Table 2.

Radio observation summary for the SUCCESS sample. Columns are: (1) Cluster name; (2) Right Ascension; (3) Declination; (4) Date of observation; (5) Telescope; (6) Observing frequency and duration; (7) Root mean square noise in the image with robust =0.0; (8) Beam and position angle (p. a.); and (9) Remark. The remarks regarding detection of diffuse radio emission (RH = radio halo, MH = Mini-halo candidate, DR = double relic, c= candidate), previous reference (if any), and comments on the data quality are provided as applicable (x  = We have not used this data due to the poor SNR of the data).

(1)(2)(3)(4)(5)(6)(7)(8)(9)
NameRAJ2000Dec.J2000DateTelescopeν, tobsrmsbeamRemark
hms|$^{\circ }\, ^{\prime }\, ^{\prime \prime }$|MHz, hmJy beam−1″ × ″, p. a.
RXC J1358.9-475013h58m42s.64-47°48 ′41″.92016-10-24GMRT325, 50.5019.4 × 6.7, 6.4°
RXC J0232.2-442002h32m18s.7-44°20′41″.02017-02-18GMRT610, 60.049.2 × 3.9, 6.3°RHb
2019-01-13MeerKAT1283, 90.00267.1 × 7.1, 86.5°RHa
MeerKAT1283, 90.0115 × 15 arcsec2
PSZ1 G313.85 + 19.2113h47m35s.80-42°28′02″.62017-01-08GMRT610, 60.06510.7 × 4.0, 14.7°
RXC J0528.9-392705h28m48s.82-39°27′40″.02016-12-13GMRT610, 70.0357.5 × 4.6, 15.9°MH
2019-01-21MeerKAT1283, 100.00267.3 × 7.3, 31.7°MHa
MeerKAT1283, 100.011615 × 15 arcsec2
A339606h28m49s.2-41°43′30″2017-02-19GMRT325, 61.514.4 × 7.5, 6.3°
A332205h10m26s.66-45°21′02″.32017-08-15GMRT610, 50.059.6 × 4.1, 14.8°MHc
2019-01-12MeerKAT1283,80.00697.6 × 7.5, 24.2°MHca
A339906h37m23s.2-48°29′16″2017-05-22GMRT610, 5--x
2019-02-17MeerKAT1283, 120.00297.5 × 7.3, −83.9°RH, DRca
MeerKAT1283, 120.01515 × 15 arcsec2
A334305h25m49s.3-47°15′20″2017-07-22GMRT610, 5--x
2019-01-11MeerKAT1283, 80.0038.1 × 7.7, 41.8°
MeerKAT1283, 80.00715 × 15 arcsec2Not shown
A393722h54m21s.1-46°20′37″2017-07-20GMRT610, 50.078.6 × 3.6, 4.9°
(1)(2)(3)(4)(5)(6)(7)(8)(9)
NameRAJ2000Dec.J2000DateTelescopeν, tobsrmsbeamRemark
hms|$^{\circ }\, ^{\prime }\, ^{\prime \prime }$|MHz, hmJy beam−1″ × ″, p. a.
RXC J1358.9-475013h58m42s.64-47°48 ′41″.92016-10-24GMRT325, 50.5019.4 × 6.7, 6.4°
RXC J0232.2-442002h32m18s.7-44°20′41″.02017-02-18GMRT610, 60.049.2 × 3.9, 6.3°RHb
2019-01-13MeerKAT1283, 90.00267.1 × 7.1, 86.5°RHa
MeerKAT1283, 90.0115 × 15 arcsec2
PSZ1 G313.85 + 19.2113h47m35s.80-42°28′02″.62017-01-08GMRT610, 60.06510.7 × 4.0, 14.7°
RXC J0528.9-392705h28m48s.82-39°27′40″.02016-12-13GMRT610, 70.0357.5 × 4.6, 15.9°MH
2019-01-21MeerKAT1283, 100.00267.3 × 7.3, 31.7°MHa
MeerKAT1283, 100.011615 × 15 arcsec2
A339606h28m49s.2-41°43′30″2017-02-19GMRT325, 61.514.4 × 7.5, 6.3°
A332205h10m26s.66-45°21′02″.32017-08-15GMRT610, 50.059.6 × 4.1, 14.8°MHc
2019-01-12MeerKAT1283,80.00697.6 × 7.5, 24.2°MHca
A339906h37m23s.2-48°29′16″2017-05-22GMRT610, 5--x
2019-02-17MeerKAT1283, 120.00297.5 × 7.3, −83.9°RH, DRca
MeerKAT1283, 120.01515 × 15 arcsec2
A334305h25m49s.3-47°15′20″2017-07-22GMRT610, 5--x
2019-01-11MeerKAT1283, 80.0038.1 × 7.7, 41.8°
MeerKAT1283, 80.00715 × 15 arcsec2Not shown
A393722h54m21s.1-46°20′37″2017-07-20GMRT610, 50.078.6 × 3.6, 4.9°

Notes.a(Knowles et al. 2022); b(Kale, Shende & Parekh 2019).

