activity
19962014
most citedEvidence for Diverse Optical Emission from Gamma-Ray Burst Sources

86 citations · 255 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2014★ 8 cited

Simultaneous optical and near-IR photometry of 4U 1957+115 - a missing secondary star

Pasi Hakala, Panu Muhli, Phil Charles

We report the results of quasi-simultaneous optical and NIR photometry of the low-mass X-ray binary, 4U 1957+115. Our observations cover B, V, R, I, J, H and K-bands and additional…

astro-ph.SR2012★ 17 cited

Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822-371

A. Somero, P. Hakala, P. Muhli +2

(Abridged) X1822-371 is the prototypical accretion disc corona X-ray source, a low-mass X-ray binary viewed at very high inclination, thereby allowing the disc structure and extend…

astro-ph.SR2011★ 5 cited

Fast Optical and X-ray Variability in the UCXB 4U0614+09

Pasi Hakala, Phil Charles, Panu Muhli

We present results from several years of fast optical photometry of 4U0614+091 (V1055 Orionis), a candidate ultracompact X-ray binary most likely consisting of a neutron star and a…

astro-ph2008★ 10 cited

Light Curve Morphology Study of UW CrB -- Evidence for a 5 d Superorbital Period

Pasi Hakala, Linnea Hjalmarsdotter, Diana C. Hannikainen +1

Since its discovery in 1990, UW CrB (also known as MS1603+2600) has remained a peculiar source without firm classification. Our current understanding is that it is an Accretion Dis…

astro-ph2007★ 20 cited

The nature of the infrared counterpart of IGR J19140+0951

D. C. Hannikainen, M. G. Rawlings, P. Muhli +3

The INTEGRAL observatory has been (re-)discovering new X-ray sources since the beginning of nominal operations in early 2003. These sources include X-ray binaries, Active Galactic…

astro-ph2004★ 20 cited

XMM-Newton observations of UW CrB -- detection of X-ray bursts and evidence for accretion disc evolution

P. Hakala, G. Ramsay, P. Muhli +4

UW CrB (MS1603+2600) is a peculiar short period X-ray binary that exhibits extraordinary optical behaviour. The optical light curve shape of the system changes drastically from nig…