The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
arXiv:astro-ph/0002234 · doi:10.1046/j.1365-8711.2000.03386.x
Abstract
We have used SCUBA to observe a complete sample of 104 galaxies selected at 60 microns from the IRAS BGS and we present here the 850 micron measurements. Fitting the 60,100 and 850 micron fluxes with a single temperature dust model gives the sample mean temperature T=36 K and beta = 1.3. We do not rule out the possibility of dust which is colder than this, if a 20 K component was present then our dust masses would increase by factor 1.5-3. We present the first measurements of the luminosity and dust mass functions, which were well fitted by Schechter functions (unlike those 60 microns). We have correlated many global galaxy properties with the submillimetre and find that there is a tendancy for less optically luminous galaxies to contain warmer dust and have greater star formation efficiencies (cf. Young 1999). The average gas-to-dust ratio for the sample is 581 +/- 43 (using both atomic and molecular hydrogen), significantly higher than the Galactic value of 160. We believe this discrepancy is due to a cold dust component at T < 20 K. There is a suprisingly tight correlation between dust mass and the mass of molecular hydrogen as estimated from CO measurements, with an intrinsic scatter of ~50%.
24 pages, 15 figures, 8 tables, accepted for publication in MNRAS
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- The Host Haloes of Lyman Break Galaxies and Sub-millimeter Sources
- Constraints on the [CII] luminosity of a proto-globular cluster at z~6 obtained with ALMA
- Dust masses and star formation in bright IRAS galaxies Application of a physical model for the interpretation of FIR observations
- Searching for the highest redshift sources in 250-500 micron submillimeter surveys
- A Search for 6.7 GHz Methanol Masers in OH Megamaser Galaxies at 0.11<z<0.27
- Dust-to-gas ratios in the starburst regions of luminous infrared galaxies
- Infrared luminosity functions and dust mass functions in the EAGLE simulation
- Gas Content and Kinematics in Clumpy, Turbulent Star-forming Disks
- Unveiling the mask on the ULIRG-to-QSO transition object [H89]1821+643 at z=0.3: a gas-poor/gas-rich galaxy merger and the implications for CO-based dynamical mass estimates
- An AzTEC 1.1-mm Survey for ULIRGs in the field of the Galaxy Cluster MS 0451.6-0305
- The composite nature of Dust-Obscured Galaxies (DOGs) at z~2-3 in the COSMOS field: I. A Far-Infrared View
- Modelling the Spoon IRS diagnostic diagram
- Deep, ultra-high-resolution radio imaging of submillimetre galaxies using Very Long Baseline Interferometry
- A Joint Model of the X-ray And Infrared Extragalactic Backgrounds: I. Model Construction And First Results
- Spatially Resolved Imaging at 350um of Cold Dust in Nearby Elliptical Galaxies
- Karl G. Jansky Very Large Array observations of cold dust and molecular gas in starbursting quasar host galaxies at z~4.5
- ASTRO-F - Super IRAS - The All Sky Infra-Red Survey
- Gigamasers: the key to the dust-obscured star-formation history of the Universe?
- Quantifying dust and the ultraviolet radiation-density in the local universe
- e-MERLIN and VLBI observations of the luminous infrared galaxy IC883: a nuclear starburst and an AGN candidate revealed
- The Radio-to-Submillimeter Flux Density Ratio of Galaxies as a Measure of Redshift
- SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy, WISE1013+6112
- SCUBA Observations of NGC 1275
- WMAP anomalous signal in the ecliptic plane
- An Investigation of the Dust Content in the Galaxy pair NGC 1512/1510 from Near-Infrared to Millimeter Wavelengths
- H-ATLAS/GAMA and HeViCS - Dusty Early-Type Galaxies in Different Environments
- Gravitational orbits in the expanding universe revisited
- The Star Formation Rate - Dense Gas Relation in the Nuclei of Nearby Galaxies
- CO Observations of the Host Galaxy of GRB000418 at z = 1.1
- Modeling the evolution of infrared luminous galaxies: the influence of the Luminosity-Temperature distribution
- Spatially Resolved Spectroscopy of Sub-mm Galaxies at z~2
- A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
- Spatially-resolved Radio-to-Far-infrared SED of the Luminous Merger Remnant NGC 1614 with ALMA and VLA
- AGN and star formation across cosmic time
- The physical properties of local (U)LIRGs: a comparison with nearby early- and late-type galaxies
- The 60-micron extragalactic background radiation intensity, dust-enshrouded AGNs and the assembly of groups and clusters of galaxies
- Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
- A broadband spectroscopic search for CO line emission in HDF850.1: the brightest submillimetre object in the Hubble Deep Field North
- Cross-Correlation of Near and Far-Infrared Background Anisotropies as Traced by Spitzer and Herschel
- Submillimetre Emission from Eta Carinae
- Sub-millimeter emission from type Ia supernova host galaxies at z=0.5
- Submillimetre Source Counts in the Fields of High-Redshift Galaxy Clusters
- Deeply Buried Nuclei in the Infrared-Luminous Galaxies NGC 4418 and Arp 220: I. ALMA Observations at 1.4-0.4 mm and Continuum Analysis
- Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies
- Herschel observations of a z~2 stellar mass selected galaxy sample drawn from the GOODS NICMOS Survey
- Dust masses, compositions, and luminosities in the nuclear disks and the diffuse circumnuclear medium of Arp220
- The infrared-luminous progenitors of high-z quasars
- An Orientation Bias in Observations of Submillimetre Galaxies
- A high dust emissivity index beta for a CO-faint galaxy in a filamentary Lyman-alpha nebula at z=3.1
- Cold Dust in (Some) High z Supernova Host Galaxies
- Far infrared constraints on the contamination by dust obscured galaxies of high-z dropout searches
- A panchromatic study of BLAST counterparts: total star-formation rate, morphology, AGN fraction and stellar mass
- Effects of dust abundance on the far-infrared colours of blue compact dwarf galaxies
- On the Detectability of the SZ Effect of Massive Young Galaxies
- The merger Seyfert galaxy Arp 220. Line and continuum absorption and emission
- VLA High Resolution 1.4 and 8.4 GHz Mapping of the Barred Galaxy NGC 3367
- Temperature Variations of the Cold Dust in the Triangulum Galaxy M33
- Molecular gas budget and characterization of intermediate-mass star-forming galaxies at
- The Extraordinary Infrared Spectrum of NGC 1222 (Mkn 603)
- The nature of sub-millimetre galaxies I: A comparison of AGN and star-forming galaxy SED fits
- Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array
- A submillimetre-bright z~3 overdensity behind a z~1 supercluster revealed by SCUBA-2 and Herschel
- Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
- A SCUBA Map in the Spitzer First Look Survey: Source Catalog and Number Counts
- Mapping the submillimeter spiral wave in NGC 6946
- Number Density Evolution of Ks -band Selected High Redshift Galaxy Populations in the AKARI North Ecliptic Pole Field
- The Circumgalactic Medium of Submillimeter Galaxies. II. Unobscured QSOs within Dusty Starbursts and QSO Sightlines with Impact Parameters below 100 Kiloparsec
- Spectroscopic follow-up of 70μm sources in Spitzer Wide-area Infrared Extragalactic Legacy Survey
- The 617 MHz - 850 m Correlation (Cosmic Rays and Cold Dust) in NGC 3044 and NGC 4157
- The host galaxies of radio-loud quasars at z>5 with ALMA
- High Star Formation Rates of Low Eddington Ratio Quasars at
- Resolving IRAS 09111-1007 at 350 microns - a different path to ULIRG formation?
- Evidence for a Dusty Dark Dwarf Galaxy in the Quadruple Lens MG0414+0534
- What determines the shape of the local (z<0.1) infrared galaxy luminosity function?
- Submillimeter Observations of Low Metallicity Galaxy NGC 4214
- Comparison of dust-to-gas ratios in luminous, ultraluminous, and hyperluminous infrared galaxies
- Revealing the Double Nucleus of NGC 4490
- Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
- Restarting radio activity and dust emission in radio-loud broad absorption line quasars
- Contribution of starburst mergers at z~1 to the strong evolution of infrared and submillimeter deep surveys
- Methods for the Pointing Reconstruction of the Planck satellite
- The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)
- IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
- PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon
- Spitzer/IRS Imaging and Spectroscopy of the luminous infrared galaxy NGC 6052 (Mrk 297)
- The dust properties of z ~ 3 MIPS-LBGs from photo-chemical models
- Deep Submillimeter Observations of Two Lyman-alpha Emitting Galaxies at z~6.5
- Star Formation and Infrared Emission in Galaxies
- Predicting the intensity mapping signal for multi- CO lines
- Dust contribution to the panchromatic galaxy emission
- On the nature of the first galaxies selected at 350 microns
- A surprising consistency between the far-infrared galaxy luminosity functions of the field and Coma
- ALMA survey of a massive node of the Cosmic Web at . II. A dynamically cold and massive disk galaxy in the proximity of a hyperluminous quasar
- A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
- Molecular Gas and Star formation in ARP 302
- Tight correlation of star formation with [Ci] and CO lines across cosmic time
- Probing Cool and Warm Infrared Galaxies using Photometric and Structural Measures
- AstroSat observations of interacting galaxies NGC 7469 and IC 5283
- Supernova dust for the extinction law in a young infrared galaxy at z = 1
- Properties of Interstellar Medium in the S0 Galaxy NGC 1222: Evidence for Shocked-enhanced Line Emission
- ATCA detections of massive molecular gas reservoirs in dusty, high-z radio galaxies
- The GLEAM 4-Jy (G4Jy) Sample: IV. Multiwavelength data and analysis
- Dust content of core-collapse supernova hosts
- What is the amount of baryonic dark matter in galaxies?
- The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
- Evolving Starburst Modeling of FIR/sub-mm/mm Line Emission. III. Application to Nearby Luminous Infrared Galaxies
- The Impact of Powerful Jets on the Far-infrared Emission of an Extreme Radio Quasar at z~6
- Resolving dust and Lyα emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS