DARKNESS: A Microwave Kinetic Inductance Detector Integral Field Spectrograph for High-contrast Astronomy
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 simultaneo...
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| Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 2018-06, Vol.130 (988), p.65001 |
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| creator | Meeker, Seth R. Mazin, Benjamin A. Walter, Alex B. Strader, Paschal Fruitwala, Neelay Bockstiegel, Clint Szypryt, Paul Ulbricht, Gerhard Coiffard, Grégoire Bumble, Bruce Cancelo, Gustavo Zmuda, Ted Treptow, Ken Wilcer, Neal Collura, Giulia Dodkins, Rupert Lipartito, Isabel Zobrist, Nicholas Bottom, Michael Shelton, J. Chris Mawet, Dimitri van Eyken, Julian C. Vasisht, Gautam Serabyn, Eugene |
| description | 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. |
| doi_str_mv | 10.1088/1538-3873/aab5e7 |
| format | Article |
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Chris ; Mawet, Dimitri ; van Eyken, Julian C. ; Vasisht, Gautam ; Serabyn, Eugene</creator><creatorcontrib>Meeker, Seth R. ; Mazin, Benjamin A. ; Walter, Alex B. ; Strader, Paschal ; Fruitwala, Neelay ; Bockstiegel, Clint ; Szypryt, Paul ; Ulbricht, Gerhard ; Coiffard, Grégoire ; Bumble, Bruce ; Cancelo, Gustavo ; Zmuda, Ted ; Treptow, Ken ; Wilcer, Neal ; Collura, Giulia ; Dodkins, Rupert ; Lipartito, Isabel ; Zobrist, Nicholas ; Bottom, Michael ; Shelton, J. Chris ; Mawet, Dimitri ; van Eyken, Julian C. ; Vasisht, Gautam ; Serabyn, Eugene ; Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><description>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.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1088/1538-3873/aab5e7</identifier><language>eng</language><publisher>Philadelphia: The Astronomical Society of the Pacific</publisher><subject>adaptive optics ; Astronomy ; ASTRONOMY AND ASTROPHYSICS ; coronagraphs ; INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY ; instrumentation: adaptive optics ; Instrumentation: coronagraphs ; instrumentation: detectors ; instrumentation: spectrographs ; Optics ; planets and satellites: detection ; spectrographs — planets and satellites: detection ; Spectrophotometers ; Spectroscopy</subject><ispartof>Publications of the Astronomical Society of the Pacific, 2018-06, Vol.130 (988), p.65001</ispartof><rights>2018. The Astronomical Society of the Pacific. All rights reserved.</rights><rights>Copyright University of Chicago Press Jun 2018</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c479t-acce449ab32e21896f6ef7f6d88d4bf40d10ea66f5772bb4ab4860d3e728bf893</citedby><cites>FETCH-LOGICAL-c479t-acce449ab32e21896f6ef7f6d88d4bf40d10ea66f5772bb4ab4860d3e728bf893</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1538-3873/aab5e7/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,777,781,882,27905,27906,53827,53874</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1511669$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Meeker, Seth R.</creatorcontrib><creatorcontrib>Mazin, Benjamin A.</creatorcontrib><creatorcontrib>Walter, Alex B.</creatorcontrib><creatorcontrib>Strader, Paschal</creatorcontrib><creatorcontrib>Fruitwala, Neelay</creatorcontrib><creatorcontrib>Bockstiegel, Clint</creatorcontrib><creatorcontrib>Szypryt, Paul</creatorcontrib><creatorcontrib>Ulbricht, Gerhard</creatorcontrib><creatorcontrib>Coiffard, Grégoire</creatorcontrib><creatorcontrib>Bumble, Bruce</creatorcontrib><creatorcontrib>Cancelo, Gustavo</creatorcontrib><creatorcontrib>Zmuda, Ted</creatorcontrib><creatorcontrib>Treptow, Ken</creatorcontrib><creatorcontrib>Wilcer, Neal</creatorcontrib><creatorcontrib>Collura, Giulia</creatorcontrib><creatorcontrib>Dodkins, Rupert</creatorcontrib><creatorcontrib>Lipartito, Isabel</creatorcontrib><creatorcontrib>Zobrist, Nicholas</creatorcontrib><creatorcontrib>Bottom, Michael</creatorcontrib><creatorcontrib>Shelton, J. Chris</creatorcontrib><creatorcontrib>Mawet, Dimitri</creatorcontrib><creatorcontrib>van Eyken, Julian C.