Precise photometry and astrometry in the core of the globular cluster NGC 6121 using PSF-R techniques
暂无分享,去创建一个
Thierry Fusco | Benoit Neichel | Julien Milli | Davide Massari | Florian Kerber | Giuliana Fiorentino | Eline Tolstoy | Olivier Beltramo-Martin | Antonino Marasco | T. Fusco | J. Milli | B. Neichel | D. Massari | G. Fiorentino | E. Tolstoy | A. Marasco | F. Kerber | O. Beltramo-Martin
[1] Jay Anderson,et al. Toward High‐Precision Astrometry with WFPC2. I. Deriving an Accurate Point‐Spread Function , 2000, astro-ph/0006325.
[2] Laurent Jolissaint,et al. Status of point spread function determination for Keck adaptive optics , 2014, Astronomical Telescopes and Instrumentation.
[3] T Fusco,et al. Pushing point-spread function reconstruction to the next level: application to SPHERE/ZIMPOL , 2020 .
[4] A. McConnachie,et al. GeMS MCAO observations of the Galactic globular cluster NGC 2808: the absolute age , 2015, 1512.03194.
[5] Davide Massari,et al. Multiple stellar populations in the globular cluster M3 (NGC 5272): a Strömgren perspective , 2016, 1603.02827.
[6] Miska Le Louarn,et al. Improvements to MASS turbulence profile estimation at Paranal , 2018, Astronomical Telescopes + Instrumentation.
[7] F. Derie,et al. Optical turbulence profiling with stereo-SCIDAR for VLT and ELT. , 2018, 1806.02585.
[8] T Fusco,et al. Off-axis point spread function characterization in laser guide star adaptive optics systems , 2018, Monthly Notices of the Royal Astronomical Society.
[9] T. Fusco,et al. SPHERE/ZIMPOL high resolution polarimetric imager , 2018, Astronomy & Astrophysics.
[10] H. Maître,et al. Estimation of the adaptive optics long-exposure point-spread function using control loop data , 1997 .
[11] E. Marchetti,et al. GeMS/GSAOI PHOTOMETRIC AND ASTROMETRIC PERFORMANCE IN DENSE STELLAR FIELDS , 2016, 1610.03489.
[12] Jessica R. Lu,et al. Astrometric performance of the Gemini multiconjugate adaptive optics system in crowded fields , 2014, 1409.0719.
[13] S. Cassisi,et al. A Large Stellar Evolution Database for Population Synthesis Studies. II. Stellar Models and Isochrones for an α-enhanced Metal Distribution , 2006 .
[14] G. Fiorentino,et al. Astrometry with MCAO: HST-GeMS proper motions in the globular cluster NGC 6681 , 2016, 1609.05923.
[15] F. Kerber,et al. Successful application of PSF-R techniques to the case of the globular cluster NGC 6121 (M 4) , 2020, Astronomy & Astrophysics.
[16] Kjetil Dohlen,et al. SPHERE ZIMPOL: overview and performance simulation , 2008, Astronomical Telescopes + Instrumentation.
[17] P. Stetson. DAOPHOT: A COMPUTER PROGRAM FOR CROWDED-FIELD STELLAR PHOTOMETRY , 1987 .
[18] Santiago Arribas,et al. The effective temperature scale of giant stars (F0–K5) - II. Empirical calibration of versus colours and [Fe/H] , 1999 .
[19] T. Fusco,et al. Optimal correction of distortion for high-angular-resolution images: Application to GeMS data , 2017, 1709.08567.
[20] Laird M. Close,et al. Analysis of isoplanatic high resolution stellar fields by the StarFinder code , 2000 .
[21] T. Fusco,et al. Turbulent and adaptive optics corrected point-spread functions as convolutive orders of the phase power spectral density , 2018, Monthly Notices of the Royal Astronomical Society.
[22] Laurent Jolissaint,et al. Determination of the optical turbulence parameters from the adaptive optics telemetry: critical analysis and on-sky validation. , 2018, Applied optics.
[23] Markus Feldt,et al. Data Reduction and Handling for SPHERE , 2008 .
[24] Peter Pessev,et al. GeMS: first on-sky results , 2012, Other Conferences.
[25] Giampaolo Piotto,et al. THE ACS SURVEY OF GLOBULAR CLUSTERS. V. GENERATING A COMPREHENSIVE STAR CATALOG FOR EACH CLUSTER , 2008 .
[26] Manash R. Samal,et al. Deep GeMS/GSAOI near-infrared observations of N159W in the Large Magellanic Cloud , 2016, 1605.07846.
[27] S. Saracino,et al. GEMINI/GeMS OBSERVATIONS UNVEIL THE STRUCTURE OF THE HEAVILY OBSCURED GLOBULAR CLUSTER LILLER 1. , 2015, 1505.00568.
[28] P L Wizinowich,et al. PRIME: PSF Reconstruction and Identification for Multiple-source characterization Enhancement – application to Keck NIRC2 imager , 2019, Monthly Notices of the Royal Astronomical Society.
[29] L. Origlia,et al. ULTRA-DEEP GEMINI NEAR-INFRARED OBSERVATIONS OF THE BULGE GLOBULAR CLUSTER NGC 6624 , 2016, 1609.02152.
[30] Peter L. Wizinowich,et al. The AIROPA software package: milestones for testing general relativity in the strong gravity regime with AO , 2016, Astronomical Telescopes + Instrumentation.
[31] Jessica R. Lu,et al. Measuring Distance and Properties of the Milky Way’s Central Supermassive Black Hole with Stellar Orbits , 2008, 0808.2870.
[32] G. Piotto,et al. Spectroscopic and photometric evidence of two stellar populations in the Galactic globular cluster NGC 6121 (M 4) , 2008, 0808.1414.
[33] Sylvain Oberti,et al. Physics-based model of the adaptive-optics-corrected point spread function , 2019, Astronomy & Astrophysics.
[34] Eleazar R. Carrasco,et al. The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS). I. A Pilot Study of the Stellar Populations in NGC 2298 and NGC 3201 , 2018, The Astrophysical Journal.
[35] A. Bellini,et al. HUBBLE SPACE TELESCOPE PROPER MOTION (HSTPROMO) CATALOGS OF GALACTIC GLOBULAR CLUSTERS. I. SAMPLE SELECTION, DATA REDUCTION, AND NGC 7078 RESULTS , 2014, 1410.5820.
[36] E. Tolstoy,et al. Three-dimensional motions in the Sculptor dwarf galaxy as a glimpse of a new era , 2017, 1711.08945.