VIRUS early installation and commissioning

Proceedings of SPIE Society of Photo-optical Instrumentation Engineers 9908 (2016)

Authors:

SE Tuttle, GJ Hill, BL Vattiat, H Lee, N Drory, A Kelz, Gavin Dalton

Abstract:

VIRUS is a massively replicated spectrograph built for HETDEX, the Hobby Eberly Telescope Dark Energy Experiment. It consists of 156 channels within 78 units fed by 34944 fibers over the 22 arcminute field of the upgraded HET. VIRUS covers a relatively narrow bandpass (350-550nm) at low resolution (R ~ 700) to target the emission of Lyman-alpha emitters (LAEs) for HETDEX. VIRUS is a first demonstration of industrial style assembly line replication in optical astronomy. Installation and testing of VIRUS units began in November of 2015. This winter we celebrated the first on sky instrument activity of the upgraded HET, using a VIRUS unit and LRS2-R (the upgraded facility Low Resolution Spectrograph for the HET). Here we describe progress in VIRUS installation and commissioning through June 2016. We include early sky data obtained to characterize spectrograph performance and on sky performance of the newly upgraded HET. As part of the instrumentation for first science light at the HET, the IFU fed spectrographs were used to test a full range of telescope system functionality including the field calibration unit (FCU).We also use placement of strategic IFUs to map the new HET field to the fiber placement, and demonstrate actuation of the dithering mechanism key to HETDEX observations.

Making SPIFFI SPIFFIER: upgrade of the SPIFFI instrument for use in ERIS and performance analysis from re-commissioning

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9908 (2016) 99080g-99080g-20

Authors:

EM George, D Gräff, H Feuchtgruber, M Hartl, F Eisenhauer, A Buron, R Davies, R Genzel, H Huber, C Rau, M Plattner, E Wiezorrek, H Weisz, P Amico, A Glindemann, G Hau, H Kuntschner

Towards integrated modelling: full image simulations for WEAVE

Proceedings of SPIE Society of Photo-optical Instrumentation Engineers 9913 (2016)

Authors:

Gavin Dalton, Sun J Ham, Scott C Trager, Don C Abrams, Piercarlo Bonifacio, J Alfonso L Aguerri, Kevin F Middleton, Chris R Benn, Kevin Rogers, Remko Stuik, Esperanza Carrasco, Antonella Vallenari, Shoko Jin, Jim R Lewis

Abstract:

We present an integrated end-end simulation of the spectral images that will be obtained by the weave spectrograph, which aims to include full modelling of all effects from the top of the atmosphere to the detector. These data are based in input spectra from a combination of library spectra and synthetic models, and will be used to provide inputs for an endend test of the full weave data pipeline and archive systems, prior to 1st light of the instrument.

Black Hole Mass Measurement in Nearby Galaxy Using Molecular Gas Dynamics

Institute of Electrical and Electronics Engineers (IEEE) (2016) 1-4

Authors:

Kyoko Onishi, Satoru Iguchi, Timothy Davis, Martin Bureau, Michele Cappellari, Leo Blitz, Marc Sarzi

Developing an integrated concept for the E-ELT Multi-Object Spectrograph (MOSAIC): design issues and trade-offs

Proceedings of SPIE Society of Photo-optical Instrumentation Engineers 9908 (2016)

Authors:

Myriam Rodrigues, Gavin Dalton, Ewan Fitzsimons, Fanny Chemla, Tim Morris, Francois Hammer, Mathieu Puech, Christopher J Evans, Pascal Jagourel

Abstract:

We present a discussion of the design issues and trade-offs that have been considered in putting together a new concept for MOSAIC, the multi-object spectrograph for the E-ELT. MOSAIC aims to address the combined science cases for E-ELT MOS that arose from the earlier studies of the multi-object and multi-adaptive optics instruments. MOSAIC combines the advantages of a highly-multiplexed instrument targeting single-point objects with one which has a more modest multiplex but can spatially resolve a source with high resolution (IFU). These will span across two wavebands: visible and near-infrared.