The SM3a Early Release Observations

Introduction

In mid-January 2000, a series of Early Release Obervations (EROs) were taken as part of the Hubble Space Telescope Servicing Mission 3a Orbital Verification. The purpose of these observations was to provide the public and the astronomical community with graphic proof that HST was again working as intended. Two targets were chosen, NGC 2392, the "Eskimo" planetary nebula, and Abell 2218, a galaxy cluster at z=0.17 known for the rich assembly of lensed arcs about its core. These objects were chosen both for their visual beauty and their scientific import. The press releases associated with these observations can be reached by clicking on the images above.

Information on our processing techniques and on how to retrieve the processed images is presented below.

NGC 2392

NGC 2392 was observed in four narrow band filters using the Wide Field and Planetary Camera 2 (WFPC2) on HST. The four filters were: F469N (HeII), F502N ([O III]), F656N (H alpha), and F658N ([N II]). Four exposures were taken in each filter with total exposure times of 1400, 400, 400, and 1400 s respectively. The exposures in each filter were taken using the standard four-point dither offsets for WFPC2. The images were combined using the "Drizzle" program. The raw data and processed individual images can be obtained from the HST archive. The drizzled, combined images used to create the press release can be retrieved here. Users wishing to do their own processing on the individual images may nonetheless find the README file in the drizzled image directory useful.

Abell 2218

Abell 2218 was observed in three different filters, F450W (B), F606W (V/R), and F814W (I). A combination of small and large dithers was used during these observations to allow a seamless joining of the images from the different WFPC2 chips. All individual exposures were 1000s long. The total exposure times were F450W, 12000s; F606W, 10,000s; and F814W, 12000s. As in the case of the NGC 2392 data, the raw data as well as processed individual images can be retrieved from the HST archive. The drizzled mosaics used for the press release are available here. Users wishing to do their own processing may nonetheless find the README file in the drizzled image directory useful. For more information on these images you can contact Andy Fruchter (STScI) or any member of the ERO Team.