Deep Astrometry of the Galactic Bulge with the HST ACS-WFC

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We report our HST determination of proper motions in the Galactic Bulge and foreground disk populations. At over 890 ks integration time in F814W, the SWEEPS transiting exoplanet search of Sahu et al. (2006) has produced the deepest image ever taken of the galactic field, allowing stellar positions to be constrained to high accuracy at unprecedented depth. With a second epoch two years later with HST/ACS with full overlap, and a third seven years earlier with WFPC2 at 60% overlap, we are able to measure the proper-motions of diskand bulge-objects, with the aim of providing better kinematic population diagnostics than has previously been possible. We discuss the techniques used to robustly measure proper-motions from our datasets, meeting the challenges of (i) high crowding, (ii) high intrinsic velocity dispersion about a small centroid offset (unlike globular cluster studies), and (iii) significant relative distortion between the ACS-WFC and WFPC2 instruments.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Deep Astrometry of the Galactic Bulge with the HST ACS-WFC does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Deep Astrometry of the Galactic Bulge with the HST ACS-WFC, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Deep Astrometry of the Galactic Bulge with the HST ACS-WFC will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1162880

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.