14 results on '"Shajib, A. J."'
Search Results
2. XI. New lensing galaxy redshift and velocity dispersion measurements from Keck spectroscopy of eight lensed quasar systems.
- Author
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Mozumdar, P., Fassnacht, C. D., Treu, T., Spiniello, C., and Shajib, A. J.
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VELOCITY measurements ,GALACTIC redshift ,QUASARS ,HUBBLE constant ,IMAGING systems ,SIGNAL-to-noise ratio - Abstract
We have measured the redshifts and single-aperture velocity dispersions of eight lens galaxies using the data collected by the Echellette Spectrograph and Imager (ESI) and Low Resolution Imaging Spectrometer (LRIS) at W.M. Keck observatory on different observing nights spread over three years (2018-2020). These results, combined with other ancillary data, such as high-resolution images of the lens systems, and time delays, are necessary to increase the sample size of the quasar-galaxy lens systems for which the Hubble constant can be measured, using the time-delay strong lensing method, hence increasing the precision of its inference. Typically, the 2D spectra of the quasar-galaxy lens systems get spatially blended due to seeing by ground-based observations. As a result, the extracted lensing galaxy (deflector) spectra become significantly contaminated by quasar light, which affects the ability to extract meaningful information about the deflector. To account for spatial blending and extract less contaminated and higher signal-to-noise ratio (S/N) 1D spectra of the deflectors, a forward modeling method has been implemented. From the extracted spectra, we have measured redshifts using prominent absorption lines and single aperture velocity dispersions using the penalized pixel fitting code ppxf. In this paper, we report the redshifts and single aperture velocity dispersions of eight lens galaxies - J0147+4630, B0445+123, B0631+519, J0659+1629, J08182613, J0924+0219, J1433+6007, and J1817+2729. Among these systems, six do not have previously measured velocity dispersions; for the other two, our measurements are consistent with previously reported values. Additionally, we have measured the previously unknown redshifts of the deflectors in J08182613 and J1817+2729 to be 0:866 ± 0:002 and 0:408 ± 0:002, respectively. [ABSTRACT FROM AUTHOR]
- Published
- 2023
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3. The Hubble Constant from Strongly Lensed Supernovae with Standardizable Magnifications.
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Birrer, Simon, Dhawan, Suhail, and Shajib, Anowar J.
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HUBBLE constant ,SUPERNOVAE ,GRAVITATIONAL lenses ,PHYSICAL cosmology ,TIME series analysis ,OBSERVATORIES - Abstract
The dominant uncertainty in the current measurement of the Hubble constant (H
0 ) with strong gravitational lensing time delays is attributed to uncertainties in the mass profiles of the main deflector galaxies. Strongly lensed supernovae (glSNe) can provide, in addition to measurable time delays, lensing magnification constraints when knowledge about the unlensed apparent brightness of the explosion is imposed. We present a hierarchical Bayesian framework to combine a data set of SNe that are not strongly lensed and a data set of strongly lensed SNe with measured time delays. We jointly constrain (i) H0 using the time delays as an absolute distance indicator, (ii) the lens model profiles using the magnification ratio of lensed and unlensed fluxes on the population level, and (iii) the unlensed apparent magnitude distribution of the SN population and the redshiftâ€"luminosity relation of the relative expansion history of the universe. We apply our joint inference framework on a future expected data set of glSNe and forecast that a sample of 144 glSNe of Type Ia with well-measured time series and imaging data will measure H0 to 1.5%. We discuss strategies to mitigate systematics associated with using absolute flux measurements of glSNe to constrain the mass density profiles. Using the magnification of SN images is a promising and complementary alternative to using stellar kinematics. Future surveys, such as the Rubin and Roman observatories, will be able to discover the necessary number of glSNe, and with additional follow-up observations, this methodology will provide precise constraints on mass profiles and H0 . [ABSTRACT FROM AUTHOR]- Published
- 2022
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4. Improved time-delay lens modelling and H0 inference with transient sources.
