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39,559 results on '"Koopman"'

201. A Comparison of a Postal Survey and Mixed-Mode Survey Using a Questionnaire on Patients’ Experiences With Breast Care

Author

Zuidgeest, Marloes, Hendriks, Michelle, Koopman, Laura, Spreeuwenberg, Peter, and Rademakers, Jany

Subjects
Computer applications to medicine. Medical informatics, R858-859.7, Public aspects of medicine, RA1-1270
Abstract

BackgroundThe Internet is increasingly considered to be an efficient medium for assessing the quality of health care seen from the patients’ perspective. Potential benefits of Internet surveys such as time efficiency, reduced effort, and lower costs should be balanced against potential weaknesses such as low response rates and accessibility for only a subset of potential participants. Combining an Internet questionnaire with a traditional paper follow-up questionnaire (mixed-mode survey) can possibly compensate for these weaknesses and provide an alternative to a postal survey. ObjectiveTo examine whether there are differences between a mixed-mode survey and a postal survey in terms of respondent characteristics, response rate and time, quality of data, costs, and global ratings of health care or health care providers (general practitioner, hospital care in the diagnostic phase, surgeon, nurses, radiotherapy, chemotherapy, and hospital care in general). MethodsDifferences between the two surveys were examined in a sample of breast care patients using the Consumer Quality Index Breast Care questionnaire. We selected 800 breast care patients from the reimbursement files of Dutch health insurance companies. We asked 400 patients to fill out the questionnaire online followed by a paper reminder (mixed-mode survey) and 400 patients, matched by age and gender, received the questionnaire by mail only (postal survey). Both groups received three reminders. ResultsThe respondents to the two surveys did not differ in age, gender, level of education, or self-reported physical and psychological health (all Ps > .05). In the postal survey, the questionnaires were returned 20 days earlier than in the mixed-mode survey (median 12 and 32 days, respectively; P < .001), whereas the response rate did not differ significantly (256/400, 64.0% versus 242/400, 60.5%, respectively; P = .30). The costs were lower for the mixed-mode survey (€2 per questionnaire). Moreover, there were fewer missing items (3.4% versus 4.4%, P = .002) and fewer invalid answers (3.2% versus 6.2%, P < .001) in the mixed-mode survey than in the postal survey. The answers of the two respondent groups on the global ratings did not differ. Within the mixed-mode survey, 52.9% (128/242) of the respondents filled out the questionnaire online. Respondents who filled out the questionnaire online were significantly younger (P < .001), were more often highly educated (P = .002), and reported better psychological health (P = .02) than respondents who filled out the paper questionnaire. Respondents to the paper questionnaire rated the nurses significantly more positively than respondents to the online questionnaire (score 9.2 versus 8.4, respectively; χ21 = 5.6). ConclusionsMixed-mode surveys are an alternative method to postal surveys that yield comparable response rates and groups of respondents, at lower costs. Moreover, quality of health care was not rated differently by respondents to the mixed-mode or postal survey. Researchers should consider using mixed-mode surveys instead of postal surveys, especially when investigating younger or more highly educated populations.

Published
2011
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202. Etanercept in juvenile idiopathic arthritis: Who will benefit?

Author

van den Berg JM, Swart JF, Dolman KM, Gorter SL, Koopman-Keemink Y, Twilt M, Hoppenreijs EPAH, ten Cate R, Armbrust W, Prince FHM, Otten MH, Wulffraat NM, van Rossum MAJ, and van Suijlekom-Smit LWA

Subjects
Pediatrics, RJ1-570, Diseases of the musculoskeletal system, RC925-935
Published
2011
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203. The Validity and Responsiveness of the Patient-Specific Functional Scale in Patients With First Carpometacarpal Osteoarthritis

Author

van der Avoort, Dirk-Johannes Jacobus Cornelis, Bijlsma, Ward Rogier, Michiel Blomme, Richard Arjen, de Boer, Herman Luitzen, van Couwelaar, Gijs Marijn, Debeij, Jan, Dekker, Jak, Feitz, Reinier, Fink, Alexandra, Harmsen, Kennard, Hoogendam, Lisa, Hovius, Steven Eric Ruden, van Huis, Rob, Koch, Richard, van Kooij, Yara Eline, Koopman, Jaimy Emerentiana, Kroeze, Alexander, Loos, Nina Louisa, Moojen, Thybout Matthias, van der Oest, Mark Johannes Willem, Pennehouat, Pierre-Yves Alain Adriaan, de Ridder, Willemijn Anna, de Schipper, Johannes Pieter, Schoneveld, Karin, Selles, Ruud Willem, Slijper, Harm Pieter, Smit, Jeronimus Maria, Smit, Xander, Souer, John Sebastiaan, ter Stege, Marloes Hendrina Paulina, Temming, Johannes Frederikes Maria, Teunissen, Joris Sebastiaan, van Uchelen, Jeroen Hein, Veltkamp, Joris Jan, Vermeulen, Guus Maarten, Walbeehm, Erik Taco, Wouters, Robbert Maarten, Zöphel, Oliver Theodor, Zuidam, Jelle Michiel, van Kooij, Yara E., ter Stege, Marloes H.P., de Ridder, Willemijn A., Hovius, Steven E.R., MacDermid, Joy C., Selles, Ruud W., and Wouters, Robbert M.

Published
2024
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204. Dietary and lifestyle inflammation scores in relation to colorectal cancer recurrence and all-cause mortality: A longitudinal analysis

Author

van Halteren, Henk K., Dekker, Jan Willem T., Sommeijer, Dirkje W., Sonneveld, Dirk J.A., Terheggen, Frederiek, Sie, Mark P.S., Wesselink, Evertine, Boshuizen, Hendriek C., van Lanen, Anne-Sophie, Kok, Dieuwertje E., Derksen, Jeroen W.G., Smit, Karel C., de Wilt, Johannes H.W., Koopman, Miriam, May, Anne M., Kampman, Ellen, and van Duijnhoven, Fränzel J.B.

Published
2024
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207. Upfront resection versus no resection of the primary tumor in patients with synchronous metastatic colorectal cancer: the randomized phase III CAIRO4 study conducted by the Dutch Colorectal Cancer Group and the Danish Colorectal Cancer Group

Author

Vincent, Jeroen, Wegdam, Johannes A., Haberkorn, Brigitte C.M., van der Harst, Erwin, Hendriks, Mathijs P., Schreurs, W.H. Hermien, Cense, Huib A., Rietbroek, Ron C., de Gier, Marie-José, van Breugel, Edwin A., de Vos, Aad I., Brosens, Rebecca P.M., Doornebosch, P.G., de Jongh, Felix E., Vles, Wouter J., den Boer, Marien O., Leijtens, Jeroen W.A., Gelderblom, A.J. Hans, Peeters, Koen C.M.J., Kuenen, Bart C., Pultrum, Bareld B., van Dodewaard-de Jong, Joyce M., Consten, Esther C.J., van de Wouw, A.J. Yes, Konsten, J.L.M., Hoekstra, R., Lutke Holzik, Martijn F., Vos, Allert H., van Hoogstraten, M.J., Schlesinger, Nis H., Creemers, Geert-Jan, de Hingh, Ignace H.J.T., Kjær, Monica L., Petersen, Lone N., Seiersen, Michael, Altaf, Rahim, van Cruijsen, Hester, Hess, Daniël A., van Leeuwen-Snoeks, Lobke L., Pronk, Apollo, Baeten, Coen I.M., van der Deure, Wendy M., Bosscha, Koop, Schut, Heidi, Leclercq, W.K.G., Simkens, L.H.J., Reijnders, Koen, van Arkel, Kees, van Grevenstein, W.M.U. Helma, van de Ven, Anthony W.H., Vuylsteke, Ronald J.C.L.M., Kuijer, Philomeen, Bakker, Sandra D., Goei, Hauwy, Helgason, Helgi H., van Acker, Gijs J.D., Temizkan, Mehmet, van Tilburg, Marc W.A., Gerhards, Michael F., Kerver, E.D., Gootjes, Elske, Nieboer, Peter, Bleeker, Wim A., Bleeker, G.R., van der Kruijssen, D.E.W., Elias, S.G., van de Ven, P.M., van Rooijen, K.L., Lam-Boer, J.’t, Mol, L., Punt, C.J.A., Sommeijer, D.W., Tanis, P.J., Nielsen, J.D., Yilmaz, M.K., van Riel, J.M.G.H., Wasowiz-Kemps, D.K., Loosveld, O.J.L., van der Schelling, G.P., de Groot, J.W.B., van Westreenen, H.L., Jakobsen, H.L., Fromm, A.L., Hamberg, P., Verseveld, M., Jaensch, C., Liposits, G.I., van Duijvendijk, P., Oulad Hadj, J., van der Hoeven, J.A.B., Trajkovic, M., de Wilt, J.H.W., and Koopman, M.

