Search Results - "Driver, Simon"

MEASUREMENTS OF EXTRAGALACTIC BACKGROUND LIGHT FROM THE FAR UV TO THE FAR IR FROM DEEP GROUND- AND SPACE-BASED GALAXY COUNTS by Driver, Simon P., Andrews, Stephen K., Davies, Luke J., Robotham, Aaron S. G., Wright, Angus H., Windhorst, Rogier A., Cohen, Seth, Emig, Kim, Jansen, Rolf A., Dunne, Loretta

“…ABSTRACT We combine wide and deep galaxy number-count data from the Galaxy And Mass Assembly, COSMOS/G10, Hubble Space Telescope (HST) Early Release Science,…”
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Deep Extragalactic VIsible Legacy Survey (DEVILS): SED fitting in the D10-COSMOS field and the evolution of the stellar mass function and SFR–M⋆ relation by Thorne, Jessica E, Robotham, Aaron S G, Davies, Luke J M, Bellstedt, Sabine, Driver, Simon P, Bravo, Matías, Bremer, Malcolm N, Holwerda, Benne W, Hopkins, Andrew M, Lagos, Claudia del P, Phillipps, Steven, Siudek, Malgorzata, Taylor, Edward N, Wright, Angus H

“…ABSTRACT We present catalogues of stellar masses, star formation rates (SFRs), and ancillary stellar population parameters for galaxies spanning 0 < z < 9 from…”
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From the far-ultraviolet to the far-infrared – galaxy emission at 0 ≤ z ≤ 10 in the shark semi-analytic model by Lagos, Claudia del P, Robotham, Aaron S G, Trayford, James W, Tobar, Rodrigo, Bravo, Matías, Bellstedt, Sabine, Davies, Luke J M, Driver, Simon P, Elahi, Pascal J, Obreschkow, Danail, Power, Chris

“…ABSTRACT We combine the shark semi-analytic model of galaxy formation with the prospect software tool for spectral energy distribution (SED) generation to…”
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The need for speed: escape velocity and dynamical mass measurements of the Andromeda galaxy by Kafle, Prajwal R, Sharma, Sanjib, Lewis, Geraint F, Robotham, Aaron S G, Driver, Simon P

“…Abstract Our nearest large cosmological neighbour, the Andromeda galaxy (M31), is a dynamical system, and an accurate measurement of its total mass is central…”
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GAMA/G10-COSMOS/3D-HST: the 0 < z < 5 cosmic star formation history, stellar-mass, and dust-mass densities by Driver, Simon P, Andrews, Stephen K, da Cunha, Elisabete, Davies, Luke J, Lagos, Claudia, Robotham, Aaron S G, Vinsen, Kevin, Wright, Angus H, Alpaslan, Mehmet, Bland-Hawthorn, Joss, Bourne, Nathan, Brough, Sarah, Bremer, Malcolm N, Cluver, Michelle, Colless, Matthew, Conselice, Christopher J, Dunne, Loretta, Eales, Steve A, Gomez, Haley, Holwerda, Benne, Hopkins, Andrew M, Kafle, Prajwal R, Kelvin, Lee S, Loveday, Jon, Liske, Jochen, Maddox, Steve J, Phillipps, Steven, Pimbblet, Kevin, Rowlands, Kate, Sansom, Anne E, Taylor, Edward, Wang, Lingyu, Wilkins, Stephen M

“…Abstract We use the energy-balance code magphys to determine stellar and dust masses, and dust corrected star formation rates for over 200 000 GAMA galaxies,…”
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Galaxy and mass assembly (GAMA): the inferred mass–metallicity relation from z = 0 to 3.5 via forensic SED fitting by Bellstedt, Sabine, Robotham, Aaron S G, Driver, Simon P, Thorne, Jessica E, Davies, Luke J M, Holwerda, Benne W, Hopkins, Andrew M, Lara-Lopez, Maritza A, López-Sánchez, Ángel R, Phillipps, Steven

“…ABSTRACT We analyse the metallicity histories of ∼4500 galaxies from the GAMA survey at z < 0.06 modelled by the SED-fitting code ProSpect using an evolving…”
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Galaxy And Mass Assembly (GAMA): a forensic SED reconstruction of the cosmic star formation history and metallicity evolution by galaxy type by Bellstedt, Sabine, Robotham, Aaron S G, Driver, Simon P, Thorne, Jessica E, Davies, Luke J M, Lagos, Claudia del P, Stevens, Adam R H, Taylor, Edward N, Baldry, Ivan K, Moffett, Amanda J, Hopkins, Andrew M, Phillipps, Steven