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Ding, Xuheng, Liao, Kai, Birrer, Simon, Shajib, Anowar J, Treu, Tommaso, and Yang, Lilan
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GRAVITATIONAL lenses ,QUASARS ,GAMMA ray bursts ,HUBBLE constant ,GRAVITATIONAL waves ,SPACE telescopes ,COSMOGRAPHY - Abstract
Strongly lensed explosive transients such as supernovae, gamma-ray bursts, fast radio bursts, and gravitational waves are very promising tools to determine the Hubble constant (H
0 ) in the near future in addition to strongly lensed quasars. In this work, we show that the transient nature of the point source provides an advantage over quasars: The lensed host galaxy can be observed before or after the transient's appearance. Therefore, the lens model can be derived from images free of contamination from bright point sources. We quantify this advantage by comparing the precision of a lens model obtained from the same lenses with and without point sources. Based on Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) observations with the same sets of lensing parameters, we simulate realistic mock data sets of 48 quasar lensing systems (i.e. adding AGN in the galaxy centre) and 48 galaxy–galaxy lensing systems (assuming the transient source is not visible but the time delay and image positions have been or will be measured). We then model the images and compare the inferences of the lens model parameters and H0 . We find that the precision of the lens models (in terms of the deflector mass slope) is better by a factor of 4.1 for the sample without lensed point sources, resulting in an increase of H0 precision by a factor of 2.9. The opportunity to observe the lens systems without the transient point sources provides an additional advantage for time-delay cosmography over lensed quasars. It facilitates the determination of higher signal-to-noise stellar kinematics of the main deflector, and thus its mass density profile, which, in turn plays a key role in breaking the mass-sheet degeneracy and constraining H0 . [ABSTRACT FROM AUTHOR]- Published
- 2021
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5. Time delay lens modelling challenge.
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Ding, X, Treu, T, Birrer, S, Chen, G C-F, Coles, J, Denzel, P, Frigo, M, Galan, A, Marshall, P J, Millon, M, More, A, Shajib, A J, Sluse, D, Tak, H, Xu, D, Auger, M W, Bonvin, V, Chand, H, Courbin, F, and Despali, G
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HUBBLE constant ,GRAVITATIONAL lenses ,DATA analysis ,MEASURING instruments ,TIME delay systems ,LENSES - Abstract
In recent years, breakthroughs in methods and data have enabled gravitational time delays to emerge as a very powerful tool to measure the Hubble constant H
0 . However, published state-of-the-art analyses require of order 1 yr of expert investigator time and up to a million hours of computing time per system. Furthermore, as precision improves, it is crucial to identify and mitigate systematic uncertainties. With this time delay lens modelling challenge, we aim to assess the level of precision and accuracy of the modelling techniques that are currently fast enough to handle of order 50 lenses, via the blind analysis of simulated data sets. The results in Rungs 1 and 2 show that methods that use only the point source positions tend to have lower precision (|$10\!-\!20{{\ \rm per\ cent}}$|) while remaining accurate. In Rung 2, the methods that exploit the full information of the imaging and kinematic data sets can recover H0 within the target accuracy (| A | < 2 per cent) and precision (<6 per cent per system), even in the presence of a poorly known point spread function and complex source morphology. A post-unblinding analysis of Rung 3 showed the numerical precision of the ray-traced cosmological simulations to be insufficient to test lens modelling methodology at the percent level, making the results difficult to interpret. A new challenge with improved simulations is needed to make further progress in the investigation of systematic uncertainties. For completeness, we present the Rung 3 results in an appendix and use them to discuss various approaches to mitigating against similar subtle data generation effects in future blind challenges. [ABSTRACT FROM AUTHOR]- Published
- 2021
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6. TDCOSMO: IV. Hierarchical time-delay cosmography – joint inference of the Hubble constant and galaxy density profiles.
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Birrer, S., Shajib, A. J., Galan, A., Millon, M., Treu, T., Agnello, A., Auger, M., Chen, G. C.-F., Christensen, L., Collett, T., Courbin, F., Fassnacht, C. D., Koopmans, L. V. E., Marshall, P. J., Park, J.-W., Rusu, C. E., Sluse, D., Spiniello, C., Suyu, S. H., and Wagner-Carena, S.
