Harps-N: the new planet hunter at TNG

By R. Cosentino, C. Lovis, F. Pepe, A. Collier Cameron, D. Latham, E. Molinari, S. Udry, N. Bezawada, M. Black, Andrew J. Born and 38 more. Other Conferences, 2012

285 citations recorded by the source corpus.

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

View Paper: https://www.semanticscholar.org/paper/6f34770aeaec93d3a7a06dc514265b8ab4507d59

How researchers see this paper

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

In Astronomy and Astrophysics

1. D. Charbonneau
2. J. Johnson
3. J. Southworth
4. S. Udry
5. M. Mayor
6. Timothy Morton
7. J. Winn
8. Andrew Vanderburg

In Atomic and Molecular Physics, and Optics

1. J. Johnson
2. C. Dressing
3. B. Bowler
4. S. Udry
5. M. Mayor
6. D. Charbonneau
7. F. Pepe
8. C. Lovis

In Instrumentation

1. D. Charbonneau
2. J. Johnson
3. J. Southworth
4. S. Udry
5. C. Dressing
6. Timothy Morton
7. B. Bowler
8. Andrew Vanderburg

Citations in the corpus

• CHARACTERIZING K2 PLANET DISCOVERIES: A SUPER-EARTH TRANSITING THE BRIGHT K DWARF HIP 116454 (2014, methodology): “HARPS-N Spectroscopy We obtained 44 spectra of HIP 116454 on 33 different nights between July and October of 2014 with the HARPS-N spectrograph (Cosentino et al. 2012) on the 3.57m Telescopio Nazionale Galileo (TNG) on La Palma Island, Spain to measure precise radial velocities and determine the…”
• THE MASS OF Kepler-93b AND THE COMPOSITION OF TERRESTRIAL PLANETS (2014, methodology): “The main differences are that HARPS-N is fed by octagonal fibers rather than circular fibers to improve the scrambling of the light and features a monolithic 4096 x 4096 CCD instead of the dual CCD configuration used for the HARPS focal plane (Cosentino et al. 2012).”
• THE KEPLER-10 PLANETARY SYSTEM REVISITED BY HARPS-N: A HOT ROCKY WORLD AND A SOLID NEPTUNE-MASS PLANET (2014, methodology): “We monitored the RV variation of Kepler-10 with the HARPS-N spectrograph installed on the 3.57-m Telescopio Nazionale Galileo at the Spanish Observatorio del Roque de los Muchachos, La Palma Island, Spain (Cosentino et al. 2012).”
• EXTRACTING RADIAL VELOCITIES OF A- AND B-TYPE STARS FROM ECHELLE SPECTROGRAPH CALIBRATION SPECTRA (2015, unknown): “…particularly with the construction of environmentally-stabilized spectrometers such as the HARPS-South and -North spectrographs (Mayor et al. 2003; Cosentino et al. 2012), SOPHIE at Haute-Provence (Bouchy et al. 2009), CHIRON at CTIO (Schwab et al. 2010), and the Planet Finder Spectrograph (PFS)…”