Table A.2
Rediscovered lenses identified in this study.
IAU Name | ID | RA | Dec | rare (″) | instru. | filter | mag | re (″) | q | PA | class | clust. | z | reference |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
A grade Lenses | ||||||||||||||
HAH 7001426.3 − 302255.3 | 199 | 3.60962 | −30.38202 | 1 | ACS | f814w | 18.9 | 0.55 | 0.72 | −137.7 | Arc | RClust125 | 0.24 ★ | Pawase et al. (2014) |
HAH 7015242.4 − 135618.2 | 200 | 28.17683 | −13.93838 | 0.97 | ACS | f775w | 21.4 | 0.30 | 0.92 | −96.3 | Arc | RClust126 | Grillo et al. (2008) | |
HAH 7032940.8 − 021318.5 | 201 | 52.42010 | −2.22180 | 0.82 | ACS | f435w | 22.2 | 0.67 | 0.94 | −148.2 | Arc | RClust127 | Desprez et al. (2018) | |
HAH 7033238.2 − 275653.3 | 202 | 53.15930 | −27.94810 | 1.67 | ACS | f606w | 21.0 | 1.08 | 0.53 | −124.5 | Arc | More et al. (2011) | ||
HAH 7033304.4 − 065144.3 | 203 | 53.26850 | −6.86230 | 0.83 | IR | f160w | 19.7 | 0.69 | 0.75 | 104.2 | Arc | RClust128 | 0.57 P | Sharon et al. (2020) |
HAH 7041604.1 − 240522.2 | 204 | 64.01720 | −24.08950 | 1.2 | ACS | f814w | 20.0 | 0.57 | 0.32 | 28.6 | Arc | RClust129 | 0.4 P★ | Diego et al. (2015) |
HAH 7045400.6 − 030833.8 | 205 | 73.50260 | −3.14280 | 1.88 | ACS | f814w | 17.0 | 3.45 | 0.69 | −8.6 | Arc | RClust130 | Schirmer et al. (2010) | |
HAH 7045413.1 + 025733.8 | 206 | 73.55475 | 2.95939 | 2.6 | ACS | f814w | 16.5 | 2.55 | 0.96 | −3.0 | Ring | RClust131 | Clowe et al. (2012) | |
HAH 7074450.9 + 392736.0 | 207 | 116.21211 | 39.45986 | unfit | ACS | f606w | 22.5 | 1.43 | 0.39 | 21.7 | Arc | RClust132 | 0.62 P★ | Horesh et al. (2010) |
HAH 7091617.5 − 002405.9 | 208 | 139.07306 | −0.40164 | 0.74 | ACS | f814w | Arc | RClust133 | Clowe et al. (2012) | |||||
HAH 7095921.8 + 020638.5 | 209 | 149.84068 | 2.11064 | 0.71 | ACS | f814w | 20.5 | 0.34 | 0.78 | 49.4 | Quad | 0.58 P | Faure et al. (2008) | |
HAH 7095930.9 + 023427.8 | 210 | 149.87890 | 2.57440 | 0.92 | ACS | f814w | 21.9 | 0.38 | 0.61 | −69.8 | Arc | 0.89 ★ | Lagattuta et al. (2010) | |
HAH 7095956.0 +021901.8 | 211 | 149.98330 | 2.31719 | 2.36 | ACS | f814w | 22.9 | 4.65 | 0.21 | 10.7 | Arc | 0.93 ★ | More et al. (2012) | |
2.36 | ACS | f814w | 21.3 | 0.74 | 0.88 | −64.5 | Arc | 0.93 ★ | ||||||
HAH 7100012.6 + 022015.8 | 212 | 150.05258 | 2.33772 | 0.73 | ACS | f814w | 19.3 | 0.49 | 0.81 | 5.9 | Arc | RClust134 | 0.37 P | Cabanac et al. (2007) |
HAH 7100018.5 + 023845.6 | 213 | 150.07700 | 2.64600 | 1.51 | ACS | f814w | 23.6 | 0.12 | 0.71 | 10.8 | Arc | RClust135 | 0.42 P★ | Cabanac et al. (2007) |