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HUBBLE constant , *COSMOGRAPHY , *GRAVITATIONAL lenses , *ELLIPTICAL galaxies , *SPECTRAL imaging , *DARK matter - Abstract
The H0LiCOW collaboration inferred via strong gravitational lensing time delays a Hubble constant value of H0 = 73.3−1.8+1.7 H 0 = 73. 3 − 1.8 + 1.7 $ H_0 = 73.3^{+1.7}_{-1.8} $ km s−1 Mpc−1, describing deflector mass density profiles by either a power-law or stars (constant mass-to-light ratio) plus standard dark matter halos. The mass-sheet transform (MST) that leaves the lensing observables unchanged is considered the dominant source of residual uncertainty in H0. We quantify any potential effect of the MST with a flexible family of mass models, which directly encodes it, and they are hence maximally degenerate with H0. Our calculation is based on a new hierarchical Bayesian approach in which the MST is only constrained by stellar kinematics. The approach is validated on mock lenses, which are generated from hydrodynamic simulations. We first applied the inference to the TDCOSMO sample of seven lenses, six of which are from H0LiCOW, and measured H0 = 74.5−6.1+5.6 H 0 = 74. 5 − 6.1 + 5.6 $ H_0 = 74.5^{+5.6}_{-6.1} $ km s−1 Mpc−1. Secondly, in order to further constrain the deflector mass density profiles, we added imaging and spectroscopy for a set of 33 strong gravitational lenses from the Sloan Lens ACS (SLACS) sample. For nine of the 33 SLAC lenses, we used resolved kinematics to constrain the stellar anisotropy. From the joint hierarchical analysis of the TDCOSMO+SLACS sample, we measured H0 = 67.4−3.2+4.1 H 0 = 67. 4 − 3.2 + 4.1 $ H_0 = 67.4^{+4.1}_{-3.2} $ km s−1 Mpc−1. This measurement assumes that the TDCOSMO and SLACS galaxies are drawn from the same parent population. The blind H0LiCOW, TDCOSMO-only and TDCOSMO+SLACS analyses are in mutual statistical agreement. The TDCOSMO+SLACS analysis prefers marginally shallower mass profiles than H0LiCOW or TDCOSMO-only. Without relying on the form of the mass density profile used by H0LiCOW, we achieve a ∼5% measurement of H0. While our new hierarchical analysis does not statistically invalidate the mass profile assumptions by H0LiCOW – and thus the H0 measurement relying on them – it demonstrates the importance of understanding the mass density profile of elliptical galaxies. The uncertainties on H0 derived in this paper can be reduced by physical or observational priors on the form of the mass profile, or by additional data. [ABSTRACT FROM AUTHOR]
- Published
- 2020
- Full Text
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7. H0LiCOW XII. Lens mass model of WFI2033 − 4723 and blind measurement of its time-delay distance and H0.
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Rusu, Cristian E, Wong, Kenneth C, Bonvin, Vivien, Sluse, Dominique, Suyu, Sherry H, Fassnacht, Christopher D, Chan, James H H, Hilbert, Stefan, Auger, Matthew W, Sonnenfeld, Alessandro, Birrer, Simon, Courbin, Frederic, Treu, Tommaso, Chen, Geoff C-F, Halkola, Aleksi, Koopmans, Léon V E, Marshall, Philip J, and Shajib, Anowar J
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GRAVITATIONAL lenses ,SPECTRAL imaging ,SPACE telescopes ,DISTANCES ,VELOCITY measurements ,HUBBLE constant - Abstract
We present the lens mass model of the quadruply-imaged gravitationally lensed quasar WFI2033 − 4723, and perform a blind cosmographical analysis based on this system. Our analysis combines (1) time-delay measurements from 14 yr of data obtained by the COSmological MOnitoring of GRAvItational Lenses (COSMOGRAIL) collaboration, (2) high-resolution Hubble Space Telescope imaging, (3) a measurement of the velocity dispersion of the lens galaxy based on ESO-MUSE data, and (4) multi-band, wide-field imaging and spectroscopy characterizing the lens environment. We account for all known sources of systematics, including the influence of nearby perturbers and complex line-of-sight structure, as well as the parametrization of the light and mass profiles of the lensing galaxy. After unblinding, we determine the effective time-delay distance to be |$4784_{-248}^{+399}~\mathrm{Mpc}$| , an average precision of |$6.6{{\ \rm per\ cent}}$|. This translates to a Hubble constant |$H_{0} = 71.6_{-4.9}^{+3.8}~\mathrm{km~s^{-1}~Mpc^{-1}}$| , assuming a flat ΛCDM cosmology with a uniform prior on Ω
m in the range [0.05, 0.5]. This work is part of the H0 Lenses in COSMOGRAIL's Wellspring (H0LiCOW) collaboration, and the full time-delay cosmography results from a total of six strongly lensed systems are presented in a companion paper (H0LiCOW XIII). [ABSTRACT FROM AUTHOR]- Published
- 2020
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8. A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging.
