STRIDES: automated uniform models for 30 quadruply imaged quasars

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 518:1 (2022) 1260-1300

Authors:

T Schmidt, T Treu, S Birrer, AJ Shajib, C Lemon, M Millon, D Sluse, A Agnello, T Anguita, MW Auger-Williams, RG McMahon, V Motta, P Schechter, C Spiniello, I Kayo, F Courbin, S Ertl, CD Fassnacht, JA Frieman, A More, S Schuldt, SH Suyu, M Aguena, F Andrade-Oliveira, J Annis, D Bacon, E Bertin, D Brooks, DL Burke, A Carnero Rosell, M Carrasco Kind, J Carretero, C Conselice, M Costanzi, LN da Costa, MES Pereira, J De Vicente, S Desai, P Doel, S Everett, I Ferrero, D Friedel, J García-Bellido, E Gaztanaga, D Gruen, RA Gruendl, J Gschwend, G Gutierrez, SR Hinton, DL Hollowood, K Honscheid, DJ James, K Kuehn, O Lahav, F Menanteau, R Miquel, A Palmese, F Paz-Chinchón, A Pieres, AA Plazas Malagón, J Prat, M Rodriguez-Monroy, AK Romer, E Sanchez, V Scarpine, I Sevilla-Noarbe, M Smith, E Suchyta, G Tarle, C To, TN Varga

The Dark Energy Survey supernova program: cosmological biases from supernova photometric classification

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 518:1 (2022) 1106-1127

Authors:

M Vincenzi, M Sullivan, A Möller, P Armstrong, BA Bassett, D Brout, D Carollo, A Carr, TM Davis, C Frohmaier, L Galbany, K Glazebrook, O Graur, L Kelsey, R Kessler, E Kovacs, GF Lewis, C Lidman, U Malik, RC Nichol, B Popovic, M Sako, D Scolnic, M Smith, G Taylor, BE Tucker, P Wiseman, M Aguena, S Allam, J Annis, J Asorey, D Bacon, E Bertin, D Brooks, DL Burke, A Carnero Rosell, J Carretero, FJ Castander, M Costanzi, LN da Costa, MES Pereira, J De Vicente, S Desai, HT Diehl, P Doel, S Everett, I Ferrero, B Flaugher, P Fosalba, J Frieman, J García-Bellido, DW Gerdes, D Gruen, G Gutierrez, SR Hinton, DL Hollowood, K Honscheid, DJ James, K Kuehn, N Kuropatkin, O Lahav, TS Li, M Lima, MAG Maia, JL Marshall, R Miquel, R Morgan, RLC Ogando, A Palmese, F Paz-Chinchón, A Pieres, AA Plazas Malagón, K Reil, A Roodman, E Sanchez, M Schubnell, S Serrano, I Sevilla-Noarbe, E Suchyta, G Tarle, C To, TN Varga, J Weller, RD Wilkinson

MIGHTEE: deep 1.4 GHz source counts and the sky temperature contribution of star forming galaxies and active galactic nuclei

Monthly Notices of the Royal Astronomical Society Oxford University Press 520:2 (2022) 2668-2691

Authors:

Cl Hale, Ih Whittam, Mj Jarvis, Pn Best, Nl Thomas, I Heywood, M Prescott, N Adams, J Afonso, Fangxia An, Raa Bowler, Jd Collier, Rhw Cook, R Davé, Bs Frank, M Glowacki, Pw Hatfield, S Kolwa, Cc Lovell, N Maddox, L Marchetti, Lk Morabito, E Murphy, I Prandoni, Z Randriamanakoto, Ar Taylor

Abstract:

We present deep 1.4 GHz source counts from ∼5 deg2 of the continuum Early Science data release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration (MIGHTEE) survey down to S1.4GHz ∼15 μJy. Using observations over two extragalactic fields (COSMOS and XMM-LSS), we provide a comprehensive investigation into correcting the incompleteness of the raw source counts within the survey to understand the true underlying source count population. We use a variety of simulations that account for: errors in source detection and characterisation, clustering, and variations in the assumed source model used to simulate sources within the field and characterise source count incompleteness. We present these deep source count distributions and use them to investigate the contribution of extragalactic sources to the sky background temperature at 1.4 GHz using a relatively large sky area. We then use the wealth of ancillary data covering a subset of the COSMOS field to investigate the specific contributions from both active galactic nuclei (AGN) and star forming galaxies (SFGs) to the source counts and sky background temperature. We find, similar to previous deep studies, that we are unable to reconcile the sky temperature observed by the ARCADE 2 experiment. We show that AGN provide the majority contribution to the sky temperature contribution from radio sources, but the relative contribution of SFGs rises sharply below 1 mJy, reaching an approximate 15-25 per cent contribution to the total sky background temperature (Tb ∼100 mK) at ∼15 μJy.

The luminous type Ia supernova 2022ilv and its early excess emission

(2022)

Authors:

Shubham Srivastav, SJ Smartt, ME Huber, G Dimitriadis, KC Chambers, Michael D Fulton, Thomas Moore, FP Callan, James H Gillanders, K Maguire, M Nicholl, Luke J Shingles, SA Sim, KW Smith, JP Anderson, Thomas de Boer, Ting-Wan Chen, Hua Gao, DR Young

Ion microscope imaging mass spectrometry using a Timepix3-based optical camera

Journal of the American Society for Mass Spectrometry American Chemical Society 33:12 (2022) 2328-2332

Authors:

Daniel Wood, Robert J Burleigh, Natasha Smith, Daniela Bortoletto, Mark Brouard, Michael Burt, Andrei Nomerotski, Richard Plackett, Ian Shipsey

Abstract:

Ion microscopy allows for high-throughput mass spectrometry imaging. In order to resolve congested mass spectra, a high degree of timing precision is required from the microscope detector. In this paper we present an ion microscope mass spectrometer that uses a Timepix3 hybrid pixel readout with an optimal 1.56 ns resolution. A novel triggering technique is also employed to remove the need for an external time-to-digital converter (TDC) and allow the experiment to be performed using a low-cost and commercially available readout system. Results obtained from samples of rhodamine B demonstrate the application of multimass imaging sensors for microscope mass spectrometry imaging with high mass resolution.