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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Aayush Saxena

Postdoctoral Research Assistant

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Cosmology
  • Galaxy formation and evolution
aayush.saxena@physics.ox.ac.uk
Denys Wilkinson Building, room 558
Aayush Saxena's website
  • About
  • Publications

Revealing new high redshift quasar populations through Gaussian mixture model selection

ArXiv 2201.11724 (2022)

Authors:

JD Wagenveld, A Saxena, KJ Duncan, HJA Röttgering, M Zhang
Details from ArXiV

Low frequency radio properties of the z >  5 quasar population⋆

Astronomy & Astrophysics EDP Sciences 656 (2021) a137

Authors:

AJ Gloudemans, KJ Duncan, HJA Röttgering, TW Shimwell, BP Venemans, PN Best, M Brüggen, G Calistro Rivera, A Drabent, MJ Hardcastle, GK Miley, DJ Schwarz, A Saxena, DJB Smith, WL Williams
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No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $\mathbf{3.1 \lesssim z \lesssim 3.5}$

ArXiv 2109.03662 (2021)

Authors:

A Saxena, L Pentericci, RS Ellis, L Guaita, A Calabrò, D Schaerer, E Vanzella, R Amorín, M Bolzonella, M Castellano, F Fontanot, NP Hathi, P Hibon, M Llerena, F Mannucci, A Saldana-Lopez, M Talia, G Zamorani
Details from ArXiV

The VANDELS Survey: new constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 z < 5.5

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 505:4 (2021) 4798-4812

Authors:

A Saxena, RS Ellis, PU Förster, A Calabrò, L Pentericci, AC Carnall, M Castellano, F Cullen, A Fontana, M Franco, JPU Fynbo, A Gargiulo, B Garilli, NP Hathi, DJ McLeod, R Amorín, G Zamorani
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HELP: the Herschel Extragalactic Legacy Project

Monthly Notices of the Royal Astronomical Society Oxford University Press 507:1 (2021) 129-155

Authors:

R Shirley, K Duncan, Mc Campos Varillas, Pd Hurley, K Malek, Y Roehlly, Mwl Smith, H Aussel, T Bakx, V Buat, D Burgarella, N Christopher, S Duivenvoorden, S Eales, A Efstathiou, Ea Gonzalez Solares, M Griffin, M Jarvis, B Lo Faro, L Marchetti, I McCheyne, A Papadopoulos, K Penner, E Pons, M Prescott, E Rigby, H Rottgering, A Saxena, J Scudder, M Vaccari, L Wang, Sj Oliver

Abstract:

We present the Herschel Extragalactic Legacy Project (HELP). This project collates, curates, homogenizes, and creates derived data products for most of the premium multiwavelength extragalactic data sets. The sky boundaries for the first data release cover 1270 deg2 defined by the Herschel SPIRE extragalactic survey fields; notably the Herschel Multi-tiered Extragalactic Survey (HerMES) and the Herschel Atlas survey (H-ATLAS). Here, we describe the motivation and principal elements in the design of the project. Guiding principles are transparent or 'open' methodologies with care for reproducibility and identification of provenance. A key element of the design focuses around the homogenization of calibration, meta data, and the provision of information required to define the selection of the data for statistical analysis. We apply probabilistic methods that extract information directly from the images at long wavelengths, exploiting the prior information available at shorter wavelengths and providing full posterior distributions rather than maximum-likelihood estimates and associated uncertainties as in traditional catalogues. With this project definition paper, we provide full access to the first data release of HELP; Data Release 1 (DR1), including a monolithic map of the largest SPIRE extragalactic field at 385 deg2 and 18 million measurements of PACS and SPIRE fluxes. We also provide tools to access and analyse the full HELP data base. This new data set includes far-infrared photometry, photometric redshifts, and derived physical properties estimated from modelling the spectral energy distributions over the full HELP sky. All the software and data presented is publicly available.
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