white dwarfs in the het dark energy experiment bárbara g. castanheira the university of texas at...

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White Dwarfs in the HET Dark Energy Experiment Bárbara G. Castanheira The University of Texas at Austin Universität Wien 17 th European White Dwarf Workshop – Tübingen, August 16-20, 2010

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White Dwarfs in the HET Dark Energy Experiment

Bárbara G. Castanheira

The University of Texas at AustinUniversität Wien

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Hobby-Eberly Telescope

Location: McDonald Observatory (30° 40' N)

Low cost: 15-20% of the cost of a 9 m telescope

Primary mirror: 11.1 x 9.8 m (9.2 m effective aperture)

91 hexagonal mirrors

Fixed elevation angle of 55o (tilted Arecibo design)

Access 81% of the sky

Queue schedule

Instruments: HRS, LRS, MRS

Model for SALT

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX: HET Dark Energy Experiment

Goal: probe dark energy

Observations: ~ 1400 hours in 3 years

Technique: expansion of the universe at 0<z<4

Main targets: Lyman-α emitting galaxies

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

(Hill et al. 2008)

Dark energy:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Supernovae discovery of accelerated expansion

Within GR: smooth energy with large negative pressure

75% of the universe

Acceleration began at z~0.4 and t~10Gyr

(Frieman et al. 2008)

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Destiny of the universe depends critically upon the nature of dark energy!

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX field:

VIRUS-P Review: Visual Integral-field Replicable Unit

Spectrograph - Prototype

1.9’x1.9’ FOV at 2.7 m HJST

1/3 fill factor

Largest FOV of any existing IFU

4.2’’ diameter fibers on sky

3500-5800Å wavelength range

R=1000 @ 5000Å

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Flux calibrating the pilot survey:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Feige 34

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 1:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 2:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 3:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 4:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 5:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 6:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Feige 34:

VIRUS-P

2.7m HJST

6x120s

V=11.2

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX details:

150 VIRUS3500-5500Å~3400 spectraFOV 22arcminResolution ~5Å~140 nights, 3 years

PARALLEL SURVEY

(Drory 2010)

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

White Dwarfs in HETDEX

~20000 White Dwarfs

Magnitude limited sample

For V=22, S/N=3

Main and Parallel surveys

A powerful survey!

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX current status:

Schedule: late 2011

VIRUS-P at HET

Replication of spectrographs

Software (CURE or VACCINE & DIAGNOSE)

Additional science

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

White dwarf science goals:

WD Luminosity Function

New candidates of pulsators (2.1m)

New “flavors” of WDs?

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

[email protected]

Danke! Obrigada!