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Chen, Geoff C-F, Fassnacht, Christopher D, Suyu, Sherry H, Rusu, Cristian E, Chan, James H H, Wong, Kenneth C, Auger, Matthew W, Hilbert, Stefan, Bonvin, Vivien, Birrer, Simon, Millon, Martin, Koopmans, Léon V E, Lagattuta, David J, McKean, John P, Vegetti, Simona, Courbin, Frederic, Ding, Xuheng, Halkola, Aleksi, Jee, Inh, and Shajib, Anowar J
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ADAPTIVE optics ,GRAVITATIONAL lenses ,TIME delay systems ,HUBBLE constant ,SPACE telescopes ,DARK matter - Abstract
We present the measurement of the Hubble constant, H
0 , with three strong gravitational lens systems. We describe a blind analysis of both PG 1115+080 and HE 0435−1223 as well as an extension of our previous analysis of RXJ 1131−1231. For each lens, we combine new adaptive optics (AO) imaging from the Keck Telescope, obtained as part of the SHARP (Strong-lensing High Angular Resolution Programme) AO effort, with Hubble Space Telescope (HST) imaging, velocity dispersion measurements, and a description of the line-of-sight mass distribution to build an accurate and precise lens mass model. This mass model is then combined with the COSMOGRAIL-measured time delays in these systems to determine H0 . We do both an AO-only and an AO + HST analysis of the systems and find that AO and HST results are consistent. After unblinding, the AO-only analysis gives |$H_{0}=82.8^{+9.4}_{-8.3}~\rm km\, s^{-1}\, Mpc^{-1}$| for PG 1115+080, |$H_{0}=70.1^{+5.3}_{-4.5}~\rm km\, s^{-1}\, Mpc^{-1}$| for HE 0435−1223, and |$H_{0}=77.0^{+4.0}_{-4.6}~\rm km\, s^{-1}\, Mpc^{-1}$| for RXJ 1131−1231. The joint AO-only result for the three lenses is |$H_{0}=75.6^{+3.2}_{-3.3}~\rm km\, s^{-1}\, Mpc^{-1}$|. The joint result of the AO + HST analysis for the three lenses is |$H_{0}=76.8^{+2.6}_{-2.6}~\rm km\, s^{-1}\, Mpc^{-1}$|. All of these results assume a flat Λ cold dark matter cosmology with a uniform prior on Ωm in [0.05, 0.5] and H0 in [0, 150] |$\rm km\, s^{-1}\, Mpc^{-1}$|. This work is a collaboration of the SHARP and H0LiCOW teams, and shows that AO data can be used as the high-resolution imaging component in lens-based measurements of H0 . The full time-delay cosmography results from a total of six strongly lensed systems are presented in a companion paper. [ABSTRACT FROM AUTHOR]- Published
- 2019
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9. H0LiCOW – IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant.
