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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”).

(a)

Approximate. See Sect. 3 for detailed implementation;

(b)

250, 350, 500 μm obtained in coordinated observations by the HerMES key program (Oliver et al. 2011);

(c)

in array coordinates, true position angle on sky will depend for these fields on execution date of the observation.

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