Version 1.34.4
Seeing-limited mode
Diffraction-limited mode
Strehl ratio:
Point source
Extended source
Template Spectrum: B0V A0V F0V G0V K0V M0V E0_galaxy Sa_galaxy Sb_galaxy Sc_galaxy uniform Redshift:
Blackbody with T= K
Single line with ...
... Wavelength: ... Flux: ... Width:
micron erg/s/cm2 Å
Target magnitude (Vega): U B V R I z J H K Ks Br_gam FeII H2 P_beta P_gam J_low J_high Y1 Y2 OH_1060 OH_1190 HeI OrderSep = mag (mag/sq.arcsec for extended sources)
LUCIFER 1
LUCIFER 2
Imaging mode
Spectroscopic mode
Filter: z J H K Ks Br_gam FeII H2 P_beta P_gam J_low J_high Y1 Y2 OH_1060 OH_1190 HeI OrderSep clear
Camera: N1.8 N3.75
Slit width: 0.25 0.50 0.75 1.00
Central wavelength of the grating in µm / Number of lines per millimeter: 1.00 / 210 1.25 / 210 1.65 / 210 1.93 / 200 2.15 / 150 2.20 / 210
Water vapor: 1.00 1.60 3.00 mm
Airmass: 1.00 1.25 1.50 1.75 2.00 2.50
Seeing: arcsec
Sky brightness for the zenith (Vega): mag/sq.arcsec pure black-body spectrum, no sky lines
Background file with 1.6 mm water vapor and selected airmass
Theoretical background spectrum
SNR
Total exposure time sec
Detector Integration Time (DIT): sec (the minimum DIT is 1.98 sec)
Help
Send comments to A.Germeroth(at)lsw.uni-heidelberg.de