“…ABSTRACT We apply the spectral energy distribution (SED) fitting code ProSpect to multiwavelength imaging for ∼7000 galaxies from the GAMA survey at z < 0.06,…”
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Effects of wearing a cloth face mask on performance, physiological and perceptual responses during a graded treadmill running exercise test by Driver, Simon, Reynolds, Megan, Brown, Katelyn, Vingren, Jakob L, Hill, David W, Bennett, Monica, Gilliland, Taylor, McShan, Evan, Callender, Librada, Reynolds, Erin, Borunda, Nate, Mosolf, John, Cates, Casey, Jones, Alan

“…To (1) determine if wearing a cloth face mask significantly affected exercise performance and associated physiological responses, and (2) describe perceptual…”
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Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis by Kelvin, Lee S., Driver, Simon P., Robotham, Aaron S. G., Hill, David T., Alpaslan, Mehmet, Baldry, Ivan K., Bamford, Steven P., Bland-Hawthorn, Joss, Brough, Sarah, Graham, Alister W., Häussler, Boris, Hopkins, Andrew M., Liske, Jochen, Loveday, Jon, Norberg, Peder, Phillipps, Steven, Popescu, Cristina C., Prescott, Matthew, Taylor, Edward N., Tuffs, Richard J.

“…We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital…”
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Quantifying cosmic variance by Driver, Simon P., Robotham, Aaron S. G.

“…We determine an expression for the cosmic variance of any ‘normal’ galaxy survey based on examination of M*± 1 mag galaxies in the Sloan Digital Sky Survey…”
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Galaxy And Mass Assembly (GAMA): the stellar mass budget by galaxy type by Moffett, Amanda J., Ingarfield, Stephen A., Driver, Simon P., Robotham, Aaron S. G., Kelvin, Lee S., Lange, Rebecca, Meštrić, Uroš, Alpaslan, Mehmet, Baldry, Ivan K., Bland-Hawthorn, Joss, Brough, Sarah, Cluver, Michelle E., Davies, Luke J. M., Holwerda, Benne W., Hopkins, Andrew M., Kafle, Prajwal R., Kennedy, Rebecca, Norberg, Peder, Taylor, Edward N.

“…We report an expanded sample of visual morphological classifications from the Galaxy and Mass Assembly survey phase two, which now includes 7556 objects…”
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The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology-Density Relation in Clusters by Brough, Sarah, van de Sande, Jesse, Owers, Matt S., d'Eugenio, Francesco, Sharp, Rob, Cortese, Luca, Scott, Nicholas, Croom, Scott M., Bassett, Rob, Bekki, Kenji, Bland-Hawthorn, Joss, Bryant, Julia J., Davies, Roger, Drinkwater, Michael J., Driver, Simon P., Foster, Caroline, Goldstein, Gregory, López-Sánchez, Á. R., Medling, Anne M., Sweet, Sarah M., Taranu, Dan S., Tonini, Chiara, Yi, Sukyoung K., Goodwin, Michael, Lawrence, J. S., Richards, Samuel N.

“…We examine the kinematic morphology of early-type galaxies (ETGs) in eight galaxy clusters in the Sydney-AAO Multi-object Integral-field spectrograph Galaxy…”
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Galaxy And Mass Assembly (GAMA): assimilation of KiDS into the GAMA database by Bellstedt, Sabine, Driver, Simon P, Robotham, Aaron S G, Davies, Luke J M, Bogue, Cameron R J, Cook, Robin H W, Hashemizadeh, Abdolhosein, Koushan, Soheil, Taylor, Edward N, Thorne, Jessica E, Turner, Ryan J, Wright, Angus H

“…ABSTRACT The Galaxy And Mass Assembly Survey (GAMA) covers five fields with highly complete spectroscopic coverage (>95 per cent) to intermediate depths (r <…”
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EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin2 of Deep, Blank Fields from the PEARLS Survey and Public JWST Data by Adams, Nathan J., Conselice, Christopher J., Austin, Duncan, Harvey, Thomas, Ferreira, Leonardo, Trussler, James, Juodžbalis, Ignas, Li, Qiong, Windhorst, Rogier, Cohen, Seth H., Jansen, Rolf A., Summers, Jake, Tompkins, Scott, Driver, Simon P., Robotham, Aaron, D’Silva, Jordan C. J., Yan, Haojing, Coe, Dan, Frye, Brenda, Grogin, Norman A., Koekemoer, Anton M., Marshall, Madeline A., Pirzkal, Nor, Ryan, Russell E., Maksym, W. Peter, Rutkowski, Michael J., Willmer, Christopher N. A., Hammel, Heidi B., Nonino, Mario, Bhatawdekar, Rachana, Wilkins, Stephen M., Bradley, Larry D., Broadhurst, Tom, Cheng, Cheng, Dole, Hervé, Hathi, Nimish P., Zitrin, Adi

