Calibrating Cepheid Sequences in Nearby Galaxies

Metcalfe, N.; Shanks, T.

VST ATLAS: Science Goals and Status (2012)
Conference Proceeding
Shanks, T., & Metcalfe, N. (2012). VST ATLAS: Science Goals and Status. In Science from the Next Generation Imaging and Spectroscopic Surveys, ESO Garching, 15-18 October 2012

CEOI microslice spectrograph (2012)
Conference Proceeding
Content, R., Blake, S., Dunlop, C., Nandi, D., Sharples, R., Talbot, G., …Luke, P. (2012). CEOI microslice spectrograph. . https://doi.org/10.1117/12.927267

VXMS: the VISTA extreme multiplex spectrograph (2012)
Conference Proceeding
Content, R., Shanks, T., Sharples, R., Bramall, D., & Percival, W. (2012). VXMS: the VISTA extreme multiplex spectrograph. . https://doi.org/10.1117/12.927260

Cosmological Parameters 2006 (2007)
Conference Proceeding
Sánchez, A., & Baugh, C. (2007). Cosmological Parameters 2006. In N. Metcalfe, & T. Shanks (Eds.), Cosmic Frontiers: proceedings of a conference held at Department of Physics, Durham University, Durham, UK, 31 July-4 August 2006

Recent measurements of the cosmic microwave background radiation (CMB), particularly when combined with other datasets, have revolutionised our knowledge of the values of the basic cosmological parameters. Here we summarize the state of play at the e... Read More about Cosmological Parameters 2006.

Do Galaxies Form at High Redshift? (2002)
Conference Proceeding
Metcalfe, N., Shanks, T., Fong, D., McCracken, H. J., Campos, A., Gardner, J. P., & Thompson, D. (2002). Do Galaxies Form at High Redshift?.

Studying Large-scale Structure with the 2dF Galaxy Redshift Survey (2002)
Conference Proceeding
Peacock, J. A., & et al. (2002). Studying Large-scale Structure with the 2dF Galaxy Redshift Survey. In N. Metcalfe, & T. Shanks (Eds.),

Evidence for Galaxy Formation at High Redshift. (2001)
Conference Proceeding
Shanks, T., Metcalfe, N., Fong, D., McCracken, H., Campos, A., & Thompson, D. (2001). Evidence for Galaxy Formation at High Redshift. In M. Harwit, & M. G. Hauser (Eds.),

We present new evidence that simple evolutionary models where the star-formation rate in galaxies increases exponentially with redshift but the space density of galaxies remains constant with redshift, give very precise fits to the number count of Ly... Read More about Evidence for Galaxy Formation at High Redshift..

Galaxy Clustering in the Herschel Deep Field. (2000)
Conference Proceeding
McCracken, H., Metcalfe, N., Shanks, T., Fong, R., Campos, A., & Gardner, J. P. (2000). Galaxy Clustering in the Herschel Deep Field. In A. Mazure, O. Le Fèvre, & V. Le Brun (Eds.),

Integral Field and Multi-Object Spectroscopy with the NGST. (1998)
Conference Proceeding
Davies, R., Allington-Smith, J., Metcalfe, N., & Shanks, T. (1998). Integral Field and Multi-Object Spectroscopy with the NGST. In B. Kaldeich (Ed.),

Galaxy Counts; Sizes; Colours and Redshifts in the Hubble Deep Field. (1998)
Conference Proceeding
Shanks, T., Metcalfe, N., Fong, R., McCracken, H., Campos, A., & Gardner, J. (1998). Galaxy Counts; Sizes; Colours and Redshifts in the Hubble Deep Field. In S. D'Odorico, A. Fontana, & E. Giallongo (Eds.),

Galaxy Counts, Colours and Redshifts in the Hubble and Herschel Deep Fields. (1997)
Conference Proceeding
Shanks, T., Metcalfe, N., Campos, A., Fong, R., & Gardner, J. (1997). Galaxy Counts, Colours and Redshifts in the Hubble and Herschel Deep Fields. In N. R. Tanvir, A. Aragon-Salamanca, & J. V. Wall (Eds.),

Faint Galaxy Number Counts. (1996)
Conference Proceeding
Metcalfe, N., Shanks, T., Fong, R., Gardner, J., & Roche, N. (1996). Faint Galaxy Number Counts. In R. Bender, & R. Davies (Eds.),

The Faint Galaxy Contribution to the X-ray Background (1996)
Conference Proceeding
Shanks, T., Almaini, O., Boyle, B., della Ceca, R., Done, C., Georgantopoulos, I., …C., G. (1996). The Faint Galaxy Contribution to the X-ray Background.

Photometric Calibration and Large-Scale Clustering in the Universe. (1994)
Conference Proceeding
Fong, R., Metcalfe, N., & Shanks, T. (1994). Photometric Calibration and Large-Scale Clustering in the Universe. In H. T. MacGillivray, E. B. Thomson, B. M. Lasker, I. N. Reid, D. F. Malin, R. M. West, & H. Lorenz (Eds.),

Galaxy Number-Counts to B =28m (1994)
Conference Proceeding
Metcalfe, N., Shanks, T., Roche, N., & Fong, R. (1994). Galaxy Number-Counts to B =28m. In H. MacGillivray, E. Thomson, B. Lasker, I. Reid, D. Malin, R. West, & H. Lorenz (Eds.),

Galaxy Clustering to B = 27m. (1994)
Conference Proceeding
Roche, N., Shanks, T., Metcalfe, N., & Fong, R. (1994). Galaxy Clustering to B = 27m. In H. MacGillivray, E. Thomson, B. Lasker, I. Reid, D. Malin, R. West, & H. Lorenz (Eds.),

A Virgo Galaxy Resolved via WHT MARTINI Image Sharpening (1993)
Conference Proceeding
Shanks, T., Tanvir, N., Doel, A., Dunlop, C., Major, J., & Myers, R. (1993). A Virgo Galaxy Resolved via WHT MARTINI Image Sharpening.

Galaxy Number-Counts to B = 28m (1993)
Conference Proceeding
Metcalfe, N., Shanks, T., Roche, N., & Fong, R. (1993). Galaxy Number-Counts to B = 28m. In C. W. Akerlof, & M. A. Srednicki (Eds.),

A High Resolution, Ground Based Observation of a Virgo Galaxy (1991)
Conference Proceeding
Shanks, T., Tanvir, N., Doel, P., Dunlop, C., Myers, R., Major, J., …O'Kane, P. (1991). A High Resolution, Ground Based Observation of a Virgo Galaxy.

Calibrating Cepheid Sequences in Nearby Galaxies (1991)
Conference Proceeding
Metcalfe, N., & Shanks, T. (1991). Calibrating Cepheid Sequences in Nearby Galaxies.

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