IMACS: The Inamori-Magellan Areal Camera and Spectrograph on Magellan-Baade

By A. Dressler, B. Bigelow, T. Hare, B. Sutin, I. Thompson, G. Burley, H. Epps, A. Oemler, A. Bagish, C. Birk and 5 more. 2011

248 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/15b6f22f4efc244b2476d3298304990d6ea06719

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Citations in the corpus

The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample (2017, methodology): “…Magellan Echellette (MagE; Marshall et al. 2008) on the 6.5 m Magellan Clay telescope, the Inamori-Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2011) on the 6.5 m Magellan Baade telescope, the ISIS spectrograph on the WHT,24 and DEIMOS (Faber et al. 2003) on the 10 m Keck…”
COSMOLOGICAL CONSTRAINTS FROM MEASUREMENTS OF TYPE Ia SUPERNOVAE DISCOVERED DURING THE FIRST 1.5 yr OF THE Pan-STARRS1 SURVEY (2013, background): “…Echellette (MagE; Marshall et al. 2008) on the 6.5- m Magellan Clay telescope, and the Inamori-Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2011) on the 6.5-m Magellan Baade telescope, and the ISIS spectrograph on the WHT. Nod-and-shuffle techniques (Glazebrook &…”
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta (2017, methodology): “Subsequently, we obtained optical spectra with the 6.5-m Magellan/Baade telescope equipped with the Inamori Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2011).”
Six months of multiwavelength follow-up of the tidal disruption candidate asassn-14li and implied tde rates from asas-sn (2015, background): “…et al. 1998) mounted on the Fred L. Whipple Observatory Tillinghast 1.5-m telescope (3700−9000 Å, R ∼ 3 Å), and the Inamori Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2011) mounted on the Las Campanas Observatory Magellan-Baade 6.5-m telescope (3650−9740 Å, R ∼ 8…”
STELLAR MASSES FROM THE CANDELS SURVEY: THE GOODS-SOUTH AND UDS FIELDS (2014, methodology): “The IMACS spectroscopic observations were reduced using the COSMOS data reduction pipeline developed at the Carnegie Observatories27 (Dressler et al. 2011).”
TYPE Iax SUPERNOVAE: A NEW CLASS OF STELLAR EXPLOSION (2012, methodology): “…(Buzzoni et al. 1984) on the ESO 3.6 m telescope, the LDSS3 spectrograph19 on the Magellan Clay 6.5 m telescope, the IMACS spectrograph (Dressler et al. 2011) on the Magellan Baade 6.5 m telescope, and the Low Resolution Imaging Spectrometer (LRIS; Oke et al. 1995) on the 10 m Keck I…”
The SAGA Survey. I. Satellite Galaxy Populations around Eight Milky Way Analogs (2017, methodology): “Data were reduced using the COSMOS software (Dressler et al. 2011).”
SILVERRUSH. IV. Lyα luminosity functions at z = 5.7 and 6.6 studied with ∼1300 Lyα emitters on the 14–21 deg2 sky (2017, methodology): “…spectroscopic redshifts are obtained by our past and present programs with Subaru/Faint Object Camera and Spectrograph (FOCAS; Kashikawa et al. 2002), Magellan/Low Dispersion Survey Spectrograph 3 (LDSS3), and Magellan/Inamori Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2011).”
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): “…at the APO 3.5-m, Boller & Chivens CCD Spectrograph (CCDS) at the MDM 2.4-m and 1.3-m, OSMOS at the MDM 2.4-m, and the Inamori-Magellan Areal Camera & Spectrograph (IMACS; Dressler et al. 2011) at the Magellan 6.5-m were all reduced with standard routines in the IRAFtwodspec andonedspec packages.”
Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky (2017, result): “In addition to the observations described above, we in- clude results of our observations with the Inamori Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2011) on the Magellan I Baade telescope in 2007 – 2011 (PI: M. Ouchi).”
Farthest Neighbor: The Distant Milky Way Satellite Eridanus II (2016, methodology): “…procedures include bias subtraction, removal of read-out pattern noise, an initial wavelength solution and slit mapping with the Cosmos pipeline (Dressler et al. 2011), and a refined wavelength calibration and spectral extraction using an IMACS pipeline derived from the DEEP2 data reduction…”