Table 6.
Multiwavelength data of the target galaxies.
Galaxy | X-rays | Ref | UV | Ref | Visible | Ref |
---|---|---|---|---|---|---|
4262 | Chandra | 1 | GALEX, UVIT | 8,9,TW | CFHT, HST | 10,11,TW |
4429 | Chandra | 1 | GALEX, UVIT | 9,TW | CFHT, HST | 11,12,TW |
4459 | Chandra, XMM | 1,2 | GALEX | 9 | CFHT, HST | 10,11,TW |
4469 | Chandra | 1 | GALEX | 9 | CFHT, HST | 11,TW |
4476 | Chandra, XMM | 1,2 | GALEX, UVIT | 9,TW | CFHT, HST | 10,11,TW |
4477 | Chandra, XMM | 2,3,4 | GALEX | 9 | CFHT, HST | 11,TW |
4526 | Chandra, XMM | 2,4 | GALEX | 9 | CFHT, HST | 10,11,TW |
4552 | Chandra, XMM | 4,5,6,7 | GALEX | 9 | CFHT, HST | 10,11,TW |
Galaxy | IR | Ref | CO | Ref | HI | Ref |
4262 | WISE, Spitzer, Herschel | 13,13,15,16 | IRAM | 18 | WSRT | 24,25 |
4429 | WISE, Spitzer, Herschel | 13,13,15,16 | CARMA, ALMA | 12,19 | WSRT | 26 |
4459 | WISE, Spitzer, Herschel | 13,13,15,16 | CARMA, ALMA, IRAM | 18,21,TW | WSRT | 26 |
4469 | WISE, Spitzer, Herschel | 13,13,15,16 | Arecibo | 27 | ||
4476 | WISE, Spitzer, Herschel | 13,17,TW | CARMA, ALMA | 21,TW | WSRT | 26 |
4477 | WISE, Spitzer, Herschel | 13,13,15,16 | CARMA, PdBI, IRAM | 18,22 | WSRT | 26 |
4526 | WISE, Spitzer, Herschel | 13,13,15,16 | CARMA, ALMA, IRAM | 18,23,TW | Arecibo | 27 |
4552 | WISE, Spitzer, Herschel | 13,13,15,16 | IRAM | 18 | WSRT | 26 |
References. (1) Chandra data archive (P.Is.: Treu, Soria, Ptak, Gultekin); (2) XMM data archive (P.Is.: David, Forman, Sanders, Jansen, Boehringer, Turner, Aschenbach, Irwin); (3) Li et al. (2018); (4) Kim et al. (2019); (5) Machacek et al. (2006a); (6) Machacek et al. (2006b); (7) Kraft et al. (2017); (8) Bettoni et al. (2010); (9) Boselli et al. (2011); (10) Côté et al. (2004); (11) Ferrarese et al. (2012); (12) Davis et al. (2018); (13) Wright et al. (2010); (14) Bendo et al. (2012a); (15) Cortese et al. (2014); (16) Ciesla et al. (2012); (17) Auld et al. (2013); (18) Combes et al. (2007); (19) Alatalo et al. (2013); (20) Young et al. (2008); (21) Young (2002); (22) Crocker et al. (2011); (23) Utomo et al. (2015); (24) Krumm et al. (1985); (25) Oosterloo et al. (2010); (26) Serra et al. (2012); (27) Haynes et al. (2018).
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