Zobrazeno 1 - 10
of 2 523
pro vyhledávání: '"D. Heath"'
Autor:
Driver, Simon P., Bellstedt, Sabine, Robotham, Aaron S. G., Baldry, Ivan K., Davies, Luke J., Liske, Jochen, Obreschkow, Danail, Taylor, Edward N., Wright, Angus H., Alpaslan, Mehmet, Bamford, Steven P., Bauer, Amanda E., Bland-Hawthorn, Joss, Bilicki, Maciej, Bravo, Matias, Brough, Sarah, Casura, Sarah, Cluver, Michelle E., Colless, Matthew, Conselice, Christopher J., Croom, Scott M., de Jong, Jelte, D'Eugenio, Franceso, De Propris, Roberto, Dogruel, Burak, Drinkwater, Michael J., Dvornik, Andrej, Farrow, Daniel J., Frenk, Carlos S., Giblin, Benjamin, Graham, Alister W., Grootes, Meiert W., Gunawardhana, Madusha L. P., Hashemizadeh, Abdolhosein, Haussler, Boris, Heymans, Catherine, Hildebrandt, Hendrik, Holwerda, Benne W., Hopkins, Andrew M., Jarrett, Tom H., Jones, D. Heath, Kelvin, Lee S., Koushan, Soheil, Kuijken, Konrad, Lara-Lopez, Maritza A., Lange, Rebecca, Lopez-Sanchez, Angel R., Loveday, Jon, Mahajan, Smriti, Meyer, Martin, Moffett, Amanda J., Napolitano, Nicola R., Norberg, Peder, Owers, Matt S., Radovich, Mario, Raouf, Mojtaba, Peacock, John A., Phillipps, Steven, Pimbblet, Kevin A., Popescu, Cristina, Said, Khaled, Sansom, Anne E., Seibert, Mark, Sutherland, Will J., Thorne, Jessica E., Tuffs, Richard J., Turner, Ryan, van der Wel, Arjen, van Kampen, Eelco, Wilkins, Steve M.
In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earlier surveys, results in 330542 redshifts across five sky regions coveri
Externí odkaz:
http://arxiv.org/abs/2203.08539
Autor:
de Diego, José A., Nadolny, Jakub, Bongiovanni, Ángel, Cepa, Jordi, Pović, Mirjana, García, Ana María Pérez, Torres, Carmen P. Padilla, Lara-López, Maritza A., Cerviño, Miguel, Martínez, Ricardo Pérez, Alfaro, Emilio J., Castañeda, Héctor O., Fernández-Lorenzo, Miriam, Gallego, Jesús, González, J. Jesús, González-Serrano, J. Ignacio, Pintos-Castro, Irene, Sánchez-Portal, Miguel, Cedrés, Bernab, González-Otero, Mauro, Jones, D. Heath, Bland-Hawthorn, Joss
Publikováno v:
A&A 638, A134 (2020)
Context. The accurate classification of hundreds of thousands of galaxies observed in modern deep surveys is imperative if we want to understand the universe and its evolution. Aims. Here, we report the use of machine learning techniques to classify
Externí odkaz:
http://arxiv.org/abs/2005.07228
Autor:
Bongiovanni, Ángel, Ramón-Pérez, Marina, García, Ana María Pérez, Cerviño, Miguel, Cepa, Jordi, Nadolny, Jakub, Martínez, Ricardo Pérez, Alfaro, Emilio J., Castañeda, Héctor, Cedrés, Bernabé, de Diego, José A., Ederoclite, Alessandro, Fernández-Lorenzo, Mirian, Gallego, Jesús, González, J. Jesús, González-Serrano, J. Ignacio, Lara-López, Maritza A., Gómez, Iván Oteo, Torres, Carmen P. Padilla, Pintos-Castro, Irene, Pović, Mirjana, Sánchez-Portal, Miguel, Jones, D. Heath, Bland-Hawthorn, Joss, Cabrera-Lavers, Antonio
Publikováno v:
A&A 637, C2 (2020)
The OTELO survey is a very deep, blind exploration of a selected region of the Extended Groth Strip and is designed for finding emission-line sources (ELSs). The survey design, observations, data reduction, astrometry, and photometry, as well as the
Externí odkaz:
http://arxiv.org/abs/2002.08978
Autor:
Bongiovanni, Ángel, Ramón-Pérez, Marina, García, Ana Mará Pérez, Cepa, Jordi, Cerviño, Miguel, Nadolny, Jakub, Martínez, Ricardo Pérez, Navarro, Emilio J. Alfaro, Castañeda, Héctor O., de Diego, José Antonio, Ederoclite, Alessandro, Fernández-Lorenzo, Mirian, Gallego, Jesús, González, J. Jesús, González-Serrano, J. Ignacio, Lara-López, Maritza A., Gómez, Iván Oteo, Torres, Carmen P. Padilla, Pintos-Castro, Irene, Pović, Mirjana, Sánchez-Portal, Miguel, Jones, D. Heath, Bland-Hawthorn, Joss, Cabrera-Lavers, Antonio
Publikováno v:
A&A, 631A (2019), 9B
The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The OTELO survey aims to provide the deepest narrow-band survey to date in terms of minimum detectable flux and emission line equivalent width
Externí odkaz:
http://arxiv.org/abs/2001.11519
2MTF - VII. 2MASS Tully-Fisher survey final data release: distances for 2,062 nearby spiral galaxies
Autor:
Hong, Tao, Staveley-Smith, Lister, Masters, Karen L., Springob, Christopher M., Macri, Lucas M., Koribalski, Barbel S., Jones, D. Heath, Jarrett, Tom H., Crook, Aidan C., Howlett, Cullan, Qin, Fei
