Erratum: Evolution of star formation in the UKIDSS Ultra Deep Survey Field - I. Luminosity functions and cosmic star formation rate out to z = 1.6

Monthly Notices of the Royal Astronomical Society Oxford University Press 446:1 (2015) 941-942

Authors:

Alyssa B Drake, Chris Simpson, Chris A Collins, Phil A James, Ivan K Baldry, Masami Ouchi, Matt J Jarvis, David G Bonfield, Yoshiaki Ono, Philip N Best, Gavin Dalton, James S Dunlop, Ross J McLure, Daniel JB Smith

Investigating the origin of harmonics in a 230 GHz local oscillator

Proceedings of the International Symposium on Space Terahertz Technology IEEE (2015)

Authors:

Boon Tan, Andre Hector, Brian N Ellison, Ghassan Yassin, Jamie Leech

Abstract:

The presence of spurious frequency tones emanating from a harmonically generated local oscillator (LO) signal can significantly degrade the performance of a SuperconductorInsulator-Superconductor (SIS) tunnel junction mixer [1]. The existence of harmonics is often revealed by distorted I-V curves obtained when pumping the SIS device with the LO. We have investigated this effect by using a commercially available source and correlating the photon step induced I-V curve structure with a direct frequency measurement made via a Fourier Transform Spectrometer (FTS) and a spectrum analyser. Our results suggest that intermixing frequency products are generated within the first, low frequency, stage of the LO chain, and these unwanted signals are converted to high frequency tones through subsequent stages of LO amplification and frequency up-conversion. The experimental work has been performed by using measurement facilities available at the University of Oxford and the Rutherford Appleton Laboratory (RAL), UK.

Multi-wavelength studies of high-latitude black-Hole X-ray transients

Proceedings of Science 1-5-June-2015 (2015)

Authors:

PA Charles, AW Shaw, M Coriat, P Gandhi, LJ Townsend, P Woudt, J Casares, DL Foster, MM Kotze, D Steeghs, RP Fender, AA Zdziarski

Abstract:

Over the last 25 years ∼75% of the low-mass X-ray binary X-ray transients have been shown to contain black-hole compact objects, based on optical spectroscopy of their kinematics when in quiescence. Because many of these systems are extremely faint in quiescence and unobservable, we have utilised the method of studying them when in X-ray outburst that exploits the fluores- cence features produced by X-ray irradiation of the donor's inner face, thereby allowing us to track the motion of the donor. Such outbursts are unpredictable and hence these studies must necessarily be through Target-of-Opportunity programs, and hence are ideal for SALT for accessible targets. Here we report on our SALT ToO studies of two transients, both believed to contain black holes and both at high galactic latitude.

Probing primordial non-Gaussianity via iSW measurements with SKA continuum surveys

Journal of Cosmology and Astroparticle Physics IOP Publishing 2015:01 (2015) 042-042

Authors:

Alvise Raccanelli, Olivier Doré, David J Bacon, Roy Maartens, Mario G Santos, Stefano Camera, Tamara M Davis, Michael J Drinkwater, Matt Jarvis, Ray Norris, David Parkinson

Testing an array of 350 GHz drilled smoothwall horns using a vector near-field beam scanner

26th International Symposium on Space Terahertz Technology, ISSTT 2015 (2015)

Authors:

PK Grimes, E Tong, L Zeng, J Leech, G Yassin

Abstract:

We describe near-field tests and results of an 8 pixel close-packed feedhorn array that will be a key component of an 8 pixel prototype 350 GHz SIS mixer array receiver prototype under construction at SAO. We have fabricated an array of smooth walled multiple flare angle feedhorns by direct drilling into a single block of aluminum. Testing of the feedhorns was carried out using a nearfield scanner and a vector network analyzer based on custom built transmitters and receivers and an HP vector voltmeter. The vector nearfield data is transformed to the farfield radiation pattern using Python code based on the NF2FF Matlab script[1].