Asset Details
Do you wish to reserve the book?
Improvements to the image processing of HST NICMOS observationswith multiple readouts
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
Improvements to the image processing of HST NICMOS observationswith multiple readouts
Do you wish to request the book?
Improvements to the image processing of HST NICMOS observationswith multiple readouts
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Journal Article
Improvements to the image processing of HST NICMOS observationswith multiple readouts
2005
Overview
We report on improvements made to the standard NICMOS processing pipeline. The calculation of the uncertainties on the signal accumulation rate has been modified to include the statistical correlations between the consecutive readouts. In order to correct a problem with the existing cosmic ray rejection algorithm, we have developed and implemented a joint fit procedure, where the accumulating signal is fit as linear functions of time with the same rate both before and after the cosmic ray (CR) impact. We also accounted for inter-pixel correlations in the CR-affected region. The new processing is most relevant for deep observations of faint targets, and for PSF fitting, for which unbiased measurements of accurate error estimates are important. We show examples of these improvements for deep NIC2 images of high-redshift supernova from the Supernova Cosmology Project.
