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10 results on '"Giulia Collura"'

1. A high efficiency photon veto for the Light Dark Matter eXperiment

Author

The LDMX collaboration, Torsten Åkesson, Nikita Blinov, Lene Bryngemark, Owen Colegrove, Giulia Collura, Craig Dukes, Valentina Dutta, Bertrand Echenard, Thomas Eichlersmith, Craig Group, Joshua Hiltbrand, David G. Hitlin, Joseph Incandela, Gordan Krnjaic, Juan Lazaro, Amina Li, Jeremiah Mans, Phillip Masterson, Jeremy McCormick, Omar Moreno, Geoffrey Mullier, Akshay Nagar, Timothy Nelson, Gavin Niendorf, James Oyang, Reese Petersen, Ruth Pöttgen, Philip Schuster, Harrison Siegel, Natalia Toro, Nhan Tran, and Andrew Whitbeck

Subjects
Beyond Standard Model, Dark matter, Fixed target experiments, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract Fixed-target experiments using primary electron beams can be powerful discovery tools for light dark matter in the sub-GeV mass range. The Light Dark Matter eXperiment (LDMX) is designed to measure missing momentum in high-rate electron fixed-target reactions with beam energies of 4 GeV to 16 GeV. A prerequisite for achieving several important sensitivity milestones is the capability to efficiently reject backgrounds associated with few-GeV bremsstrahlung, by twelve orders of magnitude, while maintaining high efficiency for signal. The primary challenge arises from events with photo-nuclear reactions faking the missing-momentum property of a dark matter signal. We present a methodology developed for the LDMX detector concept that is capable of the required rejection. By employing a detailed Geant4-based model of the detector response, we demonstrate that the sampling calorimetry proposed for LDMX can achieve better than 10 −13 rejection of few-GeV photons. This suggests that the luminosity-limited sensitivity of LDMX can be realized at 4 GeV and higher beam energies.

Published
2020
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2. DARKNESS: A Microwave Kinetic Inductance Detector Integral Field Spectrograph for High-contrast Astronomy

Author

Seth R. Meeker, Benjamin A. Mazin, Alex B. Walter, Paschal Strader, Neelay Fruitwala, Clint Bockstiegel, Paul Szypryt, Gerhard Ulbricht, Grégoire Coiffard, Bruce Bumble, Gustavo Cancelo, Ted Zmuda, Ken Treptow, Neal Wilcer, Giulia Collura, Rupert Dodkins, Isabel Lipartito, Nicholas Zobrist, Michael Bottom, J. Chris Shelton, Dimitri Mawet, Julian C. van Eyken, Gautam Vasisht, and Eugene Serabyn

Published
2018
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3. Second generation readout for large format photon counting microwave kinetic inductance detectors

Author

Ted Zmuda, John I. Bailey, Nicholas Zobrist, Gustavo Cancelo, Giulia Collura, Isabel Lipartito, Neelay Fruitwala, Paschal Strader, Alex B. Walter, Neal Wilcer, Ken Treptow, Benjamin A. Mazin, and Chris Stoughton

Subjects
Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, Large format, computer.software_genre, 01 natural sciences, Multiplexing, 010305 fluids & plasmas, Optics, 0103 physical sciences, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010302 applied physics, Physics, Signal processing, Pixel, business.industry, Firmware, Bandwidth (signal processing), Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Photon counting, business, Astrophysics - Instrumentation and Methods for Astrophysics, computer, Microwave
Abstract

We present the development of a second generation digital readout system for photon counting microwave kinetic inductance detector (MKID) arrays operating in the optical and near-IR wavelength bands. Our system retains much of the core signal processing architecture from the first generation system, but with a significantly higher bandwidth, enabling readout of kilopixel MKID arrays. Each set of readout boards is capable of reading out 1024 MKID pixels multiplexed over 2 GHz of bandwidth; two such units can be placed in parallel to read out a full 2048 pixel microwave feedline over a 4 -- 8 GHz band. As in the first generation readout, our system is capable of identifying, analyzing, and recording photon detection events in real time with a time resolution of order a few microseconds. Here, we describe the hardware and firmware, and present an analysis of the noise properties of the system. We also present a novel algorithm for efficiently suppressing IQ mixer sidebands to below -30 dBc., 12 pages, 12 figures

Published
2020

4. Design and Performance of Hafnium Optical and Near-IR Kinetic Inductance Detectors

Author

Noah Swimmer, Miguel Daal, Clint Bockstiegel, Nicholas Zobrist, Isabel Lipartito, Giulia Collura, Neelay Fruitwala, Sarah Steiger, Alex B. Walter, Benjamin A. Mazin, Gregoire Coiffard, and Bruce Bumble

