HOPCAT, 6dF - PowerPoint PPT Presentation

About This Presentation
Title:

HOPCAT, 6dF

Description:

ASTRON The Netherlands, AAO Sydney, WIYN Tucson. etc. ... SUMSS Sydney University Molonglo Sky Survey. 304 Sumss HOPCAT matches. Galaxy Density ... – PowerPoint PPT presentation

Number of Views:59
Avg rating:3.0/5.0
Slides: 18
Provided by: aao2
Category:
Tags: 6df | hopcat | sydney

less

Transcript and Presenter's Notes

Title: HOPCAT, 6dF


1
HOPCAT, 6dF Star Formation Rates
  • Marianne T. Doyle
  • Ph.D. Project

2
Content
Supervisor Michael J. Drinkwater UQ Assoc.
Supervisors Elaine Sadler Uni Sydney John Ross
- UQ Collaborators David J. Rohde - UQ Mike
Read WFAU Edinburgh Baerbel Koribalski ATNF,
Epping HIPASS Team ATNF Parkes Epping,
Universities of Melbourne, Cardiff, Western
Sydney Macarthur, Wales, Swinburne, Technology
Sydney, New Mexico, Manchester, Colorado, Sydney,
Leicester ASTRON The Netherlands, AAO
Sydney, WIYN Tucson etc.......
  • The HIPASS - 6dFGS Connection
  • My Project
  • Investigate the question How does star formation
    depend upon environment and other factors?
  • Finding optical counterparts for the HIPASS
    catalogue
  • Investigating the Morphology-density relation
    using Star Formation Rates, Star Formation
    Efficiency and Galaxy Density

3
The 6dFGS - HIPASS Connection
  • HI Parkes Sky Survey (HIPASS)
  • HI blind radio survey of the southern sky up to
    Dec2o
  • October 2001 2710 additional targets were
    added to the 6dfGS (Thank you Michael Drinkwater)
  • Optical objects included are
  • within 5 arcmin of the HIPASS positions
  • R mag lt 17
  • NOT already in one of the official optical
    target lists for 6dF
  • 341 - highest priority multiple matches to radio
    position 1558 - main sample 811 - faint sample
    (16.7ltRlt17)

4
My PhD Project
  • The question How does the conversion of hydrogen
    to stars (star formation) depend upon environment
    and other factors?
  • Testing two theories
  • Either fewer star forming galaxies actually
    form in regions of high galaxy density,
  • OR
  • There are physical processes that directly
    suppresses star formation.

5
Steps
  • Use radio detected galaxy sample instead of
    optical sample
  • Optical samples are biased towards star forming
    galaxies which is what we are trying to measure.
  • Star Formation Rate (SFR)
  • Star Formation Efficiency (SFE)
  • Local galaxy density

6
Optical Counterpart - HOPCAT
  • HIPASS Catalogue (HICAT) contains 4315 HI radio
    sources
  • Find optical counterparts
  • Accurate galaxy position needed to measure
    luminosity to calculate SFR
  • Search for Dark Galaxies

7
Optical Data
  • OPTICAL IMAGES
  • SuperCOSMOS 15 x 15 Images
  • 7 radius Radio-Optical position uncertainty
  • IMAGE ANALYSIS
  • SExtractor Image Analysis.

8
Is that the right galaxy?
  • Many images have multiple galaxies
  • Crosscheck HIPASS velocity with optical or high
    resolution radio velocities
  • Published velocities NED
  • Information from catalogues, surveys the
    literature Data varies in quality
  • Need a high quality dataset
  • 6dF velocities (Kindly supplied by Heath)
  • Developed an automated visual interactive program
    ADRIC

9
Results
  • Optically Matched with velocity 58 2516
  • Single Match (44 - 1882)
  • Compact group member (14 - 634)
  • Optically Matched with no velocity 26 1107
  • Single Match (20 - 851)
  • Compact group member (6 - 256)
  • No Guess 11 476
  • Several galaxies no velocities
  • Blank Field 5 216
  • No visible galaxy

10
Any Isolated Dark Galaxies in HIPASS?
  • 4315 HI detected objects
  • Extinction cut at ABj lt 1 - 3692 objects
  • Use only blank fields - 13 objects
  • Take out over crowded fields - 2 object remaining
  • 2 remaining objects?
  • 1 is a very faint previously observed galaxy in
    the Centaurus group
  • 1 ruled out with Narrow-band follow-up
    observations at Parkes as a non-detection
  • Conclusion No isolated dark galaxies are present
    in the HIPASS survey

11
HOPCATs Galaxy density coverage
  • Solution?
  • ATCA high resolution HI observations to
    find/confirm optical counterpart in regions of
    high galaxy density
  • Galaxies in regions with Low galaxy density?
  • Large sample
  • Galaxies in regions with High galaxy density?
  • Very small sample

12
Star Formation Density
  • SUMSS radio continuum data
  • 304 Sumss HOPCAT matches
  • Galaxy Density
  • 10th Galaxy radius
  • Galaxy number / degree2
  • Star Formation Rate
  • Star Formation Efficiency

13
(No Transcript)
14
Star Formation Rate Vs Density
15
Star Formation Efficiency Vs Density
  • SUMSS Sydney University Molonglo Sky Survey
  • 304 Sumss HOPCAT matches
  • Galaxy Density
  • 10th Galaxy radius
  • Galaxy number / degree2

16
Summary
  • 2710 optical galaxies near HIPASS positions were
    added to the 6dFGS list

17
ADRIC interactive visual matching program
Write a Comment
User Comments (0)
About PowerShow.com