The First Galaxies and Galaxy Clusters Export

@inproceedings{citeulike:4510879, abstract = {Obvious targets for Extremely Large Telescopes are high-redshift galaxies and galaxy (proto-)clusters. However, due to the extremely small field-of-view of such telescopes, finding such objects, notably the rarer proto-clusters, is best be done using other facilities. The very helpful negative K-correction experienced in the far-IR to mm wavebands makes surveys in these wavebands the ideal pathfinders for high-z ELT targets.}, author = {{Kampen}, {van E.}}, booktitle = {Science with the VLT in the ELT Era}, citeulike-article-id = {4510879}, citeulike-linkout-0 = {http://dx.doi.org/10.1007/978-1-4020-9190-2_31}, citeulike-linkout-1 = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2009svlt.conf..183V}, doi = {10.1007/978-1-4020-9190-2_31}, editor = {{moorwood}, A.}, keywords = {elt, evolution, formation, galaxy, high-z}, posted-at = {2009-05-13 23:27:18}, priority = {2}, title = {{The First Galaxies and Galaxy Clusters}}, url = {http://dx.doi.org/10.1007/978-1-4020-9190-2_31}, year = {2009} }

TY - CONF ID - citeulike:4510879 L3 - citeulike-article-id:4510879 N2 - Obvious targets for Extremely Large Telescopes are high-redshift galaxies and galaxy (proto-)clusters. However, due to the extremely small field-of-view of such telescopes, finding such objects, notably the rarer proto-clusters, is best be done using other facilities. The very helpful negative K-correction experienced in the far-IR to mm wavebands makes surveys in these wavebands the ideal pathfinders for high-z ELT targets. TI - {The First Galaxies and Galaxy Clusters} T2 - Science with the VLT in the ELT Era KW - elt KW - evolution KW - formation KW - galaxy KW - high-z AU - Kampen}, {van A2 - {moorwood}, A PY - 2009/// UR - http://dx.doi.org/10.1007/978-1-4020-9190-2_31 ER -