“…We present an analysis of the ultraviolet luminosity function (UV LF) and star formation rate density of distant galaxies (7.5 < z < 13.5) in the “blank”…”
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MegaMorph - multiwavelength measurement of galaxy structure: complete Sérsic profile information from modern surveys by Häußler, Boris, Bamford, Steven P., Vika, Marina, Rojas, Alex L., Barden, Marco, Kelvin, Lee S., Alpaslan, Mehmet, Robotham, Aaron S. G., Driver, Simon P., Baldry, I. K., Brough, Sarah, Hopkins, Andrew M., Liske, Jochen, Nichol, Robert C., Popescu, Cristina C., Tuffs, Richard J.

“…In this paper, we demonstrate a new method for fitting galaxy profiles which makes use of the full multiwavelength data provided by modern large…”
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Galaxy And Mass Assembly (GAMA): mass–size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology by Lange, Rebecca, Driver, Simon P., Robotham, Aaron S. G., Kelvin, Lee S., Graham, Alister W., Alpaslan, Mehmet, Andrews, Stephen K., Baldry, Ivan K., Bamford, Steven, Bland-Hawthorn, Joss, Brough, Sarah, Cluver, Michelle E., Conselice, Christopher J., Davies, Luke J. M., Haeussler, Boris, Konstantopoulos, Iraklis S., Loveday, Jon, Moffett, Amanda J., Norberg, Peder, Phillipps, Steven, Taylor, Edward N., López-Sánchez, Ángel R., Wilkins, Stephen M.

“…We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01 < z < 0.1 (8399 galaxies in g to Ks bands) to derive the stellar…”
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The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products by Scott, Nicholas, van de Sande, Jesse, Croom, Scott M, Groves, Brent, Owers, Matt S, Poetrodjojo, Henry, D’Eugenio, Francesco, Medling, Anne M, Barat, Dilyar, Barone, Tania M, Bland-Hawthorn, Joss, Brough, Sarah, Bryant, Julia, Cortese, Luca, Foster, Caroline, Green, Andrew W, Oh, Sree, Colless, Matthew, Drinkwater, Michael J, Driver, Simon P, Goodwin, Michael, Gunawardhana, Madusha L P, Federrath, Christoph, Harischandra, Lloyd, Jin, Yifei, Lawrence, J S, Lorente, Nuria P, Mannering, Elizabeth, O’Toole, Simon, Richards, Samuel N, Sanchez, Sebastian F, Schaefer, Adam L, Sealey, Katrina, Sharp, Rob, Sweet, Sarah M, Taranu, Dan S, Varidel, Mathew

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A Log-Quadratic Relation for Predicting Supermassive Black Hole Masses from the Host Bulge Sérsic Index by Graham, Alister W, Driver, Simon P

“…We reinvestigate the correlation between black hole mass and bulge concentration. With an increased galaxy sample (totaling 27) and updated estimates of galaxy…”
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Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST by Smail, Ian, Dudzevičiūtė, Ugnė, Gurwell, Mark, Fazio, Giovanni G., Willner, S. P., Swinbank, A. M., Arumugam, Vinodiran, Summers, Jake, Cohen, Seth H., Jansen, Rolf A., Windhorst, Rogier A., Meena, Ashish, Zitrin, Adi, Keel, William C., Cheng, Cheng, Coe, Dan, Conselice, Christopher J., D’Silva, Jordan C. J., Driver, Simon P., Frye, Brenda, Grogin, Norman A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Pirzkal, Nor, Robotham, Aaron, Rutkowski, Michael J., Ryan Jr, Russell E., Tompkins, Scott, Willmer, Christopher N. A., Yan, Haojing, Broadhurst, Thomas J., Diego, José M., Kamieneski, Patrick, Yun, Min

“…Abstract We present a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope…”
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Deep Extragalactic VIsible Legacy Survey (DEVILS): identification of AGN through SED fitting and the evolution of the bolometric AGN luminosity function by Thorne, Jessica E, Robotham, Aaron S G, Davies, Luke J M, Bellstedt, Sabine, Brown, Michael J I, Croom, Scott M, Delvecchio, Ivan, Groves, Brent, Jarvis, Matt J, Shabala, Stanislav S, Seymour, Nick, Whittam, Imogen H, Bravo, Matias, Cook, Robin H W, Driver, Simon P, Holwerda, Benne, Phillipps, Steven, Siudek, Malgorzata

“…ABSTRACT Active galactic nuclei (AGN) are typically identified through radio, mid-infrared, or X-ray emission or through the presence of broad and/or narrow…”
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