Subjects
Materials science, Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), chemistry.chemical_element, FOS: Physical sciences, 02 engineering and technology, 01 natural sciences, Resonator, Electrical resistivity and conductivity, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010302 applied physics, Superconductivity, Resistive touchscreen, business.industry, Detector, Instrumentation and Detectors (physics.ins-det), 021001 nanoscience & nanotechnology, Hafnium, chemistry, Density of states, Optoelectronics, 0210 nano-technology, business, Astrophysics - Instrumentation and Methods for Astrophysics, Microwave
Abstract

We report on the design and performance of microwave kinetic inductance detectors (MKIDs) sensitive to single photons in the optical to near-infrared range using hafnium as the sensor material. Our test device had a superconducting transition temperature of 395 mK and a room temperature normal state resistivity of 97 μ Ω cm with RRR = 1.6. Resonators on the device displayed internal quality factors of around 200 000. Similar to the analysis of MKIDs made from other highly resistive superconductors, we find that modeling the temperature response of the detector requires an extra broadening parameter in the superconducting density of states. Finally, we show that this material and design is compatible with a full-array fabrication process, which resulted in pixels with decay times of about 40 μs and resolving powers of ∼9 at 800 nm.We report on the design and performance of microwave kinetic inductance detectors (MKIDs) sensitive to single photons in the optical to near-infrared range using hafnium as the sensor material. Our test device had a superconducting transition temperature of 395 mK and a room temperature normal state resistivity of 97 μ Ω cm with RRR = 1.6. Resonators on the device displayed internal quality factors of around 200 000. Similar to the analysis of MKIDs made from other highly resistive superconductors, we find that modeling the temperature response of the detector requires an extra broadening parameter in the superconducting density of states. Finally, we show that this material and design is compatible with a full-array fabrication process, which resulted in pixels with decay times of about 40 μs and resolving powers of ∼9 at 800 nm.

Published
2019
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5. Active speckle control with microwave kinetic inductance detectors (Conference Presentation)

Author

Isabel Lipartito, Julien Lozi, Giulia Collura, Michael Bottom, Olivier Guyon, Alex B. Walter, Benjamin A. Mazin, Clinton Bockstiegel, Neelay Fruitwala, and Seth R. Meeker

Subjects
Wavefront, Physics, Pixel, business.industry, Noise (electronics), law.invention, Speckle pattern, Optics, Cardinal point, law, Sensitivity (control systems), business, Adaptive optics, Coronagraph
Abstract

We present the development and testing of focal plane wavefront control techniques that utilize microwave kinetic inductance detectors (MKIDs) as a focal plane IFU. MKIDs are ideally suited to this application, as they are energy resolving, and have single photon sensitivity, zero read noise, and microsecond time resolution. These characteristics enable much higher feedback rates than conventional systems; for the first time, focal plane measurements may be used to correct atmospheric aberrations in addition to quasistatics. A variety of approaches are under development, including conventional speckle nulling, as well as more advanced approaches such as linear dark field control. We have developed an MKID-specific speckle nulling code for DARKNESS, a 10,000 pixel MKID IFU behind the stellar double coronagraph (SDC) and PALM-3000 (P3K) AO system at Palomar observatory. Our code implements the algorithm described in (Bottom, et. al, 2016) with minor modifications. To facilitate high feedback rates on sky, the code is optimized for computational speed, and implements low-latency communications to both P3K and the MKID readout. It is also capable of integrating with P3K in closed loop operation. Using our code, we have demonstrated quasi-static speckle nulling at a 1 Hz feedback rate in the laboratory. We hope to demonstrate rates ~10-100 Hz in the near future. In addition to continuing our work with DARKNESS, we will adapt our code to MEC, a 20,000 pixel MKID IFU behind the Subaru coronagraphic extreme adaptive optics system (SCExAO) at Subaru observatory. MEC is scheduled to commission in January 2018.

