Dust content of core-collapse supernova hosts

Abstract

We study a small sample of z=0.1-0.6 core-collapse supernova (CCSN) host galaxies. Continuum observations at 250GHz have been performed with MAMBO at the IRAM-30m telescope. None of these sources has been detected and the error-weighted mean flux is 0.25+/-0.32 mJy. Upper limits on their dust masses are derived and the corresponding sample mean corresponds to 1.4 +/- 2.2 x 10^8 Msol. These results are comparable with previous submillimetre observations of SN-Ia hosts performed by Farrah et al. and by Clements et al. We conclude that CCSN hosts are not extreme at millimetre wavelengths, and as confirmed with the optical luminosities of a subset of our sample, they are typical of the local galaxy population.

5 pages, 1 figure, accepted for publication in Astronomy and Astrophysics

References in corpus (45)

• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
• High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Cosmological Results from High-z Supernovae
• The Star Formation History of Field Galaxies
• Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
• A Redshift Survey of the Submillimeter Galaxy Population
• Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust Enshrouded Star Formation Rate
• Submillimeter Galaxies
• A Precise Distance Indicator: Type Ia Supernova Multicolor Light Curve Shapes
• The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
• High-resolution Millimeter Imaging of Submillimeter Galaxies
• An interferometric CO survey of luminous submm galaxies
• Star formation efficiency in galaxy interactions and mergers: a statistical study
• A median redshift of 2.4 for galaxies bright at submillimetre wavelengths
• The SCUBA Local Universe Galaxy Survey II. 450 micron data - evidence for cold dust in bright IRAS Galaxies
• Resolving the Submillimeter Background: the 850-micron Galaxy Counts
• The Origin of Cosmic Dust
• SCUBA observations of galaxies with metallicity measurements: a new method for determining the relation between submm luminosity and dust mass
• The Morphology of Type Ia Supernovae Light Curves
• Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35
• A submillimetre survey of the star-formation history of radio galaxies
• Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant
• Infrared to millimetre photometry of ultra-luminous IR galaxies: new evidence favouring a 3-stage dust model
• Radio Constraints on the Identifications and Redshifts of Submm Galaxies
• VLBI Images of 49 Radio Supernovae in Arp 220
• Observations of a z=1.44 Dusty, Ultraluminous Galaxy and Implications for Deep Sub-mm Surveys
• A Spitzer Space Telescope Study of SN 2003gd: Still No Direct Evidence that Core-Collapse Supernovae are Major Dust Factories
• Evidence for a Major Merger Origin of High Redshift Sub-millimeter Galaxies
• Brief Note: Analytical Fit to the Luminosity Distance for Flat Cosmologies with a Cosmological Constant
• The Properties of Microjansky Radio Sources in the HDF-N, SSA13, and SSA22 Fields
• Extending the infrared radio correlation
• Adaptive Optics Discovery of Supernova 2004ip in the Nuclear Regions of the Luminous Infrared Galaxy IRAS 18293-3413
• Revised masses of dust and gas of SLUGS FIR bright galaxies based on a recent CO survey
• The Sub-parsec Scale Radio Properties of Southern Starburst Galaxies. I. Supernova Remnants, the Supernova Rate, and the Ionised Medium in the NGC 253 Starburst
• The ultraviolet properties of Luminous Infrared Galaxies at z ~ 0.7: is there any evolution in their dust attenuation?
• The FIR-Radio Relationship at High and Low Redshift
• Evolution of Dust Extinction and Supernova Cosmology
• Quantifying dust and the ultraviolet radiation-density in the local universe
• Properties of SN-host galaxies
• Dust in the Host Galaxies of Supernovae
• Sub-millimeter emission from type Ia supernova host galaxies at z=0.5
• Cold Dust in (Some) High z Supernova Host Galaxies
• Molecular content of a type-Ia SN host galaxy at z=0.6