2016
Collaboration, Planck et al. “Planck 2015 Results. XII. Full Focal Plane Simulations.” \aap 594 (2016): A12.
Collaboration, Planck et al. “Planck 2015 Results. XXVIII. The Planck Catalogue of Galactic Cold Clumps.” \aap 594 (2016): A28.
Collaboration, Planck et al. “Planck 2015 Results. XI. CMB Power Spectra, Likelihoods, and Robustness of Parameters.” \aap 594 (2016): A11.
Collaboration, Planck et al. “Planck 2015 Results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources.” \aap 594 (2016): A27.
Collaboration, Planck et al. “Planck 2015 Results. X. Diffuse Component Separation: Foreground Maps.” \aap 594 (2016): A10.
Collaboration, Planck et al. “Planck 2015 Results. XXVI. The Second Planck Catalogue of Compact Sources.” \aap 594 (2016): A26.
Collaboration, Planck et al. “Planck 2015 Results. IX. Diffuse Component Separation: CMB Maps.” \aap 594 (2016): A9.
Collaboration, Planck et al. “Planck 2015 Results. XXV. Diffuse Low-Frequency Galactic Foregrounds.” \aap 594 (2016): A25.
Collaboration, Planck et al. “Planck 2015 Results. VIII. High Frequency Instrument Data Processing: Calibration and Maps.” \aap 594 (2016): A8.
Collaboration, Planck et al. “Planck 2015 Results. XXIV. Cosmology from Sunyaev-Zeldovich Cluster Counts.” \aap 594 (2016): A24.
Collaboration, Planck et al. “Planck 2015 Results. VII. High Frequency Instrument Data Processing: Time-Ordered Information and Beams.” \aap 594 (2016): A7.
Collaboration, Planck et al. “Planck 2015 Results. XXIII. The Thermal Sunyaev-Zeldovich Effect-Cosmic Infrared Background Correlation.” \aap 594 (2016): A23.
Collaboration, Planck et al. “Planck 2015 Results. I. Overview of Products and Scientific Results.” \aap 594 (2016): A1.
Collaboration, Planck et al. “Planck Intermediate Results. LII. Planet Flux Densities.” ArXiv e-prints (2016): n. pag. Print.
Collaboration, Planck et al. “Planck 2015 Results. XXII. A Map of the Thermal Sunyaev-Zeldovich Effect.” \aap 594 (2016): A22.
Collaboration, Planck et al. “Planck Intermediate Results. LI. Features in the Cosmic Microwave Background Temperature Power Spectrum and Shifts in Cosmological Parameters.” ArXiv e-prints (2016): n. pag. Print.
Collaboration, Planck et al. “Planck Intermediate Results. XLIX. Parity-Violation Constraints from Polarization Data.” \aap 596 (2016): A110.
Collaboration, Planck et al. “Planck 2015 Results. XXI. The Integrated Sachs-Wolfe Effect.” \aap 594 (2016): A21.
Collaboration, Planck et al. “Planck Intermediate Results. XXXVIII. E- and B-Modes of Dust Polarization from the Magnetized Filamentary Structure of the Interstellar Medium.” \aap 586 (2016): A141.
Collaboration, Planck et al. “Planck Intermediate Results. XLVIII. Disentangling Galactic Dust Emission and Cosmic Infrared Background Anisotropies.” \aap 596 (2016): A109.
Collaboration, Planck et al. “Planck 2015 Results. XX. Constraints on Inflation.” \aap 594 (2016): A20.
Collaboration, Planck et al. “Planck Intermediate Results. XXXVII. Evidence of Unbound Gas from the Kinetic Sunyaev-Zeldovich Effect.” \aap 586 (2016): A140.
2015
Gudmundsson, J. E. et al. “The Thermal Design, Characterization, and Performance of the SPIDER Long-Duration Balloon Cryostat.” Cryogenics 72 (2015): 65–76.
Collaboration, BICEP2 et al. “Antenna-Coupled TES Bolometers Used in BICEP2, Keck Array, and Spider.” \apj 812 (2015): 176.
Collaboration, Planck et al. “Planck Intermediate Results. XXVIII. Interstellar Gas and Dust in the Chamaeleon Clouds As Seen by Fermi LAT and Planck.” \aap 582 (2015): A31.
Collaboration, Planck et al. “Planck Intermediate Results. XXVI. Optical Identification and Redshifts of Planck Clusters With the RTT150 Telescope.” \aap 582 (2015): A29.
Collaboration, Planck et al. “Planck Intermediate Results. XXV. The Andromeda Galaxy As Seen by Planck.” \aap 582 (2015): A28.
Collaboration, Planck et al. “Planck 2013 Results. XXXII. The Updated Planck Catalogue of Sunyaev-Zeldovich Sources.” \aap 581 (2015): A14.
Collaboration, Gudmundsson Spider. “The Thermal Design, Characterization, and Performance of the SPIDER Long-Duration Balloon Cryostat.” arXiv 1506.06953v2 (2015): n. pag.
Abstract
We describe the Spider ight cryostat, which is designed to cool six millimeter-wavelength telescopes during an Antarctic
long-duration balloon ight. The cryostat, one of the largest to have own on a stratospheric payload, uses liquid 4He
to deliver cooling power to stages at 4.2 and 1.6 K. Stainless steel capillaries facilitate a high ow impedance connection
between the main liquid helium tank and a smaller superuid tank, allowing the latter to operate at 1.6 K as long as
there is liquid in the 4.2 K main tank. Each telescope houses a closed cycle 3He adsorption refrigerator that further cools
the focal planes down to 300 mK. Liquid helium vapor from the main tank is routed through heat exchangers that cool
radiation shields, providing negative thermal feedback. The system performed successfully during a 17 day ight in the
2014{2015 Antarctic summer. The cryostat had a total hold time of 16.8 days, with 15.9 days occurring during ight.
2000
Jones, W.C. “A Three-Stage Helium Sorption Refrigerator for Cooling of Infrared Detectors to 280 MK,.” Cryogenics 40(11).685 (2000): n. pag. Print.