Measuring the disc-jet correlation in SWIFT J1753.5-0127

Simultaneous observations of hard state LMXBs with XMMNewton and the ISAACinfrared camera on the VLT can reveal the direct connection between accretiondisc variability and variations from the jet. A recent triggered observation ofGX 3394 revealed the first such correlation and showed, surprisingly, that thedisc is better correlated with the jet IR emission than the powerlaw is,suggesting that the disc plays a key role in powering the jet. Here we requestan XMMNewton open time observation (30 ksec exposure) simultaneous withVLTISAAC (3 hours) observations of the persistent. LMXB SWIFTvirgulJ1753.50127(with a supporting optical observation to be proposed for separately), todetermine whether this exciting result can be applied more generally. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]