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TELESCOPE:   SOAR
SEMESTER:    2018A
CODE:        2018A-0920
PI:          I Fuentes Morales
TITLE:       Recovery of novae after the eruption
STARTDATE:   2018-05-14
ENDDATE:     2018-05-15
SUBMIT:      2018-05-10.17:53:56
OBSERVER:    Irma Fuentes Morales
OBSERVEREM:  irma.fuentes@uv.cl
INSTITUTION: Chile
INSTRUMENT:  Goodman HTS
STARTDATE:   2018-05-14
CAMERA:      Red Camera
GRATINGS:    
FILTERS:     V, Halpha and [SII]
OBJFILE:     target_SOAR_coordinates.txt
FINDFILE:
FINDURL:
INSTRUCT.BOT We need to change the setup form sent previously, since we have recently noticed that we are more likely to identify nova if a [SII] narrow filfer is used (instead of an R filter). For this reason it is necessary that we use V, Halpha and [SII] filters. INSTRUCT.EOT Goodman_HTS.EOT