MAssive Cluster Survey

{{more citations needed|date=December 2012}}

{{Infobox astronomical survey}}

The MAssive Cluster Survey (MACS){{cite journal|last=Ebeling|first=Harald|author2=Alastair Edge|author3=J. Patrick Henry|title=MACS: A Quest for the Most Massive Galaxy Clusters in the Universe|journal=Astrophysical Journal|volume=553|date=2001|issue=2|page=668|doi=10.1086/320958|bibcode = 2001ApJ...553..668E |arxiv = astro-ph/0009101 |s2cid=15324781 }}{{cite journal|last=Ebeling|first=Harald|author2=Elizabeth Barrett |author3=David Donovan |author4=Cheng-Jiun Ma |author5=Alastair Edge |author6=Leon van Speybroeck |title=A Complete Sample of 12 Very X-Ray Luminous Galaxy Clusters at z > 0.5|journal=Astrophysical Journal Letters|volume=661|date=2007|issue=661|page=33|doi=10.1086/518603|bibcode = 2007ApJ...661L..33E |arxiv = astro-ph/0703394 |s2cid=118914497 }} compiled and characterized a sample of very X-ray luminous (and thus, by inference, massive), distant clusters of galaxies. The sample comprises 124 spectroscopically confirmed clusters at 0.3 < z < 0.7. Candidates were selected from the ROSAT All-Sky Survey data.[http://www.ifa.hawaii.edu/~ebeling/clusters/MACS.html MAssive Cluster Survey (MACS)]

Cluster candidates that are south of declination -40° cannot be observed from Mauna Kea and fit into the Southern MACS (SMACS) extension. They are also being investigated when facilities are available.{{Cite journal |last1=Repp |first1=A |last2=Ebeling |first2=H |date=2018-09-01 |title=Science from a glimpse: Hubble SNAPshot observations of massive galaxy clusters |journal=Monthly Notices of the Royal Astronomical Society |volume=479 |issue=1 |pages=844–864 |doi=10.1093/mnras/sty1489 |doi-access=free |issn=0035-8711|arxiv=1706.01263 }}

History

One of the galaxy clusters, MACS J0647+7015 was found to have gravitationally lensed the most distant galaxy (MACS0647-JD) then ever imaged, in 2012, by CLASH. The first statistical study of X-ray cavities in distant clusters of galaxies was performed by analyzing the Chandra X-ray observations of MACS. Out of 76 clusters representing a sample of the most luminous X-ray clusters, observers found 13 cut and clear cavities and 7 possible cavities. A new radio halo, as well as a relic applicant, were found in MACS, with the help of the Giant Meterwave Radio Telescope and the Karoo Array Telescope-7. The discovered radio halo has a largest linear scale of about 0.9Mpc. X-ray chosen clusters are almost free of projection effects because they are composed of intrinsically massive, gravitationally collapsed systems.

MACS team

The MACS team consists of:

Survey notation

Objects are labelled as JHHMM.m+DDMM where HHMM+DDMM are the coordinates in the J2000 system. Here H, D, and M refer to hours, degrees, and minutes, respectively, and m refers to tenths of minutes of time.

  • HH Hours of right ascension
  • MM.m Minutes of right ascension or declination
  • DD.d Degrees in declination

Southern MAssive Cluster Survey

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The Southern MAssive Cluster Survey (SMACS) involved the Hubble Space Telescope.

Notable surveyed objects

class="wikitable sortable"
| Survey objectRight ascensionDeclinationNotes
| MACS J0025.4-1222{{RA|00|25.4}}{{DEC
12|22}}
| MACS J0358.8-2955{{RA|03|58.8}}{{DEC
29.5}}Part of Abell 3192[https://science.nasa.gov/missions/hubble/hubble-views-a-double-cluster-of-glowing-galaxies/ NASA: Hubble Views a Double Cluster of Glowing Galaxies]
| MACS J0416.1-2403{{RA|04|16|9.9}}{{DEC|−24|03|58}}
| MACS J0647+7015{{RA|06|47}}{{DEC|+70|15}}
| MACS J0717.5+3745{{RA|07|17.5}}{{DEC|+37|45}}
| SMACS J0723.3–7327{{RA|07|23}}{{DEC
73|27}}Subject of first JWST deep field
| MACS J1149 Lensed Star 1{{RA|11|49|35.59}}{{DEC|22|23|47.4}}Blue supergiant star observed through a gravitational lens
| MACS 1423-z7p64{{RA|14|23}}{{DEC|24|04}}Most distant galaxy known as of April 2017
| MACS 2129-1{{RA|21|29}}{{DEC|−1}}

References

{{Reflist}}