Comparison of designs of off-axis Gregorian telescopes for millimeter-wave large focal-plane arrays.

We compare the diffraction-limited field of view (FOV) provided by four types of off-axis Gregorian telescopes: the classical Gregorian, the aplanatic Gregorian, and the designs that cancel astigmatism and both astigmatism and coma. The analysis is carried out with telescope parameters that are appropriate for satellite and balloonborne millimeter- and submillimeter-wave astrophysics. We find that the design that cancels both coma and astigmatism provides the largest flat FOV, approximately 21 square deg. We also find that the FOV can be increased by approximately 15% by means of optimizing the shape and location of the focal surface.

[1]  C. Dragone,et al.  The radiation pattern and impedance of offset and symmetrical near-field Cassegrainian and Gregorian antennas , 1974 .

[2]  C. Dragone,et al.  Offset multireflector antennas with perfect pattern symmetry and polarization discrimination , 1978, The Bell System Technical Journal.

[3]  Y. Mizuguchi,et al.  Offset Gregorian antenna , 1978 .

[4]  F. Brickell,et al.  Dual offset reflectors shaped for zero cross-polarisation and prescribed aperture illumination , 1979 .

[5]  C. Dragone,et al.  A first-order treatment of aberrations in Cassegrainian and Gregorian antennas , 1982 .

[6]  C. Dragone,et al.  First-order correction of aberrations in Cassegrainian and Gregorian antennas , 1983 .

[7]  Terry S. Mast,et al.  Optical Design And Instrumentation Of The Keck Observatory , 1986, Astronomical Telescopes and Instrumentation.

[8]  James J. Bock,et al.  Silicon nitride micromesh bolometer arrays for SPIRE , 1998, Astronomical Telescopes and Instrumentation.

[9]  James J. Bock,et al.  Bolocam: a millimeter-wave bolometric camera , 1998, Astronomical Telescopes and Instrumentation.

[10]  Dominic J. Benford,et al.  Development of a broadband submillimeter grating spectrometer , 1998, Astronomical Telescopes and Instrumentation.

[11]  Eugene E. Haller,et al.  Bolometer array development at the Max-Planck-Institut fuer Radioastronomie , 1998, Astronomical Telescopes and Instrumentation.

[12]  Hilo,et al.  SCUBA: A Common - user submillimetre camera operating on the James Clerk Maxwell telescope , 1998, astro-ph/9809122.

[13]  Patrice Rey,et al.  New technological development for far-infrared bolometer arrays , 1999, Defense, Security, and Sensing.

[14]  L. Page The MAP satellite mission to map the CMB anisotropy , 2000, astro-ph/0012214.

[15]  Jean-Bernard Riti,et al.  Very wide band telescope for Planck using optical and radio frequency techniques , 2000, Astronomical Telescopes + Instrumentation.

[16]  V. V. Hristov,et al.  MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10'-5° , 2000, astro-ph/0005123.

[17]  Adrian T. Lee,et al.  Monolithic arrays of absorber-coupled voltage-biased superconducting bolometers , 2000 .

[18]  K. Ganga,et al.  First Results from Viper: Detection of Small-scale Anisotropy at 40 GHz , 1999, The Astrophysical journal.

[19]  A. Melchiorri,et al.  A flat Universe from high-resolution maps of the cosmic microwave background radiation , 2000, Nature.

[20]  Christopher W. O'Dell,et al.  A Limit on the Large Angular Scale Polarization of the Cosmic Microwave Background , 2001 .

[21]  et al,et al.  Archeops: a high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies , 2001 .

[22]  D. Barkats,et al.  New Limits on the Polarized Anisotropy of the Cosmic Microwave Background at Subdegree Angular Scales , 2000, astro-ph/0204438.