activity
19982005
most citedAn ISOCAM survey through gravitationally lensing galaxy clusters

124 citations · 149 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph2005★ 3 cited

ISO observations of the interacting galaxy Markarian 297: with the powerful supernova remnant 1982aa

L. Metcalfe, B. O'Halloran, B. McBreen +10

Markarian (Mkn) 297 is a complex system with two interacting galaxies. Observations were made with ISO using ISOCAM, ISOPHOT and LWS. We present ISOCAM maps at 6.7, 7.7, 12 and 14.…

astro-ph2005★ 8 cited

ISO observations of the Wolf-Rayet galaxies NGC 5430, NGC 6764, Mrk 309 and VII Zw 19

B. O'Halloran, B. McBreen, L. Metcalfe +2

Observations of four WR galaxies (NGC 5430, NGC 6764, Mrk 309 and VII Zw 19) using the Infrared Space Observatory are presented here. ISOCAM maps of NGC 5430, Mrk 309 and NGC 6764…

astro-ph2003★ 124 cited

An ISOCAM survey through gravitationally lensing galaxy clusters

L. Metcalfe, J. -P. Kneib, B. McBreen +11

ISOCAM was used to perform a deep survey through three gravitationally lensing clusters of galaxies. Nearly seventy sq. arcmin were covered over the clusters A370, A2218 and A2390.…

astro-ph2002★ 12 cited

ISO observations of Hickson Compact Group 31 with the central Wolf-Rayet galaxy NGC 1741

B. O'Halloran, L. Metcalfe, B. McBreen +5

Hickson Compact Group (HCG) 31, consisting of the Wolf-Rayet galaxy NGC 1741 and its irregular dwarf companions, was observed using the Infrared Space Observatory. The deconvolved…

astro-ph2000

ISO observations of the Wolf-Rayet galaxy NGC 7714 and its companion object NGC 7715

B. O'Halloran, L. Metcalfe, M. Delaney +5

The interacting system Arp 284 consisting of the Wolf-Rayet galaxy NGC 7714 and its irregular companion NGC 7715 was observed using the Infrared Space Observatory. Deconvolved ISOC…

astro-ph2000★ 1 cited

ISO observations of a sample of 60 micron peaker galaxies

R. J. Laureijs, D. Watson, L. Metcalfe +9

The sample of IRAS galaxies with spectral energy distributions that peak near 60 microns are called Sixty Micron Peakers (SMPs or 60PKs). Their generally peculiar and amorphous mor…