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Holland, Heinrich; Holland, Doris

doi:10.1007/978-3-322-92161-1_12

Cited by 253 publications

(294 citation statements)

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“…On UT 2004 August 28, 1 hr of photometry data each at both 850 and 450 m were obtained in good weather ( 850 m ¼ 0:3) 11 The NDWFS catalogs and a description of the naming conventions are available at http://www.noao.edu /noao/noaodeep/index.html. using SCUBA (Holland et al 1999) on the James Clerk Maxwell Telescope (JCMT). The data were reduced using SURF (Jenness & Lightfoot 1998) and flux calibrated against CRL 2688.…”

Section: Submillimeter Imaging and Photometrymentioning

confidence: 99%

MIPS J142824.0+352619: A Hyperluminous Starburst Galaxy atz= 1.325

Borys¹,

Blain²,

Dey³

et al. 2006

ApJ

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Using the SHARC-II camera at the Caltech Submillimeter Observatory to obtain 350 m images of sources detected with the MIPS instrument on Spitzer, we have discovered a remarkable object at z ¼ 1:325 AE 0:002 with an apparent far-infrared luminosity of 3:2(AE0:7) ; 10 13 L . Unlike other z > 1 sources of comparable luminosity selected from mid-IR surveys, MIPS J142824.0+352619 lacks any trace of AGN activity, and is likely a luminous analog of galaxies selected locally by IRAS, or at high redshift in the submillimeter. This source appears to be lensed by a foreground elliptical galaxy at z ¼ 1:034, although the amplification is likely modest (P10). We argue that the contribution to the observed optical/near-IR emission from the foreground galaxy is small, and hence are able to present the restframe UV through radio spectral energy distribution of this galaxy. Due to its unusually high luminosity, MIPS J142824.0+352619 presents a unique chance to study a high-redshift dusty starburst galaxy in great detail.

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Section: Submillimeter Imaging and Photometrymentioning

confidence: 99%

MIPS J142824.0+352619: A Hyperluminous Starburst Galaxy atz= 1.325

Borys¹,

Blain²,

Dey³

et al. 2006

ApJ

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“…New instruments have recently been developed at submillimeter wavelengths that greatly enhance our capability in this area (Hunter, Benford, & Serabyn 1996 ;Cunningham et al 1994). In this paper, we present maps of dust emission around 21 cores in various evolutionary states using the Submillimetre Common User Bolometer Arrray (SCUBA) (Holland et al 1999) at wavelengths of 1.3 mm, 850 km, and 450 km. By mapping the extended dust emission, we can probe the density structure from 7A to 100A (for the nearest sources in our sample, at 125 pc, these angles correspond to 870 AU to 12,500 AU).…”

Section: Introductionmentioning

confidence: 99%

Tracing the Mass during Low‐Mass Star Formation. I. Submillimeter Continuum Observations

Shirley

Evans

Rawlings

et al. 2000

ASTROPHYS J SUPPL S

244

348

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We have obtained 850 and 450 km continuum maps of 21 low-mass cores with SEDs ranging from pre-protostellar to Class I (18 K), using SCUBA at the JCMT. In this paper we present K \ T bol \ 370 the maps, radial intensity proÐles, and photometry. Pre-protostellar cores do not have power-law intensity proÐles, whereas the intensity proÐles of Class 0 and Class I sources can be Ðtted with power laws over a large range of radii. A substantial number of sources have companion sources within a few arcminutes (two out of Ðve pre-protostellar cores, nine out of 16 Class 0/I sources). The mean separation between sources is 10,800 AU. The median separation is 18,000 AU including sources without companions as a lower limit. The mean value of the spectral index between 450 and 850 km is 2.8^0.4, with pre-protostellar cores having slightly lower spectral indices (2.5^0.4). The mean mass of the sample, based on the dust emission in a 120A aperture, is 1.1^0.9For the sources Ðtted by power-law M _ . intensity distributions the mean value of m is 1.52^0.45 for Class 0 and I sources, at 850 km and 1.44^0.25 at 450 km. Based on a simple analysis, assuming the emission is in the Rayleigh-Jeans limit and that these values of m translate into power-law density distribu-T d (r) P r~0.4, tions (n P r~p) with p D 2.1. However, we show that this result may be changed by more careful consideration of e †ects such as beam size and shape, Ðnite outer radii, more realistic and failure of the T d (r), Rayleigh-Jeans approximation.

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“…This effectively circumvents the time constraint for obtaining large samples of objects with the present-generation submillimeter imaging instruments, SCUBA (Holland et al 1999) and MAMBO (Bertoldi et al 2000). These surveys (BCR, C01) have used the bimodal break in the apparent optical magnitudes of radio source identifications lying at I $ 24 , selecting only the relatively faint sources for submillimeter follow-up-the optically faint radio sources (OFRS).…”

Section: Introductionmentioning

confidence: 99%

Understanding the Nature of Optically Faint Radio Sources and Their Connection to the Submillimeter Population

Chapman

Lewis

Scott

et al. 2002

ApJ

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We present a sample of 43 submillimeter sources detected (at >3 ) drawn from our program to follow up optically faint radio sources with the Submillimeter Common User Bolometric Array (SCUBA) instrument. These sources already have associated radio and, in many cases, optical identifications, and many are also detected at 450 lm. We compare these with 12 submillimeter sources drawn from the literature, which were discovered in blank-field mapping campaigns but also have radio detections. We then use this total sample (55 sources) to study and model the evolution of dusty galaxies. A correlation is observed in the submillimeter/radio color-magnitude diagram (CMD), which can be modeled by strong luminosity evolution. The selection effects of the radio/optical preselection technique are determined from the models, and a corrected redshift distribution is constrained using a range of model assumptions. The temperature/redshift effects on the 450 lm detected subset of our sample are studied in relation to the models, and prospects for improved measurements in the shorter submillimeter wavelength windows (450 and 350 lm) are explored.

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Cited by 253 publications

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MIPS J142824.0+352619: A Hyperluminous Starburst Galaxy atz= 1.325

MIPS J142824.0+352619: A Hyperluminous Starburst Galaxy atz= 1.325

Tracing the Mass during Low‐Mass Star Formation. I. Submillimeter Continuum Observations

Understanding the Nature of Optically Faint Radio Sources and Their Connection to the Submillimeter Population

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