1 / 12

Multi Cycle Treasury Program

Multi Cycle Treasury Program. Multi Cycle Treasury Program. Multi Cycle Treasury Program. Dr. Julianne Dalcanton (University of Washington) Dr. Eric F. Bell (University of Michigan) Dr. Luciana C. Bianchi (The Johns Hopkins University)

guang
Download Presentation

Multi Cycle Treasury Program

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Multi Cycle Treasury Program

  2. Multi Cycle Treasury Program

  3. Multi Cycle Treasury Program Dr. Julianne Dalcanton (University of Washington) Dr. Eric F. Bell (University of Michigan) Dr. Luciana C. Bianchi (The Johns Hopkins University) Dr. Nelson C. Caldwell (Smithsonian Institution Astrophysical Observatory) Dr. Andrew Dolphin (Raytheon Company) Dr. Karoline Gilbert (University of Washington) Dr. Leo Girardi (Osservatorio Astronomico di Padova) Dr. Stephanie Gogarten (University of Washington) Dr. Karl D. Gordon (Space Telescope Science Institute) Dr. Puragra Guhathakurta (University of California - Santa Cruz) Dr. Paul W. Hodge (University of Washington) Dr. Jon A. Holtzman (New Mexico State University) Mr. L. C. Johnson (University of Washington) Dr. Jason S. Kalirai (Space Telescope Science Institute) Dr. C. S. Kochanek (The Ohio State University) Dr. Dustin Lang (Princeton University) Dr. Soeren S. Larsen (Universiteit Utrecht, Sterrekundig Instituut Netherlands) Dr. Tod R. Lauer (National Optical Astronomy Observatories) Dr. Adam Leroy (Associated Universities, Inc.) Dr. Jason Lee Melbourne (California Institute of Technology) Dr. Knut A.G. Olsen (National Optical Astronomy Observatories) Dr. Hans-Walter Rix (Max-Planck-Institut fur Astronomie) Mr. Keith Rosema (Random Walk Group) Dr. Abhijit Saha (National Optical Astronomy Observatories) Dr. Ata Sarajedini (University of Florida) Dr. Anil C. Seth (Smithsonian Institution Astrophysical Observatory) Dr. Evan D. Skillman (University of Minnesota) Dr. Krzysztof Z. Stanek (The Ohio State University) Mr. Dan Weisz (University of Minnesota) Dr. Benjamin F. Williams (University of Washington)

  4. Multi Cycle Treasury Program

  5. Multi Cycle Treasury Program T. Brown et al. (2003)

  6. 1.) ACS/WFC3 Exploratory Survey Of M31's Evolution (AWESOME) 2.) Hubble's Andromeda Panchromatic Panoramic Imaging (HAPPI -- this is a direct reference to ANGST and ANGRRR).   3.) Stellar Evolution in Andromeda Legacy Survey (SEALS) 4.) Andromeda Survey of Stellar Evolution and Time (ASSET) 5.) Andromeda Survey of Stellar Evolution and Stellar States (ASSESS) 6.) A Panchromatic Hubble Andromeda Treasury (PHAT) 7.) The Great Andromeda Survey (GAS). 8.) The Andromeda Project 9.) Project Andromeda 10.) The Andromeda Hubble Atlas (AHA) 11.) Quarter of Andromeda Treasury Survey (QATS) 12.) Panchromatic Hubble Andromeda and Triangulum Survey (PHAT Survey) 13.) Panchromatic Imaging of Triangulum and Andromeda (PITA) 14.) Multiwavelength Mapping of M31 and M33 (MMMM) 15.) Wide-field Hubble Imaging of M31/M33 (WHIM) 16.) Wide-field High-resolution Imaging: Panchromatic Landscape of Andromeda and its Satellite with Hubble (WHIPLASH) 17.) Detailed Imaging of Nearby Galaxies: Boring into Andromeda and Triangulum (DINGBAT) 18.) Panchromatic Imaging of Nearby Galaxies (PING) 19.) Wide-field Imaging of Nearby Galaxies: Stellar Populations in Andromeda and its Neighbor (WINGSPAN) 20.) Wide-field Hubble Imaging of M31/M33 Stars In Color: Astrophysical Labratories (WHIMSICAL) 21.) Stellar Populations of Andromeda and Triangulum (SPAT) 22.) Near-infrared and Optical Survey of Two Resolved and Extended SpiralS (NOSTRESS) 23.) Hubble Ultrawide Multiwavelength M31 and M33 Survey (HUMMMS) 24.) Multiwavelength Andromeda and Triangulum Ultrawide Realization Experiment (MATURE) 25.) Multiwavelength M31 and M33 Ultrawide Survey Campaign Legacy Experiment (MMMUSCLE) 26.) Multiwavelength Andromeda and Triangulum Hubble Survey (MATHS) 27.) Survey with Hubble of Andromeda and Triangulum (SHAT) -- just kidding. 28.) Hubble Areal Mapping of M31 and M33 (HAMMM) 29.) Panchromatic Ultrawide M31 and M33 Extragalactic Legacy (PUMMEL) 30.) Panchromatic Hubble Ultrawide Galaxy Legacy Y-word (PHUGLY) -- also just kidding. 31.) Resolving Andromeda and Triangulum (RAT) 32.) Triangulum/Andromeda Survey Program (TASP) 33.) Galaxy Laboratories: Observing Andromeda and Triangulum (GLOAT) 34.) Galaxy Laboratories Observed with Hubble: the Andromeda and Triangulum Survey (GLOwHATS) Multi Cycle Treasury Program Step 1: Come up with an Acronym

