Earlier reports | Convert Day of Year |
Daily Report #6155
Period Covered:
08:00 pm May 20, 2013 - 07:59 pm May 21, 2013
(DOY 141/0000z - 141/2359z)
This report was generated by the HST Automated Report System @2013-05-22 17:02:00 GMT
Significant Spacecraft Anomalies: (The following are preliminary reports of potential non-nominal performance that will be investigated.) HSTARs: none COMPLETED OPS REQUEST: none COMPLETED OPS NOTES: none FGS ACQ STATUS: SCHEDULED SUCCESSFUL FGS GSAcq 8 8 FGS REAcq 8 8 OBAD with Maneuver 8 8 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
12468 | Keith Noll, NASA Goddard Space Flight Center | How Fast Did Neptune Migrate? A Search for Cold Red Resonant Binaries |
12880 | Adam Riess, The Johns Hopkins University | The Hubble Constant: Completing HST's Legacy with WFC3 |
12908 | Paul Goudfrooij, Space Telescope Science Institute | What Causes Extended Main Sequence Turn-offs in Intermediate-Age Star Clusters? |
12964 | Marina Rejkuba, European Southern Observatory - Germany | Probing the outermost halo in a giant galaxy: is it metal-poor and where does it end? |
12976 | Ian Roederer, Carnegie Institution of Washington | The Most Complete Template for r-process Nucleosynthesis beyond the Solar System |
13000 | Sungryong Hong, National Optical Astronomy Observatory, AURA | Impact of Environments on Lyman alpha Emitting Galaxies at High Redshift {z ~ 2.7} |
13031 | William Grundy, Lowell Observatory | Testing Collisional Grinding in the Kuiper Belt |
13051 | Jonathan Nichols, University of Leicester | Long term observations of Saturn's northern auroras |
Calibration Observations Scheduled | ||
13075 | John Biretta, Space Telescope Science Institute | UVIS CCD Daily Monitor C |
13132 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 2 |
13145 | Stephen Holland, Space Telescope Science Institute | MAMA Spectroscopic Sensitivity and Focus Monitor Cycle 20 |
13151 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 2 |