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Observing the host galaxies of high-redshift quasars with JWST: predictions from the BLUETIDES simulation

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posted on 2023-06-10, 06:53 authored by Madeline A Marshall, Stuart J B Wyithe, Rogier A Windhorst, Tiziana D Matteo, Yueying Ni, Stephen WilkinsStephen Wilkins, Rupert A C Croft, Mira Mechtley
The bright emission from high-redshift quasars completely conceals their host galaxies in the rest-frame ultraviolet/optical, with detection of the hosts in these wavelengths eluding even the Hubble Space Telescope (HST) using detailed point spread function (PSF) modelling techniques. In this study, we produce mock images of a sample of z = 7 quasars extracted from the BLUETIDES simulation, and apply Markov chain Monte Carlo-based PSF modelling to determine the detectability of their host galaxies with the James Webb Space Telescope (JWST). While no statistically significant detections are made with HST, we predict that at the same wavelengths and exposure times JWST NIRCam imaging will detect ~ 50 per cent of quasar host galaxies. We investigate various observational strategies, and find that NIRCam wide-band imaging in the long-wavelength filters results in the highest fraction of successful quasar host detections, detecting > 80 per cent of the hosts of bright quasars in exposure times of 5 ks. Exposure times of > 5 ks are required to detect the majority of host galaxies in the NIRCam wide-band filters, however, even 10 ks exposures with MIRI result in < 30 per cent successful host detections. We find no significant trends between galaxy properties and their detectability. The PSF modelling can accurately recover the host magnitudes, radii, and spatial distribution of the larger scale emission, when accounting for the central core being contaminated by residual quasar flux. Care should be made when interpreting the host properties measured using PSF modelling.

History

Publication status

  • Published

File Version

  • Accepted version

Journal

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

Publisher

Oxford University Press (OUP)

Issue

1

Volume

506

Page range

1209-1228

Department affiliated with

  • Physics and Astronomy Publications

Full text available

  • Yes

Peer reviewed?

  • Yes

Legacy Posted Date

2023-04-24

First Open Access (FOA) Date

2023-04-24

First Compliant Deposit (FCD) Date

2023-04-21

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