Zobrazeno 1 - 10
of 172
pro vyhledávání: '"Skelton, Rosalind E."'
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:
Simons, Raymond C., Papovich, Casey, Momcheva, Ivelina G., Brammer, Gabriel, Estrada-Carpenter, Vicente, Finkelstein, Steven L., Gosmeyer, Catherine M., Matharu, Jasleen, Trump, Jonathan R., Backhaus, Bren E., Cheng, Yingjie, Cleri, Nikko J., Ferguson, Henry C., Finlator, Kristian, Giavalisco, Mauro, Ji, Zhiyuan, Jung, Intae, Lotz, Jennifer M., O'Brien, Rosalia, Skelton, Rosalind E., Tilvi, Vithal, Weiner, Benjamin
We present an overview of the CANDELS Lyman-a Emission At Reionization (CLEAR) survey. CLEAR is a 130 orbit program of the Hubble Space Telescope using the Wide Field Camera 3 (WFC3) IR G102 grism. CLEAR targets 12 pointings divided between the GOODS
Externí odkaz:
http://arxiv.org/abs/2303.09570
Autor:
Momcheva, Ivelina G., Brammer, Gabriel B., van Dokkum, Pieter G., Skelton, Rosalind E., Whitaker, Katherine E., Nelson, Erica J., Fumagalli, Mattia, Maseda, Michael V., Leja, Joel, Franx, Marijn, Rix, Hans-Walter, Bezanson, Rachel, Cunha, Elisabete Da, Dickey, Claire, Schreiber, Natascha M. Förster, Illingworth, Garth, Kriek, Mariska, Labbé, Ivo, Lange, Johannes Ulf, Lundgren, Britt F., Magee, Daniel, Marchesini, Danilo, Oesch, Pascal, Pacifici, Camilla, Patel, Shannon G., Price, Sedona, Tal, Tomer, Wake, David A., van der Wel, Arjen, Wuyts, Stijn
We present reduced data and data products from the 3D-HST survey, a 248-orbit HST Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five CANDELS fields: AEGIS, COSMOS, GOODS-S, and UDS, along with WFC3 H-140 imaging, p
Externí odkaz:
http://hdl.handle.net/10150/621407
http://arizona.openrepository.com/arizona/handle/10150/621407
http://arizona.openrepository.com/arizona/handle/10150/621407
Autor:
Bezanson, Rachel, Wake, David A., Brammer, Gabriel B., Dokkum, Pieter G. van, Franx, Marijn, Labbé, Ivo, Leja, Joel, Momcheva, Ivelina G., Nelson, Erica J., Quadri, Ryan F., Skelton, Rosalind E., Weiner, Benjamin J., Whitaker, Katherine E.
We present a study of photometric redshift accuracy in the 3D-HST photometric catalogs, using 3D-HST grism redshifts to quantify and dissect trends in redshift accuracy for galaxies brighter than JH(IR) > 24 with an unprecedented and representative h
Externí odkaz:
http://hdl.handle.net/10150/621218
http://arizona.openrepository.com/arizona/handle/10150/621218
http://arizona.openrepository.com/arizona/handle/10150/621218
Autor:
Mowla, Lamiya A., Cutler, Sam E., Brammer, Gabriel B., Momcheva, Ivelina G., Whitaker, Katherine E., van Dokkum, Pieter G., Bezanson, Rachel S., Schreiber, Natascha M. Forster, Franx, Marijn, Iyer, Kartheik G., Marchesini, Danilo, Muzzin, Adam, Nelson, Erica J., Skelton, Rosalind E., Snyder, Gregory F., Wake, David A., Wuyts, Stijn, van der Wel, Arjen
The 3D-Drift And SHift (3D-DASH) program is a \textit{Hubble Space Telescope} WFC3 F160W imaging and G141 grism survey of the equatorial COSMOS field. 3D-DASH extends the legacy of HST near-infrared imaging and spectroscopy to degree-scale swaths of
Externí odkaz:
http://arxiv.org/abs/2206.01156
Autor:
Bok, Jamie, Cluver, Michelle E., Jarrett, Thomas H., Skelton, Rosalind E., Jones, Michael G., Verdes-Montenegro, Lourdes
We extend the analysis of Bok et al. (2020) in which the HI content of isolated galaxies from the AMIGA sample and selected paired galaxies from ALFALFA were examined as a potential driver of galaxy location on the WISE mid-infrared SFR-Mstar sequenc
Externí odkaz:
http://arxiv.org/abs/2204.05180
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
Autor:
Nelson, Erica J., Tacchella, Sandro, Diemer, Benedikt, Leja, Joel, Hernquist, Lars, Whitaker, Katherine E., Weinberger, Rainer, Pillepich, Annalisa, Nelson, Dylan, Terrazas, Bryan A., Nevin, Rebecca, Brammer, Gabriel B., Burkhart, Blakesley, Cochrane, Rachel, van Dokkum, Pieter, Johnson, Benjamin D., Mowla, Lamiya, Pakmor, Rudiger, Skelton, Rosalind E., Speagle, Joshua, Springel, Volker, Torrey, Paul, Vogelsberger, Mark, Wuyts, Stijn
We compare the star forming main sequence (SFMS) -- both integrated and resolved on 1kpc scales -- between the high-resolution TNG50 simulation of IllustrisTNG and observations from the 3D-HST slitless spectroscopic survey at z~1. Contrasting integra
Externí odkaz:
http://arxiv.org/abs/2101.12212
Autor:
Bok, Jamie, Skelton, Rosalind E., Cluver, Michelle E., Jarrett, Thomas H., Jones, Michael G., Verdes-Montenegro, Lourdes
Using mid-infrared star formation rate and stellar mass indicators in $\textit{WISE}$, we construct and contrast the relation between star formation rate and stellar mass for isolated and paired galaxies. Our samples comprise a selection of AMIGA (is
Externí odkaz:
http://arxiv.org/abs/2009.14585
Autor:
Hill, Allison R., van der Wel, Arjen, Franx, Marijn, Muzzin, Adam, Skelton, Rosalind E., Momcheva, Iva, van Dokkum, Pieter, Whitaker, Katherine E.
We investigate the median flattening of galaxies at $0.2
Externí odkaz:
http://arxiv.org/abs/1901.02009