HUBBLE SPACE TELESCOPE DAILY REPORT #2898 PERIOD COVERED: 0000Z (UTC) 06/20/01 - 0000Z (UTC) 06/21/01 Daily Status Report as of 172/0000Z 1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED: 1.1 Completed Three Sets of WF/PC-2 8828 (Cycle 9 Supplemental Darks pt3/3) The WF/PC-2 was used to obtain three dark frames every day to provide data for monitoring and characterizing the evolution of hot pixels. The proposal completed with no reported problems. 1.2 Completed Two Sets of WF/PC-2 8592 (Pixel Microlensing of M87) The WF/PC-2 was used to undertake a pixel microlensing study of M87 in order to: 1} probe the lower end of the M87 IMF via star-star lensing, 2} possibly obtain the first evidence of Massive Compact Objects (MACHOs) in the halo of a galaxy other than our own, and 3} search for intracluster MACHOs. The proposal completed nominally. 1.3 Completed Two Sets of WF/PC-2 8601 (A Snapshot Survey of Probable Nearby Galaxies) The WF/PC-2 was used to continue the very successful snapshot survey in order to use the high spatial resolution of HST to determine whether selected galaxies are nearby on the basis of resolution into stars, and the magnitudes and colors of the brightest stars. There were no reported problems. 1.4 Completed WF/PC-2 9140 (Is GRO J1655-40 a Runaway Black Hole?) The WF/PC-2 was used to examine the formation of black holes which is one of the most intriguing problems in astronomy. In the case of stellar-mass black holes, several theories propose that they are born with large space velocities. To test this idea we wish to determine the space velocity of X-ray Nova Scorpii 1994 {GRO J16155-40}, which is one of the best black hole candidates of stellar mass, and a source of jets with apparent superluminal motions. This intriguing object is located ~eq 2.5^degrees above the galactic plane and the center of mass of the system is known to be moving with a large anomalous radial velocity with respect to the Local Standard of Rest. Since GRO J16155-40 has already been imaged with the WFPC2 in 1995, one more image with the same instrumental set-up could allow us to measure its expected proper motion with an accuracy of a few percent. This observation may provide the first unambiguous evidence for a black hole formed in the Milky Way that is migrating into intergalactic space. 1.5 Completed WF/PC-2 8177 (Investigating Type Ia Supernovae and an Accelerating Universe) The WF/PC-2 was used to obtain rest frame U and B photometry for four z~ 0.85 Supernova (SN) Ia. These observations will be coupled to ground-based rest frame V photometry and spectra. These data, combined with previous samples, will extend the D_L vs. z diagram for SN Ia to z~0.85, and allow us to discriminate the redshift dependence of supernova magnitudes in an accelerating Universe from that expected to result from systematic effects such as age of the stellar population, chemical evolution, a drift in the properties of dust, and weak gravitational lensing. The proposal completed with no reported problems. 1.6 Completed WF/PC-2 9086 (Investigating the Formation History of Spiral Galaxy Halos) The WF/PC-2 was used to make observations in order to constrain the origin of spiral galaxy halos by studying stellar populations near the tip of the red giant branch. This will be the first systematic study of this population in external galaxies and will quadruple the sample of normal spiral galaxies for which the halo metallicity distribution function is measured. This larger sample will permit study of the relationship between the bulge, disk, and halo components and between halos and globular systems. Such correlations will in turn provide indications as to whether the halo, bulge, and globular cluster systems built up nearly simultaneously in the early universe or were accreted over time through different kinds of merging events. The proposal completed nominally. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions: 5 Successful: 5 Scheduled Re-acquisitions: 10 Successful: 10 2.2 FHST Updates: Scheduled: 10 Successful: 10 2.3 Operations Notes: The STIS instrument remains in safe mode. The SSR EDAC error counter was cleared once per ROP SR-1A. Operations personnel participated in GSFC Internal Simulation #9 (EVA-3/PCU) yesterday from 8:00 a.m. until just past midnight. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of normal science observations and calibrations. /CAW