Zobrazeno 1 - 10
of 332
pro vyhledávání: '"Cook Robin"'
Autor:
Hansen, Samuel P., Lagos, Claudia D. P., Bonato, Matteo, Cook, Robin H. W., Davies, Luke J. M., Delvecchio, Ivan, Tompkins, Scott A.
We present a model of radio continuum emission associated with star formation (SF) and active galactic nuclei (AGN) implemented in the Shark semi-analytic model of galaxy formation. SF emission includes free-free and synchrotron emission, which depen
Externí odkaz:
http://arxiv.org/abs/2405.05586
Autor:
Cook, Robin H. W., Davies, Luke J. M., Rhee, Jonghwan, Hale, Catherine L., Bellstedt, Sabine, Thorne, Jessica E., Delvecchio, Ivan, Collier, Jordan D., Dodson, Richard, Driver, Simon P., Holwerda, Benne W., Jarvis, Matt J., Knowles, Kenda, Lagos, Claudia, Maddox, Natasha, Meyer, Martin, Robotham, Aaron S. G., Roychowdhury, Sambit, Rozgonyi, Kristof, Seymour, Nicholas, Siudek, Malgorzata, Whiting, Matthew, Whittam, Imogen
The tight relationship between infrared luminosity (L$_\mathrm{TIR}$) and 1.4 GHz radio continuum luminosity (L$_\mathrm{1.4GHz}$) has proven useful for understanding star formation free from dust obscuration. Infrared emission in star-forming galaxi
Externí odkaz:
http://arxiv.org/abs/2405.00337
Autor:
Bellstedt, Sabine, Robotham, Aaron S. G., Driver, Simon P., Lagos, Claudia del P., Davies, Luke J. M., Cook, Robin H. W.
We present the first look at star formation histories of galaxy components using ProFuse, a new technique to model the 2D distribution of light across multiple wavelengths using simultaneous spectral and spatial fitting of purely imaging data. We pre
Externí odkaz:
http://arxiv.org/abs/2307.02788
Autor:
Thorne, Jessica E., Robotham, Aaron S. G., Bellstedt, Sabine, Davies, Luke J. M., Cook, Robin H. W., Cortese, Luca, Holwerda, Benne, Phillipps, Steven, Siudek, Malgorzata
Gas-phase metallicities of galaxies are typically measured through auroral or nebular emission lines, but metallicity also leaves an imprint on the overall spectral energy distribution (SED) of a galaxy and can be estimated through SED fitting. We us
Externí odkaz:
http://arxiv.org/abs/2210.13696
Autor:
Sinigaglia, Francesco, Rodighiero, Giulia, Elson, Ed, Vaccari, Mattia, Maddox, Natasha, Frank, Bradley S., Jarvis, Matt J., Oosterloo, Tom, Davé, Romeel, Salvato, Mara, Baes, Maarten, Bellstedt, Sabine, Bisigello, Laura, Collier, Jordan D., Cook, Robin H. W., Davies, Luke J. M., Delhaize, Jacinta, Driver, Simon P., Foster, Caroline, Kurapati, Sushma, Lagos, Claudia del P., Lidman, Christopher, Piña, Pavel E. Mancera, Meyer, Martin J., Mogotsi, K. Moses, Pan, Hengxing, Ponomareva, Anastasia A., Prandoni, Isabella, Rajohnson, Sambatriniaina H. A., Robotham, Aaron S. G., Santos, Mario G., Sekhar, Srikrishna, Spekkens, Kristine, Thorne, Jessica E., van der Hulst, Jan M., Wong, O. Ivy
We present the first measurements of HI galaxy scaling relations from a blind survey at $z>0.15$. We perform spectral stacking of 9023 spectra of star-forming galaxies undetected in HI at $0.23
Externí odkaz:
http://arxiv.org/abs/2208.01121
Autor:
Cook, Robin M.1,2 (AUTHOR) michelephant@savetheelephants.org, Henley, Michelle D.2,3,4 (AUTHOR)
Publikováno v:
Diversity (14242818). Sep2024, Vol. 16 Issue 9, p577. 8p.
Autor:
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
Active galactic nuclei (AGN) are typically identified through radio, mid-infrared, or X-ray emission or through the presence of broad and/or narrow emission lines. AGN can also leave an imprint on a galaxy's spectral energy distribution (SED) through
Externí odkaz:
http://arxiv.org/abs/2112.06366