Population statistics of intermediate mass black holes in dwarf galaxies using the NewHorizon simulation

(2022)

Authors:

Rs Beckmann, Y Dubois, M Volonteri, Ca Dong-P谩ez, M Trebitsch, J Devriendt, S Kaviraj, T Kimm, S Peirani

Exhaustive Symbolic Regression

(2022)

Authors:

Deaglan J Bartlett, Harry Desmond, Pedro G Ferreira

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 M枚ller, 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 Garc铆a-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-Chinch贸n, A Pieres, AA Plazas Malag贸n, 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聽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 (OUP) (2022)

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 Dav茅, 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:

Abstract We present deep 1.4聽GHz source counts from 鈭�5聽deg2 of the continuum Early Science data release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration (MIGHTEE) survey down to S1.4GHz 鈭�15 渭Jy. 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聽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聽per聽cent contribution to the total sky background temperature (Tb 鈭�100 mK) at 鈭�15 渭Jy.

First insights into the ISM at z > 8 with JWST: possible physical implications of a high [O iii] 位4363/[O iii] 位5007

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 518:1 (2022) 592-603

Authors:

Harley Katz, Aayush Saxena, Alex J Cameron, Stefano Carniani, Andrew J Bunker, Santiago Arribas, Rachana Bhatawdekar, Rebecca AA Bowler, Kristan NK Boyett, Giovanni Cresci, Emma Curtis-Lake, Francesco D鈥橢ugenio, Nimisha Kumari, Tobias J Looser, Roberto Maiolino, Hannah 脺bler, Chris Willott, Joris Witstok