Published
2018

6. MEC: the MKID exoplanet camera for high contrast astronomy at Subaru (Conference Presentation)

Author

Nicholas Zobrist, Benjamin B. Mazin, Paul Szypryt, Clint Bockstiegel, Gregoire Coiffard, Giulia Collura, Julien Lozi, Olivier Guyon, Neelay Fruitwala, Nemanja Jovanovic, Seth R. Meeker, Alex B. Walter, Paschal Strader, and Isabel Lipartito

Subjects
Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astrophysics::Cosmology and Extragalactic Astrophysics, Wavefront sensor, Exoplanet, law.invention, Integral field spectrograph, law, Planet, Astrophysics::Solar and Stellar Astrophysics, Gemini Planet Imager, Astrophysics::Earth and Planetary Astrophysics, Subaru Telescope, Coronagraph, Circumstellar habitable zone, Astrophysics::Galaxy Astrophysics
Abstract

Direct Imaging of exoplanets is one of the most technically difficult techniques used to study exoplanets, but holds immense promise for not just detecting but characterizing planets around the nearest stars. Ambitious instruments at the world’s largest telescopes have been built to carry out this science: the Gemini Planet Imager (GPI), SPHERE at VLT, SCExAO at Subaru, and the P1640 and Stellar Double Coronagraph (SDC) at Palomar. These instruments share a common archetype consisting of an extreme AO system feeding a coronagraph for on-axis stellar light rejection followed by a focal plane Integral Field Spectrograph (IFS). They are currently limited by uncontrolled scattered and diffracted light which produces a coherent speckle halo in the image plane. A number of differential imaging schemes exist to mitigate these issues resulting in star-planet contrast ratios as deep as ~10^-6 at low angular separations. Surpassing this contrast limit requires high speed active speckle nullification from a focal plane wavefront sensor (FPWS) and new processing techniques. MEC, the Microwave Kinetic Inductance Detector (MKID) Exoplanet Camera, is a J-band IFS module behind Subaru Telescope’s SCExAO system. MEC is capable of producing an image cube several thousand times a second without the read noise that dominates conventional high speed IFUs. This enables it to integrate with SCExAO as an extremely fast FPWS while eliminating non-common path aberrations by doubling as a science camera. Key science objectives can be further explored if longer wavelengths (H and K band) are simultaneously sent to CHARIS for high resolution spectroscopy. MEC, to be commissioned at Subaru in early 2018, is the second MKID IFS for high contrast imaging following DARKNESS’ debut at Palomar in July 2016. MEC will follow up on young planets and debris disks discovered in the SEEDS survey or by Project 1640 as well as discover self-luminous massive planets. The increased sensitivity, combined with the advanced coronagraphs in SCExAO which have inner working angles (IWAs) as small as 0.03” at 1.2 μm, allows young Jupiter-sized objects to be imaged as close as 4 AU from their host star. If the wavefront control enabled by MEC is fully realized, it may begin to probe the reflected light of giant planets around some nearby stars, opening a new parameter space for direct imaging targeting older stars. While direct imaging of reflected light exoplanets is the most challenging of the scientific goals, it is a promising long-term path towards characterization of habitable planets around nearby stars using Extremely Large Telescopes (ELTs). With diameters of about 30-m, an ELT can resolve the habitable zones of nearby M-type stars, for which an Earth-sized planet would be at ~10^-7 contrast at 1 μm. This will complement future space-based high contrast optical imaging targeting the wider habitable zones of sun-like stars for ~10^-10 contrast earth analogs. We will present lessons learned from the first few months of MEC’s operation including initial lab and on-sky (weather permitting) results. We already have preliminary data from Palomar testing a new statistical speckle discrimination post-processing technique using the photon arrival time measured with MKIDs. Residual stellar light in the form of a speckle masquerading as a planetary companion is pulled from a modified Rician distribution and can be statistically discerned from a true off-axis Poisson point source. Additionally, the progress of active focal plane wavefront control will be briefly discussed.

Published
2018

7. Search for Optical Pulsation in M82 X-2

Author

Giulia Collura, Paul Szypryt, T. A. Prince, Seth R. Meeker, Paschal Strader, Ben Mazin, Clinton Bockstiegel, and Alex B. Walter

Subjects
Physics, Wavelength range, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, law.invention, Telescope, Pulsar, Space and Planetary Science, Observatory, law, 0103 physical sciences, Statistical analysis, M82 X-2, 010306 general physics, Sinusoidal modulation, 010303 astronomy & astrophysics
Abstract

We report on a search for optical pulsation from M82 X-2 over a range of periods. M82 X-2 is an X-ray pulsar with a 1.37s average spin period and a 2.5 day sinusoidal modulation. The observations were done with the ARray Camera for Optical to Near-IR Spectrophotometry at the 200 inch Hale telescope at the Palomar Observatory. We performed H test and χ^2 statistical analysis. No significant optical pulsations were found in the wavelength range of 3000–11000 A with a pulsation period between 1.36262 and 1.37462 s. We found an upper limit on pulsed emission in the 4000–8000 A wavelength range to be fainter than ~20.5 mag_(AB) , corresponding to ~23 μJy.

