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  1. No Access

    Article

    Single Pixel Performance of the Kinetic Inductance Detectors for the Terahertz Intensity Mapper

    The Terahertz Intensity Mapper (TIM) is a NASA far-infrared balloon mission designed to perform [CII] intensity map** of the peak of cosmic star formation. To achieve this goal, TIM will fly two grating spec...

    R. M. J. Janssen, R. Nie, B. Bumble, L.-J. Liu in Journal of Low Temperature Physics (2023)

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    Article

    Design of the Kinetic Inductance Detector Based Focal Plane Assembly for the Terahertz Intensity Mapper

    We report on the kinetic inductance detector (KID) array focal plane assembly design for the Terahertz Intensity Mapper (TIM). Each of the 2 arrays consists of 4 wafer-sized dies (quadrants), and the overall a...

    L.-J. Liu, R. M. J. Janssen, C. M. Bradford in Journal of Low Temperature Physics (2022)

  3. No Access

    Article

    SPT-SLIM: A Line Intensity Map** Pathfinder for the South Pole Telescope

    The South Pole Telescope Summertime Line Intensity Mapper (SPT-SLIM) is a pathfinder experiment that will demonstrate the use of on-chip filter-bank spectrometers for mm-wave line intensity map**. The SPT-SL...

    K. S. Karkare, A. J. Anderson, P. S. Barry in Journal of Low Temperature Physics (2022)

  4. No Access

    Article

    Absorber Design and Optimization of Kinetic Inductance Detectors for the Terahertz Intensity Mapper

    We discuss the design and optimization of the absorber for Terahertz Intensity Mapper, a balloon-borne kinetic inductance detector spectrometer. The novel “chain-link” absorber design offers excellent performa...

    R. Nie, R. M. J. Janssen, C. M. Bradford in Journal of Low Temperature Physics (2022)

  5. Article

    Author Correction: A massive core for a cluster of galaxies at a redshift of 4.3

    Change history: In this Letter, the Acknowledgements section should have included the following sentence: “The National Radio Astronomy Observatory is a facility of the National Science Foundation operated und...

    T. B. Miller, S. C. Chapman, M. Aravena, M. L. N. Ashby, C. C. Hayward in Nature (2018)

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    Article

    A massive core for a cluster of galaxies at a redshift of 4.3

    Massive galaxy clusters have been found that date to times as early as three billion years after the Big Bang, containing stars that formed at even earlier epochs13. The high-redshift progenitors of these galaxy...

    T. B. Miller, S. C. Chapman, M. Aravena, M. L. N. Ashby, C. C. Hayward in Nature (2018)

  7. No Access

    Article

    Galaxy growth in a massive halo in the first billion years of cosmic history

    Two extremely massive galaxies are seen 800 million years after the Big Bang, showing the rapid growth of early structure and marking the most massive halo known in that era.

    D. P. Marrone, J. S. Spilker, C. C. Hayward, J. D. Vieira, M. Aravena in Nature (2018)

  8. No Access

    Article

    Dusty starburst galaxies in the early Universe as revealed by gravitational lensing

    A spectroscopic redshift survey of extraordinarily bright millimetre-wave-selected sources of carbon monoxide line emission — originating from star-forming molecular gas — shows that at least ten of these sour...

    J. D. Vieira, D. P. Marrone, S. C. Chapman, C. De Breuck, Y. D. Hezaveh, A. Weiβ in Nature (2013)

  9. No Access

    Article

    A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies

    X-ray, optical and infrared observations reveal a very high rate of star formation in the core of an extremely luminous galaxy cluster; this starburst seems to be triggered by a cooling flow of the dense intra...

    M. McDonald, M. Bayliss, B. A. Benson, R. J. Foley, J. Ruel, P. Sullivan in Nature (2012)

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    Article

    Optical and Thermal Properties of ANL/KICP Polarization Sensitive Bolometers for SPTpol

    We present recent optical and thermal characterizations of polarization sensitive mm-wave bolometers fabricated at Argonne National Lab. The devices are designed to measure the polarization of the Cosmic Micro...

    C. L. Chang, P. Ade, K. Aird, J. Austermann, J. Beall in Journal of Low Temperature Physics (2012)

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    Article

    An Overview of the SPTpol Experiment

    In 2012 the South Pole Telescope (SPT) will begin a 625 deg2 survey to measure the polarization anisotropy of the cosmic microwave background (CMB). Observations of the CMB B-mode angular power spectrum will be u...

    L. Bleem, P. Ade, K. Aird, J. Austermann, J. Beall in Journal of Low Temperature Physics (2012)

  12. No Access

    Article

    SMA observations of the magnetic fields around a low-mass protostellar system

    Observations of the submillimeter polarized dust emission is an important tool to study the role of the magnetic fields in the evolutions of molecular clouds and in the star formation processes. The Submillim...

    J. M. Girart, R. Rao, D. P. Marrone in Astrophysics and Space Science (2008)

  13. No Access

    Chapter and Conference Paper

    SMA observations of the magnetic fields around a low-mass protostellar system

    Observations of the submillimeter polarized dust emission is an important tool to study the role of the magnetic fields in the evolutions of molecular clouds and in the star formation processes. The Submillime...

    J. M. Girart, R. Rao, D. P. Marrone in Science with the Atacama Large Millimeter Array (2008)

  14. No Access

    Chapter and Conference Paper

    The Polarization Properties of Sgr A∗ at Submillimeter Wavelengths

    We have placed an upper limit on the magnitude of the rotation measure of 7 × 10^5 rad m-2 for the putative Faraday screen (magnetized plasma) in front of Sgr A*, the radio source associated with the black hole i...

    J.M. Moran, D.P. Marrone, J.-H. Zhao, R. Rao in Relativistic Astrophysics Legacy and Cosmo… (2007)