ARCHIVED SOURCE · SCRIPTS AND NETWORK DISABLED
TARGET
INSTRUMENT
RITCHEY-CHRÉTIEN 1.8M
PRIMARY / F8.0
WINDOW
22:42 – 01:16
STATE
FILTER
Hα / 6nm
REFERENCE
SEE OBSERVATION / 26-0814-A
PRIMARY TEMP−12.4°C
MIRROR DELTA+0.3°C
DOME HUMIDITY34%
WIND8km/h
TRACKING ERROR0.18arcsec
SEEING1.4arcsec FWHM
FIG. 07 / RC1.8 OPTICAL SYSTEM — SECTION
INCOMING LIGHT
PRIMARY MIRROR / M1
01 ∅1800mm / ZERODUR
SECONDARY MIRROR / M2
02 ∅280mm / CONVEX HYPERBOLIC
CASSEGRAIN FOCUS
03 F/8.0 / 14400mm EFL
FILTER WHEEL
04 8-POSITION / 50mm SLOTS
CCD DETECTOR
05 4096×4096 / 0.12 arcsec/px
01
PRIMARY MIRROR
02
SECONDARY MIRROR
03
FOCAL PLANE
04
FILTER WHEEL
05
CCD DETECTOR
RECORDTARGETSTARTEXPOSUREFILTERSTATEREV
26-0814-ANGC 700022:421800sACTIVER01
26-0813-CM4223:10600sOIIICOMPLETER03
26-0812-BNGC 89121:553600sBVRCOMPLETER02
26-0811-ANGC 239222:081200sSIICOMPLETER04
26-0809-DM5722:30900sARCHIVEDR02
NOTE A / OBS 26-0814-A / NGC 7000
Seeing improved significantly after 23:00 local. Hα exposures showing clear filament structure in the Cygnus Wall region — recommend increasing integration time for follow-up run. Guiding stable at 0.18 arcsec rms throughout. Schedule B-filter comparison set for next available window.
DR. K. VALLANCE — NSO STAFF ASTRONOMER — 26-0814 / 23:44 UT
CAUTION
04.2 / THERMAL TOLERANCE LIMIT
Calibration values are invalid after thermal differential between primary mirror and ambient air exceeds ±2.0°C. If this condition is encountered, suspend science exposures, allow 30-minute thermal soak period, and re-run flat-field sequence before resuming. Do not apply archived calibration frames.

Northstar Observatory operates from a high-altitude site at 2,840 meters above sea level, selected for exceptional atmospheric stability and low light pollution. The facility supports a dedicated research program in narrow-band nebular imaging and variable star monitoring.

The primary instrument, a 1.8-meter Ritchey-Chrétien reflector, was commissioned in 2018 following a decade of optical development. The telescope operates robotically during approved observation windows, with remote oversight available from partnering institutions. All acquired data enters the public archive 12 months after collection.

NSO operates in partnership with four regional universities. Observing time is allocated by proposal on a semester basis. The facility's technical documentation, instrument calibration records, and observation logs are maintained as part of the operational record and are referenced throughout this interface.