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The Galactic Halo as seen by Pan-STARRS1

The Galactic Halo as seen by Pan-STARRS1

The Galactic Halo as seen by Pan-STARRS1

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A <strong>Pan</strong>-<strong>STARRS1</strong> View of<br />

the Sagittarius Stream<br />

Colin Slater<br />

Eric Bell (Michigan)<br />

Eddie Schlafly (Harvard -> MPIA)<br />

Mario Juric (Harvard -> LSST)<br />

Nicol<strong>as</strong> Martin (MPIA -> Str<strong>as</strong>bourg)<br />

Hans-Walter Rix (MPIA)<br />

+ PS1 Collaboration


PS1 Survey<br />

1.8 m telescope on Haleakala, 3º FoV<br />

Covers all sky North of -30º (3π)<br />

~40 sec exposures in grizy, cadence optimized for<br />

moving objects<br />

12 fields targeted for Medium Deep survey


Data Processing<br />

Photometric catalogs produced nightly<br />

Images are not stacked nightly<br />

All current 3π catalogs are merged from single-epoch<br />

data<br />

Stacking is underway but CPU-intensive<br />

Survey is übercalibrated (Schlafly et al. 2012, better than 10mmag)


PS1 Coverage<br />

Main Sequence<br />

Turn-off Stars:<br />

0.0 < (g-r) < 0.4


Sagittarius Map<br />

SDSS<br />

Sgr<br />

PS1


Main Sequence Turn-off<br />

l=90º<br />

l=90º<br />

Anti-<br />

GC<br />

GC<br />

l=270º<br />

l=270º


Distance Me<strong>as</strong>urements<br />

Stream visible in MSTO<br />

MSTO is a relatively poor distance indicator<br />

Red Clump is more precise<br />

Combine both for best me<strong>as</strong>urement


Background Regions<br />

Faint Arm Regions<br />

Bright Arm Regions


Example Region CMD<br />

RC<br />

RC


Bright Arm


Faint Arm


Calibration<br />

Sgr dwarf is in PS1 data<br />

P1,<br />

Use dwarf RC to calibrate distances to the stream<br />

Minimizes effects of stellar population differences and<br />

survey differences


Me<strong>as</strong>ured Distances<br />

Bright Arm<br />

Faint Arm<br />

Faint arm consistently closer


Comparison to Models<br />

● Bright Arm<br />

Faint Arm<br />

■ Cetus<br />

Model from Law & Majewski (2010)<br />

Northern points from Niederste-Ostholt et al. (2011)<br />

Cetus from Newberg et al. (2009)


Summary<br />

Sgr stream is bifurcated in North and South<br />

RC is a useful distance indicator for Sgr<br />

Distance to the stream matches model expectations<br />

Faint arm is consistently closer<br />

Unlikely to be confused with Cetus


Origin of Bifurcation<br />

Multiple wraps: unlikely<br />

Internal rotation: unlikely<br />

(Fellhauer+06, but see Yanny+09)<br />

(Peñarrubia+10, but see Peñarrubia+11)<br />

No evidence of internal rotation<br />

Existing sims disagree with trailing arm<br />

Double accretion Plausible Unknown.<br />

Complex dwarf structure Unknown.

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