المؤلفون: Cecil, T., Albert, C., Anderson, A. J., Barry, P. S., Benson, B., Cotter, C., Chang, C., Dobbs, M., Dibert, K., Gualtieri, R., Karkare, K. S., Lisovenko, M., Marrone, D. P., Montgomery, J., Pan, Z., Robson, G., Rouble, M., Shirokoff, E., Smecher, G., Wang, G., Yefremenko, V.

المصدر: IEEE Transactions on Applied Superconductivity; August 2023, Vol. 33 Issue: 5 p1-6, 6p

مستخلص: Line Intensity Mapping (LIM) is a new observational technique that uses low-resolution observations of line emission to efficiently trace the large-scale structure of the Universe out to high redshift. Common mm/sub-mm emission lines are accessible from ground-based observatories, and the requirements on the detectors for LIM at mm-wavelengths are well matched to the capabilities of large-format arrays of superconducting sensors. We describe the development of an $ R$ = $\lambda / \Delta \lambda = 300$ on-chip superconducting filter-bank spectrometer covering the 120–180 GHz band for future mm-LIM experiments, focusing on SPT-SLIM, a pathfinder LIM instrument for the South Pole Telescope. Radiation is coupled from the telescope optical system to the spectrometer chip via an array of feedhorn-coupled orthomode transducers. Superconducting microstrip transmission lines then carry the signal to an array of channelizing half-wavelength resonators, and the output of each spectral channel is sensed by a lumped element kinetic inductance detector (leKID). Key areas of development include incorporating new low-loss dielectrics to improve both the achievable spectral resolution and optical efficiency and development of a robust fabrication process to create a galvanic connection between ultra-pure superconducting thin-films to realize multi-material (hybrid) leKIDs. We provide an overview of the spectrometer design, fabrication process, and prototype devices.

المؤلفون: Zmuidzinas, Jonas, Gao, Jian-Rong, Montgomery, J., Anderson, A. J., Avva, J. S., Bender, A. N., Dobbs, M. A., Dutcher, D., Elleflot, T., Foster, A., Groh, J. C., Holzapfel, W. L., Howe, D., Huang, N., Lowitz, A. E., Noble, G. I., Pan, Z., Rahlin, A., Riebel, D., Smecher, G., Suzuki, A., Whitehorn, N.

المصدر: Proceedings of SPIE; December 2020, Vol. 11453 Issue: 1 p114530X-114530X-22, 11338493p

