Potential CL sources from our list of CL candidates identified through their current optical variability and the criteria mentioned in the comments.
Name . | Ra . | Dec . | z . | MJD . | fiberid . | plate . | Comments . |
---|---|---|---|---|---|---|---|
ZTF18aalmtum | 136.365522 | 17.928647 | 0.40 | 56 246 | 330 | 5769 | Increasing MIR fluxes and W1–W2. |
ZTF18aaodaie/ZTF21ackxdiy | 191.572165 | 28.342741 | 0.10 | 54 205 | 442 | 2238 | Increasing MIR fluxes and W1–W2. |
ZTF18aaoudgg | 221.975974 | 28.556697 | 0.16 | 53 764 | 134 | 2141 | Increasing MIR fluxes and W1–W2. |
ZTF18acakoya/ZTF18abtndvk | 43.709715 | −2.797898 | 0.12 | 56 978 | 181 | 7823 | Increasing MIR fluxes and W1–W2. |
ZTF19adcfhxp | 143.823381 | 34.320597 | 0.45 | 56 336 | 727 | 5805 | Increasing MIR fluxes and W1–W2. |
ZTF20acpcfgt | 339.995984 | 0.860685 | 0.38 | 52 201 | 620 | 674 | Increasing MIR and optical fluxes and W1–W2. |
ZTF21abjprnu | 230.292534 | 20.544009 | 0.14 | 54 328 | 421 | 2159 | Increasing MIR and optical fluxes. Decreasing W1–W2, but still W1–W2 > 0.7 |
ZTF21abdvcpz | 335.843667 | 0.771973 | 0.22 | 52 140 | 454 | 375 | Increasing MIR fluxes and W1–W2. |
ZTF21abmjobi | 358.363382 | 0.123463 | 0.17 | 52 523 | 520 | 684 | Increasing MIR and optical fluxes and W1–W2. |
Name . | Ra . | Dec . | z . | MJD . | fiberid . | plate . | Comments . |
---|---|---|---|---|---|---|---|
ZTF18aalmtum | 136.365522 | 17.928647 | 0.40 | 56 246 | 330 | 5769 | Increasing MIR fluxes and W1–W2. |
ZTF18aaodaie/ZTF21ackxdiy | 191.572165 | 28.342741 | 0.10 | 54 205 | 442 | 2238 | Increasing MIR fluxes and W1–W2. |
ZTF18aaoudgg | 221.975974 | 28.556697 | 0.16 | 53 764 | 134 | 2141 | Increasing MIR fluxes and W1–W2. |
ZTF18acakoya/ZTF18abtndvk | 43.709715 | −2.797898 | 0.12 | 56 978 | 181 | 7823 | Increasing MIR fluxes and W1–W2. |
ZTF19adcfhxp | 143.823381 | 34.320597 | 0.45 | 56 336 | 727 | 5805 | Increasing MIR fluxes and W1–W2. |
ZTF20acpcfgt | 339.995984 | 0.860685 | 0.38 | 52 201 | 620 | 674 | Increasing MIR and optical fluxes and W1–W2. |
ZTF21abjprnu | 230.292534 | 20.544009 | 0.14 | 54 328 | 421 | 2159 | Increasing MIR and optical fluxes. Decreasing W1–W2, but still W1–W2 > 0.7 |
ZTF21abdvcpz | 335.843667 | 0.771973 | 0.22 | 52 140 | 454 | 375 | Increasing MIR fluxes and W1–W2. |
ZTF21abmjobi | 358.363382 | 0.123463 | 0.17 | 52 523 | 520 | 684 | Increasing MIR and optical fluxes and W1–W2. |
Potential CL sources from our list of CL candidates identified through their current optical variability and the criteria mentioned in the comments.
Name . | Ra . | Dec . | z . | MJD . | fiberid . | plate . | Comments . |
---|---|---|---|---|---|---|---|
ZTF18aalmtum | 136.365522 | 17.928647 | 0.40 | 56 246 | 330 | 5769 | Increasing MIR fluxes and W1–W2. |
ZTF18aaodaie/ZTF21ackxdiy | 191.572165 | 28.342741 | 0.10 | 54 205 | 442 | 2238 | Increasing MIR fluxes and W1–W2. |
ZTF18aaoudgg | 221.975974 | 28.556697 | 0.16 | 53 764 | 134 | 2141 | Increasing MIR fluxes and W1–W2. |
ZTF18acakoya/ZTF18abtndvk | 43.709715 | −2.797898 | 0.12 | 56 978 | 181 | 7823 | Increasing MIR fluxes and W1–W2. |
ZTF19adcfhxp | 143.823381 | 34.320597 | 0.45 | 56 336 | 727 | 5805 | Increasing MIR fluxes and W1–W2. |
ZTF20acpcfgt | 339.995984 | 0.860685 | 0.38 | 52 201 | 620 | 674 | Increasing MIR and optical fluxes and W1–W2. |
ZTF21abjprnu | 230.292534 | 20.544009 | 0.14 | 54 328 | 421 | 2159 | Increasing MIR and optical fluxes. Decreasing W1–W2, but still W1–W2 > 0.7 |
ZTF21abdvcpz | 335.843667 | 0.771973 | 0.22 | 52 140 | 454 | 375 | Increasing MIR fluxes and W1–W2. |
ZTF21abmjobi | 358.363382 | 0.123463 | 0.17 | 52 523 | 520 | 684 | Increasing MIR and optical fluxes and W1–W2. |
Name . | Ra . | Dec . | z . | MJD . | fiberid . | plate . | Comments . |
---|---|---|---|---|---|---|---|
ZTF18aalmtum | 136.365522 | 17.928647 | 0.40 | 56 246 | 330 | 5769 | Increasing MIR fluxes and W1–W2. |
ZTF18aaodaie/ZTF21ackxdiy | 191.572165 | 28.342741 | 0.10 | 54 205 | 442 | 2238 | Increasing MIR fluxes and W1–W2. |
ZTF18aaoudgg | 221.975974 | 28.556697 | 0.16 | 53 764 | 134 | 2141 | Increasing MIR fluxes and W1–W2. |
ZTF18acakoya/ZTF18abtndvk | 43.709715 | −2.797898 | 0.12 | 56 978 | 181 | 7823 | Increasing MIR fluxes and W1–W2. |
ZTF19adcfhxp | 143.823381 | 34.320597 | 0.45 | 56 336 | 727 | 5805 | Increasing MIR fluxes and W1–W2. |
ZTF20acpcfgt | 339.995984 | 0.860685 | 0.38 | 52 201 | 620 | 674 | Increasing MIR and optical fluxes and W1–W2. |
ZTF21abjprnu | 230.292534 | 20.544009 | 0.14 | 54 328 | 421 | 2159 | Increasing MIR and optical fluxes. Decreasing W1–W2, but still W1–W2 > 0.7 |
ZTF21abdvcpz | 335.843667 | 0.771973 | 0.22 | 52 140 | 454 | 375 | Increasing MIR fluxes and W1–W2. |
ZTF21abmjobi | 358.363382 | 0.123463 | 0.17 | 52 523 | 520 | 684 | Increasing MIR and optical fluxes and W1–W2. |
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