The HectoMAP Cluster Survey. II. X-Ray Clusters
Abstract
Here, we apply a friends-of-friends algorithm to the HectoMAP redshift survey and cross-identify associated X-ray emission in the ROSAT All-Sky Survey data (RASS). The resulting flux-limited catalog of X-ray cluster surveys is complete to a limiting flux of ~3 × 10–13 erg s–1 cm–2 and includes 15 clusters (7 newly discovered) with redshifts z ≤ 0.4. HectoMAP is a dense survey (~1200 galaxies deg–2) that provides ~50 members (median) in each X-ray cluster. We provide redshifts for the 1036 cluster members. Subaru/Hyper Suprime-Cam imaging covers three of the X-ray systems and confirms that they are impressive clusters. The HectoMAP X-ray clusters have an L X–σ cl scaling relation similar to that of known massive X-ray clusters. The HectoMAP X-ray cluster sample predicts ~12,000 ± 3000 detectable X-ray clusters in RASS to the limiting flux, comparable with previous estimates.
- Authors:
-
[1];
[1];
[4];
[5];
- Smithsonian Astrophysical Observatory, Cambridge, MA (United States)
- Max-Planck-Institut fur extraterrestrische Physik, Garching (Germany)
- Univ. di Torino, Torino (Italy); Istituto Nazionale di Fisica Nucleare (INFN), Torino (Italy)
- Korea Institute for Advanced Study, Seoul (Republic of Korea)
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Western Washington Univ., Bellingham, WA (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1437171
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 855; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; galaxies: clusters: general; galaxies: clusters: individual (A2198); large-scale structure of universe; X-rays: galaxies: clusters
Citation Formats
Sohn, Jubee, Chon, Gayoung, Bohringer, Hans, Geller, Margaret J., Diaferio, Antonaldo, Hwang, Ho Seong, Utsumi, Yousuke, and Rines, Kenneth J. The HectoMAP Cluster Survey. II. X-Ray Clusters. United States: N. p., 2018.
Web. doi:10.3847/1538-4357/aaac7a.
Sohn, Jubee, Chon, Gayoung, Bohringer, Hans, Geller, Margaret J., Diaferio, Antonaldo, Hwang, Ho Seong, Utsumi, Yousuke, & Rines, Kenneth J. The HectoMAP Cluster Survey. II. X-Ray Clusters. United States. https://doi.org/10.3847/1538-4357/aaac7a
Sohn, Jubee, Chon, Gayoung, Bohringer, Hans, Geller, Margaret J., Diaferio, Antonaldo, Hwang, Ho Seong, Utsumi, Yousuke, and Rines, Kenneth J. Sat .
"The HectoMAP Cluster Survey. II. X-Ray Clusters". United States. https://doi.org/10.3847/1538-4357/aaac7a. https://www.osti.gov/servlets/purl/1437171.
@article{osti_1437171,
title = {The HectoMAP Cluster Survey. II. X-Ray Clusters},
author = {Sohn, Jubee and Chon, Gayoung and Bohringer, Hans and Geller, Margaret J. and Diaferio, Antonaldo and Hwang, Ho Seong and Utsumi, Yousuke and Rines, Kenneth J.},
abstractNote = {Here, we apply a friends-of-friends algorithm to the HectoMAP redshift survey and cross-identify associated X-ray emission in the ROSAT All-Sky Survey data (RASS). The resulting flux-limited catalog of X-ray cluster surveys is complete to a limiting flux of ~3 × 10–13 erg s–1 cm–2 and includes 15 clusters (7 newly discovered) with redshifts z ≤ 0.4. HectoMAP is a dense survey (~1200 galaxies deg–2) that provides ~50 members (median) in each X-ray cluster. We provide redshifts for the 1036 cluster members. Subaru/Hyper Suprime-Cam imaging covers three of the X-ray systems and confirms that they are impressive clusters. The HectoMAP X-ray clusters have an L X–σ cl scaling relation similar to that of known massive X-ray clusters. The HectoMAP X-ray cluster sample predicts ~12,000 ± 3000 detectable X-ray clusters in RASS to the limiting flux, comparable with previous estimates.},
doi = {10.3847/1538-4357/aaac7a},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 855,
place = {United States},
year = {Sat Mar 10 00:00:00 EST 2018},
month = {Sat Mar 10 00:00:00 EST 2018}
}
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