المؤلفون: Lystrup, Makenzie, Perrin, Marshall D., Hazumi, M., Ade, P.A.R., Adler, A., Allys, E., Arnold, K., Auguste, D., Aumont, J., Aurlien, R., Austermann, J., Baccigalupi, C., Banday, A. J., Banjeri, R., Barreiro, R. B., Basak, S., Beall, J., Beck, D., Beckman, S., Bermejo, J., de Bernardis, P., Bersanelli, M., Bonis, J., Borrill, J., Boulanger, F., Bounissou, S., Brilenkov, M., Brown, M., Bucher, M., Calabrese, E., Campeti, P., Carones, A., Casas, F. J., Challinor, A., Chan, V., Cheung, K., Chinone, Y., Cliche, J. F., Colombo, L., Columbro, F., Cubas, J., Cukierman, A., Curtis, D., D'Alessandro, G., Dachlythra, N., De Petris, M., Dickinson, C., Diego-Palazuelos, P., Dobbs, M., Dotani, T., Duband, L., Duff, S., Duval, J. M., Ebisawa, K., Elleflot, T., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Finelli, F., Flauger, R., Franceschet, C., Fuskeland, U., Galloway, M., Ganga, K., Gao, J. R., Genova-Santos, R., Gerbino, M., Gervasi, M., Ghigna, T., Gjerløw, E., Gradziel, M. L., Grain, J., Grupp, F., Gruppuso, A., Gudmundsson, J. E., de Haan, T., Halverson, N. W., Hargrave, P., Hasebe, T., Hasegawa, M., Hattori, M., Henrot-Versillé, S., Herman, D., Herranz, D., Hill, C. A., Hilton, G., Hirota, Y., Hivon, E., Hlozek, R. A., Hoshino, Y., de la Hoz, E., Hubmayr, J., Ichiki, K., Iida, T., Imada, H., Ishimura, K., Ishino, H., Jaehnig, G., Kaga, T., Kashima, S., Katayama, N., Kato, A., Kawasaki, T., Keskitalo, R., Kisner, T., Kobayashi, Y., Kogiso, N., Kogut, A., Kohri, K., Komatsu, E., Komatsu, K., Konishi, K., Krachmalnicoff, N., Kreykenbohm, I., Kuo, C. L., Kushino, A., Lamagna, L., Lanen, J. V., Lattanzi, M., Lee, A. T., Leloup, C., Levrier, F., Linder, E., Louis, T., Luzzi, G., Maciaszek, T., Maffei, B., Maino, D., Maki, M., Mandelli, S., Martinez-Gonzalez, E., Masi, S., Matsumura, T., Mennella, A., Migliaccio, M., Minami, Y., Mitsuda, K., Montgomery, J., Montier, L., Morgante, G., Mot, B., Murata, Y., Murphy, J. A., Nagai, M., Nagano, Y., Nagasaki, T., Nagata, R., Nakamura, S., Namikawa, T., Natoli, P., Nerval, S., Nishibori, T., Nishino, H., Noviello, F., O'Sullivan, C., Ogawa, H., Ogawa, H., Oguri, S., Ohsaki, H., Ohta, I. S., Okada, N., Okada, N., Pagano, L., Paiella, A., Paoletti, D., Patanchon, G., Peloton, J., Piacentini, F., Pisano, G., Polenta, G., Poletti, D., Prouvé, T., Puglisi, G., Rambaud, D., Raum, C., Realini, S., Reinecke, M., Remazeilles, M., Ritacco, A., Roudil, G., Rubino-Martin, J. A., Russell, M., Sakurai, H., Sakurai, Y., Sandri, M., Sasaki, M., Savini, G., Scott, D., Seibert, J., Sekimoto, Y., Sherwin, B., Shinozaki, K., Shiraishi, M., Shirron, P., Signorelli, G., Smecher, G., Stever, S., Stompor, R., Sugai, H., Sugiyama, S., Suzuki, A., Suzuki, J., Svalheim, T. L., Switzer, E., Takaku, R., Takakura, H., Takakura, S., Takase, Y., Takeda, Y., Tartari, A., Taylor, E., Terao, Y., Thommesen, H., Thompson, K. L., Thorne, B., Toda, T., Tomasi, M., Tominaga, M., Trappe, N., Tristram, M., Tsuji, M., Tsujimoto, M., Tucker, C., Ullom, J., Vermeulen, G., Vielva, P., Villa, F., Vissers, M., Vittorio, N., Wehus, I., Weller, J., Westbrook, B., Wilms, J., Winter, B., Wollack, E. J., Yamasaki, N. Y., Yoshida, T., Yumoto, J., Zannoni, M., Zonca, A.

المصدر: Proceedings of SPIE; December 2020, Vol. 11443 Issue: 1 p114432F-114432F-20, 11328789p

