Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Shipley, Heath V."'
Autor:
Nedkova, Kalina V., Häußler, Boris, Marchesini, Danilo, Brammer, Gabriel B., Feinstein, Adina D., Johnston, Evelyn J., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Martis, Nicholas S., Muzzin, Adam, Rafelski, Marc, Shipley, Heath V., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E.
Using deep imaging from the CANDELS and HFF surveys, we present bulge+disc decompositions with GalfitM for $\sim$17,000 galaxies over $0.2 \leq z\leq 1.5$. We use various model parameters to select reliable samples of discs and bulges, and derive the
Externí odkaz:
http://arxiv.org/abs/2406.14613
Autor:
Nedkova, Kalina V., Häußler, Boris, Marchesini, Danilo, Dimauro, Paola, Brammer, Gabriel, Eigenthaler, Paul, Feinstein, Adina D., Ferguson, Henry C., Huertas-Company, Marc, Johnston, Evelyn J., Kado-Fong, Erin, Kartaltepe, Jeyhan S., Labbé, Ivo, Lange-Vagle, Daniel, Martis, Nicholas S., McGrath, Elizabeth J., Muzzin, Adam, Oesch, Pascal, Ordenes-Briceño, Yasna, Puzia, Thomas, Shipley, Heath V., Simmons, Brooke D., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E.
We reliably extend the stellar mass-size relation over $0.2\leq z \leq2$ to low stellar mass galaxies by combining the depth of Hubble Frontier Fields (HFF) with the large volume covered by CANDELS. Galaxies are simultaneously modelled in multiple ba
Externí odkaz:
http://arxiv.org/abs/2106.07663
We calibrate the integrated luminosity from the polycyclic aromatic hydrocarbon (PAH) features at 6.2\micron, 7.7\micron\ and 11.3\micron\ in galaxies as a measure of the star-formation rate (SFR). These features are strong (containing as much as 5-1
Externí odkaz:
http://arxiv.org/abs/1601.01698
Autor:
Shipley, Heath V., Papovich, Casey, Rieke, George H., Dey, Arjun, Jannuzi, Buell T., Moustakas, John, Weiner, Benjamin
We use Spitzer IRS spectroscopy to study the nature 65 IR-luminous galaxies at 0.02 < z < 0.6 with F(24micron) > 1.2mJy. The IRS spectra cover wavelengths spanning the PAH features and important atomic diagnostic lines. Our sample corresponds to L(IR
Externí odkaz:
http://arxiv.org/abs/1304.5231