Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Lea M. Z. Hagen"'
Autor:
Alexander Belles, Marjorie Decleir, William P. Bowman, Lea M. Z. Hagen, Caryl Gronwall, Michael H. Siegel
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 1, p 54 (2023)
We present Swift/Ultraviolet Optical Telescope (UVOT) integrated light photometry of the Spitzer Infrared Nearby Galaxies Survey (SINGS) and the Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH) samples of nearby galaxie
Externí odkaz:
https://doaj.org/article/bfa755bbcb094cf7bac62b422df467fe
Autor:
Christopher J. R. Clark, Julia C. Roman-Duval, Karl D. Gordon, Caroline Bot, Matthew W. L. Smith, Lea M. Z. Hagen
Publikováno v:
The Astrophysical Journal, Vol 946, Iss 1, p 42 (2023)
We explore evolution in the dust-to-gas ratio with density within four well-resolved Local Group galaxies—the LMC, SMC, M31, and M33. We do this using new Herschel maps, which restore extended emission that was missed by previous Herschel reduction
Externí odkaz:
https://doaj.org/article/fb38e902d20b41c2b28506ee2c0fa6b9
Autor:
Shubham Kanodia, Joseph O'Rourke, Candace Gray, Ming Zhao, Suzanne L. Hawley, Leo J. Liu, Gudmundur Stefansson, Paul Robertson, Heather Knutson, William Ketzeback, Joseph Huehnerhoff, Brett M. Morris, Suvrath Mahadevan, R. J. McMillan, Leslie Hebb, Chad F. Bender, Yiting Li, Thomas G. Beatty, Theodore Rudyk, Jack Dembicky, Jason T. Wright, Lea M. Z. Hagen, John P. Wisniewski, Samuel Halverson
We demonstrate a path to hitherto unachievable differential photometric precisions from the ground, both in the optical and near-infrared (NIR), using custom-fabricated beam-shaping diffusers produced using specialized nanofabrication techniques. Suc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e22a841b4d2784d98c29451c9271e89
https://resolver.caltech.edu/CaltechAUTHORS:20171006-092659962
https://resolver.caltech.edu/CaltechAUTHORS:20171006-092659962
Publikováno v:
The Astronomical Journal. 158:35
As part of the Swift/UVOT Stars Survey, we present near-ultraviolet point-source photometry for 103 Galactic open clusters. These data, taken over the span of the mission, provide a unique and unprecedented set of near-ultraviolet point-source photom
Autor:
J. E. Ryon, Santiago Erroz-Ferrer, Elena A. N. Mohd Noh Velastín, Lea M. Z. Hagen, Johan H. Knapen
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 436:3135-3146
Autor:
Kristina Nyland, Mark Seibert, Jeffrey A. Rich, Lisa M. Young, Barry F. Madore, Lea M. Z. Hagen, Marie Treyer, James D. Neill, Alex Hagen
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2016, 826 (2), ⟨10.3847/0004-637X/826/2/210⟩
NASA Astrophysics Data System
The Astrophysical Journal, American Astronomical Society, 2016, 826 (2), ⟨10.3847/0004-637X/826/2/210⟩
The Astrophysical Journal, 2016, 826 (2), ⟨10.3847/0004-637X/826/2/210⟩
NASA Astrophysics Data System
The Astrophysical Journal, American Astronomical Society, 2016, 826 (2), ⟨10.3847/0004-637X/826/2/210⟩
We provide evidence that UGC1382, long believed to be a passive elliptical galaxy, is actually a giant low surface brightness (GLSB) galaxy which rivals the archetypical GLSB Malin 1 in size. Like other GLSB galaxies, it has two components: a high su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec17ceefd0d61ceabf077647b13c1fd1
https://hal.science/hal-01440682
https://hal.science/hal-01440682
Autor:
Alex Hagen, Caryl Gronwall, Lea M. Z. Hagen, Michael H. Siegel, Erik A. Hoversten, Stefan Immler
Publikováno v:
NASA Astrophysics Data System
We present the first results from the Swift Ultraviolet Survey of the Magellanic Clouds (SUMaC), the highest resolution ultraviolet (UV) survey of the Magellanic Clouds yet completed. In this paper, we focus on the Small Magellanic Cloud (SMC). When
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4a018a8f3bf23d26b0105e25948df6e
Autor:
Lea M. Z. Hagen, Stefan Immler, Angelica Vargas, Michael H. Siegel, Caryl Gronwall, Erik A. Hoversten
Publikováno v:
Scopus-Elsevier
When measuring star formation rates using ultraviolet light, correcting for dust extinction is a critical step. However, with the variety of dust extinction curves to choose from, the extinction correction is quite uncertain. Here, we use Swift/UVOT
Autor:
E. A. Hoversten, Alex Hagen, Caryl Gronwall, Christopher Wolf, Michael H. Siegel, M. J. Page, Lea M. Z. Hagen
We use deep Swift UV/Optical Telescope (UVOT) near-ultraviolet (1600A to 4000A) imaging of the Chandra Deep Field South to measure the rest-frame far-UV (FUV; 1500A) luminosity function (LF) in four redshift bins between z=0.2 and 1.2. Our sample inc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3040d978357b76753d3e6ab843e0b76
http://arxiv.org/abs/1505.00798
http://arxiv.org/abs/1505.00798
We present the results of our ongoing investigation into the properties of hot stars and young stellar populations using the Swift/UVOT telescope. We present UVOT photometry of open and globular clusters and show that UVOT is capable of characterizin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b92c0d589388b52ab7656fa498ca332c
http://arxiv.org/abs/1504.02369
http://arxiv.org/abs/1504.02369