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About the Data Q&A category
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0
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542
|
September 29, 2017
|
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Rubin Seeing Band Distribution
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2
|
84
|
April 21, 2021
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Amending the alert schema for PLAsTiCC simulations
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3
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65
|
April 15, 2021
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Bright Star Saturation
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3
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133
|
December 16, 2020
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Data access policy for alerts during commissioning
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2
|
111
|
September 22, 2020
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In-kind Program Update: Exceptions to the Proposal Deadline, Interim Data Access in 2021
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0
|
465
|
September 12, 2020
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Large cutouts in sample alerts
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5
|
210
|
August 3, 2020
|
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How will users access Year One AP Templates
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1
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132
|
June 3, 2020
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Will DIA Objects be matched between DRP and AP?
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10
|
227
|
June 3, 2020
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Access to forced photometry and postage stamps defined by sky position (not DIAForcedSource position)
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2
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221
|
February 19, 2020
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For how long will forced photometry be run on DIAObjects, after discovery?
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2
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289
|
February 19, 2020
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Alert format, serialization, and transport
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3
|
352
|
October 14, 2019
|
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Loading large numbers of catalogs with the Butler
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|
2
|
225
|
August 8, 2019
|
|
LSST Answers to Community Broker FAQs
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0
|
843
|
August 2, 2019
|
|
Testing methods to mitigate the effects of saturation
|
|
8
|
596
|
January 10, 2019
|
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Identifying Suddenly Saturated Objects in the Prompt Pipeline
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|
1
|
364
|
November 27, 2018
|
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Will there be a live feed of the telescope schedule during operations?
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2
|
317
|
September 7, 2018
|
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Data Model for variable sources at time of Data Releases?
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5
|
655
|
July 2, 2018
|
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Availability of residual images?
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|
1
|
550
|
February 23, 2018
|
|
LSST Filters versus SDSS
|
|
5
|
1491
|
November 28, 2017
|
|
CCD Nonlinearity Near Saturation
|
|
12
|
949
|
October 24, 2017
|
|
How will the difference imaging pipeline respond to marginally resolved sources?
|
|
2
|
597
|
October 17, 2017
|