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Birrer, S, Treu, T, Rusu, C E, Bonvin, V, Fassnacht, C D, Chan, J H H, Agnello, A, Shajib, A J, Chen, G C-F, Auger, M, Courbin, F, Hilbert, S, Sluse, D, Suyu, S H, Wong, K C, Marshall, P, Lemaux, B C, and Meylan, G
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HUBBLE constant ,QUASARS ,DARK matter ,SPACE telescopes ,ANGULAR distance ,DARK energy - Abstract
We present a blind time-delay strong lensing (TDSL) cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 . We combine the relative time delay between the quasar images, Hubble Space Telescope imaging, the Keck stellar velocity dispersion of the lensing galaxy, and wide-field photometric and spectroscopic data of the field to constrain two angular diameter distance relations. The combined analysis is performed by forward modelling the individual data sets through a Bayesian hierarchical framework, and it is kept blind until the very end to prevent experimenter bias. After unblinding, the inferred distances imply a Hubble constant H
0 = 68.8 |$^{+5.4}_{-5.1}$| km s−1 Mpc−1 , assuming a flat Λ cold dark matter cosmology with uniform prior on Ωm in [0.05, 0.5]. The precision of our cosmographic measurement with the doubly imaged quasar SDSS 1206+4332 is comparable with those of quadruply imaged quasars and opens the path to perform on selected doubles the same analysis as anticipated for quads. Our analysis is based on a completely independent lensing code than our previous three H0LiCOW systems and the new measurement is fully consistent with those. We provide the analysis scripts paired with the publicly available software to facilitate independent analysis (footnote with link to www.h0licow.org). The consistency between blind measurements with independent codes provides an important sanity check on lens modelling systematics. By combining the likelihoods of the four systems under the same prior, we obtain H0 = 72.5 |$^{+2.1}_{-2.3}$| km s−1 Mpc−1 . This measurement is independent of the distance ladder and other cosmological probes. [ABSTRACT FROM AUTHOR]- Published
- 2019
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10. Improving time-delay cosmography with spatially resolved kinematics.
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Shajib, Anowar J., Treu, Tommaso, and Agnello, Adriano
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COSMOGRAPHY , *GRAVITATIONAL lenses , *QUASARS , *HUBBLE constant , *DARK matter , *SIMULATION methods & models - Abstract
Strongly gravitational lensed quasars can be used to measure the so-called time-delay distance DΔt, and thus the Hubble constant H0 and other cosmological parameters. Stellar kinematics of the deflector galaxy play an essential role in this measurement by: (i) helping break the masssheet degeneracy; (ii) determining in principle the angular diameter distance Dd to the deflector and thus further improving the cosmological constraints. In this paper we simulate observations of lensed quasars with integral field spectrographs and show that spatially resolved kinematics of the deflector enables further progress by helping break the mass-anisotropy degeneracy. Furthermore, we use our simulations to obtain realistic error estimates with current/upcoming instruments like OSIRIS on Keck and NIRSPEC on the James Webb Space Telescope for both distances (typically ~6 per cent on DΔt and ~10 per cent on Dd). We use the error estimates to compute cosmological forecasts for the sample of nine lenses that currently have wellmeasured time delays and deep Hubble Space Telescope images and for a sample of 40 lenses that is projected to be available in a few years through follow-up of candidates found in ongoing wide field surveys. We find that H0 can be measured with 2 per cent (1 per cent) precision from nine (40) lenses in a flat Λcold dark matter cosmology. We study several other cosmological models beyond the flat Λcold dark matter model and find that time-delay lenses with spatially resolved kinematics can greatly improve the precision of the cosmological parameters measured by cosmic microwave background data. [ABSTRACT FROM AUTHOR]
- Published
- 2018
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11. H0LiCOW-XIII. A 2.4 per cent measurement of H-0 from lensed quasars: 5.3 sigma tension between early- and late-Universe probes
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Wong, Kenneth C., Suyu, Sherry H., Chen, Geoff C-F, Rusu, Cristian E., Millon, Martin, Sluse, Dominique, Bonvin, Vivien, Fassnacht, Christopher D., Taubenberger, Stefan, Auger, Matthew W., Birrer, Simon, Chan, James H. H., Courbin, Frederic, Hilbert, Stefan, Tihhonova, Olga, Treu, Tommaso, Agnello, Adriano, Ding, Xuheng, Jee, Inh, Komatsu, Eiichiro, Shajib, Anowar J., Sonnenfeld, Alessandro, Blandford, Roger D., Koopmans, Leon V. E., Marshall, Philip J., and Meylan, Georges
