Methods for identifying high‐redshift galaxy cluster candidates-Reference-Cited by-同舟云学术

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Methods for identifying high‐redshift galaxy cluster candidates

Published:2019-08 Issue:7 Volume:340 Page:618-621
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr

Author:

Pinter Sandor¹²,Balázs Lajos G.²³,Bagoly Zsolt⁴,Horvath Istvan¹,Rácz István I.¹⁴,Tóth Viktor L.²

Affiliation:

1. Department of Natural ScienceNational University of Public Service Budapest Hungary

2. Department of AstronomyEötvös University Budapest Hungary

3. MTA CSFK Konkoly Observatory Budapest Hungary

4. Physics of Complex Systems DepartmentEötvös University Budapest Hungary

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.201913665

Reference31 articles.

1. The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library

2. Amati L. Atteia J.‐L. Balazs L.et al.2013 White paper arXiv:1306.5259.

3. Gamma photometric redshifts for long gamma-ray bursts

4. A giant ring-like structure at 0.78 < z < 0.86 displayed by GRBs

5. Photometric redshifts for the SDSS Data Release 12

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