Overview:
The Herschel
Lensing Survey (HLS) is a large extensive imaging
survey of massive galaxy clusters in the
far-infrared and submillimeter using the Herschel
Space Observatory. Its main scientific goals
are the following:
- To detect and study infrared/submillimeter galaxies
that are below
the nominal confusion limit of Herschel by
taking advantage of the strong gravitational lensing
power of massive galaxy clusters.
- To discover exceptionally
bright (Speak>100 mJy) lensed infrared/submillimeter
galaxies that will allow a variety of
detailed multi-wavelength follow-up observations.
- To examine infrared/submillimeter properties of galaxies in dense
environment (i.e., cluster members).
- To investigate the Sunyaev-Zel'dovich (SZ) effect through
the detection of the increment signal.
In terms of design, the HLS consists of the following two
types of surveys:
- HLS-deep: Deep
PACS (100/160 µm; 7'x7') and SPIRE (250/350/500 µm;
15'x15') imaging of 54 X-ray-luminous (i.e., massive)
clusters (including 24/25 CLASH clusters).
- HLS-snapshot:
Shallow (but nearly confusion-limited) SPIRE
(250/350/500 µm; 15'x15') imaging of 527 X-ray- or
SZ-selected massive clusters (including 148 SPT
clusters).
The following table provides more detailed information on
individual Herschel programs:
|
Cycle
|
Title
|
Tobs (hrs)
|
#clusters
|
HLS-deep I
|
0
|
"The Herschel
Lensing Survey"
Open-Time Key Program (OTKP)
|
318.2
|
44
|
HLS-deep II
|
2
|
"Herschel
Lensing Survey II": Completing the Herschel
Legacy with the HST/MCT CLASH Sample"
|
48.2
|
10
|
HLS-snapshot I
|
1
|
"SPIRE
Snapshot Survey of Massive Galaxy Clusters"
|
27.3
|
279
|
HLS-snapshot II
|
2
|
"SPIRE
Snapshot Survey II: Using SPT/CODEX Massive
Clusters as Powerful Gravitational Lenses"
|
25
|
248
|
|
|
Total
|
418.7
|
581
|
History:
In its original design, the Herschel Lensing Survey (HLS)
was conceived as a deep PACS and SPIRE imaging survey of
~40 massive clusters (HLS-deep I). However, the
discovery of an exceptionally bright cluster-lensed
submillimeter galaxy (the Eyelash) by Swinbank et al.
(2010) suggested that surveying a much larger cluster
sample would likely find similarly spectacular lensed
galaxies. Therefore, we started a second survey,
conducting shallower SPIRE-only imaging of ~280 clusters
selected from the ROSAT Millennium Cluster Sample
constructed by H. Ebeling (HLS-snapshot I). The
success of these two programs motivated us to expand
the surveys even further in Cycle 2 by (i)
completing the deep PACS and SPIRE coverage for the
HST/MCT CLASH sample by observing the remaining 10
clusters (HLS-deep II), and (ii) continuing the snapshot
survey by observing a sample of another ~250 clusters at
higher redshift (z>0.3) selected from the SPT and CODEX
clusters (HLS-snapshot II). Unfortunately, we ended
up missing one CLASH cluster because the CLASH team later
replaced A963 with A1423, the latter of which has not been
targeted by Herschel.
To make it simple, we refer to the combination of our four
Herschel programs as the Herschel
Lensing Survey (HLS), and define two
sub-programs, HLS-deep and HLS-snapshot, as described above. We keep the distinction between
the surveys I's and II's only interenally since the
corresponding Co-I's and data-sharing policies may differ.
|