Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Hung, Chao-Ling"'
Autor:
Manning, Sinclaire M., Casey, Caitlin M., Hung, Chao-Ling, Battye, Richard, Brown, Michael L., Jackson, Neal, Abdalla, Filipe, Chapman, Scott, Demetroullas, Constantinos, Drew, Patrick, Hales, Christopher A., Harrison, Ian, Riseley, Christopher J., Sanders, David B., Watson, Robert A.
We present optical and near-infrared imaging covering a $\sim$1.53 deg$^2$ region in the Super-Cluster Assisted Shear Survey (SuperCLASS) field, which aims to make the first robust weak lensing measurement at radio wavelengths. We derive photometric
Externí odkaz:
http://arxiv.org/abs/2003.01735
Autor:
Battye, Richard A., Brown, Michael L., Casey, Caitlin M., Harrison, Ian, Jackson, Neal J., Smail, Ian, Watson, Robert A., Hales, Christopher A., Manning, Sinclaire M., Hung, Chao-Ling, Riseley, Christopher J., Abdalla, Filipe B., Birkinshaw, Mark, Demetroullas, Constantinos, Chapman, Scott, Beswick, Robert J., Muxlow, Tom W. B., Bonaldi, Anna, Camera, Stefano, Hillier, Tom, Kay, Scott T., Peters, Aaron, Sanders, David B., Thomas, Daniel B., Thomson, A. P., Tunbridge, Ben, Whittaker, Lee
The SuperCLuster Assisted Shear Survey (SuperCLASS) is a legacy programme using the e-MERLIN interferometric array. The aim is to observe the sky at L-band (1.4 GHz) to a r.m.s. of 7 uJy per beam over an area of ~1 square degree centred on the Abell
Externí odkaz:
http://arxiv.org/abs/2003.01734
Autor:
Mann, Andrew W., Dupuy, Trent, Kraus, Adam L., Gaidos, Eric, Ansdell, Megan, Ireland, Michael, Rizzuto, Aaron C., Hung, Chao-Ling, Dittmann, Jason, Factor, Samuel, Feiden, Gregory, Martinez, Raquel A., Ruiz-Rodriguez, Dary, Thao, Pa Chia
Publikováno v:
2019 ApJ 871 63
The mass-luminosity relation for late-type stars has long been a critical tool for estimating stellar masses. However, there is growing need for both a higher-precision relation and a better understanding of systematic effects (e.g., metallicity). He
Externí odkaz:
http://arxiv.org/abs/1811.06938
Autor:
Koss, Michael J., Blecha, Laura, Bernhard, Phillip, Hung, Chao-Ling, Lu, Jessica R., Trakhtenbrot, Benny, Treister, Ezequiel, Weigel, Anna, Sartori, Lia F., Mushotzky, Richard, Schawinski, Kevin, Ricci, Claudio, Veilleux, Sylvain, Sanders, David B.
Major galaxy mergers are thought to play an important part in fuelling the growth of supermassive black holes. However, observational support for this hypothesis is mixed, with some studies showing a correlation between merging galaxies and luminous
Externí odkaz:
http://arxiv.org/abs/1811.03641
Autor:
Drew, Patrick M., Casey, Caitlin M., Burnham, Anne D., Hung, Chao-Ling, Kassin, Susan A., Simons, Raymond C., Zavala, Jorge A.
Observations of the baryon to dark matter fraction in galaxies through cosmic time are a fundamental test for galaxy formation models. Recent observational studies have suggested that some disk galaxies at $z>1$ host declining rotation curves, in con
Externí odkaz:
http://arxiv.org/abs/1811.01958
Autor:
Casey, Caitlin M., Narayanan, Desika, Carilli, Chris, Champagne, Jaclyn, Hung, Chao-Ling, Dave, Romeel, Decarli, Roberto, Murphy, Eric J., Popping, Gergo, Riechers, Dominik, Somerville, Rachel S., Walter, Fabian
The next generation Very Large Array (ngVLA) will revolutionize our understanding of the distant Universe via the detection of cold molecular gas in the first galaxies. Its impact on studies of galaxy characterization via detailed gas dynamics will p
Externí odkaz:
http://arxiv.org/abs/1810.08258
Autor:
Shi, Ke, Lee, Kyoung-Soo, Dey, Arjun, Huang, Yun, Malavasi, Nicola, Hung, Chao-Ling, Inami, Hanae, Ashby, Matthew, Duncan, Kenneth, Xue, Rui, Reddy, Naveen, Hong, Sungryong, Jannuzi, Buell T., Cooper, Michael C., Gonzalez, Anthony H., Röttgering, Huub J. A., Best, Phillip N., Tasse, Cyril
We present a detailed census of galaxies in and around PC217.96+32.3, a spectroscopically confirmed Coma analog at z=3.78. Diverse galaxy types identified in the field include Lya emitters (LAEs), massive star-forming galaxies, and ultra-massive gala
Externí odkaz:
http://arxiv.org/abs/1808.07065
Autor:
Hung, Chao-Ling, Hayward, Christopher C., Yuan, Tiantian, Boylan-Kolchin, Michael, Faucher-Giguère, Claude-André, Hopkins, Philip, Kereš, Dušan, Murray, Norman, Wetzel, Andrew
One important result from recent large integral field spectrograph (IFS) surveys is that the intrinsic velocity dispersion of galaxies traced by star-forming gas increases with redshift. Massive, rotation-dominated discs are already in place at z~2,
Externí odkaz:
http://arxiv.org/abs/1806.04233
Autor:
Casey, Caitlin M., Zavala, Jorge A., Spilker, Justin, da Cunha, Elisabete, Hodge, Jacqueline, Hung, Chao-Ling, Staguhn, Johannes, Finkelstein, Steven L., Drew, Patrick
Though half of cosmic starlight is absorbed by dust and reradiated at long wavelengths (3$\mu$m-3mm), constraints on the infrared through millimeter galaxy luminosity function (the `IRLF') are poor in comparison to the rest-frame ultraviolet and opti
Externí odkaz:
http://arxiv.org/abs/1805.10301
Autor:
Lee, Kyoung-Soo, Dey, Arjun, Matheson, Thomas, Shi, Ke, Hung, Chao-Ling, Xue, Rui, Inami, Hanae, Huang, Yun, Lee, Khee-Gan, Ashby, Matthew L. N., Jannuzi, Buell, Reddy, Naveen, Hong, Sungryong, Mo, Wenli, Malavasi, Nicola
We report the discovery and spectroscopic confirmation of a very large star-forming Lyman Break galaxy, G6025, at z_spec=3.721+/-0.003. In the rest-frame ~2100A, G6025 subtends ~24 kpc in physical extent when measured from the 1.5-sigma isophote, in
Externí odkaz:
http://arxiv.org/abs/1803.07145