We present the final distance measurements for the 2MASS Tully-Fisher (2MTF) survey. The final 2MTF catalogue contains 2,062 nearby spiral galaxies in the CMB frame velocity range of 600 km s$^{-1}$ $< cz < 10,000$ km s$^{-1}$ with a mean velocity of
Externí odkaz:
http://arxiv.org/abs/1905.08530
Autor:
Green, Andrew W., Croom, Scott M., Scott, Nicholas, Cortese, Luca, Medling, Anne M., D'Eugenio, Francesco, Bryant, Julia J., Bland-Hawthorn, Joss, Allen, J. T., Sharp, Rob, Ho, I-Ting, Groves, Brent, Drinkwater, Michael J., Mannering, Elizabeth, Harischandra, Lloyd, van de Sande, Jesse, Thomas, Adam D., O'Toole, Simon, McDermid, Richard M., Vuong, Minh, Sealey, Katrina, Bauer, Amanda E., Brough, S., Catinella, Barbara, Cecil, Gerald, Colless, Matthew, Couch, Warrick J., Driver, Simon P., Federrath, Christoph, Foster, Caroline, Goodwin, Michael, Hampton, Elise J., Hopkins, A. M., Jones, D. Heath, Konstantopoulos, Iraklis S., Lawrence, J. S., Leon-Saval, Sergio G., Liske, Jochen, Lopez-Sanchez, Angel R., Lorente, Nuria P. F., Mould, Jeremy, Obreschkow, Danail, Owers, Matt S., Richards, Samuel N., Robotham, Aaron S. G., Schaefer, Adam L., Sweet, Sarah M., Taranu, Dan S., Tescari, Edoardo, Tonini, Chiara, Zafar, T.
We present the first major release of data from the SAMI Galaxy Survey. This data release focuses on the emission-line physics of galaxies. Data Release One includes data for 772 galaxies, about 20% of the full survey. Galaxies included have the reds
Externí odkaz:
http://arxiv.org/abs/1707.08402
Autor:
Howlett, Cullan, Staveley-Smith, Lister, Elahi, Pascal J., Hong, Tao, Jarrett, Tom H., Jones, D. Heath, Koribalski, Bärbel S., Macri, Lucas M., Masters, Karen L., Springob, Christopher M.
We present measurements of the velocity power spectrum and constraints on the growth rate of structure $f\sigma_{8}$, at redshift zero, using the peculiar motions of 2,062 galaxies in the completed 2MASS Tully-Fisher survey (2MTF). To accomplish this
Externí odkaz:
http://arxiv.org/abs/1706.05130
Autor:
da Cunha, Elisabete, Hopkins, Andrew M., Colless, Matthew, Taylor, Edward N., Blake, Chris, Howlett, Cullan, Magoulas, Christina, Lucey, John R., Lagos, Claudia, Kuehn, Kyler, Gordon, Yjan, Barat, Dilyar, Bian, Fuyan, Wolf, Christian, Cowley, Michael J., White, Marc, Achitouv, Ixandra, Bilicki, Maciej, Bland-Hawthorn, Joss, Bolejko, Krzysztof, Brown, Michael J. I., Brown, Rebecca, Bryant, Julia, Croom, Scott, Davis, Tamara M., Driver, Simon P., Filipovic, Miroslav D., Hinton, Samuel R., Johnston-Hollitt, Melanie, Jones, D. Heath, Koribalski, Baerbel, Kleiner, Dane, Lawrence, Jon, Lorente, Nuria, Mould, Jeremy, Owers, Matt S., Pimbblet, Kevin, Tinney, C. G., Tothill, Nicholas F. H., Watson, Fred
Publikováno v:
2017PASA...34...47D
Taipan is a multi-object spectroscopic galaxy survey starting in 2017 that will cover 2pi steradians over the southern sky, and obtain optical spectra for about two million galaxies out to z<0.4. Taipan will use the newly-refurbished 1.2m UK Schmidt
Externí odkaz:
http://arxiv.org/abs/1706.01246
We examine the HI-to-stellar mass ratio (HI fraction) for galaxies near filament backbones within the nearby Universe ($d <$ 181 Mpc). This work uses the 6 degree Field Galaxy Survey and the Discrete Persistent Structures Extractor to define the fila
Externí odkaz:
http://arxiv.org/abs/1701.03467
Autor:
van de Sande, Jesse, Bland-Hawthorn, Joss, Fogarty, Lisa M. R., Cortese, Luca, d'Eugenio, Francesco, Croom, Scott M., Scott, Nicholas, Allen, James T., Brough, Sarah, Bryant, Julia J., Cecil, Gerald, Colless, Matthew, Couch, Warrick J., Davies, Roger, Elahi, Pascal J., Foster, Caroline, Goldstein, Greg, Goodwin, Michael, Groves, Brent, Ho, I-Ting, Jeong, Hyunjin, Jones, D. Heath, Konstantopoulos, Iraklis S., Lawrence, Jon S., Leslie, Sarah K., Lopez-Sanchez, Angel R., McDermid, Richard M., McElroy, Rebecca, Medling, Anne M., Oh, Sree, Owers, Matt S., Richards, Samuel N., Schaefer, Adam L., Sharp, Rob, Sweet, Sarah M., Taranu, Dan, Tonini, Chiara, Walcher, C. Jakob, Yi, Sukyoung K.
Recent cosmological hydrodynamical simulations suggest that integral field spectroscopy can connect the high-order stellar kinematic moments h3 (~skewness) and h4 (~kurtosis) in galaxies to their cosmological assembly history. Here, we assess these r
Externí odkaz:
http://arxiv.org/abs/1611.07039