Published
2017

8. Large-format platinum silicide microwave kinetic inductance detectors for optical to near-IR astronomy

Author

Bruce Bumble, Clinton Bockstiegel, Nicholas Zobrist, Seth R. Meeker, G. Ulbricht, Gregoire Coiffard, Isabel Lipartito, Miguel Daal, Paul Szypryt, B. A. Mazin, Neelay Fruitwala, Giulia Collura, and Alex B. Walter

Subjects
Materials science, Physics - Instrumentation and Detectors, Silicon, business.industry, Detector, chemistry.chemical_element, FOS: Physical sciences, Large format, Substrate (electronics), Instrumentation and Detectors (physics.ins-det), 01 natural sciences, Atomic and Molecular Physics, and Optics, Platinum silicide, chemistry.chemical_compound, Optics, chemistry, 0103 physical sciences, Sapphire, 010306 general physics, business, Tin, Astrophysics - Instrumentation and Methods for Astrophysics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Microwave
Abstract

We have fabricated and characterized 10,000 and 20,440 pixel Microwave Kinetic Inductance Detector (MKID) arrays for the Dark-speckle Near-IR Energy-resolved Superconducting Spectrophotometer (DARKNESS) and the MKID Exoplanet Camera (MEC). These instruments are designed to sit behind adaptive optics systems with the goal of directly imaging exoplanets in a 800-1400 nm band. Previous large optical and near-IR MKID arrays were fabricated using substoichiometric titanium nitride (TiN) on a silicon substrate. These arrays, however, suffered from severe non-uniformities in the TiN critical temperature, causing resonances to shift away from their designed values and lowering usable detector yield. We have begun fabricating DARKNESS and MEC arrays using platinum silicide (PtSi) on sapphire instead of TiN. Not only do these arrays have much higher uniformity than the TiN arrays, resulting in higher pixel yields, they have demonstrated better spectral resolution than TiN MKIDs of similar design. PtSi MKIDs also do not display the hot pixel effects seen when illuminating TiN on silicon MKIDs with photons with wavelengths shorter than 1 um., Comment: 16 pages, 8 figures, published in Optics Express

Published
2017
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9. First evidence for off-shell production of the Higgs boson and measurement of its width

