DARKNESS: A Microwave Kinetic Inductance Detector Integral Field Spectrograph for High-contrast Astronomy

被引：57

作者：

Meeker, Seth R. ^{[1
,2
]}

Mazin, Benjamin A. ^{[1
]}

Walter, Alex B. ^{[1
]}

Strader, Paschal ^{[3
]}

Fruitwala, Neelay ^{[1
]}

Bockstiegel, Clint ^{[1
]}

Szypryt, Paul ^{[1
]}

Ulbricht, Gerhard ^{[4
]}

Coiffard, Gregoire ^{[1
]}

Bumble, Bruce ^{[2
]}

Cancelo, Gustavo ^{[5
]}

Zmuda, Ted ^{[5
]}

Treptow, Ken ^{[5
]}

Wilcer, Neal ^{[5
]}

Collura, Giulia ^{[1
]}

Dodkins, Rupert ^{[6
]}

Lipartito, Isabel ^{[1
]}

Zobrist, Nicholas ^{[1
]}

Bottom, Michael ^{[2
]}

Shelton, J. Chris ^{[2
]}

Mawet, Dimitri ^{[7
]}

van Eyken, Julian C. ^{[8
]}

Vasisht, Gautam ^{[2
]}

Serabyn, Eugene ^{[2
]}

机构：

[1] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[2] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[3] Dominican Sch Philosophy & Theol, Berkeley, CA 94708 USA

[4] Dublin Inst Adv Studies, Sch Cosm Phys, Dublin 4, Ireland

[5] Fermilab Natl Accelerator Lab, Pine St, Bataravia, IL 60510 USA

[6] Univ Oxford, Dept Phys, Oxford OX1 3RH, England

[7] CALTECH, Dept Astron, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[8] CALTECH, IPAC, Mail Code 100-22,1200 E Calif Blvd, Pasadena, CA USA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 2018年 / 130卷 / 988期

关键词：

instrumentation: adaptive optics; instrumentation: detectors; instrumentation: spectrographs; Instrumentation: coronagraphs; planets and satellites: detection; ADAPTIVE OPTICS SYSTEM; NEAR-IR; FAINT COMPANIONS; DYNAMIC-RANGE; IMAGES; LIMITS; CORONAGRAPH; TELESCOPES; SPECKLES;

D O I：

10.1088/1538-3873/aab5e7

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present DARKNESS (the DARK-speckle Near-infrared Energy-resolving Superconducting Spectrophotometer), the first of several planned integral field spectrographs to use optical/near-infrared Microwave Kinetic Inductance Detectors (MKIDs) for high-contrast imaging. The photon counting and simultaneous low-resolution spectroscopy provided by MKIDs will enable real-time speckle control techniques and post-processing speckle suppression at frame rates capable of resolving the atmospheric speckles that currently limit high-contrast imaging from the ground. DARKNESS is now operational behind the PALM-3000 extreme adaptive optics system and the Stellar Double Coronagraph at Palomar Observatory. Here, we describe the motivation, design, and characterization of the instrument, early on-sky results, and future prospects.

引用

页数：16

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