Image Sensors for Precision Astronomy (ISPA)
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
The 4th workshop on Image Sensors for Precision Astronomy (ISPA) convenes astronomers and detector experts to address the challenges of making state-of-the-art measurements with imperfect detectors. Attendees will assess the impact of detector systematics on science goals and discuss strategies for characterization, calibration, and mitigation.
The scope of ISPA includes detector issues in any sensor type which affect applications such as photometry, astrometry, spectroscopy, coronagraphy, and shape measurement. ISPA was previously called PACCD - Precision Astronomy with fully depleted CCDs.
For remote connection please use:
Zoom https://stanford.zoom.us/j/355334733 (see zoom introduction)
US phone numbers: +1 415 762 9988; +1 646 568 7788; list for other countries; meeting ID: 355334733
Please email suggestions of any kind to Andrei Nomerotski.
Event ID: ISPA2018
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08:00
Light Breakfast Cahill foyer
Cahill foyer
Pick up your badge. Claim a dinner reservation. Put up your poster or give your presentation to Pavan Bilgi who will upload it for you.
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1
Welcome Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Jonas Zmuidzinas (Director, Caltech Optical Observatories) -
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Introductory talk Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Pierre Antilogus (LPNHE Paris) -
3
How well do we understand NIR sensors? Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
A review of how well we understand NIR detectors, directed at defining where the edges of our understanding lie. The goal is to promote discussion of the way forward for precision astronomy using these complicated devices.
Speaker: Roger Smith (Caltech) -
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Characterization of a 15 μm Cutoff HgCdTe Detector Array for Astronomy Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Mario Cabrera (Rochester) -
10:20
Coffee Break Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
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5
Linearity calibration Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Bernard Rauscher (Goddard Space Flight Center) -
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Calibrating WFIRST Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Susana Deustua (STSci) -
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Near Infrared Detectors and Precision Radial Velocity Measurements Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Gautam Vasisht (JPL) -
12:15
Lunch on Cahill Patio Head South towards sports field
Head South towards sports field
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Brighter-Fatter, crosshatch in NIR Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Eric Huff (JPL) -
9
The Brighter Fatter Effect in H4RG-10 Detectors Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Ami Choi (OSU) -
10
Interpixel Capacitive Coupling in Hybridized Arrays Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Kevan Donlon (RIT) -
15:15
Group Photo Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
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15:25
Coffee break Cahill Foyer
Cahill Foyer
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11
How I Learned to Stop Worrying and Love The Cold: Microwave Kinetic Inductance Detectors for Optical and Near-IR Astronomy Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Prof. Ben Mazin (UCSB) -
12
Moving Forward with SAPHIRA Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Dani Atkinson (Goddard) -
13
1 min poster talks Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
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14
Poster Session and reception Cahill foyer
Cahill foyer
Lively discussion with drinks and nibbles in Cahill foyer. Posters will be just outside.
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a) Tree rings in LSST production sensors: their dependence on radius, wavelength, and back bias voltageSpeakers: Hye Yun Park (Stony Brook Unversity, Broookhave National Laboratory), Andrei Nomerotski, Dmitri Tsybychev
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b) Correcting crosshatch pattern in H2RG for high precision near-infrared RV in HPFSpeakers: Joe Ninan (Pennsylvania State Unviersity), The HPF Team
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c) Recent STA Technology DevelopmentsSpeakers: Gregory Bredthauer (Semiconductor Technology Associates, Inc.), Joseph Tufts, Kasey Boggs
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d) Detector related challenges for high-precision radial-velocity spectrographsSpeakers: Andreas Seifahrt (University of Chicago), Julian Stürmer, Jacob Bean
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e) Next-to-leading-order terms for the brighter/fatter effect in thick CCDs: Are perturbations linear over 3 orders of magnitude?Speaker: Andy Rasmussen (SLAC National Accelerator Laboratory)
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f) Persistance suppresion by resetting while idlingSpeakers: Tim Greffe (Caltech), Roger Smith (Caltech)
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g) Precision Radial Velocity Measurements with an STA 1600 Detector from EXPRESSpeakers: Lily Zhao (Yale University), Debra Fischer, Colby Jurgenson, Dave Sawyer, Tyler McCracken, Andrew Szymkowiak, John Brewer, Ryan Blackman, Ryan Petersburg, Allen Davis, Joel Ong
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h) The bias shift in LSST sensorsSpeaker: Yousuke Utsumi (SLAC National Accelerator Laboratory/Stanford University)
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i) Establishing a Laboratory for Optical Sensor Testing at FZUSpeaker: Asen Christov (Institute of Physics, CAS Prague)
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j) Biased Moments of Subpixel SourcesSpeaker: Andrew Bradshaw (University of California at Davis)
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k) The Detector System for the NEID Doppler SpectrometerSpeakers: Cullen Blake (University of Pennsylvania), Dan Li (NOAO), Joseph Tufts (STA, Inc.)