Published
2024
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210. Prognostic value of liver metastases in colorectal cancer treated by systemic therapy: An ARCAD pooled analysis

Author

Cohen, Romain, Raeisi, Morteza, Chibaudel, Benoist, Shi, Qian, Yoshino, Takayuki, Zalcberg, John R., Adams, Richard, Cremolini, Chiara, Van Cutsem, Eric, Heinemann, Volker, Tabernero, Josep, Punt, Cornelis J.A., Arnold, Dirk, Hurwitz, Herbert I., Douillard, Jean-Yves, Venook, Alan P., Saltz, Leonard B., Maughan, Timothy S., Kabbinavar, Fairooz, Bokemeyer, Carsten, Grothey, Axel, Mayer, Robert J., Kaplan, Richard, Tebbutt, Niall C., Randolph Hecht, J., Giantonio, Bruce J., Díaz-Rubio, Eduardo, Sobrero, Alberto F., Peeters, Marc, Koopman, Miriam, Goldberg, Richard M., Andre, Thierry, and de Gramont, Aimery

Published
2024
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212. Safety and Effectiveness of Pulsed Field Ablation for Atrial Fibrillation in Patients With Heart Failure

Author

Turagam, Mohit K., Neuzil, Petr, Schmidt, Boris, Reichlin, Tobias, Neven, Kars, Metzner, Andreas, Hansen, Jim, Blaauw, Yuri, Maury, Philippe, Arentz, Thomas, Sommer, Philipp, Anic, Ante, Anselme, Frederic, Boveda, Serge, Deneke, Tom, Willems, Stephan, van der Voort, Pepijn, Tilz, Roland, Funasako, Moritoshi, Scherr, Daniel, Wakili, Reza, Steven, Daniel, Kautzner, Josef, Vijgen, Johan, Jais, Pierre, Petru, Jan, Chun, Julian, Roten, Laurent, Füting, Anna, Lemoine, Marc D., Ruwald, Martin, Mulder, Bart A., Rollin, Anne, Lehrmann, Heiko, Fink, Thomas, Jurisic, Zrinka, Chaumont, Corentin, Adelino, Raquel, Nentwich, Karin, Gunawardene, Melanie, Ouss, Alexandre, Heeger, Christian-Hendrik, Manninger, Martin, Bohnen, Jan-Eric, Sultan, Arian, Peichl, Petr, Koopman, Pieter, Derval, Nicolas, Kueffer, Thomas, Reinsch, Nico, and Reddy, Vivek Y.

Published
2024
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214. Transcriptional and functional profiling identifies inflammation and endothelial-to-mesenchymal transition as potential drivers for phenotypic heterogeneity within a cohort of endothelial colony forming cells

Author

Brands, Martijn, Koopman, Sjoerd, Bukkems, Laura, Cloesmeijer, Michael, Janssen, Alexander, Fijnvandraat, Karin, Gouw, Samantha, Mathôt, Ron, Haverman, Lotte, van den Akker, Emile, van den Biggelaar, Maartje, de Haas, Masja, Meijer, Sander, Voorberg, Jan, Del Castillo Alferez, Jessica, Zhang, Huan, Boender, Johan, Meijer, Stephan, Meijer, Karina, de Jong, Sean, Goedhart, Geertje, van der Bom, Anske, Bos, Mettine, Eikenboom, Jeroen, van der Meer, Felix, Laan, Sebastiaan, Schols, Saskia, Bierings, Ruben, Burdorf, Lex, Cnossen, Marjon, Hazelzet, Jan, Huisman, Elise, Kruip, Marieke, Leebeek, Frank, van Leeuwen, Nikki, Lingsma, Hester, de Maat, Moniek, van Moort, Iris, Polinder, Suzanne, Reitsma, Simone, Roest, Eliza, Arisz, Ryanne, Romano, Lorenzo, Al Arashi, Wala, van Hoorn, Shannon, Goedhart, Tine, Mussert, Caroline, Prameyllawati, Diaz, Uyl, Carin, Jansen, Nathalie, Fischer, Kathelijn, Ploos van Amstel, Hans Kristian, Urbanus, Rolf, Zivkovic, Minka, Bredenoord, Annelien, van der Graaf, Rieke, Baas, Lieke, Schutgens, Roger, Driessens, Mariëtte, Laan, Sebastiaan N.J., de Boer, Suzan, Dirven, Richard J., Kuipers, Thomas B., and Mei, Hailiang

Published
2024
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215. Intradermal delivery of the third dose of the mRNA-1273 SARS-CoV-2 vaccine: safety and immunogenicity of a fractional booster dose

Author

Roozen, Geert V.T., Prins, Manon L.M., Prins, Corine, Janse, Jacqueline J., de Gruyter, Heidi L.M., Pothast, Cilia R., Huisman, Wesley, Koopman, Jan Pieter R., Lamers, Olivia A.C., Kuijer, Marjan, Myeni, Sebenzile K., van Binnendijk, Rob S., Hartog, Gerco den, Heemskerk, Mirjam H.M., Jochems, Simon P., Feltkamp, Mariet C.W., Kikkert, Marjolein, Rosendaal, Frits R., Roestenberg, Meta, Visser, Leo G., and Roukens, Anna H.E.

Published
2024
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219. Atacama Cosmology Telescope: Constraints on prerecombination early dark energy

Author

Hill, J Colin, Calabrese, Erminia, Aiola, Simone, Battaglia, Nicholas, Bolliet, Boris, Choi, Steve K, Devlin, Mark J, Duivenvoorden, Adriaan J, Dunkley, Jo, Ferraro, Simone, Gallardo, Patricio A, Gluscevic, Vera, Hasselfield, Matthew, Hilton, Matt, Hincks, Adam D, Hložek, Renée, Koopman, Brian J, Kosowsky, Arthur, La Posta, Adrien, Louis, Thibaut, Madhavacheril, Mathew S, McMahon, Jeff, Moodley, Kavilan, Naess, Sigurd, Natale, Umberto, Nati, Federico, Newburgh, Laura, Niemack, Michael D, Page, Lyman A, Partridge, Bruce, Qu, Frank J, Salatino, Maria, Schillaci, Alessandro, Sehgal, Neelima, Sherwin, Blake D, Sifón, Cristóbal, Spergel, David N, Staggs, Suzanne T, Storer, Emilie R, van Engelen, Alexander, Vavagiakis, Eve M, Wollack, Edward J, and Xu, Zhilei

Subjects
Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract

The early dark energy (EDE) scenario aims to increase the value of the Hubble constant (H0) inferred from cosmic microwave background (CMB) data over that found in the standard cosmological model (ΛCDM), via the introduction of a new form of energy density in the early Universe. The EDE component briefly accelerates cosmic expansion just prior to recombination, which reduces the physical size of the sound horizon imprinted in the CMB. Previous work has found that nonzero EDE is not preferred by Planck CMB power spectrum data alone, which yield a 95% confidence level (C.L.) upper limit fEDE99.7% C.L.: fEDE=0.091-0.036+0.020, with H0=70.9-2.0+1.0 km/s/Mpc (both 68% C.L.). From a model-selection standpoint, we find that EDE is favored over ΛCDM by these data at roughly 3σ significance. In contrast, a joint analysis of the full Planck and ACT data yields no evidence for EDE, as previously found for Planck alone. We show that the preference for EDE in ACT alone is driven by its TE and EE power spectrum data. The tight constraint on EDE from Planck alone is driven by its high-ℓ TT power spectrum data. Understanding whether these differing constraints are physical in nature, due to systematics, or simply a rare statistical fluctuation is of high priority. The best-fit EDE models to ACT and Planck exhibit coherent differences across a wide range of multipoles in TE and EE, indicating that a powerful test of this scenario is anticipated with near-future data from ACT and other ground-based experiments.