</creatorcontrib><creatorcontrib>Vasisht, Gautam</creatorcontrib><creatorcontrib>Serabyn, Eugene</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><title>DARKNESS: A Microwave Kinetic Inductance Detector Integral Field Spectrograph for High-contrast Astronomy</title><title>Publications of the Astronomical Society of the Pacific</title><addtitle>Publ. Astron. Soc. Pac</addtitle><description>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.</description><subject>adaptive optics</subject><subject>Astronomy</subject><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>coronagraphs</subject><subject>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</subject><subject>instrumentation: adaptive optics</subject><subject>Instrumentation: coronagraphs</subject><subject>instrumentation: detectors</subject><subject>instrumentation: spectrographs</subject><subject>Optics</subject><subject>planets and satellites: detection</subject><subject>spectrographs — planets and satellites: detection</subject><subject>Spectrophotometers</subject><subject>Spectroscopy</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp1kM9PwyAcxYnRxPnj7pHoUeugpZR6azbnzPyROD0TSsFhZqnANP730tToRbmQvO97Ly8fAI4wOseIsTHOM5ZkrMjGQtS5KrbA6EfaBiOEEEloytAu2PP-BSGMGUYjYKbVw-Lucrm8gBW8NdLZD_Gu4MK0KhgJr9tmI4NopYJTFZQM1kUtqGcn1nBm1LqByy7KzkalW0Ed73PzvEqkbYMTPsDKx2NrXz8PwI4Wa68Ov_998DS7fJzMk5v7q-tJdZNIUpQhEVIqQkpRZ6lKMSuppkoXmjaMNaTWBDUYKUGpzosirWsiasIoajJVpKzWrMz2wfHQa30w3EsTZ6_inDbO5DjHmNLedDKYOmffNsoH_mI3ro27eBofJXmW59GFBlfE4r1TmnfOvAr3yTHiPXXeI-Y9Yj5Qj5HTIWJs99vZCd9xnCFexgyiecTPu0ZH99kf7n_LvwA1XZHJ</recordid><startdate>20180601</startdate><enddate>20180601</enddate><creator>Meeker, Seth R.</creator><creator>Mazin, Benjamin A.</creator><creator>Walter, Alex B.</creator><creator>Strader, Paschal</creator><creator>Fruitwala, Neelay</creator><creator>Bockstiegel, Clint</creator><creator>Szypryt, Paul</creator><creator>Ulbricht, Gerhard</creator><creator>Coiffard, Grégoire</creator><creator>Bumble, Bruce</creator><creator>Cancelo, Gustavo</creator><creator>Zmuda, Ted</creator><creator>Treptow, Ken</creator><creator>Wilcer, Neal</creator><creator>Collura, Giulia</creator><creator>Dodkins, Rupert</creator><creator>Lipartito, Isabel</creator><creator>Zobrist, Nicholas</creator><creator>Bottom, Michael</creator><creator>Shelton, J. 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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.</abstract><cop>Philadelphia</cop><pub>The Astronomical Society of the Pacific</pub><doi>10.1088/1538-3873/aab5e7</doi><tpages>16</tpages><oa>free_for_read</oa></addata></record> |
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| subjects | adaptive optics Astronomy ASTRONOMY AND ASTROPHYSICS coronagraphs INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY instrumentation: adaptive optics Instrumentation: coronagraphs instrumentation: detectors instrumentation: spectrographs Optics planets and satellites: detection spectrographs — planets and satellites: detection Spectrophotometers Spectroscopy |
| title | DARKNESS: A Microwave Kinetic Inductance Detector Integral Field Spectrograph for High-contrast Astronomy |
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