Author

Tumasyan, Armen, Wolfgang Adam, Andrejkovic, Janik Walter, Thomas Bergauer, Suman Chatterjee, Damanakis, Konstantinos, Marko Dragicevic, Alberto Escalante del Valle, Fruehwirth, Rudolf, Manfred Jeitler, Krammer, Natascha, Lukas Lechner, Liko, Dietrich, Mikulec, Ivan, Paulitsch, Peter, Pitters, Florian Michael, Jochen Schieck, Schoefbeck Robert, Schwarz, Dennis, Sebastian Templ, Wolfgang Waltenberger, Claudia-Elisabeth Wulz, Chekhovsky, Vladimir, Litomin, Aliaksandr, Vladimir Makarenko, Darwish, Mohamed Rashad, Wolf, Eddi A., Tahys Janssen, Kello, Tomas, Aleksandra Lelek, Rejeb Sfar, Haifa, Pierre Van Mechelen, Putte, Senne, Nick van Remortel, Emil Sørensen Bols, Hondt, Jorgen D., Moor, Alexandre, Delcourt, Martin, Hesham El Faham, Steven Lowette, Seth Moortgat, Alexander Morton, Denise Müller, Abanti Ranadhir Sahasransu, Stefaan Tavernier, Doninck, Walter, David Vannerom, Beghin, Diego, Bugra Bilin, Barbara Clerbaux, Lentdecker, Gilles, Laurent Favart, Amandeep Kaur Kalsi, Lee, Kyeongpil, Mahdavikhorrami, Mostafa, Inna Makarenko, Santiago Paredes Saenz, Pétré, Laurent, Andrey Popov, Postiau, Nicolas, Elizabeth Rose Starling, Laurent Thomas, Vanden Bemden, Max, Catherine Vander Velde, Pascal Vanlaer, Tom Cornelis, Dobur, Didar, Joscha Knolle, Lambrecht, Luka, Mestdach, Gianny, Marek Niedziela, Rendón, César, Roskas, Christos, Samalan, Amrutha, Kirill Skovpen, Michael Tytgat, Den Bossche, Niels, Vermassen, Basile, Wezenbeek, Liam, Benecke, Anna, Agni Bethani, Bruno, Giacomo, Florian Bury, Claudio Caputo, Pieter David, Christophe Delaere, Izzeddin Suat Donertas, Andrea Giammanco, Jaffel, Khawla, Sandhya Jain, Lemaitre, Vincent, Kuntal Mondal, Prisciandaro, Jessica, Taliercio, Angela, Maksym Teklishyn, Tran, Tu Thong, Pietro Vischia, Sébastien Wertz, Gilvan Alves, Hensel, Carsten, Arthur Moraes, Rebello Teles, P., Walter Luiz Aldá Júnior, Miguel Pereira, Barroso Ferreira Filho, Mapse, Brandao Malbouisson, Helena, Wagner de Paula Carvalho, Chinellato, Jose, Eliza Melo da Costa, Da Silveira, G. G., Dilson De Jesus Damiao, Dos Santos Sousa, Vitor, Fonseca de Souza Sandro, Maria Clemencia Mora Herrera, Mota Amarilo, Kevin, Mundim, L., Nogima, Helio, Santoro, Alberto, Sheila Silva do Amaral, Andre Sznajder, Thiel, Mauricio, Felipe Araujo, Antonio Vilela Pereira, Cesar Augusto Bernardes, Luigi Calligaris, Thiago Rafael Fernandez Perez Tomei, Eduardo de Moraes Gregores, Dener de Souza Lemos, Pedro Galli Mercadante, Sergio Novaes, Padula, Sandra S., Aleksandrov, Aleksandar, Gueorgui Antchev, Hadjiiska, Roumyana, Iaydjiev, Plamen, Misheva, Milena, Rodozov, Mircho, Shopova, Mariana, Sultanov, Georgi, Dimitrov, Anton, Ivanov, Todor, Leandar Litov, Pavlov, Borislav, Petkov, Peicho, Petrov, Anton, Tongguang Cheng, Javaid, Tahir, Mittal, Monika, Wang, Hanwen, Yuan, Li, Muhammad Ahmad, Bauer, Gerry, Candan Dozen, Zhen Hu, Jordan Martins, Wang, Yi, Yi, Kai, Émilien Chapon, Guoming Chen, Hesheng Chen, Mingshui Chen, Iemmi, Fabio, ANSHUL KAPOOR, Leggat, Duncan, Liao, Hongbo, Zhenan Liu, Vukasin Milosevic, fabio monti, Ram Krishna Sharma, Junquan Tao, Thomas-Wilsker, Joshuha, Jin Wang, Huaqiao Zhang, Jingzhou Zhao, Agapitos, Antonis, An, Ying, Ban, Yong, Chen, Cheng, Andrew Levin, Qiang Li, Lyu, Xudong, Mao, Yajun, Qian, Si-Jin, Dayong Wang, Xiao, Jie, Yang, Heng, Lu, Meng, Zhengyun You, Gao, Xuyang, Hideki Okawa, Yu Zhang, Meng Xiao, Carlos Arturo Ávila Bernal, Andres Leonardo Cabrera Mora, Carlos Andrés Flórez, Fraga, Jorge, Mejia Guisao, Jhovanny, Ramirez, Felipe, Jose Ruiz, Giljanovic, Duje, Nikola Godinovic, Damir Lelas, Ivica Puljak, Antunovic, Zeljko, Kovac, Marko, Toni Sculac, Vuko Brigljević, Dinko Ferencek, Devdatta Majumder, Roguljic, Matej, Andrey Starodumov, Tatjana Susa, Alexandros Attikis, Christoforou, Konstantinos, Gouranga Kole, Kolosova, Marina, Konstantinou, Sotiroulla, Jehad.Mousa, Nicolaou, Charalambos, Fotios Ptochos, Razis, Panos A., Rykaczewski, Hans, Halil Saka, Finger, Miroslav, michael finger, Kveton, Antonin, Ayala, Edy, Carrera Jarrin, E., Hassan Abdalla, Salama, Elsayed, Mohammed