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19992026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 19.9k across the 124 of their papers we have counts for

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20 papers · 1 filter

astro-ph2008★ 20 cited

A linear filter to reconstruct the ISW effect from CMB and LSS observations

R. B. Barreiro, P. Vielva, C. Hernandez-Monteagudo +1

The extraction of a signal from some observational data sets that contain different contaminant emissions, often at a greater level than the signal itself, is a common problem in A…

astro-ph2008★ 15 cited

Implementation of a Fourier Matched Filter in CMB Analyses. Application to ISW Studies

Carlos Hernandez-Monteagudo

Aims: Implement a matched filter (MF) cross-correlation algorithm in multipole space and compare it to the standard Angular Cross Power Spectrum (ACPS) method. Apply both methods o…

astro-ph2008★ 10 cited

Missing baryons, bulk flows and the E-mode polarization of the Cosmic Microwave Background

Carlos Hernandez-Monteagudo, Rashid A. Sunyaev

If the peculiar motion of galaxy groups and clusters indeed resembles that of the surrounding baryons, then the kinetic Sunyaev-Zel'dovich (kSZ) pattern of those massive halos shou…

astro-ph2008★ 94 cited

Carbon monoxide line emission as a CMB foreground: tomography of the star-forming universe with different spectral resolutions

Mattia Righi, Carlos Hernandez-Monteagudo, Rashid Sunyaev

The rotational lines of carbon monoxide and the fine structure lines of CII and of the most abundant metals, emitted during the epoch of enhanced star formation in the universe, ar…

astro-ph2007★ 10 cited

Oxygen pumping II: Probing the Inhomogeneous Metal Enrichment at the Epoch of Reionization with High Frequency CMB Observations

Carlos Hernandez-Monteagudo, Zoltan Haiman, Licia Verde +1

At the epoch of reionization, when the high-redshift inter-galactic medium (IGM) is being enriched with metals, the 63.2 micron fine structure line of OI is pumped by the ~ 1300 AA…

astro-ph2007

The clustering of merging star-forming haloes: dust emission as high frequency arcminute CMB foreground

Mattia Righi, Carlos Hernandez-Monteagudo, Rashid Sunyaev

Future observations of CMB anisotropies will be able to probe high multipole regions of the angular power spectrum, corresponding to a resolution of a few arcminutes. Dust emission…

astro-ph2007★ 6 cited

The Kinetic Sunyaev-Zel'dovich Effect Due to the Electrons of Our Galaxy

Amir Hajian, Carlos Hernandez-Monteagudo, Raul Jimenez +2

We compute the effect of local electrons on the CMB temperature anisotropies. The number density and distribution of free electrons in our Galaxy has been accurately measured from…

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-ph2006★ 27 cited

The thermal Sunyaev-Zel'dovich Signature of Baryons in the Local Universe

Carlos Hernandez-Monteagudo, Hy Trac, Raul Jimenez +1

Using cosmological hydrodynamical simulations, we investigate the prospects of the thermal Sunyaev-Zel'dovich (tSZ) effect to detect the missing baryons in the local universe. We f…

astro-ph2006★ 14 cited

Tomography of the Reionization Epoch with Multifrequency CMB Observations

Carlos Hernandez-Monteagudo, Licia Verde, Raul Jimenez

We study the constraints that future multifrequency Cosmic Microwave Background (CMB) experiments will be able to set on the metal enrichment history of the Inter Galactic Medium a…

astro-ph2006

Galaxy cluster merger kinematics by Rees-Sciama effect

Matteo Maturi, Torsten Ensslin, Carlos Hernandez-Monteagudo +1

We discuss how to use the Rees-Sciama (RS) effect associated with merging clusters of galaxies to measure their kinematic properties. In a previous work (Rubino-Martin et al. 2004)…

astro-ph2005★ 65 cited

Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy

C. Hernandez-Monteagudo, L. Verde, Raul Jimenez +1

In the context of a cosmological study of the bulk flows in the Universe, we present a detailed study of the statistical properties of the kinematic Sunyaev-Zel'dovich (kSZ) effect…

astro-ph2005★ 9 cited

Spectral Indications of thermal Sunyaev-Zel'dovich Effect in Archeops and WMAP Data

C. Hernandez-Monteagudo, J. F. Macias-Perez, M. Tristram +1

In this paper, we present a joint cross-correlation analysis of the Archeops CMB maps at 143 and 217 GHz and the WMAP CMB maps at 41, 61 and 94 GHz with sky templates of projected…

astro-ph2005★ 20 cited

The imprint of cosmological hydrogen recombination lines on the power spectrum of the CMB

J. A. Rubino-Martin, C. Hernandez-Monteagudo, R. A. Sunyaev

We explore the imprint of the cosmological hydrogen recombination lines on the power spectrum of the cosmic microwave background (CMB). In particular, we focus our analysis in the…

astro-ph2004★ 11 cited

Measuring Dark Matter Flows in Merging Clusters of Galaxies

J. A. Rubino-Martin, C. Hernandez-Monteagudo, T. A. Ensslin

The Rees-Sciama effect produced in mergers of galaxy clusters is discussed, and an analytical approximation to compute this effect from numerical simulations is given. Using this a…

astro-ph2003★ 61 cited

CMB Observations and the Production of Chemical Elements at the End of the Dark Ages

K. Basu, C. Hernandez-Monteagudo, R. Sunyaev

The metallicity evolution and ionization history of the universe must leave its imprint on the Cosmic Microwave Background through resonant scattering of CMB photons by atoms, ions…

astro-ph2002★ 9 cited

Using peak distribution of the cosmic microwave background for MAP and Planck data analysis: formalism and simulations

C. Hernandez-Monteagudo, A. Kashlinsky, F. Atrio-Barandela

We implement and further refine the recently proposed method (Kashlinsky, Hernández-Monteagudo & Atrio-Barandela, 2001 - KHA) for a time efficient extraction of the power spectrum…

astro-ph2001★ 12 cited

Determining cosmic microwave background structure from its peak distribution

A. Kashlinsky, C. Hernández--Monteagudo, F. Atrio--Barandela

We present a new method for time-efficient and accurate extraction of the power spectrum from future cosmic microwave background (CMB) maps based on properties of peaks and troughs…

astro-ph2000★ 5 cited

Limits on Hot Intracluster Gas Contributions to the Tenerife Temperature Anisotropy Map

J. A. Rubino-Martin, F. Atrio-Barandela, C. Hernandez-Monteagudo

We limit the contribution of the hot intracluster gas, by means of the Sunyaev-Zel'dovich effect, to the temperature anisotropies measured by the Tenerife experiment. The data is c…

astro-ph1999★ 4 cited

On the Number Density of Sunyaev-Zel'dovich Clusters of Galaxies

C. Hern'andez-Monteagudo, F. Atrio-Barandela, J. P. Mücket

If the mean properties of clusters of galaxies are well described by the entropy-driven model, the distortion induced by the cluster population on the blackbody spectrum of the Cos…