In an era when professional astronomers G@UD KNMF @A@MCNMDC SGD M@JDC DXD @MC OGNSNFQ@OGHB OK@SDR @R RBHDMSHjB CDSDB SNQR L@MX TRDQR NE +@ 2HKK@ /@Q@M@K +2/ HMRSQTLDMSR L@X MN KNMFDQ JMNV VG@S happens exactly between the arrival of SGD OGNSNMR @S SGD CDSDBSNQ @MC SGD jQRS inspection of the new observation and SGDQD RGNTKC AD MN MDDC SN @R SGHR OQNB DRR RGNTKC AD ETKKX SQ@MRO@QDMS SN SGDL .M SGD NSGDQ G@MC SGHR SQ@MRO@QDMBX B@M be achieved only if the corresponding OQNBDRR HR UDQX QNATRS @MC CNDR MNS HL OQHMS RHFM@STQDR NE HSR NVM NM SGD C@S@ 2HMBD SGHR jM@K RSDO NE @MX LNCDQM NARDQ U@SHNM HR PTHSD BNLOKDW @MC RGNTKC AD BNLOKDSDC PTHBJKX SGDQD @QD L@MX ONSDM SH@K E@HKTQD ONHMSR @MC RN SGHR K@QFDKX HM UHRHAKD RSDO QDPTHQDR LTBG B@QD @MC DEENQS The detector may have to be cleaned of SGD QDRHCTD NE @ OQDUHNTR DWONRTQD UNKS @FDR MDDC SN AD @OOKHDC SN JDDO SGD DKDB trons generated where the photons hit SGD CDSDBSNQ @ RGTSSDQ L@X G@UD SN AD NODMDC SGD DWONRTQD SHLD LTRS AD @BBT Q@SDKX JDOS @ RGTSSDQ L@X G@UD SN AD BKNRDC @MC @ RDPTDMBDQ G@R SN FDMDQ@SD SHLD CDODMCDMS UNKS@FD O@SSDQMR SN CQHUD SGD @BBTLTK@SDC DKDBSQNMR SN SGD @LOKHjDQ NQ SN @CCQDRR D@BG OHWDK @LOKHjDQ RDPTDM SH@KKX ESDQ @LOKHjB@SHNM SGD BG@QFDR @QD BNMUDQSDC SN UNKS@FDR @MC CHFHSHRDC @MC the resulting number must be inserted @S SGD QHFGS KNB@SHNM HM SGD C@S@ AKNBJ @MC important ancillary information must be VQHSSDM SN SGD %(32 GD@CDQ VHSGNTS VGHBG SGD C@S@ AKNBJ VNTKC MNS ENQL @M HL@FD that can be processed further and scien SHjB@KKX HMSDQOQDSDC