3D-DASH

The Widest Near-Infrared Hubble Space Telescope Survey

 
 

The 3D-DASH F160W Mosaic

The 3D-Drift And SHift (3D-DASH) program is a Hubble Space Telescope WFC3 F160W imaging and G141 grism survey of the equatorial COSMOS field. 3D-DASH is the widest HST/WFC3 imaging survey in the F160W filter to date, subsuming the COSMOS-DASH pilot survey (Mowla et al. 2019b). 3D-DASH extends the legacy of HST near-infrared imaging and spectroscopy to degree-scale swaths of the sky, enabling the identification and study of distant galaxies (z > 2) that are rare or in short-lived phases of galaxy evolution at rest-frame optical wavelengths.

All our data products are available on our MAST page.

The 3D-DASH Explorer

You can now explore the entire mosaic in all available filters using the FitsMap (credit: Gabe Brammer).

Cutout and psf

You can generate point spread functions or create cutouts at any location within the 3D-DASH footprint in this notebook.

Grism Spectroscopy (G141) Coming Soon

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Grism Spectroscopy (G141) Coming Soon 〰️

 

Observation

Observed with the efficient Drift And SHift technique, the 3D-DASH F160W imaging mosaic comprises over a thousand individual WFC3 pointings built up over the course of years. The full mosaic includes all ancillary F160W data in the COSMOS field (including CANDELS).

Image credit: Ivelina Momcheva (PI)

 
 

team

Ivelina Momcheva (PI)

Rachel Bezanson, Gabriel Brammer, Sam Cuter, Marijn Franx, Kartheik Iyer, Danilo Marchesini, Lamiya Mowla, Adam Muzzin, Erica Nelson, Natascha Förster Schreiber, Rosalind Skelton, Greg Snyder, David Wake, Stijn Wuyts, Kate Whitaker, Pieter van Dokkum, Arjen van der Wel