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pro vyhledávání: '"Rozgonyi, Kristof"'
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:
Rhee, Jonghwan, Meyer, Martin, Popping, Attila, Bellstedt, Sabine, Driver, Simon P., Robotham, Aaron S. G., Whiting, Matthew, Baldry, Ivan K., Brough, Sarah, Brown, Michael J. I., Bunton, John D., Dodson, Richard, Holwerda, Benne W., Hopkins, Andrew M., Koribalski, Bärbel S., Lee-Waddell, Karen, López-Sánchez, Ángel R., Loveday, Jon, Mahony, Elizabeth, Roychowdhury, Sambit, Rozgonyi, Kristóf, Staveley-Smith, Lister
We present early science results from Deep Investigation of Neutral Gas Origins (DINGO), an HI survey using the Australian Square Kilometre Array Pathfinder (ASKAP). Using ASKAP sub-arrays available during its commissioning phase, DINGO early science
Externí odkaz:
http://arxiv.org/abs/2210.09697
Autor:
Roychowdhury, Sambit, Meyer, Martin J., Rhee, Jonghwan, Zwaan, Martin A., Chauhan, Garima, Davies, Luke J. M., Bellstedt, Sabine, Driver, Simon P., Lagos, Claudia del P., Robotham, Aaron S. G., Bland-Hawthorn, Joss, Dodson, Richard, Holwerda, Benne W., Hopkins, Andrew M., Lara-Lopez, Maritza A., Lopez-Sanchez, Angel R., Obreschkow, Danail, Rozgonyi, Kristof, Whiting, Matthew T., Wright, Angus H.
We measure how the atomic gas (HI) fraction ($f_{HI}={\rm \frac{M_{HI}}{M_{*}}}$) of groups and pairs taken as single units vary with average stellar mass ($\langle {\rm M_*} \rangle$) and average star-formation rate ($\langle {\rm SFR} \rangle$), co
Externí odkaz:
http://arxiv.org/abs/2201.03575
Akademický článek
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Autor:
Rozgonyi, Kristóf, Frey, Sándor
The observation and imaging of hundreds or thousands of radio sources with the technique of very long baseline interferometry (VLBI) is a computationally intensive task. However, these surveys allow us to conduct statistical investigations of large s
Externí odkaz:
http://arxiv.org/abs/1701.04037
Autor:
Rozgonyi, Kristóf, Frey, Sándor
Publikováno v:
Galaxies, Vol. 4, No. 3, id. 10 (2016)
The prominent flat-spectrum radio quasar J0017+8135 (S5 0014+81) at z = 3.366 is one of the most luminous active galactic nuclei (AGN) known. Its milliarcsecond-scale radio jet structure has been studied with very long baseline interferometry (VLBI)
Externí odkaz:
http://arxiv.org/abs/1608.06219
Akademický článek
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