HAH 7100108.4 + 024029.9 | 214 | 150.28495 | 2.67496 | 1.41 | ACS | f814w | 19.3 | 0.34 | 0.86 | 1.8 | Arc | 0.32 P★ | Pourrahmani et al. (2018) | |
HAH 7100133.7 + 022135.3 | 215 | 150.39058 | 2.35982 | 2.54 | ACS | f814w | 20.3 | 0.54 | 0.44 | −29.4 | Arc | RClust136 | 0.36 P | More et al. (2012) |
HAH 7100211.2 + 021139.5 | 216 | 150.54675 | 2.19429 | 3.45 | ACS | f814w | 20.5 | 1.77 | 0.46 | 13.7 | Arc | 0.7 P | Faure et al. (2008) | |
HAH 7114936.7 + 222612.0 | 217 | 177.40280 | 22.43667 | 0.859 | ACS | f814w | 19.8 | 0.48 | 0.80 | 60.8 | Cross | 0.5 P | Desprez et al. (2018) | |
HAH 7133235.0 + 503237.3 | 218 | 203.14564 | 50.54369 | 4.2 | ACS | f606w | 18.9 | 1.66 | 0.72 | −156.6 | Arc | 0.28 S | Ragozzine et al. (2012) | |
HAH 7133241.0 + 503346.3 | 219 | 203.17064 | 50.56286 | 2.52 | ACS | f606w | 18.2 | 1.89 | 0.90 | 149.3 | Ring | RClust137 | 0.28 S | Ragozzine et al. (2012) |
HAH 7135409.1 +771557.2 | 220 | 208.53795 | 77.26590 | 1.79 | ACS | f814w | 21.0 | 0.60 | 0.75 | −179.5 | Arc | RClust138 | Repp & Ebeling (2018) | |
HAH 7135409.2 + 771549.9 | 221 | 208.53816 | 77.26385 | 2.26 | ACS | f814w | 20.5 | 0.91 | 0.65 | −90.1 | Arc | RClust139 | Repp & Ebeling (2018) | |
HAH 7140237.0 + 542716.3 | 222 | 210.65450 | 54.45455 | 1.8 | ACS | f814w | 18.1 | 1.14 | 0.74 | −114.1 | Arc | Pawase et al. (2014) | ||
HAH 7141735.7 + 522646.3 | 223 | 214.39891 | 52.44621 | 1.6 | ACS | f814w | 20.2 | 0.98 | 0.62 | −142.5 | Cross | 0.59 P | Ratnatunga et al. (1995) | |
HAH 7141820.8 + 523611.1 | 224 | 214.58664 | 52.60309 | 0.81 | ACS | f814w | 21.2 | 0.62 | 0.76 | −91.0 | Arc | 0.58 S | Moustakas et al. (2007) | |
HAH 7143703.3 + 350153.3 | 225 | 219.26352 | 35.03145 | 0.65 | ACS | f814w | 22.5 | 0.36 | 0.76 | −78.8 | Ring | 0.56 P | Pawase et al. (2014) | |
HAH 7145250.0 + 580135.3 | 226 | 223.20849 | 58.02649 | 3.22 | ACS | f814w | 18.3 | 1.17 | 0.67 | 42.3 | Arc | RClust140 | 0.33 S | Repp & Ebeling (2018) |
HAH 7152745.2 + 065220.8 | 227 | 231.93830 | 6.87247 | 1.78 | UVIS | f606w | 22.0 | 0.30 | 0.33 | 39.7 | Arc | RClust141 | 0.32 P | Koester et al. (2010) |
HAH 7213512.7 − 010143.9 | 228 | 323.80296 | −1.02886 | 0.98 | ACS | f814w | 20.7 | 0.64 | 0.65 | 98.8 | Arc | RClust142 | 0.3 P | Smail et al. (2007) |
HAH 7221142.0 − 035052.4 | 229 | 332.92486 | −3.84790 | 1.15 | ACS | f814w | 21.7 | 0.19 | 0.77 | −67.4 | Cross | RClust143 | 0.42 P | Bettoni et al. (2019) |
HAH 7224851.7 − 443105.1 | 230 | 342.21568 | −44.51858 | 3.17 | ACS | f814w | 20.9 | 0.11 | 0.82 | 33.3 | Arc | RClust144 | 0.33 ★ | Guzzo et al. (2009) |
3.17 | ACS | f814w | 17.7 | 2.40 | 0.82 | −103.8 | Arc | 0.33 ★ | ||||||
3.17 | ACS | f814w | 19.0 | 3.39 | 0.86 | −10.8 | Arc | 0.33 ★ | ||||||
3.17 | ACS | f814w | 20.1 | 0.27 | 0.69 | −32.1 | Arc | 0.33 ★ | ||||||
HAH 7235130.6 − 261500.7 | 231 | 357.87744 | −26.25008 | 3.32 | ACS | f814w | 16.3 | 4.47 | 0.74 | −124.2 | Arc | 0.27 ★ | Pawase et al. (2014) | |
B grade Lenses | ||||||||||||||
HAH 7001423.0 − 302109.7 | 232 | 3.59578 | −30.35270 | 1.7 | ACS | f814w | 19.8 | 0.83 | 0.85 | 22.5 | Arc | RClust145 | 0.25 ★ | Pawase et al. (2014) |
HAH 7033153.2 − 274619.3 | 233 | 52.97181 | −27.77194 | 1.05 | ACS | f840w | 20.7 | 0.66 | 0.76 | −62.5 | Arc | 0.73 ★ | More et al. (2011) | |
HAH 7095939.1 + 023044.1 | 234 | 149.91311 | 2.51224 | 1.7 | ACS | f814w | 20.0 | 0.76 | 0.69 | 62.6 | Arc | RClust146 | 0.72 P | Faure et al. (2008) |
HAH 7100013.9 + 022249.8 | 235 | 150.05800 | 2.38050 | 1.65 | ACS | f606w | 19.3 | 1.90 | 0.79 | −110.8 | Arc | RClust147 | 0.35 S | Faure et al. (2008) |
HAH 7100047.7 + 015023.3 | 236 | 150.19854 | 1.83981 | 1.71 | ACS | f814w | 20.6 | 0.75 | 0.72 | 2.2 | Arc | RClust148 | 0.89 ★ | Faure et al. (2008) |
HAH 7100055.7 + 013821.1 | 237 | 150.23214 | 1.63919 | 1.06 | ACS | f814w | 20.9 | 0.35 | 0.95 | 92.4 | Arc | RClust149 | 0.55 P | Faure et al. (2008) |
HAH 7100056.8 + 021225.8 | 238 | 150.23661 | 2.20719 | 1.67 | ACS | f814w | 18.8 | 1.01 | 0.66 | 64.1 | Arc | 0.36 S | Faure et al. (2008) | |
HAH 7103751.4 − 124326.3 | 239 | 159.46400 | −12.72398 | 1.12 | ACS | f814w | 19.5 | 1.39 | 0.70 | −49.2 | Arc | 0.58 ★ | Pawase et al. (2014) | |
1.12 | ACS | f814w | 19.8 | 0.66 | 0.86 | −53.7 | Arc | 0.58 ★ | ||||||
HAH 7121228.4 − 121723.1 | 240 | 183.11829 | −12.29002 | 2.84 | ACS | f814w | 21.9 | 0.18 | 0.79 | −105.5 | Arc | Ebeling et al. (2019) | ||
2.84 | ACS | f814w | 20.1 | 1.03 | 0.84 | −175.4 | Arc | |||||||
HAH 7123729.9 +621300.7 | 241 | 189.37456 | 62.21685 | 2.12 | ACS | f814w | 19.9 | 0.81 | 0.91 | 48.9 | Arc | 0.49 P | Fassnacht et al. (2004) | |
HAH 7130042.7 +280523.6 | 242 | 195.17804 | 28.08989 | 1.08 | ACS | f814w | 18.2 | 1.70 | 0.61 | −118.2 | Arc | RClust150 | 0.37 S | Pawase et al. (2014) |
HAH 7131829.4 − 010421.6 | 243 | 199.62246 | −1.07267 | 0.67 | ACS | f814w | 19.9 | 0.67 | 0.84 | −85.0 | Arc | 0.66 S | Brownstein et al. (2012) | |
HAH 7141833.1 + 524352.5 | 244 | 214.63790 | 52.73126 | 0.69 | ACS | f814w | 20.5 | 1.32 | 0.68 | 97.2 | Arc | 0.47 P | Marshall et al. (2009) | |
HAH 7214014.8 − 233904.3 | 245 | 325.06171 | −23.65125 | 2.58 | ACS | f606w | 20.0 | 0.58 | 0.94 | 133.2 | Arc | Fort et al. (1992) | ||
HAH 7230824.7 − 021213.3 | 246 | 347.10300 | −2.20370 | 3.24 | ACS | f606w | 18.2 | 2.76 | 0.53 | −88.3 | Arc | RClust151 | 0.27 P | Jacobs et al. (2019) |
C grade Lenses | ||||||||||||||
HAH 7013152.3 − 133658.3 | 247 | 22.96793 | −13.61621 | 1.9 | ACS | f475w | 19.0 | 1.58 | 0.86 | −170.7 | Arc | RClust152 | Zitrin et al. (2015) | |
HAH 7071815.0 + 374200.3 | 248 | 109.56253 | 37.70009 | 1.91 | ACS | f814w | 20.6 | 0.44 | 0.96 | 61.4 | Arc | RClust153 | 0.34 P | Ebeling et al. (2014) |
HAH 7095810.1 + 022942.0 | 249 | 149.54211 | 2.49500 | 2.21 | ACS | f814w | 18.9 | 1.05 | 0.75 | −57.8 | Arc | 0.4 P | Jackson (2008) | |
HAH 7114934.3 + 222440.5 | 250 | 177.39310 | 22.41127 | 0.61 | ACS | f606w | 23.1 | 0.67 | 0.93 | 7.0 | Arc | RClust154 | 0.47 P | Morishita et al. (2017) |
HAH 7173217.5 + 193250.3 | 251 | 263.07333 | 19.54731 | 1.2 | ACS | f814w | 19.8 | 0.61 | 0.93 | 44.6 | Arc | RClust155 | Ebeling et al. (2018) | |
HAH 7203146.3 − 403705.4 | 252 | 307.94293 | −40.61818 | 1.02 | ACS | f814w | 22.4 | 0.30 | 0.76 | 0.2 | Arc | RClust156 | Richard et al. (2015) |
Notes. This table summarises a list of characteristics related to each rediscovered lens. The lens objects are named using the standard IAU name, where the acronym HAH stands for Hubble Asteroid Hunter. The lenses are grouped by grades (A,B,C) which were assigned by the authors of this paper as a qualitative assessment of the candidates. RA and Dec: right ascension and declination given in degrees of celestial coordinates J2000.0. rare: the arc radius (in arcsec) corresponding to the angular separation between the lens and the surrounding images. Instru. and filter: the HST instrument (ACS/WFC, WFC3/UVIS or WFC3/IR) and the filter with which the HST image was taken. Mag, re, q, and PA: the apparent magnitude, the effective radius (in arcsec), the axis ratio and the position angle of the foreground lens galaxy (measured from North through East, same orientation as in Figures. 2−4); these parameters were retrieved with Galfit. class: the morphological class of the source images (Arc, Quad, Ring, Double). clust.: a flag indicating the presence of a foreground or background nearby cluster, details are available in table A.3. z: the photometric (P) or spectroscopic (S) redshift, retrieved from SDSS (no mark) or NED (marked ★). The reference columns shows the paper where the strong lensing system is mentioned, as listed by the ESASky portal. Because of the complexity of lens ID 207, we did not manage to measure its arc radius. Finally, We did not manage to obtain a good model for the lens ID 208 and, therefore, left the GALFIT parameters blank.
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