Table 2.

Radio observation summary for the SUCCESS sample. Columns are: (1) Cluster name; (2) Right Ascension; (3) Declination; (4) Date of observation; (5) Telescope; (6) Observing frequency and duration; (7) Root mean square noise in the image with robust =0.0; (8) Beam and position angle (p. a.); and (9) Remark. The remarks regarding detection of diffuse radio emission (RH = radio halo, MH = Mini-halo candidate, DR = double relic, c= candidate), previous reference (if any), and comments on the data quality are provided as applicable (x  = We have not used this data due to the poor SNR of the data).

(1)(2)(3)(4)(5)(6)(7)(8)(9)
NameRAJ2000Dec.J2000DateTelescopeν, tobsrmsbeamRemark
hms|$^{\circ }\, ^{\prime }\, ^{\prime \prime }$|MHz, hmJy beam−1″ × ″, p. a.
RXC J1358.9-475013h58m42s.64-47°48 ′41″.92016-10-24GMRT325, 50.5019.4 × 6.7, 6.4°
RXC J0232.2-442002h32m18s.7-44°20′41″.02017-02-18GMRT610, 60.049.2 × 3.9, 6.3°RHb
2019-01-13MeerKAT1283, 90.00267.1 × 7.1, 86.5°RHa
MeerKAT1283, 90.0115 × 15 arcsec2
PSZ1 G313.85 + 19.2113h47m35s.80-42°28′02″.62017-01-08GMRT610, 60.06510.7 × 4.0, 14.7°
RXC J0528.9-392705h28m48s.82-39°27′40″.02016-12-13GMRT610, 70.0357.5 × 4.6, 15.9°MH
2019-01-21MeerKAT1283, 100.00267.3 × 7.3, 31.7°MHa
MeerKAT1283, 100.011615 × 15 arcsec2
A339606h28m49s.2-41°43′30″2017-02-19GMRT325, 61.514.4 × 7.5, 6.3°
A332205h10m26s.66-45°21′02″.32017-08-15GMRT610, 50.059.6 × 4.1, 14.8°MHc
2019-01-12MeerKAT1283,80.00697.6 × 7.5, 24.2°MHca
A339906h37m23s.2-48°29′16″2017-05-22GMRT610, 5--x
2019-02-17MeerKAT1283, 120.00297.5 × 7.3, −83.9°RH, DRca
MeerKAT1283, 120.01515 × 15 arcsec2
A334305h25m49s.3-47°15′20″2017-07-22GMRT610, 5--x
2019-01-11MeerKAT1283, 80.0038.1 × 7.7, 41.8°
MeerKAT1283, 80.00715 × 15 arcsec2Not shown
A393722h54m21s.1-46°20′37″2017-07-20GMRT610, 50.078.6 × 3.6, 4.9°
(1)(2)(3)(4)(5)(6)(7)(8)(9)
NameRAJ2000Dec.J2000DateTelescopeν, tobsrmsbeamRemark
hms|$^{\circ }\, ^{\prime }\, ^{\prime \prime }$|MHz, hmJy beam−1″ × ″, p. a.
RXC J1358.9-475013h58m42s.64-47°48 ′41″.92016-10-24GMRT325, 50.5019.4 × 6.7, 6.4°
RXC J0232.2-442002h32m18s.7-44°20′41″.02017-02-18GMRT610, 60.049.2 × 3.9, 6.3°RHb
2019-01-13MeerKAT1283, 90.00267.1 × 7.1, 86.5°RHa
MeerKAT1283, 90.0115 × 15 arcsec2
PSZ1 G313.85 + 19.2113h47m35s.80-42°28′02″.62017-01-08GMRT610, 60.06510.7 × 4.0, 14.7°
RXC J0528.9-392705h28m48s.82-39°27′40″.02016-12-13GMRT610, 70.0357.5 × 4.6, 15.9°MH
2019-01-21MeerKAT1283, 100.00267.3 × 7.3, 31.7°MHa
MeerKAT1283, 100.011615 × 15 arcsec2
A339606h28m49s.2-41°43′30″2017-02-19GMRT325, 61.514.4 × 7.5, 6.3°
A332205h10m26s.66-45°21′02″.32017-08-15GMRT610, 50.059.6 × 4.1, 14.8°MHc
2019-01-12MeerKAT1283,80.00697.6 × 7.5, 24.2°MHca
A339906h37m23s.2-48°29′16″2017-05-22GMRT610, 5--x
2019-02-17MeerKAT1283, 120.00297.5 × 7.3, −83.9°RH, DRca
MeerKAT1283, 120.01515 × 15 arcsec2
A334305h25m49s.3-47°15′20″2017-07-22GMRT610, 5--x
2019-01-11MeerKAT1283, 80.0038.1 × 7.7, 41.8°
MeerKAT1283, 80.00715 × 15 arcsec2Not shown
A393722h54m21s.1-46°20′37″2017-07-20GMRT610, 50.078.6 × 3.6, 4.9°

Notes.a(Knowles et al. 2022); b(Kale, Shende & Parekh 2019).

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