J/A+A/672/A114      FITS images of HST debris disks                 (Ren+, 2023)

Debris Disk Color with the Hubble Space Telescope. Ren B.B., Rebollido I., Choquet E., Zhou W.-H., Perrin M. D., Schneider G., Milli J., Wolff S.G., Chen C.H., Debes J.H., Hagan J.B., Hines D.C., Millar-Blanchaer M.A., Pueyo L., Roberge A., Serabyn E., Soummer R. <Astron. Astrophys. 672, A114 (2023)> =2023A&A...672A.114R 2023A&A...672A.114R (SIMBAD/NED BibCode)
ADC_Keywords: Stars, normal ; Interstellar medium ; Optical ; Infrared Keywords: stars: imaging - instrumentation: high angular resolution - Kuiper Belt: general - techniques: image processing Abstract: Multi-wavelength scattered light imaging of debris disks may inform dust properties including typical size and mineral composition. Existing studies have investigated a small set of individual systems across a variety of imaging instruments and filters, calling for uniform comparison studies to systematically investigate dust properties. We obtain the surface brightness of dust particles in debris disks by post-processing coronagraphic imaging observations, and compare the multi-wavelength reflectance of dust. For a sample of resolved debris disks, we perform a systematic analysis on the reflectance properties of their birth rings. We reduced the visible and near-infrared images of 23 debris disk systems hosted by A through M stars using two coronagraphs onboard the Hubble Space Telescope: the STIS instrument observations centering at 0.58um, and the NICMOS instrument at 1.12um or 1.60um. For proper recovery of debris disks, we used classical reference differential imaging for STIS, and adopted non-negative matrix factorization with forward modeling for NICMOS. By dividing disk signals by stellar signals to take into account of intrinsic stellar color effects, we systematically obtained and compared the reflectance of debris birth rings at ∼90° scattering angle. Debris birth rings typically exhibit a blue color at ∼90° scattering angle. As the stellar luminosity increases, the color tends to be more neutral. A likely L-shaped color-albedo distribution indicates a clustering of scatterer properties. The observed color trend correlates with the expected blow-out size of dust particles. The color-albedo clustering likely suggests different populations of dust in these systems. More detailed radiative transfer models with realistic dust morphology will contribute to explaining the observed color and color-albedo distribution of debris systems. Description: FITS files of disk images in STIS and NICMOS (F110W and F160W) from the Hubble Space Telescope. The stars are located at the mathematical centers of the arrays. The units are in counts per pixel per second. The STIS date were reduced with classical reference differential imaging. The NICMOS data were reduced with non-negative matrix factorization without a scaling factor here, so they are prone to over-fitting, and they are fainter than their actual surface brightness. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 35 23 List of studied stars list.dat 99 56 List of fits images fits/* . 56 Individual fits images -------------------------------------------------------------------------------- See also: J/ApJ/768/25 : Spitzer & Herschel debris disks observations (Gaspar+, 2013) J/ApJ/798/87 : Spitzer/IRS debris disk catalog. II. (Mittal+, 2015) J/A+A/591/A108 : HD61005 SPHERE H and Ks images (Olofsson+, 2016) J/A+A/595/A31 : SAM detection limits of 8 debris disks (Gauchet+, 2016) J/AJ/154/245 : Spitzer-detected debris disks imaging survey (Meshkat+, 2017) J/A+A/630/A85 : SPHERE images of HD 32297 (Bhowmik+, 2019) J/A+A/630/A142 : HR4796 debris disk Qphi and Uphi images (Olofsson+, 2019) J/A+A/635/A19 : HD 117214 debris disk polarization images (Engler+, 2020) J/A+A/646/A132 : beta Pictoris debris disk image (Janson+, 2021) J/AJ/161/78 : SPHERE astrometry for 14 debris disk stars (Matthews+, 2021) Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Star name 12- 13 I2 h RAh right ascension (J2000) 15- 16 I2 min RAm right ascension (J2000) 18- 22 F5.2 s RAs right ascension (J2000) 24 A1 --- DE- Declination sign (J2000) 25- 26 I2 deg DEd Declination (J2000) 28- 29 I2 arcmin DEm Declination (J2000) 31- 35 F5.2 arcsec DEs Declination (J2000) -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Star name 12- 13 I2 h RAh right ascension (J2000) 15- 16 I2 min RAm right ascension (J2000) 18- 22 F5.2 s RAs right ascension (J2000) 24 A1 --- DE- Declination sign (J2000) 25- 26 I2 deg DEd Declination (J2000) 28- 29 I2 arcmin DEm Declination (J2000) 31- 35 F5.2 arcsec DEs Declination (J2000) 37- 39 I3 Kibyte size Size of FITS file 41- 65 A25 --- FileName Name of FITS file, in subdirectory fits 67- 99 A33 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Bin Ren, bin.ren(at)oca.eu
(End) Patricia Vannier [CDS] 17-Feb-2023
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line