Recent Herschel observations have detected up to 0.7 Msun of cold dust surrounding SN 1987A . This discovery implies that supernovae could be responsible for the large dust masses detected in high red-shift galaxies and opens opportunities in the Herschel era for detecting and measuring accurate cold dust masses in extra-galactic supernovae. One data point from SN1987A is insufficient to resolve the fundamental question of the origin of dust in early Universe, therefore we propose Herschel PACS and SPIRE imaging observations of the two nearby supernovae SN 2004et and SN 2004dj. After SN 1987A, they are the closest well-known supernovae with evidence of dust formation from Spitzer and other ground-based observations. Our scientific goals are i) to detect far-infrared and submm emission from supernovae, ii) to understand the spectral energy distribution of the SNe for temperatures and dust composition, and iii) to estimate freshly formed dust mass. These added observations are essential to help determine if supernove are significant dust makers in the early Universe.
Publication
DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands | Clark C. J. R. et al. | Astronomy & Astrophysics Volume 609 id.A37 30 pp. | 609 | 10.1051\\/0004-6361\\/201731419 | 2018A&A...609A..37C | http://adsabs.harvard.edu/abs/2018A%26A...609A..37C
Probing the spectral shape of dust emission with the DustPedia galaxy sample | Nersesian Angelos et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2021MNRAS.506.3986N |
A nearby galaxy perspective on dust evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples | Galliano Frederic et al. | Astronomy and Astrophysics | null | null | 2021A&A...649A..18G |
Dust emissivity and absorption cross section in DustPedia late-type galaxies | Bianchi S. et al. | Astronomy and Astrophysics | null | null | 2019A&A...631A.102B |
Fraction of bolometric luminosity absorbed by dust in DustPedia galaxies | Bianchi S. et al. | Astronomy & Astrophysics Volume 620 id.A112 21 pp. | 620 | 10.1051\\/0004-6361\\/201833699 | 2018A&A...620A.112B | http://adsabs.harvard.edu/abs/2018A%26A...620A.112B
UV to submillimetre luminosity functions of TNG50 galaxies | Trcka Ana et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2022MNRAS.516.3728T |
DustPedia: A Definitive Study of Cosmic Dust in the Local Universe | Davies J. I. et al. | Publications of the Astronomical Society of the Pacific Volume 129 Issue 974 pp. 044102 (2017). | 129 | 10.1088\\/1538-3873\\/129\\/974\\/044102 | 2017PASP..129d4102D | http://adsabs.harvard.edu/abs/2017PASP..129d4102D
Instrument
PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage
2012-10-08T20:59:14Z/2013-03-01T08:32:52Z
Version
SPG v14.2.0
Mission Description
Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
European Space Agency, rho et al., 2013, 'Cold Dust in the Ejecta of Two Nearby Supernovae: Are supernovae dust producers in the early UniversequestionMark', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-9y2y1mg
