Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #7185

Period Covered:
08:00 pm March 15, 2016 - 07:59 pm March 16, 2016
(DOY 076/0000z - 076/2359z)

Flight Operations Summary

This report was generated by the HST Automated Report System @2016-03-17 17:02:00 GMT

Significant Spacecraft Anomalies: (The following are preliminary reports
of potential non-nominal performance that will be investigated.)


Program Principal Investigator Program Title
Science Observations Scheduled
14071 Sanchayeeta Borthakur, The Johns Hopkins University How are HI Disks Fed? Probing Condensation at the Disk-Halo Interface
14077 Boris Gaensicke, The University of Warwick The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps
14141 Guy Worthey, Washington State University NGSL Extension 1. Hot Stars and Evolved Stars
14254 Tommaso Treu, University of California - Los Angeles Accurate cosmography from gravitational time delays: 2.3% on H0 from deep WFC3 images of lensed quasars
14327 Saul Perlmutter, University of California - Berkeley See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts
14469 Carlo Manara, European Space Agency - ESTEC The HST-ALMA connection: measuring the FUV spectrum of a newly discovered transition disk down to the H2 and CO photodissociation regime
Calibration Observations Scheduled
14369 Matthew Bourque, Space Telescope Science Institute WFC3 UVIS Daily Monitor B
14381 Knox Long, Eureka Scientific Inc. WFC3 IR Persistence: Position Dependent Model
14382 Sylvia Baggett, Space Telescope Science Institute WFC3/UVIS contamination and stability monitor
14389 Heather Gunning, Space Telescope Science Institute WFC3 UVIS Pixel variations via int-flat monitor
14396 David Golimowski, Space Telescope Science Institute CCD Daily Monitor (Part 2)
14412 Joanna Taylor, Space Telescope Science Institute CCD Dark Monitor Part 1
14414 Joanna Taylor, Space Telescope Science Institute CCD Bias and Read Noise Monitor Part 2