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galaxy-group identification ,cosmic distance scale ,time delays ,internal structure ,gravitational lensing: strong ,Astrophysics::Cosmology and Extragalactic Astrophysics ,distance scale ,hubble constant ,cosmology: observations ,he 0435-1223 ,cosmological constraints ,gravitational lens ,cosmological parameters ,sound-horizon ,spectroscopic survey - Abstract
We present a measurement of the Hubble constant (H-0) and other cosmological parameters from a joint analysis of six gravitationally lensed quasars with measured time delays. All lenses except the first are analysed blindly with respect to the cosmological parameters. In a flat Lambda cold dark matter (Lambda CDM) cosmology, we find H-0 = 73.3(-1.8)(+1.7) km s(-1) Mpc(-1), a 2.4 per cent precision measurement, in agreement with local measurements of H-0 from type Ia supernovae calibrated by the distance ladder, but in 3.1 sigma tension with Planck observations of the cosmic microwave background (CMB). This method is completely independent of both the supernovae and CMB analyses. A combination of time-delay cosmography and the distance ladder results is in 5.3 sigma tension with Planck CMB determinations of H-0 in flat Lambda CDM. We compute Bayes factors to verify that all lenses give statistically consistent results, showing that we are not underestimating our uncertainties and are able to control our systematics. We explore extensions to flat Lambda CDM using constraints from time-delay cosmography alone, as well as combinations with other cosmological probes, including CMB observations from Planck, baryon acoustic oscillations, and type Ia supernovae. Time-delay cosmography improves the precision of the other probes, demonstrating the strong complementarity. Allowing for spatial curvature does not resolve the tension with Planck. Using the distance constraints from time-delay cosmography to anchor the type Ia supernova distance scale, we reduce the sensitivity of our H-0 inference to cosmological model assumptions. For six different cosmological models, our combined inference on H-0 ranges from similar to 73 to 78 km s(-1) Mpc(-1), which is consistent with the local distance ladder constraints.
12. TDCOSMO I. An exploration of systematic uncertainties in the inference ofH(0)from time-delay cosmography
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Shajib, Anowar J., Mozumdar, Pritom, Chen, Geoff C. -F., Treu, Tommaso, Cappellari, Michele, Knabel, Shawn, Suyu, Sherry H., Bennert, Vardha N., Frieman, Joshua A., Sluse, Dominique, Birrer, Simon, Courbin, Frederic, Fassnacht, Christopher D., Villafana, Lizvette, and Williams, Peter R.
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line-of-sight ,to-light ratio ,gravitational lensing ,data analysis ,fundamental plane ,strong ,external convergence ,spectroscopic data ,methods ,sdss-iv manga ,hubble constant ,dark-matter ,multi-gaussian expansion ,early-type galaxies - Abstract
Strong-lensing time delays enable the measurement of the Hubble constant (H0) independently of other traditional methods. The main limitation to the precision of time-delay cosmography is mass-sheet degeneracy (MSD). Some of the previous TDCOSMO analyses broke the MSD by making standard assumptions about the mass density profile of the lens galaxy, reaching 2% precision from seven lenses. However, this approach could potentially bias the H0 measurement or underestimate the errors. For this work, we broke the MSD for the first time using spatially resolved kinematics of the lens galaxy in RXJ1131 1231 obtained from the Keck Cosmic Web Imager spectroscopy, in combination with previously published time delay and lens models derived from Hubble Space Telescope imaging. This approach allowed us to robustly estimate H0, e ffectively implementing a maximally flexible mass model. Following a blind analysis, we estimated the angular diameter distance to the lens galaxy Dd = 865 +85 81 Mpc and the time-delay distance D t = 2180 +472 271 Mpc, giving H0 = 77:1 +7:3 7:1 km s 1 Mpc 1 - for a flat cold dark matter cosmology. The error budget accounts for all uncertainties, including the MSD inherent to the lens mass profile and line-of-sight e ffects, and those related to the mass-anisotropy degeneracy and projection e ffects. Our new measurement is in excellent agreement with those obtained in the past using standard simply parametrized mass profiles for this single system (H0 = 78:3 +3:4 3:3 km s 1 Mpc 1) and for seven lenses (H0 = 74:2 +1:6 1:6 km s 1 Mpc 1), or for seven lenses using single-aperture kinematics and the same maximally flexible models used by us ( H0 = 73 :3+5:8 5:8 km s 1 Mpc 1). This agreement corroborates the methodology of time-delay cosmography.
