Article (Scientific journals)
High-contrast Stellar Observations within the Diffraction Limit at the Palomar Hale Telescope
Mennesson, B.; Hanot, Charles; Serabyn, Eugene et al.
2011In Astrophysical Journal, 743, p. 178
Peer Reviewed verified by ORBi
 

Files


Full Text
MENN_giants.pdf
Author preprint (571.48 kB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
circumstellar matter; infrared: stars; instrumentation: high angular resolution; stars: individual: α Boo α Her β Peg β And α Ori ρ Per α Aur χ Cyg
Abstract :
[en] We report on high-accuracy high-resolution (<20 mas) stellar observations obtained with the Palomar Fiber Nuller (PFN), a near-infrared (sime2.2 μm) interferometric coronagraph installed at the Palomar Hale telescope. The PFN uses destructive interference between two elliptical (3 m × 1.5 m) sub-apertures of the primary to reach high dynamic range inside the diffraction limit of the full telescope. In order to validate the PFN's instrumental approach and its data reduction strategy, based on the newly developed "Null Self-Calibration" (NSC) method, we observed a sample of eight well-characterized bright giants and supergiants. The quantity measured is the source astrophysical null depth, or equivalently the object's visibility at the PFN 3.2 m interferometric baseline. For the bare stars α Boo, α Her, β And, and α Aur, PFN measurements are in excellent agreement with previous stellar photosphere measurements from long baseline interferometry. For the mass-losing stars β Peg, α Ori, ρ Per, and χ Cyg, circumstellar emission and/or asymmetries are detected. Overall, these early observations demonstrate the PFN's ability to measure astrophysical null depths below 10[SUP]-2[/SUP] (limited by stellar diameters), with 1 σ uncertainties as low as a few 10[SUP]-4[/SUP]. Such visibility accuracy is unmatched at this spatial resolution in the near-infrared and translates into a contrast better than 10[SUP]-3[/SUP] within the diffraction limit. With further improvements anticipated in 2011/2012, a state-of-the-art infrared science camera and a new extreme adaptive optics system, the PFN should provide a unique tool for the detection of hot debris disks and young self-luminous sub-stellar companions in the immediate vicinity of nearby stars.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Mennesson, B.;  Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA
Hanot, Charles ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Serabyn, Eugene;  Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA
Liewer, Kurt;  Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA
Martin, Stefan
Mawet, D.;  European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
Language :
English
Title :
High-contrast Stellar Observations within the Diffraction Limit at the Palomar Hale Telescope
Publication date :
01 December 2011
Journal title :
Astrophysical Journal
ISSN :
0004-637X
eISSN :
1538-4357
Publisher :
University of Chicago Press, Chicago, United States - Illinois
Volume :
743
Pages :
178
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 02 February 2012

Statistics


Number of views
89 (4 by ULiège)
Number of downloads
217 (0 by ULiège)

Scopus citations®
 
27
Scopus citations®
without self-citations
14
OpenCitations
 
23

Bibliography


Similar publications



Contact ORBi