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l) CCD Characterization and Modeling at UC DavisSpeakers: Craig Lage, Andrew Bradshaw, Tyson Tony (University of California at Davis), Kirk Gilmore (SLAC)
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m) Direct measurement of Kepler’s intra-pixel response functionSpeakers: Dmitry Vorobiev (Rochester Institute of Technology), Zoran Ninkov, Lexi Irwin, Kevan Donlon
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n) Strap Effects in the TESS CCDsSpeakers: Joel Villasenor, Sormeh Yazdi (Massachusetts Institute of Technology)
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o) Update on the NASA Goddard Astrophysics Division IR Detector TestbedSpeakers: Gregory Mosby (NASA Goddard Space Flight Center), Bernie Rauscher, Dani Atkinson, Alexander Kutyrev
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15
map of local restaurants Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
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19:00
Dinner at local restaurants Restaurants in Old Town
Restaurants in Old Town
See map attached to agenda introduction.This not covered by registration fee, but by paying directly you get to choose from the entire menu and will get a better meal. We have made reservations at the following restaurants. Please nominate which you prefer before lunch time on Monday so we can make sure you have a place.
www.cafesantorini.com (Mediteranean) 5 tables for 6 -- 64 W Union St, Pasadena, CA 91103
www.ilfornaio.com (Italian) 3 tables for 8 -- 24 W Union St, Pasadena, CA 91103
https://www.mipiace.com (Italian) 1 table for 12 -- 25 E Colorado Blvd, Pasadena, CA 91105
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08:00
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08:00
Light Breakfast Cahill Foyer
Cahill Foyer
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16
Uniformity and Stability of the LSST Focal Plane Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Paul O'CONNOR (Brookhaven National Laboratory) -
17
Unexpected features of bloomed images in deep depletion TESS CCDs Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Gregory Prigozhin (MIT) -
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Detector Systems Engineering for Extremely Large Instruments Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Elizabeth George (ESO) -
10:15
Coffee Break Cahill Foyer
Cahill Foyer
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19
Shape of the Photon Tranfer Curve of CCDs Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Pierre Astier (LPNHE, Paris) -
20
Automatic selection of Correlated Double Sampling timing parameters for optimal noise and linearity Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Daniel Weatherill (Oxford University) -
21
Tearing and related field distortions in deep-depletion CCDs Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Claire Juramy ( LPNHE, Paris) -
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Walk to Ath
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12:20
Athenaeum Buffet Athenaeum Al Fresco
Athenaeum Al Fresco
Outdoors if weather is nice or under clear sided tent if weather requires.
Cross at the lights, walk through the arches, turn right at the refection pond to head East past the tortoise pond, under the Lemon Scented Gums (tall Eucaltyptus), down Olive walk, past the cannon. Up a few steps to the left just before entering the Ath.
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Mitigating CTI from CCD bulk traps; Pavan Bilgi (Caltech) Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Pavan Bilgi (Caltech) -
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Investigation of Deferred Charge Effects in LSST CCD Sensors Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Snyder Adam (SLAC) -
25
Advances in Charge-Coupled Devices at MIT Lincoln Laboratory Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Chris Leitz (MIT / Lincoln Labs) -
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Impact of Detector Imperfections on Precision Radial Velocity Exoplanet Searches Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Roy Arpita (Caltech) -
15:30
Coffee Break Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
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27
EMCCDs for astrophysical use: performance, drawbacks, and lessons learned Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Erika Hamden (University of Arizona) -
28
Zero noise with skipper-CCD Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: juan estrada (fermilab) -
29
Summary Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
Speaker: Michael Seiffert (JPL) -
30
Closeout Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
Cahill Center for Astronomy & Astrophysics, Bldg. 17, Hameetman Auditorium
California Institute of Technology
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18:30
Dinner at local restaurants TBD
TBD
Arrangements TBD
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08:00