Results 81 to 90 of about 57,270 (311)
The BINGO project
Astronomy & AstrophysicsContext. Building on the transformative success of optical redshift surveys, the emerging technique of neutral hydrogen (HI) intensity mapping (IM) offers a novel probe of large-scale structure (LSS) growth and the late-time accelerated expansion of the ...Motta Pablo, Abdalla Filipe B., Novaes Camila P., Abdalla Elcio, Zhang Jiajun, Hoerning Gabriel A., Marins Alessandro, de Mericia Eduardo J., Ponte Luiza O., Queiroz Amilcar R., Villela Thyrso, Wang Bin, Wuensche Carlos A., Feng Chang, Gurjão Edmar C. +14 moredoaj +1 more sourceRNA‐Binding Proteins Shape Mammalian Retroelement RNA Fate: Lessons From HIV‐1, LINE‐1, and Related Reverse‐Transcribing Elements
Animal Research and One Health, EarlyView.RNA‐binding proteins (RBPs) and RNA‐associated factors shape retroelement RNA fate by regulating RNA processing, translation, RNP assembly and remodeling, reverse transcription, nuclear trafficking, chromatin engagement, and RNA surveillance. These pathways balance productive retroviral replication or retrotransposon insertion with RNA decay ...Mingrui Li, Zhangyuan Pan, Yongjuan Guanwiley +1 more source9. The next telescopes
, 2016 Each question that telescopes have helped answer has led to new questions: what is dark matter and dark energy? How did the first galaxies form? Are there habitable, Earth-like exoplanets?Geoff Cottrellcore +1 more sourcePrincipal Component‐Based Classification of Blazar Candidates of Uncertain Type in the 4FGL/LAT
Astronomische Nachrichten, EarlyView.ABSTRACT
We adopted principal component analysis (PCA), linear discriminant analysis (LDA), and support vector machines (SVM), to study classification for a sample of 2708 Fermi blazars: 1142 BL Lac objects (BLLs), 759 flat spectrum radio quasars (FSRQs), and 807 blazar candidates of uncertain type (BCUs).Wen‐Xin Yang, Guo‐Hai Chen, Jing‐Tian Zhu, Hong‐Guang Wang, Denis Bastieri, Xu‐Hong Ye, Jing‐Chao Liang, De‐Xiang Wu, Jiang‐He Yang, Anton A. Strigachev, Rumen S. Bachev, Jun‐Jie Feng, Yi Liu, Jun‐Hui Fan +13 morewiley +1 more sourceThe Effelsberg Direct Digitisation radio astronomy back-end framework
Astronomy & AstrophysicsContext. Modern digital radio astronomy receivers produce increasingly wide-bandwidth, high bit-rate data streams that necessitate the development of flexible, scalable, and maintainable back-end processing and recording systems.Barr Ewan D., Bansod Amit, Behrend Jan, Chen Weiwei, Esser Niclas, Men Yungpen, Winchen Tobias, Wu Jason, Bach Uwe, Connot Claus, Heininger Matthias, Jawor Jedrzej, Kasemann Christoph, Kramer Michael, Kraus Alex, Nussbaum Eddy, Polch Oliver, Wagner Jan, Wieching Gundolf +18 moredoaj +1 more sourceOverview of the medium and high frequency telescopes of the LiteBIRD space mission [PDF]
, 2020 LiteBIRD is a JAXA-led Strategic Large-Class mission designed to search for the existence of the primordial gravitational waves produced during the inflationary phase of the Universe, through the measurements of their imprint onto the polarization of the Raum C., Winter B., Ichiki K., Nakamura S., Terao Y., Borrill J., Wilms J., Sekimoto Y., Allys E., Diego-Palazuelos P., Franceschet C., Ishino H., Nagasaki T., Hilton G., Jaehnig G., Cheung K., Ganga K., Piacentini F., Cubas J., Komatsu K., Remazeilles M., Hirota Y., Namikawa T., Montier L., Takeda Y., Fuskeland U., Shirron P., Russell M., Yamasaki N. Y., Banerji R., Maffei B., Arnold K., Savini G., Matsumura T., O'sullivan C., Pagano L., Pisano G., Sasaki M., Ullom J., Realini S., Kohri K., Tomasi M., Casas F. J., Sherwin B., Masi S., Oguri S., Sugai H., Cukierman A., Dachlythra N., Yoshida T., Keskitalo R., Challinor A., Rambaud D., Scott D., Murphy J. A., Paoletti D., Gjerlow E., Seibert J., Peloton J., Maino D., Vermeulen G., Yumoto J., Grain J., Nagano Y., Aumont J., Brown M., Columbro F., Minami Y., Takakura S., Dobbs M., Flauger R., Levrier F., Gao J. R., Hubmayr J., Reinecke M., Maki M., Thorne B., Maciaszek T., Signorelli G., Kogut A., Zonca A., Duband L., Villa F., Beall J., De Petris M., Errard J., Essinger-Hileman T., Ritacco A., Vittorio N., Tristram M., Wehus I., Tucker C., Carones A., Okada N., Hill C. A., Duval J. M., Ohta I. S., Nerval S., Ade P. A. R., Hoshino Y., Bounissou S., Kreykenbohm I., Colombo L., De Bernardis P., Roudil G., Vielva P., Ohsaki H., Komatsu E., Krachmalnicoff N., Murata Y., Mandelli S., Tsuji M., Stever S., Tominaga M., Mennella A., Wollack E. J., De La Hoz E., Svalheim T. L., Puglisi G., Halverson N. W., Ebisawa K., Herman D., Nagata R., Weller J., Stompor R., Brilenkov M., Cliche J. F., Westbrook B., Curtis D., Lattanzi M., Boulanger F., Montgomery J., Duff S., Trappe N., Gruppuso A., Dickinson C., Iida T., Sakurai H., Poletti D., Auguste D., Nagai M., Bersanelli M., Chinone Y., Luzzi G., Calabrese E., Prouve T., Sakurai Y., Kogiso N., Polenta G., Eriksen H. K., Elleflot T., De Haan T., Chan V., Morgante G., Smecher G., Hattori M., Rubino-Martin J. A., Beckman S., Bonis J., Katayama N., Louis T., Switzer E., Takakura H., Lee A. T., Adler A., Migliaccio M., Dotani T., Bermejo J., Sandri M., Ogawa H., Bucher M., Takaku R., Basak S., Shinozaki K., Hivon E., Aurlien R., Thompson K. L., Kaga T., Suzuki A., Ishimura K., Tsujimoto M., Toda T., Austermann J., Patanchon G., Suzuki J., Genova-Santos R., Vissers M., Ghigna T., Hlozek R. A., Nishibori T., Gerbino M., Kato A., Natoli P., Herranz D., Imada H., Mitsuda K., Hargrave P., Banday A. J., Paiella A., Campeti P., Konishi K., Linder E., Mot B., Taylor E., Finelli F., Kuo C. L., Tartari A., Kisner T., Gradziel M. L., Kobayashi Y., Grupp F., Gervasi M., Leloup C., Nishino H., Sugiyama S., Martinez-Gonzalez E., Lamagna L., Beck D., Kushino A., Takase Y., Barreiro R. B., Baccigalupi C., Hazumi M., Henrot-Versille S., Galloway M., Thommesen H., Gudmundsson J. E., Hasebe T., Zannoni M., Hasegawa M., Kawasaki T., Shiraishi M., Kashima S., D'alessandro G., Lanen J. V. +234 morecore +1 more sourceTime-domain photometry and activity evolution of interstellar comet 3I/ATLAS with BHTOM
Astronomy & AstrophysicsContext. Time-domain photometric monitoring is essential for characterizing cometary evolution, particularly for rare interstellar objects with limited observing opportunities.
Aims.Gillan A. Fraser, Wyrzykowski Łukasz, Mikołajczyk Przemysław J., Kotysz Krzysztof, Bufanda Erica, Chandler Colin O., Fişek Süleyman, Hsieh Henry H., Kelley Michael S. P., Pessi Priscila J., Robinson James E., Aliş Sinan, Bykowski Wieńczysław, Cannon Richard E., Dominik Martin, Handzlik Barbara, İçen Mehmet, Kurowski Sebastian, Kutluay Ahmet Cem, Majumdar Joysankar, Nehir Çağlayan, O’Neill David, Ötken Sibel, Pu Kangming, Şimşir Özlem, Snodgrass Colin, Tezcan Cihan Tuğrul, Tezcan Fatma, Wicker Mauritz, Korhan Yelkenci Fuat, Żejmo Michał, Ackley Kendall, Andersen Michael, Ávalos-Vega Catalina, Belkin Sergey, Bozza Valerio, Breton Rene P., Burgdorf Martin J., Casares Jorge, Dhillon Vik, Donaldson Abbie, Dyer Martin J., Figuera Jaimes Roberto, Galloway Duncan K., Hinse Tobias C., Hundertmark Markus, Khalouei Elahe, Killestein Thomas, Kotak Rubina, Kumar Amit, Liu Feng-Yuan Frey, Longa-Peña Penelope, Lyman Joe, Mancini Luigi, Moharana Ayush, Molina Valeska, Noysena Kanthanakorn, Nuttall Laura Kate, O’Brien Paul, Okoth Vincent, Opitom Cyrielle, Pollacco Don, Rabus Markus, Ramsay Gavin, Sajadian Sedighe, Salinas San Martin A., Skottfelt Jesper, Southworth John, Steeghs Danny, Tregloan-Reed Jeremy, Ulaczyk Krzysztof, Vieliute Roberta +71 moredoaj +1 more source