Published
2022

220. The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy

Author

Hill, J. Colin, Calabrese, Erminia, Aiola, Simone, Battaglia, Nicholas, Bolliet, Boris, Choi, Steve K., Devlin, Mark J., Duivenvoorden, Adriaan J., Dunkley, Jo, Ferraro, Simone, Gallardo, Patricio A., Gluscevic, Vera, Hasselfield, Matthew, Hilton, Matt, Hincks, Adam D., Hlozek, Renee, Koopman, Brian J., Kosowsky, Arthur, La Posta, Adrien, Louis, Thibaut, Madhavacheril, Mathew S., McMahon, Jeff, Moodley, Kavilan, Naess, Sigurd, Natale, Umberto, Nati, Federico, Newburgh, Laura, Niemack, Michael D., Page, Lyman A., Partridge, Bruce, Qu, Frank J., Salatino, Maria, Schillaci, Alessandro, Sehgal, Neelima, Sherwin, Blake D., Sifon, Cristobal, Spergel, David N., Staggs, Suzanne T., Storer, Emilie R., van Engelen, Alexander, Vavagiakis, Eve M., Wollack, Edward J., and Xu, Zhilei

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology
Abstract

The early dark energy (EDE) scenario aims to increase the value of the Hubble constant ($H_0$) inferred from cosmic microwave background (CMB) data over that found in $\Lambda$CDM, via the introduction of a new form of energy density in the early universe. The EDE component briefly accelerates cosmic expansion just prior to recombination, which reduces the physical size of the sound horizon imprinted in the CMB. Previous work has found that non-zero EDE is not preferred by Planck CMB power spectrum data alone, which yield a 95% confidence level (CL) upper limit $f_{\rm EDE} < 0.087$ on the maximal fractional contribution of the EDE field to the cosmic energy budget. In this paper, we fit the EDE model to CMB data from the Atacama Cosmology Telescope (ACT) Data Release 4. We find that a combination of ACT, large-scale Planck TT (similar to WMAP), Planck CMB lensing, and BAO data prefers the existence of EDE at $>99.7$% CL: $f_{\rm EDE} = 0.091^{+0.020}_{-0.036}$, with $H_0 = 70.9^{+1.0}_{-2.0}$ km/s/Mpc (both 68% CL). From a model-selection standpoint, we find that EDE is favored over $\Lambda$CDM by these data at roughly $3\sigma$ significance. In contrast, a joint analysis of the full Planck and ACT data yields no evidence for EDE, as previously found for Planck alone. We show that the preference for EDE in ACT alone is driven by its TE and EE power spectrum data. The tight constraint on EDE from Planck alone is driven by its high-$\ell$ TT power spectrum data. Understanding whether these differing constraints are physical in nature, due to systematics, or simply a rare statistical fluctuation is of high priority. The best-fit EDE models to ACT and Planck exhibit coherent differences across a wide range of multipoles in TE and EE, indicating that a powerful test of this scenario is anticipated with near-future data from ACT and other ground-based experiments., Comment: v1: 25+20 pages, 6+18 figures, submitted to PRD; v2: 26+20 pages, 7+18 figures, results unchanged, matches PRD accepted version. MCMC chains available at https://lambda.gsfc.nasa.gov/product/act/actpol_mcmc_chains_get.html

Published
2021
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221. Pseudo Relevance Feedback with Deep Language Models and Dense Retrievers: Successes and Pitfalls

Author

Li, Hang, Mourad, Ahmed, Zhuang, Shengyao, Koopman, Bevan, and Zuccon, Guido

Subjects
Computer Science - Information Retrieval
Abstract

Pseudo Relevance Feedback (PRF) is known to improve the effectiveness of bag-of-words retrievers. At the same time, deep language models have been shown to outperform traditional bag-of-words rerankers. However, it is unclear how to integrate PRF directly with emergent deep language models. In this article, we address this gap by investigating methods for integrating PRF signals into rerankers and dense retrievers based on deep language models. We consider text-based and vector-based PRF approaches, and investigate different ways of combining and scoring relevance signals. An extensive empirical evaluation was conducted across four different datasets and two task settings (retrieval and ranking). Text-based PRF results show that the use of PRF had a mixed effect on deep rerankers across different datasets. We found that the best effectiveness was achieved when (i) directly concatenating each PRF passage with the query, searching with the new set of queries, and then aggregating the scores; (ii) using Borda to aggregate scores from PRF runs. Vector-based PRF results show that the use of PRF enhanced the effectiveness of deep rerankers and dense retrievers over several evaluation metrics. We found that higher effectiveness was achieved when (i) the query retains either the majority or the same weight within the PRF mechanism, and (ii) a shallower PRF signal (i.e., a smaller number of top-ranked passages) was employed, rather than a deeper signal. Our vector-based PRF method is computationally efficient; thus this represents a general PRF method others can use with deep rerankers and dense retrievers., Comment: Accepted to the Journal of ACM Transactions on Information Systems (TOIS)

Published
2021

228. Forearm rotation improves after corrective osteotomy in patients with symptomatic distal radius malunion

Author

Blomme, R.A.M., Smit, J.M., Harmsen, K., Halbesma, G., Vermeulen, G.M., Schipper, JP de, van Uchelen, J.H., Zöphel, O.T., Souer, J.S., Esteban Lopez, L., Fink, A., van Huis, R., Pennehouat, P.Y., Schoneveld, K., Arends, G.D., Feitz, R., Hoogendam, L., Hovius, S.E.R., van Kooij, Y.E., Koopman, J.E., van der Oest, M.J.W., de Ridder, W.A., Selles, R.W., Sikking, L., Slijper, H.P., ter Stege, M.H.P., Teunissen, J.S., Wouters, R.M., Loos, N.L., Mendelaar, N.H.A., Wijk, L van, Bijlsma, W.R., Duraku, L.S., van der Heijden, E.P.A., Hundepool, C.A., Zuidam, J.M., van Es, E.M., Dijkhof, M., van Ewijk, F.J., and Colaris, J.W.

Published
2024
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231. Host gene expression signatures to identify infection type and organ dysfunction in children evaluated for sepsis: a multicentre cohort study