المؤلفون: Lystrup, Makenzie, Perrin, Marshall D., Montier, L., Mot, B., de Bernardis, P., Maffei, B., Pisano, G., Columbro, F., Gudmundsson, J. E., Henrot-Versillé, S., Lamagna, L., Montgomery, J., Prouvé, T., Russell, M., Savini, G., Stever, S., Thompson, K. L., Tsujimoto, M., Tucker, C., Westbrook, B., Ade, P. A. R., Adler, A., Allys, E., Arnold, K., Auguste, D., Aumont, J., Aurlien, R., Austermann, J., Baccigalupi, C., Banday, A. J., Banerji, R., Barreiro, R. B., Basak, S., Beall, J., Beck, D., Beckman, S., Bermejo, J., Bersanelli, M., Bonis, J., Borrill, J., Boulanger, F., Bounissou, S., Brilenkov, M., Brown, M., Bucher, M., Calabrese, E., Campeti, P., Carones, A., Casas, F. J., Challinor, A., Chan, V., Cheung, K., Chinone, Y., Cliche, J. F., Colombo, L., Cubas, J., Cukierman, A., Curtis, D., D'Alessandro, G., Dachlythra, N., De Petris, M., Dickinson, C., Diego-Palazuelos, P., Dobbs, M., Dotani, T., Duband, L., Duff, S., Duval, J. M., Ebisawa, K., Elleflot, T., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Finelli, F., Flauger, R., Franceschet, C., Fuskeland, U., Galloway, M., Ganga, K., Gao, J. R., Genova-Santos, R., Gerbino, M., Gervasi, M., Ghigna, T., Gjerløw, E., Gradziel, M. L., Grain, J., Grupp, F., Gruppuso, A., de Haan, T., Halverson, N. W., Hargrave, P., Hasebe, T., Hasegawa, M., Hattori, M., Hazumi, M., Herman, D., Herranz, D., Hill, C. A., Hilton, G., Hirota, Y., Hivon, E., Hlozek, R. A., Hoshino, Y., de la Hoz, E., Hubmayr, J., Ichiki, K., Iida, T., Imada, H., Ishimura, K., Ishino, H., Jaehnig, G., Kaga, T., Kashima, S., Katayama, N., Kato, A., Kawasaki, T., Keskitalo, R., Kisner, T., Kobayashi, Y., Kogiso, N., Kogut, A., Kohri, K., Komatsu, E., Komatsu, K., Konishi, K., Krachmalnicoff, N., Kreykenbohm, I., Kuo, C. L., Kushino, A., Lanen, J. V., Lattanzi, M., Lee, A. T., Leloup, C., Levrier, F., Linder, E., Louis, T., Luzzi, G., Maciaszek, T., Maino, D., Maki, M., Mandelli, S., Martinez-Gonzalez, E., Masi, S., Matsumura, T., Mennella, A., Migliaccio, M., Minami, Y., Mitsuda, K., Morgante, G., Murata, Y., Murphy, J. A., Nagai, M., Nagano, Y., Nagasaki, T., Nagata, R., Nakamura, S., Namikawa, T., Natoli, P., Nerval, S., Nishibori, T., Nishino, H., O'Sullivan, C., Ogawa, H., Ogawa, H., Oguri, S., Ohsaki, H., Ohta, I. S., Okada, N., Okada, N., Pagano, L., Paiella, A., Paoletti, D., Patanchon, G., Peloton, J., Piacentini, F., Polenta, G., Poletti, D., Puglisi, G., Rambaud, D., Raum, C., Realini, S., Reinecke, M., Remazeilles, M., Ritacco, A., Roudil, G., Rubino-Martin, J. A., Sakurai, H., Sakurai, Y., Sandri, M., Sasaki, M., Scott, D., Seibert, J., Sekimoto, Y., Sherwin, B., Shinozaki, K., Shiraishi, M., Shirron, P., Signorelli, G., Smecher, G., Stompor, R., Sugai, H., Sugiyama, S., Suzuki, A., Suzuki, J., Svalheim, T. L., Switzer, E., Takaku, R., Takakura, H., Takakura, S., Takase, Y., Takeda, Y., Tartari, A., Taylor, E., Terao, Y., Thommesen, H., Thorne, B., Toda, T., Tomasi, M., Tominaga, M., Trappe, N., Tristram, M., Tsuji, M., Ullom, J., Vermeulen, G., Vielva, P., Villa, F., Vissers, M., Vittorio, N., Wehus, I., Weller, J., Wilms, J., Winter, B., Wollack, E. J., Yamasaki, N. Y., Yoshida, T., Yumoto, J., Zannoni, M., Zonca, A.

المصدر: Proceedings of SPIE; December 2020, Vol. 11443 Issue: 1 p114432G-114432G-21, 11328790p

المؤلفون: Marcote, B., Nimmo, K., Hessels, J. W. T., Tendulkar, S. P., Bassa, C. G., Paragi, Z., Keimpema, A., Bhardwaj, M., Karuppusamy, R., Kaspi, V. M., Law, C. J., Michilli, D., Aggarwal, K., Andersen, B., Archibald, A. M., Bandura, K., Bower, G. C., Boyle, P. J., Brar, C., Burke-Spolaor, S., Butler, B. J., Cassanelli, T., Chawla, P., Demorest, P., Dobbs, M., Fonseca, E., Giri, U., Good, D. C., Gourdji, K., Josephy, A., Kirichenko, A. Yu., Kirsten, F., Landecker, T. L., Lang, D., Lazio, T. J. W., Li, D. Z., Lin, H.-H., Linford, J. D., Masui, K., Mena-Parra, J., Naidu, A., Ng, C., Patel, C., Pen, U.-L., Pleunis, Z., Rafiei-Ravandi, M., Rahman, M., Renard, A., Scholz, P., Siegel, S. R., Smith, K. M., Stairs, I. H., Vanderlinde, K., Zwaniga, A. V.