13. H0LiCOW XII. Lens mass model of WFI2033 − 4723 and blind measurement of its time-delay distance and H0.
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Rusu, Cristian E, Wong, Kenneth C, Bonvin, Vivien, Sluse, Dominique, Suyu, Sherry H, Fassnacht, Christopher D, Chan, James H H, Hilbert, Stefan, Auger, Matthew W, Sonnenfeld, Alessandro, Birrer, Simon, Courbin, Frederic, Treu, Tommaso, Chen, Geoff C-F, Halkola, Aleksi, Koopmans, Léon V E, Marshall, Philip J, and Shajib, Anowar J
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GRAVITATIONAL lenses , *SPECTRAL imaging , *SPACE telescopes , *DISTANCES , *VELOCITY measurements , *HUBBLE constant - Abstract
We present the lens mass model of the quadruply-imaged gravitationally lensed quasar WFI2033 − 4723, and perform a blind cosmographical analysis based on this system. Our analysis combines (1) time-delay measurements from 14 yr of data obtained by the COSmological MOnitoring of GRAvItational Lenses (COSMOGRAIL) collaboration, (2) high-resolution Hubble Space Telescope imaging, (3) a measurement of the velocity dispersion of the lens galaxy based on ESO-MUSE data, and (4) multi-band, wide-field imaging and spectroscopy characterizing the lens environment. We account for all known sources of systematics, including the influence of nearby perturbers and complex line-of-sight structure, as well as the parametrization of the light and mass profiles of the lensing galaxy. After unblinding, we determine the effective time-delay distance to be |$4784_{-248}^{+399}~\mathrm{Mpc}$| , an average precision of |$6.6{{\ \rm per\ cent}}$|. This translates to a Hubble constant |$H_{0} = 71.6_{-4.9}^{+3.8}~\mathrm{km~s^{-1}~Mpc^{-1}}$| , assuming a flat ΛCDM cosmology with a uniform prior on Ωm in the range [0.05, 0.5]. This work is part of the H 0 Lenses in COSMOGRAIL's Wellspring (H0LiCOW) collaboration, and the full time-delay cosmography results from a total of six strongly lensed systems are presented in a companion paper (H0LiCOW XIII). [ABSTRACT FROM AUTHOR]
- Published
- 2020
- Full Text
- View/download PDF
14. Snowmass2021-Letter of interest cosmology intertwined I:Perspectives for the next decade
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Tristan L. Smith, Angela Chen, Salvatore Capozziello, Paolo de Bernardis, Micol Benetti, François R. Bouchet, Yacine Ali-Haïmoud, Tanvi Karwal, Simon Birrer, Arindam Mazumdar, David F. Mota, Marco Bruni, Florian Niedermann, Antonella Palmese, Vivian Miranda, Mikhail M. Ivanov, Carsten van de Bruck, Marika Asgari, Noemi Frusciante, Alan Heavens, Jens Chluba, Weiqiang Yang, Luis A. Anchordoqui, Agnès Ferté, David Camarena, Anton Chudaykin, Erminia Calabrese, Luca Lamagna, Anowar J. Shajib, Francesco Pace, Arman Shafieloo, Alessandro Melchiorri, Martin S. Sloth, Licia Verde, Andronikos Paliathanasis, Anil Kumar Yadav, Elia S. Battistelli, Ankan Mukherjee, Mario Ballardini, F. Piacentini, Daniela Paoletti, Dragan Huterer, Joan Solà Peracaula, Eoin Ó Colgáin, Supriya Pan, Lloyd Knox, Valerio Marra, Anjan A. Sen, J. Muir, Suresh Kumar, Adam G. Riess, Hendrik Hildebrandt, Luca Amendola, Ian Harrison, Celia Escamilla-Rivera, Olga Mena, Daniel E. Holz, Eleonora Di Valentino, Özgür Akarsu, Luca Visinelli, Deng Wang, Francis-Yan Cyr-Racine, Wendy L. Freedman, Sabino Matarrese, Shahab Joudaki, Joseph Silk, Laura Mersini-Houghton, Nikki Arendse, Julien Lesgourgues, Javier de Cruz Pérez, Alessandra Silvestri, Jo Dunkley, Vincenzo Salzano, Vivian Poulin, Valeria Pettorino, Jacques Delabrouille, Silvia