The most luminous, merger-free AGNs show only marginal correlation with bar presence

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 522:1 (2023) 211-225

Authors:

Izzy L Garland, Matthew J Fahey, Brooke D Simmons, Rebecca J Smethurst, Chris J Lintott, Jesse Shanahan, Maddie S Silcock, Joshua Smith, William C Keel, Alison Coil, Tobias Géron, Sandor Kruk, Karen L Masters, David O’Ryan, Matthew R Thorne, Klaas Wiersema

WISDOM project -- XIV. SMBH mass in the early-type galaxies NGC0612, NGC1574, and NGC4261 from CO dynamical modelling

(2023)

Authors:

Ilaria Ruffa, Timothy A Davis, Michele Cappellari, Martin Bureau, Jacob S Elford, Satoru Iguchi, Federico Lelli, Fu-Heng Liang, Lijie Liu, Anan Lu, Marc Sarzi, Thomas G Williams

SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Helium-Shell Detonation in a Star-Forming Galaxy

(2023)

Authors:

Chang Liu, Adam A Miller, Abigail Polin, Anya E Nugent, Kishalay De, Peter E Nugent, Steve Schulze, Avishay Gal-Yam, Christoffer Fremling, Shreya Anand, Igor Andreoni, Peter Blanchard, Thomas G Brink, Suhail Dhawan, Alexei V Filippenko, Kate Maguire, Tassilo Schweyer, Huei Sears, Yashvi Sharma, Matthew J Graham, Steven L Groom, David Hale, Mansi M Kasliwal, Frank J Masci, Josiah Purdum, Benjamin Racine, Jesper Sollerman, Shrinivas R Kulkarni

WEAVE-StePS - a Stellar Population Survey using WEAVE at WHT

Astronomy and Astrophysics EDP Sciences 672 (2023) A87

Authors:

Angela Iovino, Bianca Poggianti, A Mercurio, M Longhetti, Gavin Dalton, Shoko Jin, Scott Trager

Abstract:

Context. The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide valuable opportunities for forthcoming galaxy surveys through their huge multiplexing capabilities, excellent spectral resolution, and unprecedented wavelength coverage.
Aims. WEAVE is a new wide-field spectroscopic facility mounted on the 4.2 m William Herschel Telescope in La Palma. WEAVE-StePS is one of the five extragalactic surveys that will use WEAVE during its first five years of operations. It will observe galaxies using WEAVE MOS (∼950 fibres distributed across a field of view of ∼3 square degrees on the sky) in low-resolution mode (R ∼ 5000, spanning the wavelength range 3660 − 9590 Å).
Methods. WEAVE-StePS will obtain high-quality spectra (S/N ∼ 10 Å−1 at R ∼ 5000) for a magnitude-limited (IAB = 20.5) sample of ∼25 000 galaxies, the majority selected at z ≥ 0.3. The survey goal is to provide precise spectral measurements in the crucial interval that bridges the gap between LEGA-C and SDSS data. The wide area coverage of ∼25 square degrees will enable us to observe galaxies in a variety of environments. The ancillary data available in each of the observed fields (including X-ray coverage, multi-narrow-band photometry and spectroscopic redshift information) will provide an environmental characterisation for each observed galaxy.
Results. This paper presents the science case of WEAVE-StePS, the fields to be observed, the parent catalogues used to define the target sample, and the observing strategy that was chosen after a forecast of the expected performance of the instrument for our typical targets.
Conclusions. WEAVE-StePS will go back further in cosmic time than SDSS, extending its reach to encompass more than ∼6 Gyr. This is nearly half of the age of the Universe. The spectral and redshift range covered by WEAVE-StePS will open a new observational window by continuously tracing the evolutionary path of galaxies in the largely unexplored intermediate-redshift range.

SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Helium-shell Detonation in a Star-forming Galaxy

The Astrophysical Journal American Astronomical Society 946:2 (2023) 83

Authors:

Chang Liu, Adam A Miller, Abigail Polin, Anya E Nugent, Kishalay De, Peter E Nugent, Steve Schulze, Avishay Gal-Yam, Christoffer Fremling, Shreya Anand, Igor Andreoni, Peter Blanchard, Thomas G Brink, Suhail Dhawan, Alexei V Filippenko, Kate Maguire, Tassilo Schweyer, Huei Sears, Yashvi Sharma, Matthew J Graham, Steven L Groom, David Hale, Mansi M Kasliwal, Frank J Masci, Josiah Purdum, Benjamin Racine, Jesper Sollerman, Shrinivas R Kulkarni