Wfc3 - PowerPoint Presentations and PDF Documents

The New WFC3 Photometric Calibration

by alexa-scheidler

Outline. 1.) Step 1 – TV3 Calibration. 2.) Step...

WFC3 Spatial Scanning (

by calandra-battersby

Exoplanets. ). STScI. Calibration Workshop. Aug ...

WFC3 slitless spectroscopy

by lindy-dunigan

Harald Kuntschner. Martin . Kümmel. , Jeremy Wal...

CLASH:

by natalia-silvester

. C. luster . L. ensing . A. nd . S. upernova su...

Through a Lens, Darkly:

by kittie-lecroy

An Innovative. Multi-cycle Hubble Treasury Progr...

American Astronomical Society meeting, Jan 9-12, 2012, Aust

by faustina-dinatale

Acknowledgments. Zach . Berta (Harvard), the P.I....

High-

by alexa-scheidler

Redshift. Galaxies . in Cluster Fields. Wei Zhen...

How Does WFC3 Geometric Distortion Vary with Time ?

by stefany-barnette

Kozhurina-Platais. Ω. Cen observed with the . ...

Through a Lens, Darkly:

by phoebe-click

An Innovative. Multi-cycle Hubble Treasury Progr...

Avi M.

by celsa-spraggs

Mandell. NASA GSFC. Collaborators. :. Korey. Hay...

Cluster views of the high redshift universe

by tatiana-dople

Leonidas . Moustakas. , JPL/Caltech. CLASH London...

Mission Engineering and Science Analysis

by tatyana-admore

(. MESA). Jeff Valenti. What is MESA?. 2. 2012 In...

Wide-Field Slitless

by karlyn-bohler

Spectr. . scopy. with NIRISS. Van Dixon. STScI...

Avi M.

by luanne-stotts

Mandell. NASA GSFC. Collaborators. :. Korey. Hay...

Data Pipeline Wei Zheng

by kittie-lecroy

Johns Hopkins University. Requirements. Science i...

Direct Test of Brown Dwarf Models Through Secondary Eclipse Spectroscopy of LHS 6343 C

by della

William Frost. MSc - . UdeM. In collaboration with...

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