Masi, Alessio Notari, Fabio Finelli, Matteo Lucca, Luke Hart, Benjamin D. Wandelt, Will Handley, Adrià Gómez-Valent, Marco Raveri, Cristian Moreno-Pulido, Jian-Min Wang, Marc Kamionkowski, Emmanuel N. Saridakis, Spyros Basilakos, Elena Giusarma, Rafael C. Nunes, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Di Valentino, Eleonora, Anchordoqui, Luis A., Akarsu, Özgür, Ali-Haimoud, Yacine, Amendola, Luca, Arendse, Nikki, Asgari, Marika, Ballardini, Mario, Basilakos, Spyro, Battistelli, Elia, Benetti, Micol, Birrer, Simon, Bouchet, François R., Bruni, Marco, Calabrese, Erminia, Camarena, David, Capozziello, Salvatore, Chen, Angela, Chluba, Jen, Chudaykin, Anton, Colgáin, Eoin Ó, Cyr-Racine, Francis-Yan, de Bernardis, Paolo, de Cruz Pérez, Javier, Delabrouille, Jacque, Dunkley, Jo, Escamilla-Rivera, Celia, Ferté, Agnè, Finelli, Fabio, Freedman, Wendy, Frusciante, Noemi, Giusarma, Elena, Gómez-Valent, Adrià, Handley, Will, Harrison, Ian, Hart, Luke, Heavens, Alan, Hildebrandt, Hendrik, Holz, Daniel, Huterer, Dragan, Ivanov, Mikhail M., Joudaki, Shahab, Kamionkowski, Marc, Karwal, Tanvi, Knox, Lloyd, Kumar, Suresh, Lamagna, Luca, Lesgourgues, Julien, Lucca, Matteo, Marra, Valerio, Masi, Silvia, Matarrese, Sabino, Mazumdar, Arindam, Melchiorri, Alessandro, Mena, Olga, Mersini-Houghton, Laura, Miranda, Vivian, Moreno-Pulido, Cristian, Mota, David F., Muir, Jessica, Mukherjee, Ankan, Niedermann, Florian, Notari, Alessio, Nunes, Rafael C., Pace, Francesco, Paliathanasis, Androniko, Palmese, Antonella, Pan, Supriya, Paoletti, Daniela, Pettorino, Valeria, Piacentini, Francesco, Poulin, Vivian, Raveri, Marco, Riess, Adam G., Salzano, Vincenzo, Saridakis, Emmanuel N., Sen, Anjan A., Shafieloo, Arman, Shajib, Anowar J., Silk, Joseph, Silvestri, Alessandra, Sloth, Martin S., Smith, Tristan L., Solà Peracaula, Joan, van de Bruck, Carsten, Verde, Licia, Visinelli, Luca, Wandelt, Benjamin D., Wang, Deng, Wang, Jian-Min, Yadav, Anil K., Yang, Weiqiang, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Value (ethics) ,cosmological model ,Cold dark matter ,satellite: Planck ,anomaly ,dark matter: density ,01 natural sciences ,Cosmology ,NO ,symbols.namesake ,SEARCH ,0103 physical sciences ,Planck ,010303 astronomy & astrophysics ,Standard model (cryptography) ,Physics ,Hubble constant ,010308 nuclear & particles physics ,PE9_14 ,Astronomy and Astrophysics ,Cosmological model ,tension ,Data science ,Astrophysics - Cosmology and Nongalactic Astrophysics ,High Energy Physics - Phenomenology ,symbols ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Hubble's law - Abstract
The standard Lambda Cold Dark Matter cosmological model provides an amazing description of a wide range of astrophysical and astronomical data. However, there are a few big open questions, that make the standard model look like a first-order approximation to a more realistic scenario that still needs to be fully understood. In this Letter of Interest we will list a few important goals that need to be addressed in the next decade, also taking into account the current discordances present between the different cosmological probes, as the Hubble constant H-0 value, the sigma S-8(8) tension, and the anomalies present in the Planck results. Finally, we will give an overview of upgraded experiments and next-generation space-missions and facilities on Earth that will be of crucial importance to address all these questions. (C) 2021 Elsevier B.V. All rights reserved.
- Published
- 2021
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