8140\AA\ to 2200\AA. In 3 of the systems, HE0512$-$3329,…

宇宙学与河外天体物理 · 物理学 2015-05-30 José A. Muñoz , Evencio Mediavilla , Christopher S. Kochanek , Emilio Falco , Ana María Mosquera

LISA might detect gravitational waves from mergers of massive black hole binaries strongly lensed by intervening galaxies (Sereno et al. 2010). The detection of multiple gravitational lensing events would provide a new tool for cosmography.…

宇宙学与河外天体物理 · 物理学 2015-05-27 M. Sereno , Ph. Jetzer , A. Sesana , M. Volonteri

A majority of quasar surveys have been based on criteria which assume strong blue continua or a UV-excess. Any amount of dust along the line-of-sight is expected to drastically extinguish the optical/UV flux leading to a selection bias.…

天体物理学 · 物理学 2007-05-23 Frank J. Masci

The observed properties of high redshift galaxies depend on the underlying foreground distribution of large scale structure, which distorts their intrinsic properties via gravitational lensing. We focus on the regime where the dominant…

宇宙学与河外天体物理 · 物理学 2015-06-30 Anastasia Fialkov , Abraham Loeb
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