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 MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics

(2019)

Authors:

Dieu D Nguyen, Mark den Brok, Anil C Seth, Satoru Iguchi, Jenny E Greene, Timothy Davis, Masatoshi Imanishi, Takuma, Izumi, Michelle Cappellari, Nadine Neumayer, Kristina Nyland, Takafumi Tsukui, Kouichiro Nakanishi, Phuong M Nguyen, Quang L Nguyen, Sabine Thater, Martin Bureau, Kyoko Onishi, Karina T Voggel, Ngan M Le, Trung V Dinh

IRIS opens pupils' eyes to real space research

Astronomy & Geophysics Oxford University Press (OUP) 60:1 (2019) 1.22-1.24

Authors:

Peter Hatfield, W Furnell, A Shenoy, E Fox, B Parker, L Thomas, EAC Rushton

Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova

The Astrophysical Journal American Astronomical Society 871:2 (2019) 176

Authors:

Danfeng Xiang, Xiaofeng Wang, Jun Mo, Lingjun Wang, Stephen Smartt, Morgan Fraser, Shuhrat A Ehgamberdiev, Davron Mirzaqulov, Jujia Zhang, Tianmeng Zhang, Jozsef Vinko, J Craig Wheeler, Griffin Hosseinzadeh, D Andrew Howell, Curtis McCully, James M DerKacy, E Baron, Peter Brown, Xianfei Zhang, Shaolan Bi, Hao Song, Kaicheng Zhang, A Rest, Ken’ichi Nomoto, Alexey Tolstov, Sergei Blinnikov

A progenitor candidate for the type II-P supernova SN 2018aoq in NGC 4151

Astronomy & Astrophysics EDP Sciences 622 (2019) l1

Authors:

D O’Neill, R Kotak, M Fraser, SA Sim, S Benetti, SJ Smartt, S Mattila, C Ashall, E Callis, N Elias-Rosa, M Gromadzki, SJ Prentice