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19972008
most citedIs Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models

97 citations · 177 across the 11 of their papers we have counts for

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15 papers · 1 filter

astro-ph2008

The Thickness of High-Redshift Quasar Ionization Fronts as a Constraint on the Ionizing Spectral Energy Distribution

Roban Hultman Kramer, Zoltán Haiman

High-redshift quasars (z >~ 6) drive ionization fronts into the intergalactic medium (IGM). If the thickness of the front can be measured, it can provide a novel constraint on the…

astro-ph200797 cited

Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models

Sheng Wang, Lam Hui, Morgan May +1

We apply the technique of parameter-splitting to existing cosmological data sets, to check for a generic failure of dark energy models. Given a dark energy parameter, such as the e…

astro-ph200747 cited

Pre-Merger Localization of Gravitational-Wave Standard Sirens With LISA I: Harmonic Mode Decomposition

Bence Kocsis, Zoltán Haiman, Kristen Menou +1

The continuous improvement in localization errors (sky position and distance) in real time as LISA observes the gradual inspiral of a supermassive black hole (SMBH) binary can be o…

astro-ph2006

Oxygen Pumping: Mapping the Reionization Epoch with the CMB

Carlos Hernandez-Monteagudo, Zoltan Haiman, Raul Jimenez +1

We consider the pumping of the m fine structure line of neutral OI in the high--redshift intergalactic medium (IGM), in analogy with the Wouthuysen--Field effect for the 21…

astro-ph200628 cited

Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey

Wenjuan Fang, Zoltan Haiman

We study the potential of a large future weak-lensing survey to constrain dark energy properties by using both the number counts of detected galaxy clusters (sensitive primarily to…

astro-ph20054 cited

An X-ray Galaxy Cluster Survey for Investigations of Dark Energy

Z. Haiman, S. Allen, N. Bahcall +34

The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the r…