2010A&A...518L..12E


C.D.S. - SIMBAD4 rel 1.7 - 2021.02.24CET21:51:04

2010A&A...518L..12E - Astronomy and Astrophysics, volume 518, L12-12 (2010/7-2)

The Herschel Lensing Survey (HLS): overview.

EGAMI E., REX M., RAWLE T.D., PEREZ-GONZALEZ P.G., RICHARD J., KNEIB J.-P., SCHAERER D., ALTIERI B., VALTCHANOV I., BLAIN A.W., FADDA D., ZEMCOV M., BOCK J.J., BOONE F., BRIDGE C.R., CLEMENT B., COMBES F., DESSAUGES-ZAVADSKY M., DOWELL C.D., ILBERT O., IVISON R.J., JAUZAC M., LUTZ D., METCALFE L., OMONT A., PELLO R., PEREIRA M.J., RIEKE G.H., RODIGHIERO G., SMAIL I., SMITH G.P., TRAMOY G., WALTH G.L., VAN DER WERF P. and WERNER M.W.

Abstract (from CDS):

The Herschel Lensing Survey (HLS) will conduct deep PACS and SPIRE imaging of ∼40 massive clusters of galaxies. The strong gravitational lensing power of these clusters will enable us to penetrate through the confusion noise, which sets the ultimate limit on our ability to probe the Universe with Herschel. Here we present an overview of our survey and a summary of the major results from our science demonstration phase (SDP) observations of the Bullet cluster (z=0.297). The SDP data are rich and allow us to study not only the background high-redshift galaxies (e.g., strongly lensed and distorted galaxies at z=2.8 and 3.2) but also the properties of cluster-member galaxies. Our preliminary analysis shows a great diversity of far-infrared/submillimeter spectral energy distributions (SEDs), indicating that we have much to learn with Herschel about the properties of galaxy SEDs. We have also detected the Sunyaev-Zel'dovich (SZ) effect increment with the SPIRE data. The success of this SDP program demonstrates the great potential of the Herschel Lensing Survey to produce exciting results in a variety of science areas.

Abstract Copyright:

Journal keyword(s): infrared: galaxies - submillimeter: galaxies - galaxies: evolution - galaxies: high-redshift - galaxies: clusters: general

Simbad objects: 8

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Number of rows : 8

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 ClG 0451-03 ClG 04 54 10.9 -03 01 07     20.0     ~ 333 0
2 [LGH99] MS 0456.6-0305 A1 G 04 54 13.00 -03 00 55.9           ~ 5 1
3 ClG 0657-56 ClG 06 58 29.6 -55 56 39           ~ 825 1
4 ACO 2218 ClG 16 35 54.0 +66 13 00           ~ 782 1
5 NAME SMM J16359+6612.4 LeI 16 35 54.10 +66 12 23.8           ~ 29 0
6 NAME Eyelash LeG 21 35 11.60 -01 02 52.0           ~ 190 0
7 ClG J2135-0102 ClG 21 35 12.1 -01 02 57           ~ 36 0
8 NAME 1E 0657-56 Arc+Core Galaxy LeG ~ ~           ~ 10 0

    Equat.    Gal    SGal    Ecl

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