Author

Levin, Michael, Coin, Lachlan, Gormley, Stuart, Hamilton, Shea, Hoggart, Clive, Kaforou, Myrsini, Sancho-Shimizu, Vanessa, Wright, Victoria, Abdulla, Amina, Agapow, Paul, Bartlett, Maeve, Eleftherohorinou, Hariklia, Galassini, Rachel, Inwald, David, Mashbat, Meg, Menikou, Stephanie, Mustafa, Sobia, Nadel, Simon, Rahman, Rahmeen, Shailes, Hannah, Thakker, Clare, Bokhandi, S., Power, Sue, Barham, Heather, Pathan, N., Ridout, Jenna, White, Deborah, Thurston, Sarah, Faust, S., Patel, S., McCorkell, Jenni, Davies, P., Crate, Lindsey, Navarra, Helen, Carter, Stephanie, Ramaiah, R., Patel, Rekha, Tuffrey, Catherine, Gribbin, Andrew, McCready, Sharon, Peters, Mark, Hardy, Katie, Standing, Fran, O'Neill, Lauren, Abelake, Eugenia, Deep, Akash, Nsirim, Eniola, Pollard, Andrew, Willis, Louise, Young, Zoe, Royad, C., White, Sonia, Fortune, Peter-Marc, Hudnott, Phil, Martinón-Torres, Federico, Salas, Antonio, Álvez González, Fernando, Barral-Arca, Ruth, Cebey-López, Miriam, Curras-Tuala, María José, García, Natalia, García Vicente, Luisa, Gómez-Carballa, Alberto, Gómez Rial, Jose, Grela Beiroa, Andrea, Justicia Grande, Antonio, Leboráns Iglesias, Pilar, Martínez Santos, Alba Elena, Martinón-Torres, Nazareth, Martinón Sánchez, José María, Morillo Gutiérrez, Beatriz, Mosquera Pérez, Belén, Obando Pacheco, Pablo, Pardo-Seco, Jacobo, Pischedda, Sara, Rivero-Calle, Irene, Rodríguez-Tenreiro, Carmen, Redondo-Collazo, Lorenzo, Salas Ellacuriaga, Antonio, Fernández, Sonia Serén, del Sol Porto Silva, María, Vega, Ana, Vilanova Trillo, Lucía, Reyes, Susana Beatriz, Cruz León León, María, Navarro Mingorance, Álvaro, Gabaldó Barrio, Xavier, Oñate Vergara, Eider, Concha Torre, Andrés, Vivanco, Ana, Fernández, Reyes, Giménez Sánchez, Francisco, Sánchez Forte, Miguel, Rojo, Pablo, Contreras, J. Ruiz, Palacios, Alba, Epalza Ibarrondo, Cristina, Fernández Cooke, Elizabeth, Navarro, Marisa, Álvarez Álvarez, Cristina, José Lozano, María, Carreras, Eduardo, Brió Sanagustín, Sonia, Neth, Olaf, Martínez Padilla, Mª del Carmen, Prieto Tato, Luis Manuel, Guillén, Sara, Fernández Silveira, Laura, Moreno, David, de Groot, R., Tutu van Furth, A.M., van der Flier, M., Boeddha, N.P., Driessen, G.J.A., Emonts, M., Hazelzet, J.A., Kuijpers, T.W., Pajkrt, D., Sanders, E.A.M., van de Beek, D., van der Ende, A., Philipsen, H.L.A., Adeel, A.O.A., Breukels, M.A., Brinkman, D.M.C., de Korte, C.C.M.M., de Vries, E., de Waal, W.J., Dekkers, R., Dings-Lammertink, A., Doedens, R.A., Donker, A.E., Dousma, M., Faber, T.E., Gerrits, G.P.J.M., Gerver, J.A.M., Heidema, J., Homan-van der Veen, J., Jacobs, M.A.M., Jansen, N.J.G., Kawczynski, P., Klucovska, K., Kneyber, M.C.J., Koopman-Keemink, Y., Langenhorst, V.J., Leusink, J., Loza, B.F., Merth, I.T., Miedema, C.J., Neeleman, C., Noordzij, J.G., Obihara, C.C., van Overbeek- van Gils, A.L.T., Poortman, G.H., Potgieter, S.T., Potjewijd, J., Rosias, P.P.R., Sprong, T., ten Tussher, G.W., Thio, B.J., Tramper-Stranders, G.A., van Deuren, M., van der Meer, H., van Kuppevelt, A.J.M., van Wermeskerken, A.M., Verwijs, W.A., Wolfs, T.F.W., Schlapbach, Luregn J., Agyeman, Philipp, Aebi, Christoph, Giannoni, Eric, Stocker, Martin, Posfay-Barbe, Klara M., Heininger, Ulrich, Bernhard-Stirnemann, Sara, Niederer-Loher, Anita, Kahlert, Christian, Hasters, Paul, Relly, Christa, Baer, Walter, Berger, Christoph, Carrol, Enitan D., Paulus, Stéphane, Frederick, Hannah, Jennings, Rebecca, Johnston, Joanne, Kenwright, Rhian, Fink, Colin G, Pinnock, Elli, Emonts, Marieke, Agbeko, Rachel, Anderson, Suzanne, Secka, Fatou, Bojang, Kalifa, Sarr, Isatou, Kebbeh, Ngange, Sey, Gibbi, Saidykhan, Momodou, Cole, Fatoumata, Thomas, Gilleh, Antonio, Martin, Zenz, Werner, Kohlfürst, Daniela S., Binder, Alexander, Schweintzger, Nina A., Sagmeister, Manfred, Baumgart, Hinrich, Baumgartner, Markus, Behrends, Uta, Biebl, Ariane, Birnbacher, Robert, Blanke, Jan-Gerd, Boelke, Carsten, Breuling, Kai, Brunner, Jürgen, Buller, Maria, Dahlem, Peter, Dietrich, Beate, Eber, Ernst, Elias, Johannes, Emhofer, Josef, Etschmaier, Rosa, Farr, Sebastian, Girtler, Ylenia, Grigorow, Irina, Heimann, Konrad, Ihm, Ulrike, Jaros, Zdenek, Kalhoff, Hermann, Kaulfersch, Wilhelm, Kemen, Christoph, Klocker, Nina, Köster, Bernhard, Kohlmaier, Benno, Komini, Eleni, Kramer, Lydia, Neubert, Antje, Ortner, Daniel, Pescollderungg, Lydia, Pfurtscheller, Klaus, Reiter, Karl, Ristic, Goran, Rödl, Siegfried, Sellner, Andrea, Sonnleitner, Astrid, Sperl, Matthias, Stelzl, Wolfgang, Till, Holger, Trobisch, Andreas, Vierzig, Anne, Vogel, Ulrich, Weingarten, Christina, Welke, Stefanie, Wimmer, Andreas, Wintergerst, Uwe, Wüller, Daniel, Zaunschirm, Andrew, Ziuraite, Ieva, Žukovskaja, Veslava, Hibberd, Martin L., Davila, Sonia, Delany, Isabel, Schlapbach, Luregn J, Raman, Sainath, Sharp, Nathalie, Phillips, Natalie, Irwin, Adam, Balch, Ross, Harley, Amanda, Johnson, Kerry, Sever, Zoe, George, Shane, Grimwood, Keith, Snelling, Peter J, Chavan, Arjun, Kitcatt, Eleanor, Lawton, Luke, Hempenstall, Allison, Pilot, Pelista, Gibbons, Kristen S, Le Marsney, Renate, Blumenthal, Antje, Ganesamoorthy, Devika, Pardo, Carolyn, Kling, Jessica, McPherson, Stephen, MacDonald, Anna D, Bialasiewicz, Seweryn, Pham, Trang, Wilson, Clare, Sharp, Natalie, Kling, Jessica C, McPherson, Stephen J, Herberg, Jethro A, and Coin, Lachlan J M

Published
2024
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232. Impact of Left Atrial Posterior Wall Ablation During Pulsed-Field Ablation for Persistent Atrial Fibrillation

Author

Turagam, Mohit K., Neuzil, Petr, Schmidt, Boris, Reichlin, Tobias, Neven, Kars, Metzner, Andreas, Hansen, Jim, Blaauw, Yuri, Maury, Philippe, Arentz, Thomas, Sommer, Philipp, Anic, Ante, Anselme, Frederic, Boveda, Serge, Deneke, Tom, Willems, Stephan, van der Voort, Pepijn, Tilz, Roland, Funasako, Moritoshi, Scherr, Daniel, Wakili, Reza, Steven, Daniel, Kautzner, Josef, Vijgen, Johan, Jais, Pierre, Petru, Jan, Chun, Julian, Roten, Laurent, Füting, Anna, Lemoine, Marc D., Ruwald, Martin, Mulder, Bart A., Rollin, Anne, Lehrmann, Heiko, Fink, Thomas, Jurisic, Zrinka, Chaumont, Corentin, Adelino, Raquel, Nentwich, Karin, Gunawardene, Melanie, Ouss, Alexandre, Heeger, Christian-Hendrik, Manninger, Martin, Bohnen, Jan-Eric, Sultan, Arian, Peichl, Petr, Koopman, Pieter, Derval, Nicolas, Kueffer, Thomas, Reinsch, Nico, and Reddy, Vivek Y.

Published
2024
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233. Results from the UNITED study: a multicenter study validating the prognostic effect of the tumor–stroma ratio in colon cancer

Author

Petrushevska, Gordana, Bogdanovska, Magdalena, Zdravkoski, Panche, Antovic, Svetozar, Dzambaz, Darko, Karagjozov, Panche, de Cuba, Erienne M.V., Beverdam, Frédérique, Jansen, Jan, Vermaas, Maarten, Gašljević, Gorana, Kjær-Frifeldt, Sanne, Lindebjerg, Jan, Strous, Maud, Vogelaar, Jeroen F., Bulkmans, Nicole W.J., van Baarlen, Joop, Mekenkamp, Leonie, Hoekstra, Ronald, Sie, Mark, Cuatrecasas, Miriam, Simonetti, Sara, Rodrigo, María Teresa, Sanz, Iván Archilla, Guerrero Pineda, Jose, Leeuwis-Fedorovich, Natalja E., Talsma, Koen A., Souza da Silva, Ricella M., Lacle, Miangela M., Koopman, Miriam, Dekker, Jan Willem T., van Tilburg, Arjan, Nuciforo, Paolo, Villalobos Alberú, Xenia, Landolfi, Stefania, Zucchiatti, Adriana, Witteveen, Emma, Bordbar, Arad, Hendriks, Mathijs P., Arensman, René, Natu, Shonali, Maka, Noori, Mesker, Wilma E., Tollenaar, Rob A.E.M., Polack, Meaghan, Smit, Marloes A., van Pelt, Gabi W., Putter, Hein, Meershoek-Kleinenbarg, Elma, Roodvoets, Annet G.H., Crobach, Augustinus S.L.P., Gelderblom, Hans, Fontes e Sousa, Mário, Borralho Nunes, Paula, Cruz, João, Raimundo, Ana, Silva, Nelson, Brito, Maria J., Terpstra, Valeska, Zakhartseva, L.M., Al Dieri, Raed, Fléjou, Jean-François, Feakins, Roger, Dequeker, Els, Vink, Geraldine R., van Krieken, J.Han J.M., Polack, M., Smit, M.A., van Pelt, G.W., Roodvoets, A.G.H., Meershoek-Klein Kranenbarg, E., Putter, H., Gelderblom, H., Crobach, A.S.L.P., Terpstra, V., Petrushevska, G., Gašljević, G., Kjær-Frifeldt, S., de Cuba, E.M.V., Bulkmans, N.W.J., Vink, G.R., Al Dieri, R., Tollenaar, R.A.E.M., van Krieken, J.H.J.M., and Mesker, W.E.

