1
|
Romualdez LJ, Benton SJ, Brown AM, Clark P, Damaren CJ, Eifler T, Fraisse AA, Galloway MN, Gill A, Hartley JW, Holder B, Huff EM, Jauzac M, Jones WC, Lagattuta D, Leung JSY, Li L, Luu TVT, Massey RJ, McCleary J, Mullaney J, Nagy JM, Netterfield CB, Redmond S, Rhodes JD, Schmoll J, Shaaban MM, Sirks E, Tam SI. Publisher's Note: "Robust diffraction-limited near-infrared-to-near-ultraviolet wide-field imaging from stratospheric balloon-borne Platforms-Super-pressure Balloon-borne Imaging Telescope performance" [Rev. Sci. Instrum. 91, 034501 (2020)]. Rev Sci Instrum 2021; 92:019901. [PMID: 33514192 DOI: 10.1063/5.0040187] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/10/2020] [Indexed: 06/12/2023]
Affiliation(s)
- L Javier Romualdez
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Steven J Benton
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Anthony M Brown
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Paul Clark
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Christopher J Damaren
- University of Toronto Institute for Aerospace Studies (UTIAS), 4925 Dufferin Street, Toronto, Ontario, M3H 5T6, Canada
| | - Tim Eifler
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
| | - Aurelien A Fraisse
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Mathew N Galloway
- Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo 0315, Norway
| | - Ajay Gill
- Department of Astronomy, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
| | - John W Hartley
- Department of Physics, University of Toronto, 60 St. George Street, Toronto, Ontario, M5R 2M8, Canada
| | - Bradley Holder
- University of Toronto Institute for Aerospace Studies (UTIAS), 4925 Dufferin Street, Toronto, Ontario, M3H 5T6, Canada
| | - Eric M Huff
- Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - Mathilde Jauzac
- Department of Physics, Centre for Extragalactic Astronomy, Durham University, Durham DH1 3LE, United Kingdom
| | - William C Jones
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - David Lagattuta
- Department of Physics, Centre for Extragalactic Astronomy, Durham University, Durham DH1 3LE, United Kingdom
| | - Jason S-Y Leung
- Department of Astronomy, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
| | - Lun Li
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Thuy Vy T Luu
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Richard J Massey
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Jacqueline McCleary
- Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - James Mullaney
- Department of Physics and Astronomy, The University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
| | - Johanna M Nagy
- Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
| | - C Barth Netterfield
- Department of Astronomy, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
| | - Susan Redmond
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Jason D Rhodes
- Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - Jurgen Schmoll
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Mohamed M Shaaban
- Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
| | - Ellen Sirks
- Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Sut-Ieng Tam
- Department of Physics, Centre for Extragalactic Astronomy, Durham University, Durham DH1 3LE, United Kingdom
| |
Collapse
|
2
|
Romualdez LJ, Benton SJ, Brown AM, Clark P, Damaren CJ, Eifler T, Fraisse AA, Galloway MN, Gill A, Hartley JW, Holder B, Huff EM, Jauzac M, Jones WC, Lagattuta D, Leung JSY, Li L, Luu TVT, Massey RJ, McCleary J, Mullaney J, Nagy JM, Netterfield CB, Redmond S, Rhodes JD, Schmoll J, Shaaban MM, Sirks E, Tam SI. Robust diffraction-limited near-infrared-to-near-ultraviolet wide-field imaging from stratospheric balloon-borne platforms-Super-pressure Balloon-borne Imaging Telescope performance. Rev Sci Instrum 2020; 91:034501. [PMID: 32259997 DOI: 10.1063/1.5139711] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/22/2019] [Accepted: 02/10/2020] [Indexed: 06/11/2023]
Abstract
At a fraction of the total cost of an equivalent orbital mission, scientific balloon-borne platforms, operating above 99.7% of the Earth's atmosphere, offer attractive, competitive, and effective observational capabilities-namely, space-like seeing, transmission, and backgrounds-which are well suited for modern astronomy and cosmology. The Super-pressure Balloon-borne Imaging Telescope (SUPERBIT) is a diffraction-limited, wide-field, 0.5 m telescope capable of exploiting these observing conditions in order to provide exquisite imaging throughout the near-infrared to near-ultraviolet. It utilizes a robust active stabilization system that has consistently demonstrated a 48 mas 1σ sky-fixed pointing stability over multiple 1 h observations at float. This is achieved by actively tracking compound pendulations via a three-axis gimballed platform, which provides sky-fixed telescope stability at < 500 mas and corrects for field rotation, while employing high-bandwidth tip/tilt optics to remove residual disturbances across the science imaging focal plane. SUPERBIT's performance during the 2019 commissioning flight benefited from a customized high-fidelity science-capable telescope designed with an exceptional thermo- and opto-mechanical stability as well as a tightly constrained static and dynamic coupling between high-rate sensors and telescope optics. At the currently demonstrated level of flight performance, SUPERBIT capabilities now surpass the science requirements for a wide variety of experiments in cosmology, astrophysics, and stellar dynamics.
