SNIFS: a wideband integral field spectrograph with microlens arrays

By B. Lantz, G. Aldering, P. Antilogus, C. Bonnaud, L. Capoani, A. Castera, Y. Copin, D. Dubet, E. Gangler, F. Hénault and 5 more. 2003

151 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

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Citations in the corpus

STELLAR AND PLANETARY PROPERTIES OF K2 CAMPAIGN 1 CANDIDATES AND VALIDATION OF 17 PLANETS, INCLUDING A PLANET RECEIVING EARTH-LIKE INSOLATION (2015, methodology): “An optical spectrum was obtained using SNIFS (Aldering et al. 2002; Lantz et al. 2004) on the University of Hawai’i 2.2 m telescope on the night of 2015 January 30.”
HOW TO CONSTRAIN YOUR M DWARF: MEASURING EFFECTIVE TEMPERATURE, BOLOMETRIC LUMINOSITY, MASS, AND RADIUS (2015, methodology): “Optical spectra of all stars were obtained with the SuperNova Integral Field Spectrograph (SNIFS, Aldering et al. 2002; Lantz et al. 2004) on the University of Hawaii 2.2 m telescope on Mauna Kea.”
Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local H$\alpha$ (2013, methodology): “The SNfactory has observed a large sample of nearby SNe and their immediate surroundings using the SuperNova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) installed on the UH 2.2m telescope (Mauna Kea).”
Nearby Supernova Factory Observations of SN 2005gj: Another Type Ia Supernova in a Massive Circumstellar Envelope (2006, methodology): “SNIFS Spectroscopy Observations of SN 2005gj were obtained with SNIFS (Aldering et al. 2002; Lantz et al. 2004), operated by the SNfactory.”
ZODIACAL EXOPLANETS IN TIME (ZEIT). III. A SHORT-PERIOD PLANET ORBITING A PRE-MAIN-SEQUENCE STAR IN THE UPPER SCORPIUS OB ASSOCIATION (2016, methodology): “Optical Spectrum from SNIFS We obtained an optical spectrum of K2-33 on February 23, 2016 (UT) with the SuperNova Integral Field Spectrograph (SNIFS, Aldering et al. 2002; Lantz et al. 2004) on the University of Hawai’i 2.2m telescope on Maunakea.”
THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617 (2013, methodology): “The integral field unit spectrum obtained with the SupernovaIntegral Field Spectrograph (SNIFS; Lantz et al. 2004) at the University of Hawaii (UH) 2.2-m was reduced and extracted using the SNIFS Data Reduction Package (Aldering et al. 2006).”
PROSPECTING IN LATE-TYPE DWARFS: A CALIBRATION OF INFRARED AND VISIBLE SPECTROSCOPIC METALLICITIES OF LATE K AND M DWARFS SPANNING 1.5 dex (2012, methodology): “2m We obtained a visible spectrum of each companion with the SuperNova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) on the University of Hawaii 2.2m telescope atop Mauna Kea.”
The quest for dual and binary supermassive black holes: A multi-messenger view (2019, background): “2m Hawaii Telescope instrument SNIFS (Aldering et al., 2002; Lantz et al., 2004) at a spatial resolution of approximately 1.”
A SPECTROSCOPIC CATALOG OF THE BRIGHTEST (J < 9) M DWARFS IN THE NORTHERN SKY, (2012, methodology): “Spectra for a total of 901 bright M dwarf targets were collected at MDM. Additional spectra were obtained with the SuperNova Integral Field Spectrograph (SNIFS; Lantz et al. 2004) on the University of Hawaii 2.2 m telescope on Mauna Kea between February 2009 and November 2012.”
SPECTRO-THERMOMETRY OF M DWARFS AND THEIR CANDIDATE PLANETS: TOO HOT, TOO COOL, OR JUST RIGHT? (2013, methodology): “Optical spectra of both the calibration sample and the Kepler planet host sample were obtained with the SuperNova Integral Field Spectrograph (SNIFS, Aldering et al. 2002; Lantz et al. 2004) on the University of Hawaii 2.2m telescope atop Mauna Kea.”