Araştırma Makalesi
BibTex RIS Kaynak Göster

The Faintest and Closest Clusters in CFHTLS W4

Yıl 2018, , 53 - 58, 31.12.2018
https://doi.org/10.30516/bilgesci.487078

Öz

Introduction

Material and Methods

Results

Discussion

Kaynakça

  • Arnouts, S. et al., 1999, Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North, Monthly Notices of the Royal Astronomical Society, 310, 540.
  • Coleman, G. D. et al., 1980, Colors and magnitudes predicted for high redshift galaxies, The Astrophysics of Journal Suplement, 43, 393C.
  • Coupon, J. et al., 2009, Photometric redshifts for the CFHTLS T0004 deep and wide fields, Astronomy & Astrophysics, 500, 981C.
  • Feuerbacher, B. and Stoewer, H., 2006, Utilization of Space: Today and Tomorrow, Springer, ISBN: 354029970X.
  • Garilli, B., et al., 2014, The VIMOS Public Extragalactic Survey (VIPERS). First Data Release of 57 204 spectroscopic measurements, Astronomy & Astrophysics, 562A, 23G.
  • Hudelot, P. et al., 2012, T0007: The Final CFHTLS Release, CFHTLS, http://www.cfht.hawaii.edu/Science/CFHLS/T0007/, [visiting date: 1st June 2013].
  • Ilbert, O. et al., 2006, Accurate Photometric Redshifts for the CFHT Legacy Survey Calibrated Using the VIMOS VLT Deep Survey, Astronomy & Astrophysics, 457, 841.
  • İğdi-Şen, M. 2018, The Reliability of Redshift Values in Determination of Structures in the Universe, JoCREST, 4, 69-80.
  • Kinney, A. L. et al., 1996, Template Ultraviolet to Near-Infrared Spectra of Star-forming Galaxies and Their Application to K-Corrections, The Astrophysics of Journal, 467, 38.
  • Le Fèvre, O. et al., 2005, The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5, Astronomy & Astrophysics,439, 845L.
  • Terapix1, 2012, CFHTLS-Deep &Wide targets, Terapix, http://terapix.iap.fr/ cplt/T0007/table_syn_T0007.html, [visiting date: 1st January 2015].
  • Wen, Z. L.and Han, J. L., 2011, Galaxy Clusters at High Redshift and Evolution of Brightest Cluster Galaxies, The Astrophysics of Journal, 734, 68W.
Yıl 2018, , 53 - 58, 31.12.2018
https://doi.org/10.30516/bilgesci.487078

Öz

Kaynakça

  • Arnouts, S. et al., 1999, Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North, Monthly Notices of the Royal Astronomical Society, 310, 540.
  • Coleman, G. D. et al., 1980, Colors and magnitudes predicted for high redshift galaxies, The Astrophysics of Journal Suplement, 43, 393C.
  • Coupon, J. et al., 2009, Photometric redshifts for the CFHTLS T0004 deep and wide fields, Astronomy & Astrophysics, 500, 981C.
  • Feuerbacher, B. and Stoewer, H., 2006, Utilization of Space: Today and Tomorrow, Springer, ISBN: 354029970X.
  • Garilli, B., et al., 2014, The VIMOS Public Extragalactic Survey (VIPERS). First Data Release of 57 204 spectroscopic measurements, Astronomy & Astrophysics, 562A, 23G.
  • Hudelot, P. et al., 2012, T0007: The Final CFHTLS Release, CFHTLS, http://www.cfht.hawaii.edu/Science/CFHLS/T0007/, [visiting date: 1st June 2013].
  • Ilbert, O. et al., 2006, Accurate Photometric Redshifts for the CFHT Legacy Survey Calibrated Using the VIMOS VLT Deep Survey, Astronomy & Astrophysics, 457, 841.
  • İğdi-Şen, M. 2018, The Reliability of Redshift Values in Determination of Structures in the Universe, JoCREST, 4, 69-80.
  • Kinney, A. L. et al., 1996, Template Ultraviolet to Near-Infrared Spectra of Star-forming Galaxies and Their Application to K-Corrections, The Astrophysics of Journal, 467, 38.
  • Le Fèvre, O. et al., 2005, The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5, Astronomy & Astrophysics,439, 845L.
  • Terapix1, 2012, CFHTLS-Deep &Wide targets, Terapix, http://terapix.iap.fr/ cplt/T0007/table_syn_T0007.html, [visiting date: 1st January 2015].
  • Wen, Z. L.and Han, J. L., 2011, Galaxy Clusters at High Redshift and Evolution of Brightest Cluster Galaxies, The Astrophysics of Journal, 734, 68W.
Toplam 12 adet kaynakça vardır.

Ayrıntılar

Birincil Dil İngilizce
Konular Metroloji,Uygulamalı ve Endüstriyel Fizik
Bölüm Araştırma Makaleleri
Yazarlar

Mukadder İğdi-şen 0000-0002-0760-1752

Yayımlanma Tarihi 31 Aralık 2018
Kabul Tarihi 28 Aralık 2018
Yayımlandığı Sayı Yıl 2018

Kaynak Göster

APA İğdi-şen, M. (2018). The Faintest and Closest Clusters in CFHTLS W4. Bilge International Journal of Science and Technology Research, 2, 53-58. https://doi.org/10.30516/bilgesci.487078