Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Noeske, Kai"'
Autor:
Straatman, Caroline M. S., van der Wel, Arjen, Bezanson, Rachel, Pacifici, Camilla, Gallazzi, Anna, Wu, Po-Feng, Noeske, Kai, Barisic, Ivana, Bell, Eric F., Brammer, Gabriel B., Calhau, Joao, Chauke, Priscilla, Franx, Marijn, van Houdt, Josha, Labbe, Ivo, Maseda, Michael V., Munoz-Mateos, Juan C., Muzzin, Adam, van de Sande, Jesse, Sobral, David, Spilker, Justin S.
We present the second data release of the Large Early Galaxy Astrophysics Census (LEGA-C), an ESO 130-night public spectroscopic survey conducted with VIMOS on the Very Large Telescope. We release 1988 spectra with typical continuum S / N ~= 20 /Angs
Externí odkaz:
http://arxiv.org/abs/1809.08236
Autor:
Chauke, Priscilla, van der Wel, Arjen, Pacifici, Camilla, Bezanson, Rachel, Wu, Po-Feng, Gallazzi, Anna, Noeske, Kai, Straatman, Caroline, Muños-Mateos, Juan-Carlos, Franx, Marijn, Barišić, Ivana, Bell, Eric F., Brammer, Gabriel B., Calhau, Joao, van Houdt, Josha, Labbé, Ivo, Maseda, Michael V., Muzzin, Adam, Rix, Hans-Walter, Sobral, David
Using high resolution spectra from the VLT LEGA-C program, we reconstruct the star formation histories (SFHs) of 607 galaxies at redshifts $z = 0.6-1.0$ and stellar masses $\gtrsim10^{10}$M$_{\odot}$ using a custom full spectrum fitting algorithm tha
Externí odkaz:
http://arxiv.org/abs/1805.02568
Autor:
Bezanson, Rachel, van der Wel, Arjen, Pacifici, Camilla, Noeske, Kai, Barišić, Ivana, Bell, Eric F., Brammer, Gabriel B., Calhau, Joao, Chauke, Priscilla, van Dokkum, Pieter, Franx, Marijn, Gallazzi, Anna, van Houdt, Josha, Labbé, Ivo, Maseda, Michael V., Muños-Mateos, Juan Carlos, Muzzin, Adam, van de Sande, Jesse, Sobral, David, Straatman, Caroline, Wu, Po-Feng
We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at $z=0.6-1$ from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic survey. Rotation is typically probed across 10-20kpc, or to an average
Externí odkaz:
http://arxiv.org/abs/1804.02402
Autor:
Barišić, Ivana, van der Wel, Arjen, Bezanson, Rachel, Pacifici, Camilla, Noeske, Kai, Mateos, Juan C. Muñoz, Franx, Marijn, Smolčić, Vernesa, Bell, Eric F., Brammer, Gabriel, Calhau, João, Chauké, Priscilla, van Dokkum, Pieter G., van Houdt, Josha, Gallazzi, Anna, Labbé, Ivo, Maseda, Michael V., Muzzin, Adam, Sobral, David, Straatman, Caroline, Wu, Po-Feng
We investigate the stellar kinematics and stellar populations of 58 radio-loud galaxies of intermediate luminosities (L$_{3 GHz}$ $>$ 10$^{23}$ W Hz$^{-1}$ ) at 0.6 < z < 1. This sample is constructed by cross-matching galaxies from the deep VLT/VIMO
Externí odkaz:
http://arxiv.org/abs/1708.08461
Autor:
Guo, Yicheng, Ferguson, Henry C., Bell, Eric F., Koo, David C., Conselice, Christopher J., Giavalisco, Mauro, Kassin, Susan, Lu, Yu, Lucas, Ray, Mandelker, Nir, McIntosh, Daniel M., Primack, Joel R., Ravindranath, Swara, Barro, Guillermo, Ceverino, Daniel, Dekel, Avishai, Faber, Sandra M., Fang, Jerome J., Koekemoer, Anton M., Noeske, Kai, Rafelski, Marc, Straughn, Amber
Publikováno v:
ApJ 800 (2015) 39-60
Although giant clumps of stars are crucial to galaxy formation and evolution, the most basic demographics of clumps are still uncertain, mainly because the definition of clumps has not been thoroughly discussed. In this paper, we study the basic demo
Externí odkaz:
http://arxiv.org/abs/1410.7398
Autor:
Hayward, Christopher C., Lanz, Lauranne, Ashby, Matthew L. N., Fazio, Giovanni, Hernquist, Lars, Martínez-Galarza, Juan Rafael, Noeske, Kai, Smith, Howard A., Wuyts, Stijn, Zezas, Andreas
Publikováno v:
MNRAS 445 (2014) 1598-1604
The total infrared (IR) luminosity is very useful for estimating the star formation rate (SFR) of galaxies, but converting the IR luminosity into an SFR relies on assumptions that do not hold for all galaxies. We test the effectiveness of the IR lumi
Externí odkaz:
http://arxiv.org/abs/1402.0006
Autor:
Pirzkal, Nor, Rothberg, Barry, Ryan, Russell, Coe, Dan, Malhotra, Sangeeta, Rhoads, James, Noeske, Kai
In the absence of spectra, fitting template model spectra to observed photometric fluxes, known as Spectral Energy Distribution (SED) fitting, has become the workhorse for identifying high-z galaxies. In this paper, we present an analysis of the most
Externí odkaz:
http://arxiv.org/abs/1304.4594
Autor:
Kassin, Susan A., Weiner, Benjamin J., Faber, S. M., Gardner, Jonathan P., Willmer, C. N. A., Coil, Alison L., Cooper, Michael C., Devriendt, Julien, Dutton, Aaron A., Guhathakurta, Puragra, Koo, David C., Metevier, A. J., Noeske, Kai G., Primack, Joel R.
We present evidence from a sample of 544 galaxies from the DEEP2 Survey for evolution of the internal kinematics of blue galaxies with stellar masses ranging 8.0 < log M* (M_Sun) < 10.7 over 0.2
Externí odkaz:
http://arxiv.org/abs/1207.7072