The LOFAR Two-metre Sky Survey: II. First data release

Astronomy and Astrophysics EDP Sciences 622 (2019) A1

Authors:

TW Shimwell, C Tasse, MJ Hardcastle, AP Mechev, WL Williams, PN Best, HJA Röttgering, Matthew J Jarvis, Leah K Morabito, Catherine L Hale

Abstract:

The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120–168 MHz survey of the entire northern sky for which observations are now 20% complete. We present our first full-quality public data release. For this data release 424 square degrees, or 2% of the eventual coverage, in the region of the HETDEX Spring Field (right ascension 10h45m00s to 15h30m00s and declination 45°00′00″ to 57°00′00″) were mapped using a fully automated direction-dependent calibration and imaging pipeline that we developed. A total of 325 694 sources are detected with a signal of at least five times the noise, and the source density is a factor of ∼10 higher than the most sensitive existing very wide-area radio-continuum surveys. The median sensitivity is S144 MHz = 71 μJy beam−1 and the point-source completeness is 90% at an integrated flux density of 0.45 mJy. The resolution of the images is 6″ and the positional accuracy is within 0.2″. This data release consists of a catalogue containing location, flux, and shape estimates together with 58 mosaic images that cover the catalogued area. In this paper we provide an overview of the data release with a focus on the processing of the LOFAR data and the characteristics of the resulting images. In two accompanying papers we provide the radio source associations and deblending and, where possible, the optical identifications of the radio sources together with the photometric redshifts and properties of the host galaxies. These data release papers are published together with a further ∼20 articles that highlight the scientific potential of LoTSS.

The C-Band All-Sky Survey (C-BASS): Digital backend for the northern survey

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2019)

Authors:

MA Stevenson, TJ Pearson, Michael E Jones, CJ Copley, C Dickinson, JJ John, OG King, SJC Muchovej, Angela C Taylor

The C-Band All-Sky Survey (C-BASS): digital backend for the northern survey

Monthly Notices of the Royal Astronomical Society Oxford University Press 484:4 (2019) 5377-5388

Authors:

MA Stevenson, TJ Pearson, Michael Jones, CJ Copley, C Dickinson, JJ John, OG King, SJC Muchovej, Angela Taylor

Abstract:

The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarization survey at a frequency of 5 GHz, designed to provide data complementary to the all-sky surveys of WMAP and Planck and future CMB B-mode polarization imaging surveys. We describe the design and performance of the digital backend used for the northern part of the survey. In particular, we describe the features that efficiently implement the demodulation and filtering required to suppress contaminating signals in the time-ordered data, and the capability for real-time correction of detector non-linearity and receiver balance.

Towards the first detection of strongly lensed H i emission

Monthly Notices of the Royal Astronomical Society Oxford University Press 484:3 (2019) 3681-3690

Authors:

T Blecher, R Deane, Ian Heywood, D Obreschkow

Tracking the variable jets of V404 Cygni during its 2015 outburst

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 482:3 (2019) 2950-2972

Authors:

AJ Tetarenko, GR Sivakoff, JCA Miller-Jones, M Bremer, KP Mooley, RP Fender, C Rumsey, A Bahramian, D Altamirano, S Heinz, D Maitra, SB Markoff, S Migliari, MP Rupen, DM Russell, TD Russell, CL Sarazin