Elizabeth R. Stanway

Probing $\sim L_{*}$ Lyman-break Galaxies at $z\approx 7$ in GOODS-South with WFC3 on HST (2009)

Wilkins, Stephen M., Bunker, Andrew J., Ellis, Richard S., Stark, Daniel, Stanway, Elizabeth R., Chiu, Kuenley, ...

We analyse recently acquired near-infrared Hubble Space Telescope imaging of the GOODS-South field to search for star forming galaxies at z~7.0. By comparing WFC 3 0.98 micron Y-band images with ACS...

Spectral synthesis including massive binaries (2009)

Eldridge, John J., Stanway, Elizabeth R.

We have constructed a new code to produce synthetic spectra of stellar populations that includes massive binaries. We have tested this code against the broadband colours of unresolved young massive...

A Limit on the Number Density of Bright z~7 Galaxies (2008)

Stanway, Elizabeth R., Bremer, Malcolm N., Squitieri, Valentina, Douglas, Laura S., Lehnert, Matthew D.

We present a survey of bright optical dropout sources in two deep, multiwavelength surveys comprising eleven widely-separated fields, aimed at constraining the galaxy luminosity function at z~7 for...

Discovery of a single faint AGN in a large sample of z>5 Lyman break galaxies (2007)

Douglas, Laura S., Bremer, Malcolm N., Stanway, Elizabeth R., Lehnert, Matthew D.

As part of a large spectroscopic survey of z>5 Lyman break galaxies (LBGs), we have identified a single source which is clearly hosting an AGN. Out of a sample of more than fifty...

The stellar mass density at z ~6 from Spitzer imaging of i'-drop galaxies (2007)

Eyles, Laurence P., Bunker, Andrew J., Ellis, Richard S., Lacy, Mark, Stanway, Elizabeth R., Stark, Daniel P., ...

We measure the ages, stellar masses, and star formation histories of z ~6 galaxies, observed within 1 Gyr of the big bang. We use imaging from the Hubble Space Telescope (HST) and the Spitzer Space...

The GLARE Survey II. Faint z=6 Ly-alpha Line Emitters in the HUDF (2007)

Stanway, Elizabeth R, Bunker, Andrew J, Glazebrook, Karl, Abraham, Roberto G, Rhoads, James, Malhotra, Sangeeta, ...

The galaxy population at z~6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) -- the deepest imaging survey yet. A large number of high...

The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)

Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...

The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...

The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)

Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...

The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...

The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)

Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...

The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...

The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)

Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...

The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...

The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)

Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...

The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...

A Matched Catalogue i-dropout galaxies at z~6 in the Hubble Ultra Deep Field (2004)

Bunker, Andrew J, Stanway, Elizabeth R.

A recent preprint by Yan & Windhorst (astro-ph/0407493) independently repeats our selection of candidate z~6 galaxies in the Hubble Ultra Deep Field (astro-ph/0403223). The agreement of this...

Three Ly alpha emitters at z ≈ 6: early GMOS/Gemini data from the GLARE project (2004)

Stanway, Elizabeth R., Glazebrook, Karl, Bunker, Andrew J., Abraham, R. G., Hook, Isobel, Rhoads, James, ...

We report spectroscopic detection of three z ∼ 6 Lyα-emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman Alpha at Reionisation Era...

Three Ly alpha emitters at z ≈ 6: early GMOS/Gemini data from the GLARE project (2004)

Stanway, Elizabeth R., Glazebrook, Karl, Bunker, Andrew J., Abraham, R. G., Hook, Isobel, Rhoads, James, ...

We report spectroscopic detection of three z ∼ 6 Lyα-emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman Alpha at Reionisation Era (GLARE)...

Three Lyman-alpha Emitters at z approx 6: Early GMOS/Gemini Data from the GLARE Project (2003)

Stanway, Elizabeth R., Glazebrook, Karl, Bunker, Andrew J., Abraham, Roberto G., Hook, Isobel, Rhoads, James, ...

We report spectroscopic detection of three z~6 Lyman-alpha emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman-$\alpha$ at Reionisation Era...

A star-forming galaxy at z=5.78 in the Chandra Deep Field South (2003)

Bunker, Andrew J., Stanway, Elizabeth R., Ellis, Richard S., McMahon, Richard G., McCarthy, Patrick J.

We report the discovery of a luminous z=5.78 star-forming galaxy in the Chandra Deep Field South. This galaxy was selected as an `i-drop' from the GOODS public survey imaging with HST/ACS (object 3...