Table 1
PEP fields.
Field | RA | Dec | Size | PA | Wavelengths | Observations | Time |
degree, J2000 | arcmin | degree | μm | h | |||
|
|||||||
COSMOS | 150.11917 | 2.20583 | 85 × 85 | 0a | 100,160b | Nov. 2009–Jun. 2010 | 196.9 |
Lockman Hole XMM | 163.17917 | 57.48000 | 24 × 24 | 0 | 100,160b | Oct. 2009–Nov. 2009 | 32.1 |
EGS | 214.82229 | 52.82617 | 67 × 10 | 40.5 | 100,160b | May 2011–June 2011 | 34.8 |
ECDFS | 53.10417 | –27.81389 | 30 × 30 | 0 | 100,160b | Feb. 2010–Feb. 2011 | 32.8 |
GOODS-S | 53.12654 | –27.80467 | 17 × 11 | –11.3 | 70,100,160b | Jan. 2010 | 239.7 |
GOODS-N | 189.22862 | 62.23867 | 17 × 11 | 41 | 100,160b | Oct. 2009 | 25.8 |
Cl0024+16 | 6.62500 | 17.16250 | 6 × 6 | 45c | 100,160b | Jun. 2010 | 6.2 |
Abell 370 | 39.97083 | –1.57861 | 4 × 4 | 45c | 100,160b | 5.3 | |
MS0451.6-0305 | 73.55000 | –3.01667 | 4 × 4 | 45c | 100,160b | May 2010 | 5.3 |
Abell 1689 | 197.87625 | –1.34000 | 4 × 4 | 45c | 100,160b | Jan. 2011– | 13.0 |
RXJ1347.5-1145 | 206.87708 | –11.75250 | 4 × 4 | 45c | 100,160b | Feb. 2011 | 5.3 |
MS1358.4+6245 | 209.97625 | 62.51000 | 4 × 4 | 45c | 100,160b | May 2010 | 5.3 |
Abell 1835 | 210.25833 | 2.87889 | 4 × 4 | 45c | 100,160b | Feb. 2011 | 5.3 |
Abell 2218 | 248.97083 | 66.20611 | 4 × 4 | 45c | 100,160b | Oct. 2009 | 10.2 |
Abell 2219 | 250.08333 | 46.71194 | 4 × 4 | 45c | 100,160b | May 2010 | 5.3 |
Abell 2390 | 328.40417 | 17.69556 | 4 × 4 | 45c | 100,160b | May 2010 | 5.3 |
RXJ0152.7-1357 | 38.17083 | –13.96250 | 10 × 5 | 45 | 100,160,250,350,500 | Mar. 2010–Jan. 2011 | 5.8 |
MS1054.4-0321 | 164.25092 | –3.62428 | 10 × 5 | 0 | 100,160,250,350,500 | Jun. 2010–Dec. 2010 | 5.8 |
Notes. List of the six blank deep fields, ten lensing clusters, and two z ~ 1 clusters to be observed by PEP. As of early June 2011, surveys for all fields except Abell 370 and Abell 1689 are completed (see column “Observations”).
Approximate. See Sect. 3 for detailed implementation;
250, 350, 500 μm obtained in coordinated observations by the HerMES key program (Oliver et al. 2011);
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