  7. Step 2: TAC chops off 360 orbits…ouch!!! Multi Cycle Treasury Program Step 1: Come up with an Acronym …and the winner is: Panchromatic Hubble Andromeda and Triangulum Survey (PHAT Survey) (1194 orbits)

  8. 1.) ACS/WFC3 Exploratory Survey Of M31's Evolution (AWESOME) 2.) Hubble's Andromeda Panchromatic Panoramic Imaging (HAPPI -- this is a direct reference to ANGST and ANGRRR).   3.) Stellar Evolution in Andromeda Legacy Survey (SEALS) 4.) Andromeda Survey of Stellar Evolution and Time (ASSET) 5.) Andromeda Survey of Stellar Evolution and Stellar States (ASSESS) 6.) A Panchromatic Hubble Andromeda Treasury (PHAT) 7.) The Great Andromeda Survey (GAS). 8.) The Andromeda Project 9.) Project Andromeda 10.) The Andromeda Hubble Atlas (AHA) 11.) Quarter of Andromeda Treasury Survey (QATS) 12.) Panchromatic Hubble Andromeda and Triangulum Survey (PHAT Survey) 13.) Panchromatic Imaging of Triangulum and Andromeda (PITA) 14.) Multiwavelength Mapping of M31 and M33 (MMMM) 15.) Wide-field Hubble Imaging of M31/M33 (WHIM) 16.) Wide-field High-resolution Imaging: Panchromatic Landscape of Andromeda and its Satellite with Hubble (WHIPLASH) 17.) Detailed Imaging of Nearby Galaxies: Boring into Andromeda and Triangulum (DINGBAT) 18.) Panchromatic Imaging of Nearby Galaxies (PING) 19.) Wide-field Imaging of Nearby Galaxies: Stellar Populations in Andromeda and its Neighbor (WINGSPAN) 20.) Wide-field Hubble Imaging of M31/M33 Stars In Color: Astrophysical Labratories (WHIMSICAL) 21.) Stellar Populations of Andromeda and Triangulum (SPAT) 22.) Near-infrared and Optical Survey of Two Resolved and Extended SpiralS (NOSTRESS) 23.) Hubble Ultrawide Multiwavelength M31 and M33 Survey (HUMMMS) 24.) Multiwavelength Andromeda and Triangulum Ultrawide Realization Experiment (MATURE) 25.) Multiwavelength M31 and M33 Ultrawide Survey Campaign Legacy Experiment (MMMUSCLE) 26.) Multiwavelength Andromeda and Triangulum Hubble Survey (MATHS) 27.) Survey with Hubble of Andromeda and Triangulum (SHAT) -- just kidding. 28.) Hubble Areal Mapping of M31 and M33 (HAMMM) 29.) Panchromatic Ultrawide M31 and M33 Extragalactic Legacy (PUMMEL) 30.) Panchromatic Hubble Ultrawide Galaxy Legacy Y-word (PHUGLY) -- also just kidding. 31.) Resolving Andromeda and Triangulum (RAT) 32.) Triangulum/Andromeda Survey Program (TASP) 33.) Galaxy Laboratories: Observing Andromeda and Triangulum (GLOAT) 34.) Galaxy Laboratories Observed with Hubble: the Andromeda and Triangulum Survey (GLOwHATS) Multi Cycle Treasury Program Step 1: Come up with an Acronym

  9. Multi Cycle Treasury Program Science Goals • Stellar Initial Mass Function and Variations with Environment (SFR intensity, metallicity, density). • Study young and old star clusters over a range of ages and metallicity (calibration of models). • Constrain cluster formation and evolutionary processes. • Measure energetics and timescales of ISM through interplay of gas and spatially resolved SFHs. • Characterize full SEDs (spatially resolved) of x-ray binaries, SN remnants, Cepheids, PN, WR stars, • background AGN, and transients (e.g., counterparts and association with surrounding population properties). • - Provide rich probes of gas phase and interaction with SF, through sub-arcsecond extinction mapping. • Spatially resolve SFH in a Galactic bulge and disk, fully sampled over spiral arms. • Map the spiral dynamics, growth of galaxy disk and spheroid, role of tidal interactions/accretion. Bonus Massey et al. (2006) Technical Goal • Resolve M31 into 100 million stars. • Survey provides temperatures for O through M spectral types, with simultaneous • extinction mapping.

  10. Multi Cycle Treasury Program Requirements - Wide-field, high-resolution, ultra-sensitive imaging in the UV, optical, and NIR ACS + WFC3

  11. Multi Cycle Treasury Program Observing Plan -Thanks to ACS and WFC3 teams, plus Merle, Bill, and Alan!

  12. Multi Cycle Treasury Program Synergistic Spectroscopy - Keck/DEIMOS 2010 proposal submitted on Friday (PI Guhathakurta)!

More Related