Published
2024
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234. Pathological findings associated with the updated European Society of Cardiology 2022 guidelines for preoperative cardiac testing: an observational cohort modelling study

Author

Kemper, Johann, Kohaupt, Lena, Witzler, Jette, Tuzhikov, Michael, Roth, Sebastian, Stroda, Alexandra, M’Pembele, René, Tenge, Theresa, Schultze, Cornelia, Verbarg, Nele, Gehrke, Christian, Klemann, Anna Katharina, Hagebölling, Friederike, Albrecht, Svenja, Stroeder, Jakob, Schubert, Ann-Kristin, Espeter, Florian, Russe, Benedikt, Weigand, Markus A., Bergmann, Lars, Unterberg, Matthias, Bischoff, Petra, Pirzer, Raphael, Rach, Patric Rene, Ott, Klaus, Zarbock, Alexander, Kowark, Ana, Neumann, Claudia, Marchand, Bahareh, Sponholz, Christoph, Rueffert, Henrik, Kramer, Mira, Zacharowski, Kai, Meybohm, Patrick, Lindau, Simone, Carollo, Melissa, Novazzi, Cecilia, Toso, Fiorenza, Bacuzzi, Alessandro, Ragazzi, Riccardo, Volta, Carlo Alberto, De Giorgi, Francesco, Bacer, Barbara, Federico, Antonio, Chiumello, Davide, Vetrugno, Luigi, Castella, Alberto, Tesoro, Simonetta, Cotoia, Antonella, Bignami, Elena, Bellissima, Agrippino, Cortegiani, Andrea, Crisman, Marco, Toninelli, Arturo, Piazza, Ornella, Mirabella, Lucia, Bossolasco, Matteo, Bona, Francesco, Perdomo, Juan Manuel, Coca-Martinez, Miquel, Carramiñana, Albert, Servén, Marta Giné, González, Astrid Batalla, Gil Sánchez, José Maria, Becerra-Bolaños, Ángel, Rodríguez-Pérez, Aurelio, Soler, Anna Artigas, Basso, Morena, Font, Anna Peig, Vernetta, Diana, Santos, Julia Hernando, Muñoz, Enrique Alday, Olivares, Mercedes Cabellos, Marco, Gregorio, Lopez, Maria Bermudez, Barrio, Javier, Forés, María Isabel, Boix, Estefanía, Ayuso, Mercedes, Petre, Bogdan Sorel, Oprea, Ioana Sorina, Latiș, Mihai Dan, Margarit, Simona, Vasian, Horatiu, Tomescu, Dana, Cîndea, Iulia, Dirzu, Dan Sebastian, Copotoiu, Sanda-Maria, Moise, Alida, Bubenek-Turconi, Serban, Valeanu, Liana, Wanner, Patrick Mark, Djurdjevic, Mirjana, Nuth, Sandra, Seeberger, Esther, Goettel, Nicolai, Kamber, Firmin, Ganter, Michael Thomas, Gerber, Thomas Jan, Schneebeli, Daniela, Pregernig, Andreas, Grape, Sina, Tomala, Simon, Pinto, Bernardo Bollen, Żukowski, Maciej, Zegan-Barańska, Małgorzata, Karolak, Igor, Krzych, Lukasz, Czajka, Szymon, Studzińska, Dorota, Kluzik, Anna, Koszel, Tomasz, Pabjańczyk, Izabela, Gajdosz, Anna, Erkoc, Suheyla Karadag, Meco, Basak Ceyda, Koltka, Ahmet Kemalettin, Dincer, Muserref Beril, Ekmekçi, Perihan, Saracoglu, Kemal Tolga, Solmaz, Filiz Alkaya, Ozcelik, Menekse, Arun, Oguzhan, Dilmen, Ozlem Korkmaz, Preckel, Benedikt, Hollmann, Markus W., Hazen, Yannick, Donald de Boer, Hans, Epema, Anne, Koopman, Seppe, Van Lier, Felix, Pinto, Rita, Carrão, André, Ribeiro, Daniel, Mourão, Joana, Coelho, Miguel, Losa, Nuno, Santos, Nuno, Cabral, Luis, Afonso, Diana, Zenha, Sérgio, Ramos, Cristina, Hipólito, Carla, Vasilaki, Maria, Andreeva, Antonia, Zaimi, Donika, Chalkias, Athanasios, Spyraki, Maria, Rekatsina, Martina, Tsaousi, Georgia, Short, Anthony, Meier, Sonja, Madhuri, Thumuluru Kavitha, Latham, Scott, Knock, James, Drummond, Andrew, Ramsden, Fiona, Kubisz-Pudelko, Agnieszka, Walker, James, Moppett, Iain, White, Louise, Jackson, Matthew, Reschreiter, Henrik, Innes, Richard, Chew, Michelle, Kalman, Sigridur, Wallden, Jakob, Schening, Anna, Jonikaite, Lina, Enlund, Anna, De Baerdemaeker, Luc, Morrison, Stuart, Rex, Steffen, Alexis, Alexandros, Khoronenko, Viktoria E., Ovezov, Alexey, Belskii, Vladislav, Kaznacheeva, Kseniya, Gritsan, Alexey, Kuzmanovska, Biljana, Malinovska-Nikolovska, Liljana, Barisin, Stjepan, Poredos, Peter, Arabadzhieva, Daniela, Unic-Stojanovic, Dragana, Golubović, Mladjan, Fleischmann, Edith, Kotzinger, Oskar, Des Deserts, Marc Danguy, Ducrocq, Nicolas, Buggy, Donal J., Bonnet, Jean François, Cusack, Barbara, Calleja, Paul, Hasani, Antigona, Nallbani, Rajmonda, Mauermann, Eckhard, Ionescu, Daniela, Szczeklik, Wojciech, De Hert, Stefan, Filipovic, Miodrag, Beck Schimmer, Beatrice, Spadaro, Savino, Matute, Purificación, Ganter, Michael T., Turhan, Sanem C., van Waes, Judith, Lagarto, Filipa, Theodoraki, Kassiani, Gupta, Anil, Gillmann, Hans-Jörg, Guzzetti, Luca, Kotfis, Katarzyna, Larmann, Jan, Corneci, Dan, Howell, Simon J., and Lurati Buse, Giovanna

Published
2024
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237. The mass and galaxy distribution around SZ-selected clusters

