most citedXMM-Newton and Chandra Cross Calibration Using HIFLUGCS Galaxy Clusters: Systematic Temperature Differences and Cosmological Impact

185 citations · 215 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2023

Studying X-ray instruments with galaxy clusters

J. Nevalainen, S. Molendi

We applied a scientific approach to the problem of the effective area cross-calibration of the XMM-Newton EPIC instruments. Using a sample of galaxy clusters observed with the XMM-…

astro-ph.CO20237 cited

A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113

D. Spence, M. Bonamente, J. Nevalainen +5

This paper presents an analysis of XMM X--ray spectra of the quasar 1ES 1553+113, in search for absorption lines from the intervening warm--hot intergalactic medium. A search for O…

astro-ph.CO202315 cited

Cosmic gas highways in C-EAGLE simulations

I. Vurm, J. Nevalainen, S. E. Hong +3

A substantial fraction of the cosmic baryons is expected to hide in the form of diffuse warm-hot intergalactic medium (WHIM), the majority of which resides in the filaments of the…

astro-ph.CO202310 cited

Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation

T. Tuominen, J. Nevalainen, P. Heinämäki +5

The current observational status of the hot (log T(K) > 5.5) warm-hot intergalactic medium (WHIM) remains incomplete. While recent observations from stacking large numbers of Cosmi…

astro-ph.IM20142 cited

Summary of the 2014 IACHEC Meeting

David Burrows, Fabio Gastaldello, Catherine E. Grant +6

We present the main results of the 9th meeting of the International Astronomical Consortium for High Energy Calibration (IACHEC), held in Warrenton (Virginia) in May 2014. Over 50…

astro-ph.CO201428 cited

Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias

Holger Israel, Gerrit Schellenberger, Jukka Nevalainen +2

The mass of galaxy clusters can be inferred from the temperature of their X-ray emitting gas, . Their masses may be underestimated if it is assumed that the gas is…