CIRCE: The Canarias InfraRed Camera Experiment for the Gran Telescopio Canarias

The Canarias InfraRed Camera Experiment (CIRCE) is a near-infrared (1-2.5 micron) imager, polarimeter and low-resolution spectrograph operating as a visitor instrument for the Gran Telescopio Canarias 10.4-meter telescope. It was designed and built largely by graduate students and postdocs, with help from the UF astronomy engineering group, and is funded by the University of Florida and the U.S. National Science Foundation. CIRCE is intended to help fill the gap in near-infrared capabilities prior to the arrival of EMIR to the GTC, and will also provide the following scientific capabilities to compliment EMIR after its arrival: high-resolution imaging, narrowband imaging, high-time-resolution photometry, imaging polarimetry, low resolution spectroscopy. In this paper, we review the design, fabrication, integration, lab testing, and on-sky performance results for CIRCE. These include a novel approach to the opto-mechanical design, fabrication, and alignment.

[1]  Ata Sarajedini,et al.  The Stellar Populations in the Outer Regions of M33. I. Metallicity Distribution Function , 2004, astro-ph/0403525.

[2]  R. M. Hjellming,et al.  Episodic ejection of relativistic jets by the X-ray transient GRO J1655 - 40 , 1995, Nature.

[3]  Ata Sarajedini,et al.  WIYN Open Cluster Study. X. The K-Band Magnitude of the Red Clump as a Distance Indicator , 2001, astro-ph/0112251.

[4]  I. Mirabel,et al.  A superluminal source in the Galaxy , 1994, Nature.

[5]  S. J. Tingay,et al.  Relativistic motion in a nearby bright X-ray source , 1995, Nature.

[6]  J. Orosz,et al.  Optical Observations of GRO J1655–40 in Quiescence. I. A Precise Mass for the Black Hole Primary , 1996, astro-ph/9610211.

[7]  R. P. Fender,et al.  Infrared synchrotron oscillations in GRS 1915+105 , 1998 .

[8]  J. Greiner,et al.  An unusually massive stellar black hole in the Galaxy , 2001, Nature.

[9]  Stephen S. Eikenberry,et al.  The Ultraluminous X-Ray Source X-37 Is a Background Quasar in the Antennae Galaxies , 2005 .

[10]  Eikenberry,et al.  Faint Infrared Flares from the Microquasar GRS 1915+105. , 2000, The Astrophysical journal.

[11]  A. Chrysostomou,et al.  A new imaging infrared polarimeter , 1994 .

[12]  Craig Warner,et al.  Redefining the Data Pipeline Using GPUs , 2013 .

[13]  S. Eikenberry,et al.  Observations of Rapid Disk-Jet Interaction in the Microquasar GRS 1915+105 , 2005, astro-ph/0501624.

[14]  E. Oliva Wedged double Wollaston, a device for single shot polarimetric measurements , 1997 .

[15]  J. R. Houck,et al.  Possible Infrared Counterparts to the Soft Gamma-Ray Repeater SGR 1806–20 , 2001, astro-ph/0110619.

[16]  Stephen S. Eikenberry,et al.  HST NICMOS Observations of Fast Infrared Flickering in the Microquasar GRS 1915+105 , 2007, 0709.1095.

[17]  R. W. Nelson,et al.  Evidence for a Disk-Jet Interaction in the Microquasar GRS 1915+105 , 1997 .

[18]  S. S. Eikenberry,et al.  The Antennae Ultraluminous X-Ray Source, X-37, Is A Background Quasar , 2005 .