Author

Shin, T., Jain, B., Adhikari, S., Baxter, E. J., Chang, C., Pandey, S., Salcedo, A., Weinberg, D. H., Amsellem, A., Battaglia, N., Belyakov, M., Dacunha, T., Goldstein, S., Kravtsov, A. V., Varga, T. N., Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Amon, A., Andrade-Oliveira, F., Annis, J., Bacon, D., Bechtol, K., Becker, M. R., Bernstein, G. M., Bertin, E., Bocquet, S., Bond, J. R., Brooks, D., Buckley-Geer, E., Burke, D. L., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Chen, R., Choi, A., Costanzi, M., da Costa, L. N., DeRose, J., Desai, S., De Vicente, J., Devlin, M. J., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferraro, S., Ferrero, I., Ferté, A., Flaugher, B., Frieman, J., Gallardo, P. A., Gatti, M., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Harrison, I., Hartley, W. G., Hill, J. C., Hilton, M., Hinton, S. R., Hollowood, D. L., Hughes, J. P., James, D. J., Jarvis, M., Jeltema, T., Koopman, B. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Lokken, M., MacCrann, N., Madhavacheril, M. S., Maia, M. A. G., McCullough, J., McMahon, J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Myles, J., Nati, F., Navarro-Alsina, A., Niemack, M. D., Ogando, R. L. C., Page, L. A., Palmese, A., Partridge, B., Paz-Chinchón, F., Pereira, M. E. S., Pieres, A., Malagón, A. A. Plazas, Prat, J., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Romer, A. K., Rykoff, E. S., Salatino, M., Sánchez, C., Sanchez, E., Santiago, B., Scarpine, V., Schillaci, A., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Sherwin, B. D., Sifón, C., Smith, M., Soares-Santos, M., Staggs, S. T., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Troxel, M. A., Tutusaus, I., Vavagiakis, E. M., Weller, J., Wollack, E. J., Yanny, B., Yin, B., and Zhang, Y.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev-Zel'dovich-selected clusters using both weak lensing and galaxy counts. The clusters are selected from the Atacama Cosmology Telescope Data Release 5 and the galaxies from the Dark Energy Survey Year 3 dataset. With signal-to-noise of 62 (43) for galaxy (weak lensing) profiles over scales of about $0.2-20h^{-1}$ Mpc, these are the highest precision measurements for SZ-selected clusters to date. Because SZ selection closely approximates mass selection, these measurements enable several tests of theoretical models of the mass and light distribution around clusters. Our main findings are: 1. The splashback feature is detected at a consistent location in both the mass and galaxy profiles and its location is consistent with predictions of cold dark matter N-body simulations. 2. The full mass profile is also consistent with the simulations; hence it can constrain alternative dark matter models that modify the mass distribution of clusters. 3. The shapes of the galaxy and lensing profiles are remarkably similar for our sample over the entire range of scales, from well inside the cluster halo to the quasilinear regime. This can be used to constrain processes such as quenching and tidal disruption that alter the galaxy distribution inside the halo, and scale-dependent features in the transition regime outside the halo. We measure the dependence of the profile shapes on the galaxy sample, redshift and cluster mass. We extend the Diemer \& Kravtsov model for the cluster profiles to the linear regime using perturbation theory and show that it provides a good match to the measured profiles. We also compare the measured profiles to predictions of the standard halo model and simulations that include hydrodynamics. Applications of these results to cluster mass estimation and cosmology are discussed., Comment: 15 pages, 6 figures (main) + 3 pages, 6 figures (appendix), submitted to MNRAS

Published
2021
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238. The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center

Author

Guan, Yilun, Clark, Susan E., Hensley, Brandon S., Gallardo, Patricio A., Naess, Sigurd, Duell, Cody J., Aiola, Simone, Atkins, Zachary, Calabrese, Erminia, Choi, Steve K., Cothard, Nicholas F., Devlin, Mark, Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Ferraro, Simone, Hasselfield, Matthew, Hughes, John P., Koopman, Brian J., Kosowsky, Arthur B., Madhavacheril, Mathew S., McMahon, Jeff, Nati, Federico, Niemack, Michael D., Page, Lyman A., Salatino, Maria, Schaan, Emmanuel, Sehgal, Neelima, Sifón, Cristóbal, Staggs, Suzanne, Vavagiakis, Eve M., Wollack, Edward J., and Xu, Zhilei

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present arcminute-resolution intensity and polarization maps of the Galactic center made with the Atacama Cosmology Telescope (ACT). The maps cover a 32 deg$^2$ field at 98, 150, and 224 GHz with $\vert l\vert\le4^\circ$, $\vert b\vert\le2^\circ$. We combine these data with Planck observations at similar frequencies to create coadded maps with increased sensitivity at large angular scales. With the coadded maps, we are able to resolve many known features of the Central Molecular Zone (CMZ) in both total intensity and polarization. We map the orientation of the plane-of-sky component of the Galactic magnetic field inferred from the polarization angle in the CMZ, finding significant changes in morphology in the three frequency bands as the underlying dominant emission mechanism changes from synchrotron to dust emission. Selected Galactic center sources, including Sgr A*, the Brick molecular cloud (G0.253+0.016), the Mouse pulsar wind nebula (G359.23-0.82), and the Tornado supernova remnant candidate (G357.7-0.1), are examined in detail. These data illustrate the potential for leveraging ground-based Cosmic Microwave Background polarization experiments for Galactic science., Comment: 26 pages, 14 figures, accepted for publication in ApJ

Published
2021
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239. Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT

Author

Orlowski-Scherer, John, Di Mascolo, Luca, Bhandarkar, Tanay, Manduca, Alex, Mroczkowski, Tony, Amodeo, Stefania, Battaglia, Nick, Brodwin, Mark, Choi, Steve K., Devlin, Mark, Dicker, Simon, Dunkley, Jo, Gonzalez, Anthony H., Han, Dongwon, Hilton, Matt, Huffenberger, Kevin, Hughes, John P., MacInnis, Amanda, Knowles, Kenda, Koopman, Brian J., Lowe, Ian, Moodley, Kavilan, Nati, Federico, Niemack, Michael D., Page, Lyman A., Partridge, Bruce, Romero, Charles, Salatino, Maria, Schillaci, Alessandro, Sehgal, Neelima, Sifón, Cristóbal, Staggs, Suzanne, Stanford, S. A., Thornton, Robert, Vavagiakis, Eve M., Wollack, Edward J., Xu, Zhilei, and Zhu, Ningfeng

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Galaxy clusters are an important tool for cosmology, and their detection and characterization are key goals for current and future surveys. Using data from the Wide-field Infrared Survey Explorer (WISE), the Massive and Distant Clusters of WISE Survey (MaDCoWS) located 2,839 significant galaxy overdensities at redshifts $0.7\lesssim z\lesssim 1.5$, which included extensive follow-up imaging from the Spitzer Space Telescope to determine cluster richnesses. Concurrently, the Atacama Cosmology Telescope (ACT) has produced large area mm-wave maps in three frequency bands along with a large catalog of Sunyaev-Zeldovich (SZ) selected clusters, as part of its Data Release 5 (DR5). Using the maps and cluster catalog from DR5, we explore the scaling between SZ mass and cluster richness. We use complementary radio survey data from the Very Large Array, submillimeter data from Herschel, and ACT 224~GHz data to assess the impact of contaminating sources on the SZ signals. We then use a hierarchical Bayesian model to fit the mass-richness scaling relation. We find that MaDCoWS clusters have submillimeter contamination which is consistent with a gray-body spectrum, while the ACT clusters are consistent with no submillimeter emission on average. We find the best fit ACT SZ mass vs. MaDCoWS richness scaling relation has a slope of $\kappa = 1.84^{+0.15}_{-0.14}$, where the slope is defined as $M\propto \lambda_{15}^{\kappa}$ where $\lambda_{15}$ is the richness. Additionally, we find that the approximate level of in-fill of the ACT and MaDCoWS cluster SZ signals to be at the percent level, Comment: 25 pages, 17 Figures; accepted for publication in A&A

Published
2021
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240. The Atacama Cosmology Telescope: A search for Planet 9

Author

Naess, Sigurd, Aiola, Simone, Battaglia, Nick, Bond, Richard J., Calabrese, Erminia, Choi, Steve K., Cothard, Nicholas F., Halpern, Mark, Hill, J. Colin, Koopman, Brian J., Devlin, Mark, McMahon, Jeff, Dicker, Simon, Duivenvoorden, Adriaan J., Dunkley, Jo, Van Engelen, Alexander, Fanfani, Valentina, Ferraro, Simone, Gallardo, Patricio A., Guan, Yilun, Han, Dongwon, Hasselfield, Matthew, Hincks, Adam D., Huffenberger, Kevin, Kosowsky, Arthur B., Louis, Thibaut, Macinnis, Amanda, Madhavacheril, Mathew S., Nati, Federico, Niemack, Michael D., Page, Lyman, Salatino, Maria, Schaan, Emmanuel, Orlowski-Scherer, John, Schillaci, Alessandro, Schmitt, Benjamin, Sehgal, Neelima, Sifón, Cristóbal, Staggs, Suzanne, and Wollack, Edward J.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