Attia Mahmoud, yasser mohammed, Sandeep Bhowmik, Ram Krishna Dewanjee, Ehataht, Karl, Kadastik, Mario, Nandan, Saswati, Nielsen, Christine, Pata, Joosep, Martti Raidal, Tani, Laurits, Veelken, Christian, Paula Anna-Maria Eerola, Henning Kirschenmann, Kenneth Mikael Österberg, Mikko Voutilainen, Bharthuar, Shudhashil, Jens Erik Brucken, Francisco Ignacio Garcia Fuentes, Joona Havukainen, Min Suk Kim, Kinnunen, Ritva, Lampén, Tapio, Kati Lassila-Perini, Sami Lehti, Lindén, Tomas, Lotti, Mikko, Martikainen, Laura, Myllymäki, Mikael, Jennifer Ott, Rantanen, Milla-Maarit, Siikonen, Hannu, Eija Maarit Tuominen, Tuominiemi, Jorma, Panja Luukka, Petrow, Henri, Tuuva, Tuure, Chiara Amendola, Besancon, Marc, Fabrice Couderc, Dejardin, Marc, Denegri, Daniel, Faure, Jean-Louis, Federico Ferri, Ganjour, Serguei, Gras, Philippe, Gautier Hamel de Monchenault, Jarry, Patrick, Bruno Lenzi, Malcles, Julie, Rander, John, André Rosowsky, Mehmet Özgür Sahin, Savoy-Navarro, Aurore, Simkina, Polina, Maxim Titov, Geum Bong Yu, Sudha Ahuja, Florian Beaudette, Matteo Bonanomi, Buchot Perraguin, Axel, Busson, Philippe, Cappati, Alessandra, Charlot, Claude, Davignon, Olivier, Diab, Batoul, Guillaume Falmagne, Fontana Santos Alves, Bruno Afonso, Ghosh, Shamik, Raphael Granier de Cassagnac, Hakimi, Alexandre, Inna Kucher, Motta, Jona, Matthew Nguyen, Christophe Ochando, Pascal Paganini, Rembser, Jonas, Roberto Salerno, UTTIYA SARKAR, Jean-Baptiste Sauvan, Yves Sirois, Tarabini, Alessandro, Zabi, Alexandre, Amina Zghiche, Agram, Jean-Laurent, Andrea, Jeremy, Apparu, Dylan, Daniel Bloch, Bourgatte, Guillaume, Brom, Jean-Marie, Chabert, Eric Christian, Caroline Collard, Darej, Douja, Fontaine, Jean-Charles, Goerlach, Ulrich, Grimault, Clément, Le Bihan, Anne-Catherine, Emery Nibigira, Pierre Van Hove, Asilar, Ece, Stephanie Beauceron, Colin Bernet, Boudoul, Gaelle, Camen, Camille, Carle, Aurélien, Nicolas Chanon, Contardo, Didier, Pierre Depasse, El Mamouni, Houmani, Fay, Jean, Susan Gascon-Shotkin, Maxime Gouzevitch, Ille, Bernard, Laktineh, Imad Baptiste, Hugues Lattaud, Antoine Lesauvage, Morgan Lethuillier, Mirabito, Laurent, Perries, Stephane, Shchablo, Konstantin, Viola Sordini, Touquet, Gaël, Vander Donckt, Muriel, Viret, Sébastien, Lomidze, Irakli, Toriashvili, Tengizi, Tsamalaidze, Zviad, Botta, Valeria, Lutz Feld, Klein, Katja, Lipinski, Martin, Meuser, Danilo, Pauls, Alexander, Röwert, Nicolas, Schulz, Johannes, Marius Teroerde, Dodonova, Alena, Eliseev, Dmitry, Martin Erdmann, Peter Fackeldey, Fischer, Benjamin, Thomas Hebbeker, Hoepfner, Kerstin, Ivone, Francesco, Mastrolorenzo, Luca, Markus Merschmeyer, Arnd Meyer, Mocellin, Giovanni, Mondal, Spandan, Swagata Mukherjee, Dennis Noll, Novak, Andrzej, Andrey Pozdnyakov, Rath, Yannik, Reithler, Hans, Alexander Schmidt, Schuler, Simon Christoph, Archana Sharma, Vigilante, Lorenzo, Wiedenbeck, Sebastian, Zaleski, Shawn, Dziwok, Christian, Flügge, Günter, Wael Haj Ahmad, Hlushchenko, Olena, Kress, Thomas, Andreas Nowack, Pooth, Oliver, Dennis Roy, Achim Stahl, Tim Ziemons, Zotz, Alexander, Aarup Petersen, Henriette, Aldaya Martin, Maria, Asmuss, Paul, Baxter, Samuel, Bayatmakou, Maryam, Behnke, Olaf, Bermúdez Martínez, Armando, Bhattacharya, Soham, Afiq Anuar, Freya Blekman, Borras, Kerstin, Brunner, David, Alan Campbell, Andrea Cardini, Cheng, Chun, Colombina, Federica, Sandra Consuegra Rodriguez, Correia Silva, Gilson, Silva, Malinda, Didukh, Leonid, Eckerlin, Guenter, Eckstein, Doris, Luis Ignacio Estevez Banos, Oleg Filatov, Gallo, Elisabetta, Geiser, Achim, Giraldi, Angela, Greau, Guillaume, Alexander Grohsjean, Guthoff, Moritz, Abideh Jafari, Nur Zulaiha Jomhari, Hannes Jung, Ashraf Mohamed, Matthias Kasemann, hessamoddin kaveh, Claus Kleinwort, Roman Kogler, Dirk Krücker, Lange, Wolfgang, Lipka, Katerina, Lohmann, Wolfgang, Mankel, Rainer, Isabell-Alissandra Melzer-Pellmann, Mendizabal Morentin, Mikel, Metwally, Josry, Meyer, Andreas B., Mareike Meyer, Joachim Mnich, Mussgiller, Andreas, Nürnberg, Andreas, Otarid, Younes, Danyer Pérez