Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Tisanic, Kresimir"'
Autor:
Fatović, Marta, Palaversa, Lovro, Tisanić, Krešimir, Thanjavur, Karun, Ivezić, Željko, Kovačević, Andjelka B., Ilić, Dragana, Popović, Luka Č.
Publikováno v:
2023 AJ 165 138
We report the results of a search for long-period ($100
Externí odkaz:
http://arxiv.org/abs/2303.04600
Autor:
Ceraj, Lana, Smolčić, Vernesa, Delvecchio, Ivan, Butler, Andrew, Tisanić, Krešimir, Delhaize, Jacinta, Horellou, Cathy, Kartaltepe, Jeyhan, Kolokythas, Konstantinos, Leslie, Sarah, Marchesi, Stefano, Novak, Mladen, Pierre, Marguerite, Plionis, Manolis, Vardoulaki, Eleni, Zamorani, Giovanni
Publikováno v:
A&A 642, A125 (2020)
We studied a sample of 274 radio and X-ray selected quasars (XQSOs) detected in the COSMOS and XXL-S radio surveys at 3 GHz and 2.1 GHz, respectively. This sample was identified by adopting a conservative threshold in X-ray luminosity, Lx [2-10\ keV]
Externí odkaz:
http://arxiv.org/abs/2106.08786
Autor:
Molnar, Daniel Cs., Sargent, Mark T., Leslie, Sarah, Magnelli, Benjamin, Schinnerer, Eva, Zamorani, Giovanni, Delhaize, Jacinta, Smolcic, Vernesa, Tisanic, Kresimir, Vardoulaki, Eleni
The infrared-radio correlation (IRRC) underpins many commonly used radio luminosity-star formation rate (SFR) calibrations. In preparation for the new generation of radio surveys we revisit the IRRC of low-$z$ galaxies by (a) drawing on the best curr
Externí odkaz:
http://arxiv.org/abs/2103.04803
Autor:
Tisanić, Krešimir, Smolčić, V., Imbrišak, M., Bondi, M., Zamorani, G., Ceraj, L., Vardoulaki, E., Delhaize, J.
Publikováno v:
A&A 643, A51 (2020)
As the SKA is expected to be operational in the next decade, investigations of the radio sky in the range of 100 MHz to 10 GHz have become important for simulations of the SKA observations. In determining physical properties of galaxies from radio da
Externí odkaz:
http://arxiv.org/abs/2008.10969
Autor:
Tisanić, Krešimir, Smolčić, Vernesa, Delhaize, Jacinta, Novak, Mladen, Intema, Huib, Delvecchio, Ivan, Schinnerer, Eva, Zamorani, Giovanni
The infrared-radio correlation (IRRC) offers a way to assess star formation from radio emission. Multiple studies found the IRRC to decrease with increasing redshift. This may in part be due to the lack of knowledge about the possible radio spectral
Externí odkaz:
http://arxiv.org/abs/1801.08423