We use Atacama Cosmology Telescope (ACT) observations at 98 GHz (2015--2019), 150 GHz (2013--2019) and 229 GHz (2017--2019) to perform a blind shift-and-stack search for Planet 9. The search explores distances from 300 AU to 2000 AU and velocities up to 6.3 arcmin per year, depending on the distance. For a 5 Earth-mass Planet 9 the detection limit varies from 325 AU to 625 AU, depending on the sky location. For a 10 Earth-mass planet the corresponding range is 425 AU to 775 AU. The search covers the whole 18,000 square degrees of the ACT survey, though a slightly deeper search is performed for the parts of the sky consistent with Planet 9's expected orbital inclination. No significant detections are found, which is used to place limits on the mm-wave flux density of Planet 9 over much of its orbit. Overall we eliminate roughly 17% and 9% of the parameter space for a 5 and 10 Earth-mass Planet 9 respectively. We also provide a list of the 10 strongest candidates from the search for possible follow-up. More generally, we exclude (at 95% confidence) the presence of an unknown Solar system object within our survey area brighter than 4--12 mJy (depending on position) at 150 GHz with current distance $300 \text{ AU} < r < 600 \text{ AU}$ and heliocentric angular velocity $1.5'/\text{yr} < v \cdot \frac{500 \text{ AU}}{r} < 2.3'\text{yr}$, corresponding to low-to-moderate eccentricities. These limits worsen gradually beyond 600 AU, reaching 5--15 mJy by 1500 AU., Comment: 23 pages, 10 figures, 5 tables, submitted to ApJ

Published
2021
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241. The Simons Observatory: the Large Aperture Telescope (LAT)

Author

Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Beall, J. A., Bhandarkar, Tanay, Bond, J. Richard, Chesmore, Grace E., Chinone, Yuji, Choi, Steve K., Connors, Jake A., Coppi, Gabriele, Cothard, Nicholas F., Crowley, Kevin D., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duff, Shannon M., Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Gudmundsson, Jon E., Haridas, Saianeesh K., Harrington, Kathleen, Hervias-Caimapo, Carlos, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Kaneko, Daisuke, Kofman, Anna M., Koopman, Brian J., Lashner, Jack, Limon, Michele, Link, Michael J., Lucas, Tammy J., Matsuda, Frederick, McCarrick, Heather, Nati, Federico, Niemack, Michael D., Orlowski-Scherer, John, Piccirillo, Lucio, Sarmiento, Karen Perez, Schaan, Emmanuel, Silva-Feaver, Maximiliano, Sonka, Rita, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Terasaki, Tomoki, Thornton, Robert, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Whipps, Zachary, Wollack, Edward J., Zannoni, Mario, Zhu, Ningfeng, and Zonca, Andrea

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at $\sim$5200m altitude -- comprises three Small Aperture Telescopes (SATs) and one Large Aperture Telescope (LAT) at the Atacama Desert, Chile. This research note describes the design and current status of the LAT along with its future timeline., Comment: 4 pages, 1 figure

Published
2021
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242. AI Specialization for Pathways of Economic Diversification

Author

Mishra, Saurabh, Koopman, Robert, De-Prato, Giuditta, Rao, Anand, Osorio-Rodarte, Israel, Kim, Julie, Spatafora, Nikola, Strier, Keith, and Zaccaria, Andrea

Subjects
Computer Science - Computers and Society, Economics - General Economics
Abstract

The growth in AI is rapidly transforming the structure of economic production. However, very little is known about how within-AI specialization may relate to broad-based economic diversification. This paper provides a data-driven framework to integrate the interconnection between AI-based specialization with goods and services export specialization to help design future comparative advantage based on the inherent capabilities of nations. Using detailed data on private investment in AI and export specialization for more than 80 countries, we propose a systematic framework to help identify the connection from AI to goods and service sector specialization. The results are instructive for nations that aim to harness AI specialization to help guide sources of future competitive advantage. The operational framework could help inform the public and private sector to uncover connections with nearby areas of specialization., Comment: 27 pages, 20 figures, 3 tables

Published
2021

243. The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access

Author

Mallaby-Kay, Maya, Atkins, Zachary, Aiola, Simone, Amodeo, Stefania, Austermann, Jason E., Beall, James A., Becker, Daniel T., Bond, J. Richard, Calabrese, Erminia, Chesmore, Grace E., Choi, Steve K., Crowley, Kevin T., Darwish, Omar, Denison, Edwawd V., Devlin, Mark J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Ferraro, Simone, Fichman, Kyra, Gallardo, Patricio A., Golec, Joseph E., Guan, Yilun, Han, Dongwon, Hasselfield, Matthew, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hlozek, Renee, Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Koopman, Brian J., Louis, Thibaut, MacInnis, Amanda, Madhavacheril, Mathew S., McMahon, Jeff, Moodley, Kavilan, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura B., Nibarger, John P., Niemack, Michael D., Page, Lyman A., Salatino, Maria, Schaan, Emmanuel, Schillaci, Alessandro, Sehgal, Neelima, Sherwin, Blake D., Sifon, Cristobal, Simon, Sara, Staggs, Suzanne T., Storer, Emilie R., Ullom, Joel N., Van Engelen, Alexander, Van Lanen, Jeff, Vale, Leila R., Wollack, Edward J., and Xu, Zhilei

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Two recent large data releases for the Atacama Cosmology Telescope (ACT), called DR4 and DR5, are available for public access. These data include temperature and polarization maps that cover nearly half the sky at arcminute resolution in three frequency bands; lensing maps and component-separated maps covering ~ 2,100 deg^2 of sky; derived power spectra and cosmological likelihoods; a catalog of over 4,000 galaxy clusters; and supporting ancillary products including beam functions and masks. The data and products are described in a suite of ACT papers; here we provide a summary. In order to facilitate ease of access to these data we present a set of Jupyter IPython notebooks developed to introduce users to DR4, DR5, and the tools needed to analyze these data. The data products (excluding simulations) and the set of notebooks are publicly available on the NASA Legacy Archive for Microwave Background Data Analysis (LAMBDA); simulation products are available on the National Energy Research Scientific Computing Center (NERSC)., Comment: Accepted to ApJS. 21 pages, 8 figures. Data and notebooks available on LAMBDA https://lambda.gsfc.nasa.gov/product/act/

Published
2021
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244. The Simons Observatory Large Aperture Telescope Receiver

Author

Zhu, Ningfeng, Bhandarkar, Tanay, Coppi, Gabriele, Kofman, Anna M., Orlowski-Scherer, John L., Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Aiola, Simone, Austermann, Jason, Bazarko, Andrew O., Beall, James A., Bhimani, Sanah, Bond, J. Richard, Chesmore, Grace E., Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duell, Cody J., Duff, Shannon M., Dünner, Rolando, Fabbian, Giulio, Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Haridas, Saianeesh K., Harrington, Kathleen, Healy, Erin, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keatin, Brian, Kiuchi, Kenji, Koopman, Brian J., Lashner, Jack, Lee, Adrian T., Li, Yaqiong, Limon, Michele, Link, Michael, Lucas, Tammy J, McCarrick, Heather, Moore, Jenna, Nati, Federico, Newburgh, Laura B., Niemack, Michael D., Pierpaoli, Elena, Randall, Michael J., Sarmiento, Karen Perez, Saunders, Lauren J., Seibert, Joseph, Sierra, Carlos, Sonka, Rita, Spisak, Jacob, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Thornton, Robert J., Tsan, Tran, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Westbrook, Benjamin, Wollack, Edward J., and Zannoni, Mario

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The Simons Observatory (SO) Large Aperture Telescope Receiver (LATR) will be coupled to the Large Aperture Telescope located at an elevation of 5,200 m on Cerro Toco in Chile. The resulting instrument will produce arcminute-resolution millimeter-wave maps of half the sky with unprecedented precision. The LATR is the largest cryogenic millimeter-wave camera built to date with a diameter of 2.4 m and a length of 2.6 m. It cools 1200 kg of material to 4 K and 200 kg to 100 mk, the operating temperature of the bolometric detectors with bands centered around 27, 39, 93, 145, 225, and 280 GHz. Ultimately, the LATR will accommodate 13 40 cm diameter optics tubes, each with three detector wafers and a total of 62,000 detectors. The LATR design must simultaneously maintain the optical alignment of the system, control stray light, provide cryogenic isolation, limit thermal gradients, and minimize the time to cool the system from room temperature to 100 mK. The interplay between these competing factors poses unique challenges. We discuss the trade studies involved with the design, the final optimization, the construction, and ultimate performance of the system.

