SCUBA Observations of MAMBO Sources
arXiv:astro-ph/0305218 · doi:10.1046/j.1365-8711.2003.06806.x
Abstract
We have observed 23 sources from the MAMBO 1200 micron survey with SCUBA at 850 microns, detecting 19 of the sources. The sources generally have low values for the ratio of 850 micron to 1200 micron flux. Two possible explanations for the low values are either that the sources are at very high redshift or that the global properties of the dust in the MAMBO sources are different from the global properties of dust in low-redshift galaxies. If the former explanation is correct, we estimate that 15 of the MAMBO sources lie at z > 3.
MNRAS, in press
References in corpus (35)
- Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
- A Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution
- SCUBA: A common-user submillimetre camera operating on the James Clerk Maxwell Telescope
- Dusty star forming galaxies at high redshift
- The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
- The nature of faint submm-selected galaxies
- A median redshift of 2.4 for galaxies bright at submillimetre wavelengths
- The Canada-UK Deep Submillimetre Survey: First Submillimetre Images, the Source Counts, and Resolution of the Background
- The SCUBA Local Universe Galaxy Survey II. 450 micron data - evidence for cold dust in bright IRAS Galaxies
- The SCUBA 8-mJy survey - I: Sub-millimetre maps, sources and number counts
- Deep radio imaging of the SCUBA 8-mJy survey fields: sub-mm source identifications and redshift distribution
- The Radio-to-Submm Spectral Index as a Redshift Indicator
- The Nature of Radio Emission from Distant Galaxies: The 1.4 GHz Observations
- The diversity of SCUBA-selected galaxies
- SCUBA observations of galaxies with metallicity measurements: a new method for determining the relation between submm luminosity and dust mass
- The Canada-UK Deep Submillimetre Survey: The Survey of the 14-hour field
- Submillimetre and far-infrared spectral energy distributions of galaxies: the luminosity-temperature relation and consequences for photometric redshifts
- A 1.2mm MAMBO/IRAM-30m Survey of Dust Emission from the Highest Redshift PSS Quasars
- Radio Constraints on the Identifications and Redshifts of Submm Galaxies
- Observations of a z=1.44 Dusty, Ultraluminous Galaxy and Implications for Deep Sub-mm Surveys
- The Scatter in the Relationship between Redshift and the Radio-to-Submm Spectral Index
- A 250 GHz Survey of High Redshift QSOs from the Sloan Digital Sky Survey
- The Canada-UK Deep Submillimeter Survey VI: The 3-Hour Field
- The SCUBA Bright Quasar Survey (SBQS): 850micron observations of the z>4 sample
- 350 Micron Dust Emission from High Redshift Objects
- Confusion errors in astrometry and counterpart association
- Dust temperture and the submillimetre-radio flux density ratio as a redshift indicator for distant galaxies
- The far-infrared--submm spectral energy distribution of high-redshift quasars
- The coincidence and angular clustering of Chandra and SCUBA sources
- Properties of mm galaxies: Constraints from K-band blank fields
- Optically faint counterparts to the ISO-FIRBACK 170 micron population: the discovery of cold, luminous galaxies at high redshift
- Constraining the Radio-Submm Redshift Indicator using data from the SCUBA Local Universe Galaxy Survey
- XMM-Newton Surveys of the CFRS Fields - I: The Sub-mm/X-ray relation
- Submillimeter dust emission of the M17 complex measured with PRONAOS
- The Radio-to-Submillimeter Flux Density Ratio of Galaxies as a Measure of Redshift
Cited by in corpus (40)
- A Redshift Survey of the Submillimeter Galaxy Population
- The Hubble Deep Field North SCUBA Super-map IV - Characterizing submillimetre galaxies using deep Spitzer imaging
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies
- The Stellar Mass Content of Submillimeter-Selected Galaxies
- Dust in starburst nuclei and ULIRGs: SED models for observers
- A 1200 micron MAMBO Survey of ELAIS N2 and the Lockman Hole: I. Maps, sources and number counts
- A mid-infrared spectroscopic study of submillimeter galaxies: luminous starbursts at high redshift
- Spitzer observations of MAMBO galaxies: weeding out active nuclei in starbursting proto-ellipticals
- Deep 1.1 mm-wavelength imaging of the GOODS-South field by AzTEC/ASTE -- II. Redshift distribution and nature of the submillimetre galaxy population
- Gas-rich mergers and feedback are ubiqitous amongst starbursting radio galaxies, as revealed by JVLA, IRAM PdBI and Herschel
- The Bolocam Lockman Hole Millimeter-Wave Galaxy Survey: Galaxy Candidates and Number Counts
- The Properties of Sub-mm Galaxies in Hierarchical Models
- An AzTEC 1.1 mm survey of the GOODS-N field -- II. Multi-wavelength identifications and redshift distribution
- A Near-Infrared Analysis of the Submillimeter Background and the Cosmic Star-Formation History
- The Submillimetre Properties of Ultraluminous Infrared Galaxies
- A 1200-micron MAMBO survey of the GOODS-N field: a significant population of submillimetre drop-out galaxies
- Dust and star formation in distant radio galaxies
- Mid-infrared spectroscopy of two luminous submillimeter galaxies at z~2.8
- An 850 Micron SCUBA Survey of the HDF-N GOODS Region
- Cold Dust in Kepler's Supernova Remnant
- The faint counterparts of MAMBO mm sources near the NTT Deep Field
- A robust sample of submillimetre galaxies: constraints on the prevalence of dusty, high-redshift starbursts
- The sub-millimeter properties of broad absorption line quasars
- Wide-field mid-infrared and millimetre imaging of the high-redshift radio galaxy, 4C41.17
- A multi-wavelength study of the proto-cluster surrounding the z=4.1 radio galaxy TN J1338-1942
- Measurements of the dust properties in z~1-3 SMGs with ALMA
- A model for the infrared dust emission from forming galaxies
- Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts
- Accounting for the Foreground Contribution to the Dust Emission towards Kepler's Supernova Remnant
- An Improved Estimate of the Mass of Dust in Cassiopeia A
- Imaging of High Redshift Submillimeter Galaxies at 16 and 22microns with the Spitzer/IRS: Revealing a population at z>2.5
- Overdensities of SMGs around WISE-selected, ultra-luminous, high-redshift AGN
- Quasars in the MAMBO blank field survey
- Submillimeter sources behind the massive lensing clusters A370 and A2390
- Deep, ultra-high-resolution radio imaging of submillimetre galaxies using Very Long Baseline Interferometry
- Iron Needles in Supernova Remnants?
- A Deep Radio Survey of Abell 2125 I: Radio, Optical and Near-IR Observations
- Improved Templates for Photometric Redshifts of Submm Sources
- Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
- Smoking Supernovae