The Goodman spectrograph

By J. Clemens, J. Crain, R. Anderson. SPIE Astronomical Telescopes + Instrumentation, 2004

247 citations recorded by the source corpus.

Subfields: Atomic and Molecular Physics, and Optics, Instrumentation, Surfaces, Coatings and Films

View Paper: https://www.semanticscholar.org/paper/d44f4ab14feec5d6fd347617057325764f9bb592

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atomic and Molecular Physics, and Optics

1. P.-E. Tremblay
2. S. Redfield
3. B. Metzger
4. B. Gänsicke
5. A. MacFadyen
6. I. Chilingarian
7. J. Leja
8. D. Kasen

In Instrumentation

1. J. Leja
2. B. Metzger
3. E. Berger
4. C. Conroy
5. W. Fong
6. Raffaella Margutti
7. P.-E. Tremblay
8. C. Briceño

Citations in the corpus

• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale (2017, methodology): “Here, we use a spectrum obtained 1.5 days after the GW trigger with the Southern Astrophysical Research Telescope equipped with the Goodman High Throughput Spectrograph (Clemens et al. 2004).”
• 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): “We used the Goodman High Throughput Spectrograph (Clemens et al. 2004) with the 400 lines-per-mm grating and 1” slit (R ∼ 930), beginning with the blue (‘M1’; 4000–8000 Å) setting but switching to the red (‘M2’; 5000–9000 Å) setup as the spectrum evolved to redder wavelengths.”
• An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients (2018, methodology): “We obtained five spectra of AT 2018cow using the Goodman spectrograph (Clemens et al. 2004) mounted on the SOAR telescope in the time range δt∼4.6–34.2 days.”
• White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Line Widths: Kepler Observations of 27 Pulsating DA White Dwarfs through K2 Campaign 8 (2017, methodology): “All K2 fields lie along the ecliptic, so we obtained spectroscopy of all K2 DAVs with the Goodman spectrograph (Clemens et al. 2004) mounted on the 4.1m Southern Astrophysical Research (SOAR) telescope on Cerro Pachón in Chile.”