Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)

E. L. Chapin; S. C. Chapman; K. E. Coppin; M. J. Devlin; J. S. Dunlop; T. R. Greve; M. Halpern; M. F. Hasselfield; D. H. Hughes; R. J. Ivison; G. Marsden; L. Moncelsi; C. B. Netterfield; E. Pascale; D. Scott; I. Smail; M. Viero; F. Walter; A. Weiss; P. V. D. Werf

Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)

E. L. Chapin, S. C. Chapman, K. E. Coppin, M. J. Devlin, J. S. Dunlop, T. R. Greve, M. Halpern, M. F. Hasselfield, D. H. Hughes, R. J. Ivison, G. Marsden, L. Moncelsi, C. B. Netterfield, E. Pascale, D. Scott, I. Smail, M. Viero, F. Walter, A. Weiss, P. V. D. Werf

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract / Description of output

We present a joint analysis of the overlapping Balloon-borne Large Aperture Submillimetre Telescope (BLAST) 250, 350, 500um, and LABOCA 870um observations [from the LABOCA ECDFS Submm Survey (LESS) survey] of the Extended Chandra Deep Field-South. Out to z~3, the BLAST filters sample near the peak wavelength of thermal far-infrared (FIR) emission from galaxies (rest-frame wavelengths ~60-200um), primarily produced by dust heated through absorption in star-forming clouds. However, identifying counterparts to individual BLAST peaks is very challenging, given the large beams [full-width at half-maximum (FWHM) 36-60 arcsec]. In contrast, the ground-based 870um observations have a significantly smaller 19 arcsec FWHM beam, and are sensitive to higher redshifts (z~1-5, and potentially beyond) due to the more favourable negative K-correction. We use the LESS data, as well as deep Spitzer and VLA imaging, to identify 118 individual sources that produce significant emission in the BLAST bands. (6 data files).

Original language	English
Pages (from-to)	10505
Journal	VizieR On-line Data Catalog
Volume	741
Publication status	Published - 1 Oct 2011

Keywords / Materials (for Non-textual outputs)

Galaxy catalogs
X-ray sources
Millimetric/submm sources

Access to Document

http://adsabs.harvard.edu/abs/2011yCat..74110505C

Cite this

Chapin, E. L., Chapman, S. C., Coppin, K. E., Devlin, M. J., Dunlop, J. S., Greve, T. R., Halpern, M., Hasselfield, M. F., Hughes, D. H., Ivison, R. J., Marsden, G., Moncelsi, L., Netterfield, C. B., Pascale, E., Scott, D., Smail, I., Viero, M., Walter, F., Weiss, A., & Werf, P. V. D. (2011). Sub-mm observations in Extended Chandra DFS (Chapin+, 2011). VizieR On-line Data Catalog, 741, 10505. http://adsabs.harvard.edu/abs/2011yCat..74110505C

@article{c9e773f88eda4100ab9ec563686665ca,

title = "Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)",

abstract = "We present a joint analysis of the overlapping Balloon-borne Large Aperture Submillimetre Telescope (BLAST) 250, 350, 500um, and LABOCA 870um observations [from the LABOCA ECDFS Submm Survey (LESS) survey] of the Extended Chandra Deep Field-South. Out to z~3, the BLAST filters sample near the peak wavelength of thermal far-infrared (FIR) emission from galaxies (rest-frame wavelengths ~60-200um), primarily produced by dust heated through absorption in star-forming clouds. However, identifying counterparts to individual BLAST peaks is very challenging, given the large beams [full-width at half-maximum (FWHM) 36-60 arcsec]. In contrast, the ground-based 870um observations have a significantly smaller 19 arcsec FWHM beam, and are sensitive to higher redshifts (z~1-5, and potentially beyond) due to the more favourable negative K-correction. We use the LESS data, as well as deep Spitzer and VLA imaging, to identify 118 individual sources that produce significant emission in the BLAST bands. (6 data files).",

