Professor Joseph Conlon: Publications

3.55 keV photon lines from axion to photon conversion in the Milky Way and M31

Journal of Cosmology and Astroparticle Physics IOP Publishing 2014:11 (2014) 033-033

Authors:

Joseph P Conlon, Francesca V Day

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Observational consistency and future predictions for a 3.5 keV ALP to photon line

(2014)

Authors:

Pedro D Alvarez, Joseph P Conlon, Francesca V Day, MC David Marsh, Markus Rummel

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Soft X-ray excess in the Coma cluster from a Cosmic Axion Background

Journal of Cosmology and Astroparticle Physics IOP Publishing 2014:09 (2014) 026-026

Authors:

Stephen Angus, Joseph P Conlon, MC David Marsh, Andrew J Powell, Lukas T Witkowski

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3.55 keV photon line and its morphology from a 3.55 keV axionlike particle line

Physical Review D American Physical Society (APS) 90:2 (2014) 023540

Authors:

Michele Cicoli, Joseph P Conlon, MC David Marsh, Markus Rummel

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A 3.55 keV line from $\text{DM}\rightarrow a \rightarrow \gamma$: predictions for cool-core and non-cool-core clusters

(2014)

Authors:

Joseph P Conlon, Andrew J Powell

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Professor Joseph Conlon

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3.55 keV photon lines from axion to photon conversion in the Milky Way and M31

Authors:

Observational consistency and future predictions for a 3.5 keV ALP to photon line

Authors:

Soft X-ray excess in the Coma cluster from a Cosmic Axion Background

Authors:

3.55 keV photon line and its morphology from a 3.55 keV axionlike particle line

Authors:

A 3.55 keV line from $\text{DM}\rightarrow a \rightarrow \gamma$: predictions for cool-core and non-cool-core clusters

Authors:

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Professor Joseph Conlon

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3.55 keV photon lines from axion to photon conversion in the Milky Way and M31

Authors:

Observational consistency and future predictions for a 3.5 keV ALP to photon line

Authors:

Soft X-ray excess in the Coma cluster from a Cosmic Axion Background

Authors:

3.55 keV photon line and its morphology from a 3.55 keV axionlike particle line

Authors:

A 3.55 keV line from $\text{DM}\rightarrow a \rightarrow \gamma$: predictions for cool-core and non-cool-core clusters

Authors: