Discovery of giant radio sources from TGSS ADR 1: radio, optical, and infrared properties

Autor: Bhukta, Netai, Manik, Souvik, Pal, Sabyasachi, Mondal, Sushanta K.

Giant radio sources (GRSs) are the single largest astrophysical objects known in the universe that have grown to megaparsec scales ($\ge$ 0.7 Mpc). GRSs are much rarer compared with normal-sized radio galaxies. Still, the reason for the formation of

Externí odkaz: http://arxiv.org/abs/2201.12353

Tailed Radio Galaxies from the TIFR GMRT Sky Survey

Autor: Bhukta, Netai, Mondal, Sushanta K., Pal, Sabyasachi

Publikováno v: Monthly Notices of the Royal Astronomical Society, 2022, 516 (1), 372-390

We present a list of candidate tailed radio galaxies using the TIFR GMRT Sky Survey Alternative Data Release 1 (TGSS ADR1) at 150 MHz. We have visually examined 5336 image fields and found 264 candidates for the tailed galaxy. Tailed radio galaxies a

Externí odkaz: http://arxiv.org/abs/2110.05484

Comparison of $pp$ and $p \bar{p}$ differential elastic cross sections and observation of the exchange of a colorless $C$-odd gluonic compound

Autor: Abazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Alves, G. A., Antchev, G., Askew, A., Aspell, P., Jesus, A. C. S. Assis, Atanassov, I., Atkins, S., Augsten, K., Aushev, V., Aushev, Y., Avati, V., Avila, C., Badaud, F., Baechler, J., Bagby, L., Barrera, C. Baldenegro, Baldin, B., Bandurin, D. V., Banerjee, S., Barberis, E., Baringer, P., Barreto, J., Bartlett, J. F., Bassler, U., Bazterra, V., Bean, A., Begalli, M., Bellantoni, L., Berardi, V., Beri, S. B., Bernardi, G., Bernhard, R., Berretti, M., Bertram, I., Besanccon, M., Beuselinck, R., Bhat, P. C., Bhatia, S., Bhatnagar, V., Blazey, G., Blessing, S., Bloom, K., Boehnlein, A., Boline, D., Boos, E. E., Borchsh, V., Borissov, G., Borysova, M., Bossini, E., Bottigli, U., Bozzo, M., Brandt, A., Brandt, O., Brochmann, M., Brock, R., Bross, A., Brown, D., Bu, X. B., Buehler, M., Buescher, V., Bunichev, V., Burdin, S., Burkhardt, H., Buszello, C. P., Cafagna, F. S., Camacho-P'erez, E., Carvahlo, W., Casey, B. C. K., Castilla-Valdez, H., Catanesi, M. G., Caughron, S., Chakrabarti, S., Chan, K. M., Chandra, A., Chapon, E., Chen, G., Cho, S. W., Choi, S., Choudhary, B., Cihangir, S., Claes, D., Clutter, J., Cooke, M., Cooper, W. E., Corcoran, M., Couderc, F., Cousinou, M. -C., Csan'ad, M., Cs"orgHo, T., Cuth, J., Cutts, D., Das, A., Davies, G., Deile, M., de Jong, S. J., De La Cruz-Burelo, E., De Leonardis, F., D'eliot, F., Demina, R., Denisov, D., Denisov, S. P., Desai, S., Deterre, C., DeVaughan, K., Diehl, H. T., Diesburg, M., Ding, P. F., Dominguez, A., Doubek, M., Drutskoy, A., Druzhkin, D., Dubey, A., Dudko, L. V., Duperrin, A., Dutt, S., Eads, M., Edmunds, D., Eggert, K., Ellison, J., Elvira, V. D., Enari, Y., Eremin, V., Evans, H., Evdokimov, A., Evdokimov, V. N., Faur'e, A., Feng, L., Ferbel, T., Ferro, F., Fiedler, F., Fiergolski, A., Filthaut, F., Fisher, W., Fisk, H. E., Forthomme, L., Fortner, M., Fox, H., Franc, J., Fuess, S., Garbincius, P. H., Garcia, F., Garcia-Bellido, A., Garc'ia-Gonz'alez, J. A., Gavrilov, V., Geng, W., Georgiev, V., Gerber, C. E., Gershtein, Y., Giani, S., Ginther, G., Gogota, O., Golovanov, G., Grannis, P. D., Greder, S., Greenlee, H., Grenier, G., Gris, Ph., Grivaz, J. -F., Grohsjean, A., Gr"unendahl, S., Gr"unewald, M. W., Grzanka, L., Guillemin, T., Gutierrez, G., Gutierrez, P., Haley, J., Hammerbauer, J., Han, L., Harder, K., Harel, A., Hauptman, J. M., Hays, J., Head, T., Hebbeker, T., Hedin, D., Hegab, H., Heinson, A. P., Heintz, U., Hensel, C., La Cruz, I. Heredia-De, Herner, K., Hesketh, G., Hildreth, M. D., Hirosky, R., Hoang, T., Hobbs, J. D., Hoeneisen, B., Hogan, J., Hohlfeld, M., Holzbauer, J. L., Howley, I., Hubacek, Z., Hynek, V., Iashvili, I., Ilchenko, Y., Illingworth, R., Isidori, T., Ito, A. S., Ivanchenko, V., Jabeen, S., Jaffr'e, M., Janda, M., Jayasinghe, A., Jeong, M. S., Jesik, R., Jiang, P., Johns, K., Johnson, E., Johnson, M., Jonckheere, A., Jonsson, P., Joshi, J., Jung, A. W., Juste, A., Kajfasz, E., Karev, A., Karmanov, D., Kavspar, J., Katsanos, I., Kaur, M., Kaynak, B., Kehoe, R., Kermiche, S., Khalatyan, N., Khanov, A., Kharchilava, A., Kharzheev, Y. N., Kiselevich, I., Kohli, J. M., Kopal, J., Kozelov, A. V., Kraus, J., Kumar, A., Kundr'at, V., Kupco, A., Kurvca, T., Kuzmin, V. A., Lami, S., Lammers, S., Latino, G., Lebrun, P., Lee, H. S., Lee, S. W., Lee, W. M., Le, X., Lellouch, J., Li, D., Li, H., Li, L., Li, Q. Z., Lim, J. K., Lincoln, D., Lindsey, C., Linhart, R., Linnemann, J., Lipaev, V. V., Lipton, R., Liu, H., Liu, Y., Lobodenko, A., Lokajicek, M., Lokaj'ivcek, M. V., de Sa, R. Lopes, Losurdo, L., Rodr'iguez, F. Lucas, Luna-Garcia, R., Lyon, A. L., Maciel, A. K. A., Macr'i, M., Madar, R., na-Villalba, R. Maga, Malawski, M., Malbouisson, H. B., Malik, S., Malyshev, V. L., Mansour, J., Mart'inez-Ortega, J., McCarthy, R., McGivern, C. L., Meijer, M. M., Melnitchouk, A., Menezes, D., Mercadante, P. G., Merkin, M., Meyer, A., Meyer, J., Miconi, F., Minafra, N., Minutoli, S., Molina, J., Mondal, N. K., Da Motta, H., Mulhearn, M., Mundim, L., Naaranoja, T., Nagy, E., Narain, M., Nayyar, R., Neal, H. A., Negret, J. P., Nemes, F., Neustroev, P., Nguyen, H. T., Niewiadomski, H., Nov'ak, T., Nunnemann, T., Oguri, V., Oliveri, E., Oljemark, F., Orduna, J., Oriunno, M., Osman, N., "Osterberg, K., Pal, A., Palazzi, P., Parashar, N., Parihar, V., Park, S. K., Partridge, R., Parua, N., Pasechnik, R., Passaro, V., Patwa, A., Penning, B., Perfilov, M., Peroutka, Z., Peters, Y., Petridis, K., Petrillo, G., P'etroff, P., Pleier, M. -A., Podstavkov, V. M., Popov, A. V., Da Silva, W. L. Prado, Prewitt, M., Price, D., Proch'azka, J., Prokopenko, N., Qian, J., Quadt, A., Quinn, B., Quinto, M., Raben, T. G., Radermacher, E., Rangel, M., Radicioni, E., Ratoff, P. N., Ravotti, F., Razumov, I., Ripp-Baudot, I., Rizatdinova, F., Robutti, E., Rodrigues, R. F., Rominsky, M., Ross, A., Royon, C., Rubinov, P., Ruchti, R., Ruggiero, G., Saarikko, H., Sajot, G., Samoylenko, V. D., S'anchez-Hern'andez, A., Sanders, M. P., Santoro, A., Santos, A. S., Savage, G., Savitskyi, M., Sawyer, L., Scanlon, T., Schamberger, R. D., Scheglov, Y., Schellman, H., Schott, M., Schwanenberger, C., Schwienhorst, R., Scribano, A., Sekaric, J., Severini, H., Shabalina, E., Shary, V., Shaw, S., Shchukin, A. A., Shkola, O., Simak, V., Siroky, J., Skubic, P., Slattery, P., Smajek, J., Snoeys, W., Snow, G. R., Snow, J., Snyder, S., S"oldner-Rembold, S., Sonnenschein, L., Soustruznik, K., Stark, J., Stefaniuk, N., Stefanovitch, R., Ster, A., Stoyanova, D. A., Strauss, M., Suter, L., Svoisky, P., Szanyi, I., Sziklai, J., Taylor, C., Tcherniaev, E., Titov, M., Tokmenin, V. V., Tsai, Y. -T., Tsybychev, D., Tuchming, B., Tully, C., Turini, N., Urban, O., Uvarov, L., Uvarov, S., Uzunyan, S., Vacek, V., Van Kooten, R., van Leeuwen, W. M., Varelas, N., Varnes, E. W., Vasilyev, I. A., Vavroch, O., Verkheev, A. Y., Vertogradov, L. S., Verzocchi, M., Vesterinen, M., Vilanova, D., Vokac, P., Wahl, H. D., Wang, C., Wang, M. H. L. S., Warchol, J., Watts, G., Wayne, M., Weichert, J., Welti, J., Welty-Rieger, L., Williams, J., Williams, M. R. J., Wilson, G. W., Wobisch, M., Wood, D. R., Wyatt, T. R., Xie, Y., Yamada, R., Yang, S., Yasuda, T., Yatsunenko, Y. A., Ye, W., Ye, Z., Yin, H., Yip, K., Youn, S. W., Yu, J. M., Zennamo, J., Zhao, T. G., Zhou, B., Zhu, J., Zich, J., Zielinski, K., Zielinski, M., Zieminska, D., Zivkovic, L.

Publikováno v: Phys. Rev. Lett. 127, 062003 (2021)

We describe an analysis comparing the $p\bar{p}$ elastic cross section as measured by the D0 Collaboration at a center-of-mass energy of 1.96 TeV to that in $pp$ collisions as measured by the TOTEM Collaboration at 2.76, 7, 8, and 13 TeV using a mode

Externí odkaz: http://arxiv.org/abs/2012.03981

Search for X/Z-shaped radio sources from TGSS ADR 1

Autor: Bhukta, Netai, Pal, Sabyasachi, Mondal, Sushanta K.

Publikováno v: Monthly Notices of the Royal Astronomical Society, Volume 512, Issue 3, May 2022, Pages 4308-4323

A small sub-class of radio galaxies that exhibit a pair of secondary low surface brightness radio lobes oriented at an angle to the primary high surface brightness lobes are known as X-shaped radio galaxies (XRGs). In cases, it is seen that the less

Externí odkaz: http://arxiv.org/abs/2006.07219

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