Published
2021
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245. The Integration and Testing Program for the Simons Observatory Large Aperture Telescope Optics Tubes

Author

Harrington, Kathleen, Sierra, Carlos, Chesmore, Grace, Sutariya, Shreya, Ali, Aamir M., Choi, Steve K., Cothard, Nicholas F., Dicker, Simon, Galitzki, Nicholas, Ho, Shuay-Pwu Patty, Kofman, Anna M., Koopman, Brian J., Lashner, Jack, McMahon, Jeff, Niemack, Michael D., Orlowski-Scherer, John, Seibert, Joseph, Silva-Feaver, Max, Vavagiakis, Eve M., Xu, Zhilei, and Zhu, Ningfeng

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe from the Atacama Desert in Chile. In total, SO will field over 60,000 transition-edge sensor (TES) bolometers in six spectral bands centered between 27 and 280 GHz in order to achieve the sensitivity necessary to measure or constrain numerous cosmological quantities, as outlined in The Simons Observatory Collaboration et al. (2019). The 6~m Large Aperture Telescope (LAT), which will target the smaller angular scales of the CMB, utilizes a cryogenic receiver (LATR) designed to house up to 13 individual optics tubes. Each optics tube is comprised of three silicon lenses, IR blocking filters, and three dual-polarization, dichroic TES detector wafers. The scientific objectives of the SO project require these optics tubes to achieve high-throughput optical performance while maintaining exquisite control of systematic effects. We describe the integration and testing program for the SO LATR optics tubes that will verify the design and assembly of the optics tubes before they are shipped to the SO site and installed in the LATR cryostat. The program includes a quick turn-around test cryostat that is used to cool single optics tubes and validate the cryogenic performance and detector readout assembly. We discuss the optical design specifications the optics tubes must meet to be deployed on sky and the suite of optical test equipment that is prepared to measure these requirements.

Published
2021
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246. The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies

Author

Calafut, Victoria, Gallardo, Patricio A., Vavagiakis, Eve M., Amodeo, Stefania, Aiola, Simone, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia S., Beall, James A., Bean, Rachel, Bond, J. Richard, Calabrese, Erminia, Choi, Steve K., Cothard, Nicholas F., Devlin, Mark J., Duell, Cody J., Duff, S. M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dunner, Rolando, Ferraro, Simone, Guan, Yilun, Hill, J. Colin, Hilton, Matt, Hlozek, Renee, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Koopman, Brian J., Kosowsky, Arthur, Li, Yaqiong, Lokken, Martine, Madhavacheril, Mathew, McMahon, Jeff, Moodley, Kavilan, Naess, Sigurd, Nati, Federico, Newburgh, Laura B., Niemack, Michael D., Page, Lyman, Partridge, Bruce, Schaan, Emmanuel, Schillaci, Alessandro, Sifon, Cristobal, Spergel, David N., Staggs, Suzanne T., Ullom, Joel N., Vale, Leila R., Van Engelen, Alexander, Wollack, Edward J., and Xu, Zhilei

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present a 5.4$\sigma$ detection of the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect using Atacama Cosmology Telescope (ACT) and $\it{Planck}$ CMB observations in combination with Luminous Red Galaxy samples from the Sloan Digital Sky Survey (SDSS) DR15 catalog. Results are obtained using three ACT CMB maps: co-added 150 GHz and 98 GHz maps, combining observations from 2008-2018 (ACT DR5), which overlap with SDSS DR15 over 3,700 sq. deg., and a component-separated map using night-time only observations from 2014-2015 (ACT DR4), overlapping with SDSS DR15 over 2,089 sq. deg. Comparisons of the results from these three maps provide consistency checks in relation to potential frequency-dependent foreground contamination. A total of 343,647 galaxies are used as tracers to identify and locate galaxy groups and clusters from which the kSZ signal is extracted using aperture photometry. We consider the impact of various aperture photometry assumptions and covariance estimation methods on the signal extraction. Theoretical predictions of the pairwise velocities are used to obtain best-fit, mass-averaged, optical depth estimates for each of five luminosity-selected tracer samples. A comparison of the kSZ-derived optical depth measurements obtained here to those derived from the thermal SZ effect for the same sample is presented in a companion paper., Comment: 17 pages, 10 figures. Updated to match published version in PRD

Published
2021
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247. The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects

Author

Vavagiakis, Eve M., Gallardo, Patricio A., Calafut, Victoria, Amodeo, Stefania, Aiola, Simone, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia S., Beall, James A., Bean, Rachel, Bond, J. Richard, Calabrese, Erminia, Choi, Steve K., Cothard, Nicholas F., Devlin, Mark J., Duell, Cody J., Duff, S. M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dunner, Rolando, Ferraro, Simone, Guan, Yilun, Hill, J. Colin, Hilton, Matt, Hlozek, Renee, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Koopman, Brian J., Kosowsky, Arthur, Li, Yaqiong, Lokken, Martine, Madhavacheril, Mathew, McMahon, Jeff, Moodley, Kavilan, Naess, Sigurd, Nati, Federico, Newburgh, Laura B., Niemack, Michael D., Page, Lyman, Partridge, Bruce, Schaan, Emmanuel, Schillaci, Alessandro, Sifon, Cristobal, Spergel, David N., Staggs, Suzanne T., Ullom, Joel N., Vale, Leila R., Van Engelen, Alexander, Wollack, Edward J., and Xu, Zhilei

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present high signal-to-noise measurements (up to 12$\sigma$) of the average thermal Sunyaev Zel'dovich (tSZ) effect from optically selected galaxy groups and clusters and estimate their baryon content within a 2.1$^\prime$ radius aperture. Sources from the Sloan Digital Sky Survey (SDSS) Baryon Oscillation Spectroscopic Survey (BOSS) DR15 catalog overlap with 3,700 sq. deg. of sky observed by the Atacama Cosmology Telescope (ACT) from 2008 to 2018 at 150 and 98 GHz (ACT DR5), and 2,089 sq. deg. of internal linear combination component-separated maps combining ACT and $\it{Planck}$ data (ACT DR4). The corresponding optical depths, $\bar{\tau}$, which depend on the baryon content of the halos, are estimated using results from cosmological hydrodynamic simulations assuming an AGN feedback radiative cooling model. We estimate the mean mass of the halos in multiple luminosity bins, and compare the tSZ-based $\bar{\tau}$ estimates to theoretical predictions of the baryon content for a Navarro-Frenk-White profile. We do the same for $\bar{\tau}$ estimates extracted from fits to pairwise baryon momentum measurements of the kinematic Sunyaev-Zel'dovich effect (kSZ) for the same data set obtained in a companion paper. We find that the $\bar{\tau}$ estimates from the tSZ measurements in this work and the kSZ measurements in the companion paper agree within $1\sigma$ for two out of the three disjoint luminosity bins studied, while they differ by 2-3$\sigma$ in the highest luminosity bin. The optical depth estimates account for one third to all of the theoretically predicted baryon content in the halos across luminosity bins. Potential systematic uncertainties are discussed. The tSZ and kSZ measurements provide a step towards empirical Compton-$\bar{y}$-$\bar{\tau}$ relationships to provide new tests of cluster formation and evolution models., Comment: 19 pages, 9 figures

Published
2021
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248. In situ Performance of the Low Frequency Arrayfor Advanced ACTPol

Author

Li, Yaqiong, Austermann, Jason E., Beall, James A., Bruno, Sarah Marie, Choi, Steve K., Cothard, Nicholas F., Crowley, Kevin T., Duff, Shannon M., Ho, Shuay-Pwu Patty, Golec, Joseph E., Hilton, Gene C., Hasselfield, Matthew, Hubmay, Johannes, Koopman, Brian J., Lungu, Marius, McMahon, Jeff, Niemack, Michael D., Page, LymanA., Salatino, Maria, Simon, Sara M., Staggs, Suzanne T., Stevens, Jason R., Ullom, Joel N., Vavagiakis, Eve M., Wang, Yuhan, Wollack, Edward J., and Xu, Zhilei

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Advanced Atacama Cosmology Telescope Polarimeter (AdvACT) \cite{thornton} is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarization anisotropies in multiple frequencies. The low frequency (LF) array was deployed early 2020. It consists of 292 TES bolometers observing in two bands centered at 27 GHz and 39 GHz. At these frequencies, it is sensitive to synchrotron radiation from our galaxy as well as to the CMB, and complements the AdvACT arrays operating at 90, 150 and 230 GHz. We present the initial LF array on-site characterization, including the time constant, optical efficiency and array sensitivity.

Published
2021
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