Anna Moore

Prof. Dr. Anna Moore

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Research Focus & Metrics

Academic Career Length

29Years (1998-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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17 February 2016 in Nature
Verified
Journal Article
Closed access
XCXavier Clemente-Casares
Xavier Clemente-Casares
JBJesus Blanco
Jesus Blanco
PAPoornima Ambalavanan
Poornima Ambalavanan
JYJun Yamanouchi
Jun Yamanouchi
SSSantiswarup Singha
Santiswarup Singha
PSPere Santamaria
Pere Santamaria

6 October 2009 in Journal of the American Chemical Society
Verified
Journal Article
Closed access
CRChongzhao Ran
Chongzhao Ran
XXXiaoyin Xu
Xiaoyin Xu
SRScott B. Raymond
Scott B. Raymond
BFBrian J. Ferrara
Brian J. Ferrara
KNKrista Neal
Krista Neal
AMAnna Moore
Anna Moore

1 September 2018 in The Astrophysical Journal
Verified
Journal Article
Closed access
PMPatrick Morrissey
Patrick Morrissey
MMMatuesz Matuszewski
Matuesz Matuszewski
DMD. Christopher Martin
D. Christopher Martin
JNJames D. Neill
James D. Neill
HEHarland Epps
Harland Epps
RZRay Zarzaca
Ray Zarzaca
We report on the design and performance of the Keck Cosmic Web Imager (KCWI), a general purpose optical integral field spectrograph that has been installed at the Nasmyth port of the 10 m Keck II telescope on Maunakea, Hawaii. The novel design provides blue-optimized seeing-limited imaging from 350–560 nm with configurable spectral resolution from 1000–20,000 in a field of view up to 20″ × 33″. Selectable volume phase holographic (VPH) gratings and high-performance dielectric, multilayer silver, and enhanced-aluminum coatings provide end-to-end peak efficiency in excess of 45% while accommodating the future addition of a red channel that will extend wavelength coverage to 1 micron. KCWI takes full advantage of the excellent seeing and dark sky above Maunakea with an available nod-and-shuffle observing mode. The instrument is optimized for observations of faint, diffuse objects such as the intergalactic medium or cosmic web. In this paper, a detailed description of the instrument design is provided with measured performance results from the laboratory test program and 10 nights of on-sky commissioning during the spring of 2017. The KCWI team is lead by Caltech and JPL (project management, design, and implementation) in partnership with the University of California at Santa Cruz (camera optical and mechanical design) and the W. M. Keck Observatory (observatory interfaces).

11 October 2013 in Journal of the American Chemical Society
Verified
Journal Article
Closed access
XZXueli Zhang
Xueli Zhang
YTYanli Tian
Yanli Tian
ZLZeng Li
Zeng Li
XTXiaoyu Tian
Xiaoyu Tian
HSHongbin Sun
Hongbin Sun
CRChongzhao Ran
Chongzhao Ran

5 August 2014 in Nature Biotechnology
Verified
Journal Article
Closed access
PDF file
ANAnna V Naumova
Anna V Naumova
MMMike Modo
Mike Modo
AMAnna Moore
Anna Moore
CMCharles E Murry
Charles E Murry
JFJoseph A Frank
Joseph A Frank

21 July 2015 in Proceedings of the National Academy of Sciences
Verified
Journal Article
Closed access
PDF file
XZXueli Zhang
Xueli Zhang
YTYanli Tian
Yanli Tian
CZCan Zhang
Can Zhang
XTXiaoyu Tian
Xiaoyu Tian
ARAlana W. Ross
Alana W. Ross
CRChongzhao Ran
Chongzhao Ran
Significance: Drug development for Alzheimer’s disease (AD) has been largely unsuccessful to date. Although numerous agents are reportedly effective in vitro, only an inadequate number of them have been tested in vivo, partially because of the lack of reliable and cost-efficient imaging methods to monitor their in vivo therapeutic effectiveness. Several amyloid beta (Aβ)-specific PET tracers have been used for clinical studies. However, their application for monitoring drug treatment in small animals is limited. Near-infrared fluorescence (NIRF) molecular imaging is a cheap, easy-to-use, and widely available technology for small animal studies. In this report we demonstrate, for the first time to our knowledge, that NIRF imaging can be used to monitor the loading changes of Aβs in an AD mouse model.