SVO Filter Profile Service

LCO :Las Campanas Observatory
LCO/MMIRS :MMT and Magellan InfraRed Spectrograph (MMIRS) is a near infrared (NIR) imager and multi-object spectrograph with a 6.9'x 6.9' imaging field-of-view.

LCO filters: CAPSCam CCD3x3 CSP CSP2 e2v FourStar IMACS MagAOX MagIC MMIRS OGLE-IV RetroCam
SITe3 VisAO WFCCD WIRC

Filter ID	λ_ref	λ_mean	λ_eff	λ_min	λ_max	W_eff	ZP_ν	ZP_λ	Obs. Facility	Instrument	Description
LCO/MMIRS.Y	10184.73	10200.51	10166.24	9422.63	11053.60	1077.65	2093.17	6.07e-10	LCO	MMIRS	LCO, MMIRS Y
LCO/MMIRS.zJ	11987.09	12299.43	11596.80	9325.70	15270.66	5259.56	1610.71	3.59e-10	LCO	MMIRS	LCO, MMIRS zJ
LCO/MMIRS.J	12492.08	12519.14	12453.00	11489.74	13584.18	1545.83	1555.97	3.01e-10	LCO	MMIRS	LCO, MMIRS J
LCO/MMIRS.H	16373.65	16437.07	16293.40	14648.78	18266.67	2833.56	1032.51	1.17e-10	LCO	MMIRS	LCO, MMIRS H
LCO/MMIRS.Hk3	17133.67	17967.34	16070.52	12089.72	23744.87	10534.79	921.62	1.07e-10	LCO	MMIRS	LCO, MMIRS Hk3
LCO/MMIRS.Hk	17800.56	18805.54	16508.95	12245.53	25432.25	11524.42	861.27	9.47e-11	LCO	MMIRS	LCO, MMIRS Hk
LCO/MMIRS.K	21549.25	21612.26	21454.03	19540.75	23832.58	3141.31	668.27	4.35e-11	LCO	MMIRS	LCO, MMIRS K

Filter Plots

If your research benefits from the use of the SVO Filter Profile Service, we would appreciate if you could include the following acknowledgement in your publication:

This research has made use of the Spanish Virtual Observatory (https://svo.cab.inta-csic.es) project funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00

and we would appreciate if you could include the following references in your publication:

The SVO Filter Profile Service. Rodrigo, C., Solano, E., Bayo, A., 2012; https://ui.adsabs.harvard.edu/abs/2012ivoa.rept.1015R/abstract
The SVO Filter Profile Service. Rodrigo, C., Solano, E., 2020; https://ui.adsabs.harvard.edu/abs/2020sea..confE.182R/abstract