Cameron P M Bell
The intrinsic reddening of the Magellanic Clouds as traced by background galaxies – II. The Small Magellanic Cloud
Bell, Cameron P M; Cioni, Maria-Rosa L; Wright, A H; Rubele, Stefano; Nidever, David L; Tatton, Ben L; Van Loon, Jacco Th; Zaritsky, Dennis; Choi, Yumi; Choudhury, Samyaday; Clementini, Gisella; de Grijs, Richard; Ivanov, Valentin D; Majewski, Steven R; Marconi, Marcella; Martínez-Delgado, David; Massana, Pol; Muñoz, Ricardo R; Niederhofer, Florian; Noël, Noelia E D; Oliveira, Joana M; Olsen, Knut; Pennock, Clara M; Ripepi, V; Subramanian, Smitha; Vivas, A Katherina
Authors
Maria-Rosa L Cioni
A H Wright
Stefano Rubele
David L Nidever
Ben L Tatton
Jacobus Van Loon j.t.van.loon@keele.ac.uk
Dennis Zaritsky
Yumi Choi
Samyaday Choudhury
Gisella Clementini
Richard de Grijs
Valentin D Ivanov
Steven R Majewski
Marcella Marconi
David Martínez-Delgado
Pol Massana
Ricardo R Muñoz
Florian Niederhofer
Noelia E D Noël
Joana Maria Oliveira j.oliveira@keele.ac.uk
Knut Olsen
Clara M Pennock
V Ripepi
Smitha Subramanian
A Katherina Vivas
Abstract
We present a map of the total intrinsic reddening across ? 34 deg2 of the Small Magellanic Cloud (SMC) derived using optical (ugriz) and near-infrared (IR; YJKs) spectral energy distributions (SEDs) of background galaxies. The reddening map is created using a subsample of 29,274 galaxies with low levels of intrinsic reddening based on the lephare ?2 minimisation SED-fitting routine. We find statistically significant enhanced levels of reddening associated with the main body of the SMC compared with regions in the outskirts [?E(B - V) ? 0.3 mag]. A comparison with literature reddening maps of the SMC shows that, after correcting for differences in the volume of the SMC sampled, there is good agreement between our results and maps created using young stars. In contrast, we find significant discrepancies between our results and maps created using old stars or based on longer wavelength far-IR dust emission that could stem from biased samples in the former and uncertainties in the far-IR emissivity and the optical properties of the dust grains in the latter. This study represents one of the first large-scale categorisations of extragalactic sources behind the SMC and as such we provide the lephare outputs for our full sample of ~ 500,000 sources.
Citation
Bell, C. P. M., Cioni, M. L., Wright, A. H., Rubele, S., Nidever, D. L., Tatton, B. L., …Vivas, A. K. (2020). The intrinsic reddening of the Magellanic Clouds as traced by background galaxies – II. The Small Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 499(1), 993 -1004. https://doi.org/10.1093/mnras/staa2786
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 8, 2020 |
Online Publication Date | Sep 21, 2020 |
Publication Date | 2020-11 |
Publicly Available Date | May 26, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 499 |
Issue | 1 |
Pages | 993 -1004 |
DOI | https://doi.org/10.1093/mnras/staa2786 |
Keywords | surveys – dust, extinction – galaxies: ISM – Magellanic Clouds – galaxies: photometry. |
Publisher URL | https://doi.org/10.1093/mnras/staa2786 |
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