AN INTENSIVE HUBBLE SPACE TELESCOPE SURVEY FOR z>1 TYPE Ia SUPERNOVAE BY TARGETING GALAXY CLUSTERS

AN INTENSIVE HUBBLE SPACE TELESCOPE SURVEY FOR z>1 TYPE Ia SUPERNOVAE BY TARGETING GALAXY CLUSTERS
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DOI：
10.1088/0004-6256/138/5/1271
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发表时间：
2009-08
期刊：
The Astronomical Journal
影响因子：
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通讯作者：
Kyle S. Dawson;Kyle S. Dawson;G. Aldering;R. Amanullah;K. Barbary;K. Barbary;L. Barrientos;M. Brodwin;N. Connolly;A. Dey;M. Doi;M. Donahue;P. Eisenhardt;E. Ellingson;L. Faccioli;V. Fadeyev;H. Fakhouri;H. Fakhouri;A. Fruchter;D. Gilbank;M. Gladders;G. Goldhaber;G. Goldhaber;Anthony H. Gonzalez;A. Goobar;A. Gude;Takashi Hattori;H. Hoekstra;H. Hoekstra;H. Hoekstra;X. Huang;Y. Ihara;B. Jannuzi;David E. Johnston;David E. Johnston;K. Kashikawa;B. Koester;K. Konishi;M. Kowalski;C. Lidman;E. Linder;L. Lubin;J. Meyers;J. Meyers;T. Morokuma;F. Munshi;C. Mullis;T. Oda;N. Panagia;S. Perlmutter;S. Perlmutter;M. Postman;T. Pritchard;T. Pritchard;J. Rhodes;P. Rosati;David Rubin;David Rubin;D. Schlegel;A. Spadafora;S. Stanford;S. Stanford;V. Stanishev;V. Stanishev;D. Stern;M. Strovink;M. Strovink;N. Suzuki;N. Takanashi;K. Tokita;M. N. Wagner;M. N. Wagner;Lianqi Wang;N. Yasuda;H. Yee
Kyle S. Dawson;Kyle S. Dawson;G. Aldering;R. Amanullah;K. Barbary;K. Barbary;L. Barrientos;M. Brodwin;N. Connolly;A. Dey;M. Doi;M. Donahue;P. Eisenhardt;E. Ellingson;L. Faccioli;V. Fadeyev;H. Fakhouri;H. Fakhouri;A. Fruchter;D. Gilbank;M. Gladders;G. Goldhaber;G. Goldhaber;Anthony H. Gonzalez;A. Goobar;A. Gude;Takashi Hattori;H. Hoekstra;H. Hoekstra;H. Hoekstra;X. Huang;Y. Ihara;B. Jannuzi;David E. Johnston;David E. Johnston;K. Kashikawa;B. Koester;K. Konishi;M. Kowalski;C. Lidman;E. Linder;L. Lubin;J. Meyers;J. Meyers;T. Morokuma;F. Munshi;C. Mullis;T. Oda;N. Panagia;S. Perlmutter;S. Perlmutter;M. Postman;T. Pritchard;T. Pritchard;J. Rhodes;P. Rosati;David Rubin;David Rubin;D. Schlegel;A. Spadafora;S. Stanford;S. Stanford;V. Stanishev;V. Stanishev;D. Stern;M. Strovink;M. Strovink;N. Suzuki;N. Takanashi;K. Tokita;M. N. Wagner;M. N. Wagner;Lianqi Wang;N. Yasuda;H. Yee
中科院分区：
其他
文献类型：
--
作者：
Kyle S. Dawson;Kyle S. Dawson;G. Aldering;R. Amanullah;K. Barbary;K. Barbary;L. Barrientos;M. Brodwin;N. Connolly;A. Dey;M. Doi;M. Donahue;P. Eisenhardt;E. Ellingson;L. Faccioli;V. Fadeyev;H. Fakhouri;H. Fakhouri;A. Fruchter;D. Gilbank;M. Gladders;G. Goldhaber;G. Goldhaber;Anthony H. Gonzalez;A. Goobar;A. Gude;Takashi Hattori;H. Hoekstra;H. Hoekstra;H. Hoekstra;X. Huang;Y. Ihara;B. Jannuzi;David E. Johnston;David E. Johnston;K. Kashikawa;B. Koester;K. Konishi;M. Kowalski;C. Lidman;E. Linder;L. Lubin;J. Meyers;J. Meyers;T. Morokuma;F. Munshi;C. Mullis;T. Oda;N. Panagia;S. Perlmutter;S. Perlmutter;M. Postman;T. Pritchard;T. Pritchard;J. Rhodes;P. Rosati;David Rubin;David Rubin;D. Schlegel;A. Spadafora;S. Stanford;S. Stanford;V. Stanishev;V. Stanishev;D. Stern;M. Strovink;M. Strovink;N. Suzuki;N. Takanashi;K. Tokita;M. N. Wagner;M. N. Wagner;Lianqi Wang;N. Yasuda;H. Yee

文献摘要

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我们提出了一种利用哈勃太空望远镜（HST）发现和研究高红移Ia型超新星（SNe Ia）的新巡天策略。通过瞄准0.9 0.95的大质量星系团，其中9个在星系团中。该策略提供了一个SN样本，可用于解耦高红移SNe中宿主星系消光和本征颜色的影响，从而减少了SN宇宙学中最大的系统不确定性之一。
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST). By targeting massive galaxy clusters at 0.9 0.95, nine of which were in galaxy clusters. This strategy provides an SN sample that can be used to decouple the effects of host-galaxy extinction and intrinsic color in high-redshift SNe, thereby reducing one of the largest systematic uncertainties in SN cosmology.