Adán, Pitzl, Daniel, Raspereza, Alexei, Ribeiro Lopes, Beatriz, Rübenach, Jonas, Alessia Saggio, Andrej Saibel, Mykola Savitskyi, Scham, Moritz, Scheurer, Valerie, Schnake, Simon, Schütze, Paul, Christian Schwanenberger, Shchedrolosiev, Mykyta, Rafael Eduardo Sosa Ricardo, Stafford, Dominic, Nicolas Tonon, Merijn van de Klundert, Federico Vazzoler, Roberval Walsh, Walter, David, Qun Wang, Yiwen Wen, Wichmann, Katarzyna, Wiens, Lucas, Wissing, Christoph, Sebastian Wuchterl, Aggleton, Robin, Steffen Albrecht, Samuel Bein, Lisa Benato, Patrick Connor, Ksenia de Leo, Eich, Melanie, El Morabit, Karim, Feindt, Finn, Fröhlich, Alexander, Christoph Garbers, Erika Garutti, Gunnellini, Paolo, Hajheidari, Mohammadtaghi, Johannes Haller, Andreas Hinzmann, Kasieczka, Gregor, Robert Klanner, Kramer, Tobias, Kutzner, Viktor, Johannes Lange, Torben Lange, Artur Lobanov, Andrea Malara, Matthies, Christopher, ANKITA MEHTA, Louis Moureaux, Nigamova, Aliya, Pena Rodriguez, Karla Josefina, Marcel Rieger, Rieger, Oliver, Schleper, Peter, Matthias Schröder, Joern Schwandt, Jory, Stadie, Hartmut, Steinbrück, Georg, Tews, Alexandra, Irene Zoi, Janek Bechtel, Brommer, Sebastian, Burkart, Maximilian, Erik Butz, Rene Caspart, Chwalek, Thorsten, Boer, Wim, Dierlamm, Alexander, Droll, Alexander, Nils Faltermann, Giffels, Manuel, Gosewisch, Jan-Ole, Gottmann, Artur, Frank Hartmann, Heidecker, Christoph, Ulrich Husemann, Keicher, Philip, Koppenhöfer, Roland, Maier, Stefan, Soureek Mitra, Müller, Thomas, Neukum, Max, Günter Quast, Klaus Rabbertz, Rauser, Johann, Daniel Savoiu, Schnepf, Matthias, Seith, David, Shvetsov, Ivan, Simonis, Hans-Jürgen, Ralf Ulrich, Linden, Jan, Cube, Ralf Florian, Wassmer, Michael, Marc Weber, Wieland, Sebastian, Roger Wolf, Wozniewski, Sebastian, Wunsch, Stefan, Anagnostou, Georgios, Daskalakis, Georgios, Kyriakis, Aristotelis, Loukas, Demetrios, Anna Stakia, Diamantopoulou, Magda, Karasavvas, Dimitrios, Pantelis Kontaxakis, Koraka, Charis Kleio, Manousakis-Katsikakis, Arkadios, Panagiotou, Apostolos, Papavergou, Ioanna, Niki Saoulidou, Konstantinos Theofilatos, Eirini Tziaferi, Vellidis, Konstantinos, Vourliotis, Emmanouil, Bakas, Georgios, Konstantinos Kousouris, Papakrivopoulos, Ioannis, Tsipolitis, Georgios, Zacharopoulou, Anna, Adamidis, Kosmas, Bestintzanos, Ioannis, Ioannis Evangelou, Foudas, Costas, Gianneios, Paraskevas, Katsoulis, Panagiotis, Kokkas, Panagiotis, Manthos, Nikolaos, Ioannis Papadopoulos, John Strologas, Mate Csanad, Farkas, Krisztián, Mahmoud Moussa Abdelkhalek Gadallah, Sandor Lokos, Major, Péter, Koushik Mandal, Gabriella Pásztor, Rádl, Attila József, Surányi, Olivér, Gabor Veres, Márton Bartók, Bencze, Gyorgy, Csaba Hajdu, Dezso Horvath, Ferenc Siklér, Viktor Veszprémi, Czellar, Sandor, Daniele Fasanella, Francesco Fienga, János Karancsi, Molnar, Jozsef, Szillasi, Zoltan, Teyssier, Daniel, Raics, Peter, Zoltan Trocsanyi, Ujvari, 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B., Amandeep Kaur, Ahmed, Asar, Ashutosh Bhardwaj, brajesh choudhary, Gola, Mohit, Sumit Keshri, Ashok Kumar, Md Naimuddin, Priyanka, Ranjan, Kirti, Saumya, Saumya, Aashaq Shah, Bharti, Monika, Bhattacharya, Rajarshi, satyaki bhattacharya, Bhowmik, Debabrata, Dutta, Shubham, Dutta, Suchandra, bhawna gomber, Maity, Manas, Pritam Palit, PRASANT KUMAR ROUT, Saha, Gourab, Bisnupriya Sahu, Sarkar, Subir, Sharan, Manoj, Prafulla Kumar Behera, Behera, Subash Chandra, Pritam Kalbhor, Jyothsna Rani Komaragiri, Kumar, Deepak, Muhammad, Alibordi, Lata Panwar, Pradhan, Raghunath, Pujahari, Prabhat Ranjan, ashish sharma, Sikdar, Anup Kumar, Praveen Chandra Tiwari, Naskar, Kousik, Aziz, Tariq, Dugad, Shashikant, Kumar, Mintu, Mohanty, Gagan B., sudeshna banerjee, Chudasama, Ruchi, Guchait, Monoranjan, Karmakar, Saikat, Kumar, Sanjeev, Majumder, Gobinda, Mazumdar, Kajari, Soumya Mukherjee, Alpana, Alpana, Sourabh Dube, Kansal, Bhumika, Laha, Arnab, Shubham Pandey, Angira Rastogi, Seema Sharma, 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10. The MKID Exoplanet Camera for Subaru SCExAO