keywords = "Galaxy catalogs, X-ray sources, Millimetric/submm sources",

author = "Chapin, {E. L.} and Chapman, {S. C.} and Coppin, {K. E.} and Devlin, {M. J.} and Dunlop, {J. S.} and Greve, {T. R.} and M. Halpern and Hasselfield, {M. F.} and Hughes, {D. H.} and Ivison, {R. J.} and G. Marsden and L. Moncelsi and Netterfield, {C. B.} and E. Pascale and D. Scott and I. Smail and M. Viero and F. Walter and A. Weiss and Werf, {P. V. D.}",

year = "2011",

month = oct,

day = "1",

language = "English",

volume = "741",

pages = "10505",

journal = "VizieR On-line Data Catalog",

}

Chapin, EL, Chapman, SC, Coppin, KE, Devlin, MJ, Dunlop, JS, Greve, TR, Halpern, M, Hasselfield, MF, Hughes, DH, Ivison, RJ, Marsden, G, Moncelsi, L, Netterfield, CB, Pascale, E, Scott, D, Smail, I, Viero, M, Walter, F, Weiss, A & Werf, PVD 2011, 'Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)', VizieR On-line Data Catalog, vol. 741, pp. 10505. <http://adsabs.harvard.edu/abs/2011yCat..74110505C>

TY - JOUR

T1 - Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)

AU - Chapin, E. L.

AU - Chapman, S. C.

AU - Coppin, K. E.

AU - Devlin, M. J.

AU - Dunlop, J. S.

AU - Greve, T. R.

AU - Halpern, M.

AU - Hasselfield, M. F.

AU - Hughes, D. H.

AU - Ivison, R. J.

AU - Marsden, G.

AU - Moncelsi, L.

AU - Netterfield, C. B.

AU - Pascale, E.

AU - Scott, D.

AU - Smail, I.

AU - Viero, M.

AU - Walter, F.

AU - Weiss, A.

AU - Werf, P. V. D.

PY - 2011/10/1

Y1 - 2011/10/1

N2 - We present a joint analysis of the overlapping Balloon-borne Large Aperture Submillimetre Telescope (BLAST) 250, 350, 500um, and LABOCA 870um observations [from the LABOCA ECDFS Submm Survey (LESS) survey] of the Extended Chandra Deep Field-South. Out to z~3, the BLAST filters sample near the peak wavelength of thermal far-infrared (FIR) emission from galaxies (rest-frame wavelengths ~60-200um), primarily produced by dust heated through absorption in star-forming clouds. However, identifying counterparts to individual BLAST peaks is very challenging, given the large beams [full-width at half-maximum (FWHM) 36-60 arcsec]. In contrast, the ground-based 870um observations have a significantly smaller 19 arcsec FWHM beam, and are sensitive to higher redshifts (z~1-5, and potentially beyond) due to the more favourable negative K-correction. We use the LESS data, as well as deep Spitzer and VLA imaging, to identify 118 individual sources that produce significant emission in the BLAST bands. (6 data files).

AB - We present a joint analysis of the overlapping Balloon-borne Large Aperture Submillimetre Telescope (BLAST) 250, 350, 500um, and LABOCA 870um observations [from the LABOCA ECDFS Submm Survey (LESS) survey] of the Extended Chandra Deep Field-South. Out to z~3, the BLAST filters sample near the peak wavelength of thermal far-infrared (FIR) emission from galaxies (rest-frame wavelengths ~60-200um), primarily produced by dust heated through absorption in star-forming clouds. However, identifying counterparts to individual BLAST peaks is very challenging, given the large beams [full-width at half-maximum (FWHM) 36-60 arcsec]. In contrast, the ground-based 870um observations have a significantly smaller 19 arcsec FWHM beam, and are sensitive to higher redshifts (z~1-5, and potentially beyond) due to the more favourable negative K-correction. We use the LESS data, as well as deep Spitzer and VLA imaging, to identify 118 individual sources that produce significant emission in the BLAST bands. (6 data files).

KW - Galaxy catalogs

KW - X-ray sources

KW - Millimetric/submm sources

M3 - Article

VL - 741

SP - 10505

JO - VizieR On-line Data Catalog

JF - VizieR On-line Data Catalog

ER -

Sub-mm observations in Extended Chandra DFS (Chapin+, 2011)

Abstract / Description of output

Keywords / Materials (for Non-textual outputs)

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