Table 1
Chronological list of measurements of radially extended PSFs.
PSF | Fig. | Ref. | Observatory | Alt. | Telescope | Band / Line | Range | Object (Symbol) |
|
||||||||
PSFK71 | 1, 2 | 1–4 | Solar Physics | 30 | 36′′ Common reflector | ... | ~20″–180″ | stars |
1 | 2–4 | ... | 1′, 4′ | ☉ (△) | ||||
1, 2 | 3, 4 | Lowell | 2195 | 21′′ reflector | B | ~20″–5° | ♃ and 2 m star | |
1, 2 | 4 | Palomar | 1713 | 48′′ Schmidt | B | ![]() |
stars (•, ×) | |
1, 2 | Mount Wilson | 1742 | 60′′ reflector | B | –![]() |
3 stars (°) | ||
PSFK73 | 1, 2 | 5 | Palomar | 1713 | 48′′ Schmidt | B | 7″–1° | stars |
PSFP73 | 1 | 6 | Goethe Link | 293 | 16′′ reflector | B | 48″–170′ | stars, ![]() |
McDonald | 2076 | 2.1 m Otto Struve | ... | not shown | ||||
PSFS74 | 2 | 7 | Palomar | 1713 | 48′′ Schmidt | RG-1 | 100–600′′ | stars (▴) |
PSFCV, | 8 | McDonald | 2076 | 0.9 m | B | 10″–![]() |
γCMa | |
(PSFCV,1, | 1 | ... | 3.5–90′ | αCMa | ||||
PSFCV,2) | 1, 2 | ... | 1.5–90° | ☉ | ||||
PSFS90 | 2 | 9 | Calar Alto | 2168 | 1.23 m | R | ≲480″ | stars (Λ) |
PSFU91 | 2 | 10 | Kitt Peak | 2160 | 1.09 m | R | 1–975″ | stars |
PSFM92 | 2 | 11 | Kitt Peak | 2160 | 24/36′′ B. Schmidt | g | 5–92″ | HD 19445 (•) |
PSFMBH | 1 | 12 | Kitt Peak | 2160 | No. 1 0.9 m (SARA) | Harris R | 0–150′′ | two stars |
PSF![]() |
1 | |||||||
PSFV,0m, | 1, 2 | 13 | Haute-Provence | 650 | 1.2 m Newtonian | V | ≲160″ | stars |
PSFV,3m | 1 | |||||||
PSFi,0m, | 1, 2 | I | ≲160″ | stars | ||||
PSFi,3m | 1 | |||||||
PSFG05 | 2 | 14 | Las Campanas | 2282 | 40′′ Swope | Gunn i | 10–400′′ | stars |
PSFB07 | 2 | 15 | Las Campanas | 2282 | 100′′ du Pont | r | ≲400″ | stars |
PSFP,LR | 1 | 16 | Calar Alto | 2168 | 3.5 m/PMAS | Hα | –25″ | αLyr |
PSFS09 | 1 | 17 | Kitt Peak | 2160 | 24/36′′ B. