Open Access

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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