Images | NOIRLab Science

Images

0.9m Stromgren u filter

filter_u

0.9m Halpha Set #6740

W9_6740c

0.9m Halpha Set #6700

W9_6700b

0.9m Halpha Set #6660

W9_6660b

0.9m Halpha Set #6580

W9_6580b

WIYN 0.9m R filter

Rfilt

WIYN 0.9m V filter

Vfilt

WIYN 0.9m B filter

Bfilt

Bias exposure

bias

H-alpha dome flat

HAlpharaw

I dome flat

Iflatraw

R dome flat

Rflatraw

V dome flat

Vflatraw

B dome flat

Bflatraw

Bias Frame

zeroraw

The quantum efficiency of S2KB

s2kbdqe

NEWFIRM Image resized

NEWFIRM_Image_resized

NEWFIRM and Gemini FOVs

fpf2

NGs (1mm)

132_sm

KPNO Mosaic Standard UBVRI and White Filters

KPNO Mosaic Standard UBVRI and White Filters

k1001frs

k1001frs

k1001

k1001

H-band dome flat

fig8a-whirc

Photometry of a star (Ks ~ 11)

fig7-whirc

The ratio of a processed flat in Ks to that in J

fig6b-whirc

The ratio of a processed flat in Ks to that in J

fig6a-whirc

Flatfields through the Ks

fig5b-whirc

Flatfields through the J

fig5a-whirc

Linearity WHIRC 0.7v bias 17 Sep 2008 (linearity corrected with new algoritm)

fig4b-whirc

Linearity WHIRC 0.7v bias 17 Sep 2008 (raw date)

fig4a-whirc

WIYN IAS Guide Field, WTTM Deployed

fig3-whirc

J9671

J9671

J9440

J9440

J9232

J9232

J8265

J8265

J7799

J7799

H6420

H6420

H6073

H6073

K4748

K4748

K4667

K4667

K4578

K4578

K4484

K4484

K4396

K4396

K4308

K4308

K4220

K4220

K4132

K4132

L3290

L3290

L3100

L3100

L3010

L3010

L2870

L2870