المصدر: Nature; January 2020, Vol. 577 Issue: 7789 p190-194, 5p

مستخلص: Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes1,2. Their physical origin remains unknown, but dozens of possible models have been postulated3. Some FRB sources exhibit repeat bursts4–7. Although over a hundred FRB sources have been discovered8, only four have been localized and associated with a host galaxy9–12, and just one of these four is known to emit repeating FRBs9. The properties of the host galaxies, and the local environments of FRBs, could provide important clues about their physical origins. The first known repeating FRB, however, was localized to a low-metallicity, irregular dwarf galaxy, and the apparently non-repeating sources were localized to higher-metallicity, massive elliptical or star-forming galaxies, suggesting that perhaps the repeating and apparently non-repeating sources could have distinct physical origins. Here we report the precise localization of a second repeating FRB source6, FRB 180916.J0158+65, to a star-forming region in a nearby (redshift 0.0337 ± 0.0002) massive spiral galaxy, whose properties and proximity distinguish it from all known hosts. The lack of both a comparably luminous persistent radio counterpart and a high Faraday rotation measure6further distinguish the local environment of FRB 180916.J0158+65 from that of the single previously localized repeating FRB source, FRB 121102. This suggests that repeating FRBs may have a wide range of luminosities, and originate from diverse host galaxies and local environments.

المؤلفون: Zmuidzinas, Jonas, Gao, Jian-Rong, Dutcher, D., Ade, P. A. R., Ahmed, Z., Anderson, A. J., Avva, J. S., Thakur, R. Basu, Bender, A. N., Benson, B. A., Carlstrom, J. E., Carter, F. W., Cecil, T. W., Chang, C. L., Cliche, J. F., Cukierman, A., de Haan, T., Ding, J., Dobbs, M. A., Everett, W., Foster, A., Gallicchio, J., Gilbert, A., Groh, J. C., Harke-Hosemann, A. H., Guns, S. T., Halverson, N. W., Harrington, N. L., Henning, J. W., Holzapfel, W. L., Huang, N., Irwin, K. D., Jeong, O. B., Jonas, M., Khaire, T. S., Kofman, A. M., Korman, M., Kubik, D. L., Kuhlmann, S., Kuo, C.-L., Lowitz, A. E., Lee, A. T., Meyer, S. S., Michalik, D., Montgomery, J., Nadolski, A., Natoli, T., Nguyen, H., Noble, G. I., Novosad, V., Padin, S., Pan, Z., Pearson, J., Posada, C. M., Quan, W., Rahlin, A., Ruhl, J. E., Sayre, J. T., Shirokoff, E., Smecher, G., Sobrin, J. A., Stark, A. A., Story, K. T., Suzuki, A., Thompson, K. L., Tucker, C., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Yefremenko, V., Yoon, K. W., Young, M. R.

المصدر: Proceedings of SPIE; July 2018, Vol. 10708 Issue: 1 p107081Z-107081Z-13, 10601033p

المؤلفون: Lystrup, Makenzie, MacEwen, Howard A., Fazio, Giovanni G., Batalha, Natalie, Siegler, Nicholas, Tong, Edward C., Sekimoto, Y., Ade, P., Arnold, K., Aumont, J., Austermann, J., Baccigalupi, C., Banday, A., Banerji, R., Basak, S., Beckman, S., Bersanelli, M., Borrill, J., Boulanger, F., Brown, M. L., Bucher, M., Calabrese, E., Challinor, A., Chinone, Y., Columbro, F., Cukierman, A., Curtis, D., de Bernardis, P., de Petris, M., Dobbs, M., Dotani, T., Duband, L., Ducout, A., Ebisawa, K., Elleflot, T., Eriksen, H., Errard, J., Flauger, R., Franceschet, C., Fuskeland, U., Ganga, K., Gao, J.R., Ghigna, T., Grain, J., Gruppuso, A., Halverson, N., Hargrave, P., Hasebe, T., Hasegawa, M., Hattori, M., Hazumi, M., Henrot-Versille, S., Hill, C., Hirota, Y., Hivon, E., Hoang, D. T., Hubmayr, J., Ichiki, K., Imada, H., Ishino, H., Jaehnig, G., Kanai, H., Kashima, S., Kataoka, Y., Katayama, N., Kawasaki, T., Keskitalo, R., Kibayashi, A., Kikuchi, T., Kimura, K., Kisner, T., Kobayashi, Y., Kogiso, N., Kohri, K., Komatsu, E., Komatsu, K., Konishi, K., Krachmalnicoff, N., Kuo, C. L., Kurinsky, N., Kushino, A., Lamagna, L., Lee, A. T., Linder, E., Maffei, B., Maki, M., Mangilli, A., Martinez-Gonzalez, E., Masi, S., Matsumura, T., Mennella, A., Minami, Y., Mistuda, K., Molinari, D., Montier, L., Morgante, G., Mot, B., Murata, Y., Murphy, A., Nagai, M., Nagata, R., Nakamura, S., Namikawa, T., Natoli, P., Nishibori, T., Nishino, H., Noviello, F., O'Sullivan, C., Ochi, H., Ogawa, H., Ogawa, H., Ohsaki, H., Ohta, I., Okada, N., Patanchon, G., Piacentini, F., Pisano, G., Polenta, G., Poletti, D., Puglisi, G., Raum, C., Realini, S., Remazeilles, M., Sakurai, H., Sakurai, Y., Savini, G., Sherwin, B., Shinozaki, K., Shiraishi, M., Signorelli, G., Smecher, G., Stompor, R., Sugai, H., Sugiyama, S., Suzuki, A., Suzuki, J., Takaku, R., Takakura, H., Takakura, S., Taylor, E., Terao, Y., Thompson, K. L., Thorne, B., Tomasi, M., Tomida, H., Trappe, N., Tristram, M., Tsuji, M., Tsujimoto, M., Uozumi, S., Utsunomiya, S., Vittorio, N., Watanabe, N., Wehus, I., Westbrook, B., Winter, B., Yamamoto, R., Yamasaki, N. Y., Yanagisawa, M., Yoshida, T., Yumoto, J., Zannoni, M., Zonca, A.

