Zobrazeno 1 - 10
of 1 880
pro vyhledávání: '"Mullaney P"'
Autor:
Killestein, T. L., Kelsey, L., Wickens, E., Nuttall, L., Lyman, J., Krawczyk, C., Ackley, K., Dyer, M. J., Jiménez-Ibarra, F., Ulaczyk, K., O'Neill, D., Kumar, A., Steeghs, D., Galloway, D. K., Dhillon, V. S., O'Brien, P., Ramsay, G., Noysena, K., Kotak, R., Breton, R. P., Pallé, E., Pollacco, D., Awiphan, S., Belkin, S., Chote, P., Clark, P., Coppejans, D., Duffy, C., Eyles-Ferris, R., Godson, B., Gompertz, B., Graur, O., Irawati, P., Jarvis, D., Julakanti, Y., Kennedy, M. R., Kuncarayakti, H., Levan, A., Littlefair, S., Magee, M., Mandhai, S., Sánchez, D. Mata, Mattila, S., McCormac, J., Mullaney, J., Munday, J., Patel, M., Pursiainen, M., Rana, J., Sawangwit, U., Stanway, E., Starling, R., Warwick, B., Wiersema, K.
Time-domain astrophysics continues to grow rapidly, with the inception of new surveys drastically increasing data volumes. Democratised, distributed approaches to training sets for machine learning classifiers are crucial to make the most of this tor
Externí odkaz:
http://arxiv.org/abs/2406.02334
Autor:
Sazonova, Elizaveta, Morgan, Cameron R, Balogh, Michael, Alatalo, Katherine, Benavides, Jose A., Bluck, Asa, Brough, Sarah, Busa, Innocenza, Demarco, Ricardo, Donevski, Darko, Figueira, Miguel, Martin, Garreth, Mullaney, James R, Rodriguez-Gomez, Vicente, Román, Javier, Rowlands, Kate
Structural disturbances, such as galaxy mergers or instabilities, are key candidates for driving galaxy evolution, so it is important to detect and quantify galaxies hosting these disturbances spanning a range of masses, environments, and cosmic time
Externí odkaz:
http://arxiv.org/abs/2404.05792
A key feature of active galactic nuclei (AGN) is their variability across all wavelengths. Typically, AGN vary by a few tenths of a magnitude or more over periods lasting from hours to years. By contrast, extreme variability of AGN -- large luminosit
Externí odkaz:
http://arxiv.org/abs/2403.05354
Autor:
Małek, K., Junais, Pollo, A., Boquien, M., Buat, V., Salim, S., Brough, S., Demarco, R., Graham, A. W., Hamed, M., Mullaney, J. R., Romano, M., Sifón, C., Aravena, M., Benavides, J. A., Busà, I., Donevski, D., Dorey, O., Hernandez-Toledo, H. M., Nanni, A., Pearson, W. J., Pistis, F., Ragusa, R., Riccio, G., Román, J.
Large future sky surveys, such as the LSST, will provide optical photometry for billions of objects. This paper aims to construct a proxy for the far ultraviolet attenuation (AFUVp) from the optical data alone, enabling the rapid estimation of the st
Externí odkaz:
http://arxiv.org/abs/2401.12831
Efficient energy management of Distributed Renewable Energy Resources (DRER) enables a more sustainable and efficient energy ecosystem. Therefore, we propose a holistic Energy Management System (EMS), utilising the computational and energy storage ca
Externí odkaz:
http://arxiv.org/abs/2312.00587
Autor:
Molyneux, S. J., Rivera, G. Calistro, De Breuck, C., Harrison, C. M., Mainieri, V., Lundgren, A., Kakkad, D., Circosta, C., Girdhar, A., Costa, T., Mullaney, J. R., Kharb, P., Battaia, F. Arrigoni, Farina, E. P., Alexander, D. M., Ward, S. R., S., Silpa, Smit, R.
We present a comprehensive study of the molecular gas properties of 17 Type 2 quasars at $z <$ 0.2 from the Quasar Feedback Survey (L$_{[OIII]}$ > $10^{42.1}$ $\rm ergs^{-1}$), selected by their high [OIII] luminosities and displaying a large diversi
Externí odkaz:
http://arxiv.org/abs/2310.10235
Peer-to-Peer (P2P) energy trading provides various benefits over conventional wholesale energy markets and makes renewable energy more accessible. This paper proposes a novel multi-layer P2P energy trading system for microgrids based on IOTA 2.0, whi
Externí odkaz:
http://arxiv.org/abs/2210.06427
Autor:
Xiao, Mengyuan, Elbaz, David, Gómez-Guijarro, Carlos, Leroy, Lucas, Bing, Longji, Daddi, Emanuele, Magnelli, Benjamin, Franco, Maximilien, Zhou, Luwenjia, Dickinson, Mark, Wang, Tao, Rujopakarn, Wiphu, Magdis, Georgios E., Treister, Ezequiel, Inami, Hanae, Demarco, Ricardo, Sargent, Mark T., Shu, Xinwen, Kartaltepe, Jeyhan S., Alexander, David M., Béthermin, Matthieu, Bournaud, Frederic, Ciesla, Laure, Ferguson, Henry C., Finkelstein, Steven L., Giavalisco, Mauro, Gu, Qiusheng, Iono, Daisuke, Juneau, Stephanie, Lagache, Guilaine, Leiton, Roger, Messias, Hugo, Motohara, Kentaro, Mullaney, James, Nagar, Neil, Pannella, Maurilio, Papovich, Casey, Pope, Alexandra, Schreiber, Corentin, Silverman, John
Publikováno v:
A&A 672, A18 (2023)
Our current understanding of the cosmic star formation history at z>3 is primarily based on UV-selected galaxies (i.e., LBGs). Recent studies of H-dropouts have revealed that we may be missing a large proportion of star formation that is taking place
Externí odkaz:
http://arxiv.org/abs/2210.03135
Autor:
Delvecchio, I., Daddi, E., Sargent, M. T., Aird, J., Mullaney, J. R., Magnelli, B., Elbaz, D., Bisigello, L., Ceraj, L., Jin, S., Kalita, B. S., Liu, D., Novak, M., Prandoni, I., Radcliffe, J. F., Spingola, C., Zamorani, G., Allevato, V., Rodighiero, G., Smolcic, V.
Publikováno v:
A&A 668, A81 (2022)
Mapping the average AGN luminosity across galaxy populations and over time encapsulates important clues on the interplay between supermassive black hole (SMBH) and galaxy growth. This paper presents the demography, mean power and cosmic evolution of
Externí odkaz:
http://arxiv.org/abs/2209.12585
Autor:
Mong, Y. -L., Ackley, K., Killestein, T. L., Galloway, D. K., Dyer, M., Cutter, R., Brown, M. J. I., Lyman, J., Ulaczyk, K., Steeghs, D., Dhillon, V., O'Brien, P., Ramsay, G., Noysena, K., Kotak, R., Breton, R., Nuttall, L., Palle, E., Pollacco, D., Thrane, E., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B. P., Heikkila, T., Irawati, P., Kennedy, M., Levan, A., Littlefair, S., Makrygianni, L., Marsh, T., Sanchez, D. Mata, Mattila, S., Maund, J. R., McCormac, J., Mkrtichian, D., Mullaney, J., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strom, P., Tooke, S., Wiersema, K.
Developing an effective automatic classifier to separate genuine sources from artifacts is essential for transient follow-ups in wide-field optical surveys. The identification of transient detections from the subtraction artifacts after the image dif
Externí odkaz:
http://arxiv.org/abs/2209.06375