Collapse
Affiliation(s)
- L Javier Romualdez
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Steven J Benton
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Anthony M Brown
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Paul Clark
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Christopher J Damaren
- University of Toronto Institute for Aerospace Studies (UTIAS), 4925 Dufferin Street, Toronto, Ontario M3H 5T6, Canada
| | - Tim Eifler
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
| | - Aurelien A Fraisse
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Mathew N Galloway
- Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo 0315, Norway
| | - Ajay Gill
- Department of Astronomy, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, Canada
| | - John W Hartley
- Department of Physics, University of Toronto, 60 St. George Street, Toronto, Ontario M5R 2M8, Canada
| | - Bradley Holder
- University of Toronto Institute for Aerospace Studies (UTIAS), 4925 Dufferin Street, Toronto, Ontario M3H 5T6, Canada
| | - Eric M Huff
- Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - Mathilde Jauzac
- Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - William C Jones
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - David Lagattuta
- Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - Jason S-Y Leung
- Department of Astronomy, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, Canada
| | - Lun Li
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Thuy Vy T Luu
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Richard J Massey
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Jacqueline McCleary
- Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - James Mullaney
- Department of Physics and Astronomy, The University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
| | - Johanna M Nagy
- Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, Canada
| | - C Barth Netterfield
- Department of Astronomy, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, Canada
| | - Susan Redmond
- Department of Physics, Princeton University, Jadwin Hall, Princeton, New Jersey 08544, USA
| | - Jason D Rhodes
- Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - Jürgen Schmoll
- Centre for Advanced Instrumentation (CfAI), Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Mohamed M Shaaban
- Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, Canada
| | - Ellen Sirks
- Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, United Kingdom
| | - Sut-Ieng Tam
- Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| |
Collapse
|
3
|
Oshidari R, Strecker J, Chung DKC, Abraham KJ, Chan JNY, Damaren CJ, Mekhail K. Nuclear microtubule filaments mediate non-linear directional motion of chromatin and promote DNA repair. Nat Commun 2018; 9:2567. [PMID: 29967403 PMCID: PMC6028458 DOI: 10.1038/s41467-018-05009-7] [Citation(s) in RCA: 57] [Impact Index Per Article: 9.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/06/2018] [Accepted: 06/07/2018] [Indexed: 12/19/2022] Open
Abstract
Damaged DNA shows increased mobility, which can promote interactions with repair-conducive nuclear pore complexes (NPCs). This apparently random mobility is paradoxically abrogated upon disruption of microtubules or kinesins, factors that typically cooperate to mediate the directional movement of macromolecules. Here, we resolve this paradox by uncovering DNA damage-inducible intranuclear microtubule filaments (DIMs) that mobilize damaged DNA and promote repair. Upon DNA damage, relief of centromeric constraint induces DIMs that cooperate with the Rad9 DNA damage response mediator and Kar3 kinesin motor to capture DNA lesions, which then linearly move along dynamic DIMs. Decreasing and hyper-inducing DIMs respectively abrogates and hyper-activates repair. Accounting for DIM dynamics across cell populations by measuring directional changes of damaged DNA reveals that it exhibits increased non-linear directional behavior in nuclear space. Abrogation of DIM-dependent processes or repair-promoting factors decreases directional behavior. Thus, inducible and dynamic nuclear microtubule filaments directionally mobilize damaged DNA and promote repair. Following DNA damage, different processes come to action to aid repair. The authors here find that microtubule filaments within the cell nucleus capture and non-randomly mobilize damaged chromatin to mediate DNA repair.
Collapse
Affiliation(s)
- Roxanne Oshidari
- Department of Laboratory Medicine and Pathobiology, MaRS Centre, University of Toronto, West Tower, 661 University Avenue, Toronto, ON, M5G 1M1, Canada
| | - Jonathan Strecker
- Department of Molecular Genetics, MaRS Centre, University of Toronto, West Tower, 661 University Avenue, Toronto, ON, M5G 1M1, Canada.,Lunenfeld-Tanenbaum Research Institute, Mount Sinai Hospital, 600 University Avenue, Toronto, ON, M5G 1X5, Canada.,Broad Institute of MIT and Harvard, 75 Ames Street, Cambridge, MA, 02142, USA
| | - Daniel K C Chung
- Department of Laboratory Medicine and Pathobiology, MaRS Centre, University of Toronto, West Tower, 661 University Avenue, Toronto, ON, M5G 1M1, Canada
| | - Karan J Abraham
- Department of Laboratory Medicine and Pathobiology, MaRS Centre, University of Toronto, West Tower, 661 University Avenue, Toronto, ON, M5G 1M1, Canada
| | - Janet N Y Chan
- Department of Laboratory Medicine and Pathobiology, MaRS Centre, University of Toronto, West Tower, 661 University Avenue, Toronto, ON, M5G 1M1, Canada
| | - Christopher J Damaren
- Institute for Aerospace Studies, University of Toronto, 4925 Dufferin Street, Toronto, ON, M3H 5T6, Canada
| | - Karim Mekhail
- Department of Laboratory Medicine and Pathobiology, MaRS Centre, University of Toronto, West Tower, 661 University Avenue, Toronto, ON, M5G 1M1, Canada. .,Canada Research Chairs Program, University of Toronto, 1 King's College Circle, Toronto, ON, M5S 1A8, Canada.
| |
Collapse
|
4
|
Abstract
The vibration modes of a generic two-link fiexible manipulator are studied as a function of the link, rotor, and tip (statorlpayload) mass distribution. Necessary and sufficient conditions are devel oped for all vibration modes to exhibit a node at the manipulator endpoint. A rigorous treatment of the relevant kinematics and dy namics shows that this property can be closely achieved for large tip/link mass ratio and sufficiently small rotor inertia. The major impacts of this result on feedforward/feedback controller design are uncovered. First, the nonlinear joint torque to end-effector motion dynamics become essentially equivalent to those of the rigid case. Second, an output involving the endpoint rates and elastic motions is shown to possess the passivity property for suitably defined inputs. This permits the design of simple controllers that furnish endpoint stabilization with simultaneous vibration suppression. A numeri cal example is used to illustrate the results and demonstrate the achievable performance using the controller design concepts.
Collapse
|