المصدر: Proceedings of SPIE; July 2018, Vol. 10698 Issue: 1 p106981Y-106981Y-17, 10591137p

المؤلفون: Zmuidzinas, Jonas, Gao, Jian-Rong, Rouble, M., Smecher, G., Anderson, A., Barry, P. S., Dibert, K., Dobbs, M., Karkare, K. S., Montgomery, J.

المصدر: Proceedings of SPIE; August 2022, Vol. 12190 Issue: 1 p1219024-1219024-14

المؤلفون: Zmuidzinas, Jonas, Gao, Jian-Rong, Anderson, A. J., Barry, P., Bender, A. N., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Cecil, T. W., Chang, C. L., Crawford, T. M., Dibert, K. R., Dobbs, M. A., Fichman, K., Halverson, N. W., Holzapfel, W. L., Hryciuk, A., Karkare, K. S., Li, J., Lisovenko, M., Marrone, D., McMahon, J., Montgomery, J., Natoli, T., Pan, Z., Raghunathan, S., Reichardt, C. L., Rouble, M., Shirokoff, E., Smecher, G., Stark, A. A., Vieira, J. D., Young, M. R.

المصدر: Proceedings of SPIE; August 2022, Vol. 12190 Issue: 1 p1219003-1219003-26

المؤلفون: Nord, M., Basu, K., Pacaud, F., Ade, P. A. R., Bender, A. N., Benson, B. A., Bertoldi, F., Cho, H.-M., Chon, G., Clarke, J., Dobbs, M., Ferrusca, D., Halverson, N. W., Holzapfel, W. L., Horellou, C., Johansson, D., Kennedy, J., Kermish, Z., Kneissl, R., Lanting, T., Lee, A. T., Lueker, M., Mehl, J., Menten, K. M., Plagge, T., Reichardt, C. L., Richards, P. L., Schaaf, R., Schwan, D., Spieler, H., Tucker, C., Weiss, A., Zahn, O., Nord, M., Basu, K., Pacaud, F., Ade, P. A. R., Bender, A. N., Benson, B. A., Bertoldi, F., Cho, H.-M., Chon, G., Clarke, J., Dobbs, M., Ferrusca, D., Halverson, N. W., Holzapfel, W. L., Horellou, C., Johansson, D., Kennedy, J., Kermish, Z., Kneissl, R., Lanting, T., Lee, A. T., Lueker, M., Mehl, J., Menten, K. M., Plagge, T., Reichardt, C. L., Richards, P. L., Schaaf, R., Schwan, D., Spieler, H., Tucker, C., Weiss, A., Zahn, O.

المصدر: Astronomy and Astrophysics; November 2009, Vol. 506 Issue: 2 p623-636, 14p

مستخلص: Context. Observations of the Sunyaev-Zel'dovich effect (SZE) from galaxy clusters are emerging as a powerful tool in cosmology. Besides large cluster surveys, resolved SZE images of individual clusters can shed light on the physics of the intra-cluster medium (ICM) and allow accurate measurements of the cluster gas and total masses.