Author

Noah Swimmer, Sarah Steiger, Thayne Currie, Miguel Daal, Neelay Fruitwala, Kristina K. Davis, Nemanja Jovanovic, Nicholas Zobrist, Bruce Bumble, Isabel Lipartito, Paul Szypryt, John I. Bailey, Clint Bockstiegel, Sébastien Vievard, Rupert Dodkins, Gregoire Coiffard, Benjamin A. Mazin, Seth R. Meeker, Frantz Martinache, Giulia Collura, Olivier Guyon, Alexander B. Walter, Julien Lozi, Jennifer Pearl Smith, and Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France

Subjects
Physics, 010504 meteorology & atmospheric sciences, business.industry, FOS: Physical sciences, Astronomy and Astrophysics, Wavefront sensor, 01 natural sciences, Noise (electronics), Exoplanet, Speckle pattern, Cardinal point, Optics, Integral field spectrograph, [SDU]Sciences of the Universe [physics], Space and Planetary Science, 0103 physical sciences, 14. Life underwater, Astrophysics - Instrumentation and Methods for Astrophysics, business, Subaru Telescope, Adaptive optics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences
Abstract

We present the MKID Exoplanet Camera (MEC), a z through J band (800 - 1400 nm) integral field spectrograph located behind The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) at the Subaru Telescope on Maunakea that utilizes Microwave Kinetic Inductance Detectors (MKIDs) as the enabling technology for high contrast imaging. MEC is the first permanently deployed near-infrared MKID instrument and is designed to operate both as an IFU, and as a focal plane wavefront sensor in a multi-kHz feedback loop with SCExAO. The read noise free, fast time domain information attainable by MKIDs allows for the direct probing of fast speckle fluctuations that currently limit the performance of most high contrast imaging systems on the ground and will help MEC achieve its ultimate goal of reaching contrasts of $10^{-7}$ at 2$\lambda / D$. Here we outline the instrument details of MEC including the hardware, firmware, and data reduction and analysis pipeline. We then discuss MEC's current on-sky performance and end with future upgrades and plans., Comment: To be published in Publications of the Astronomical Society of the Pacific

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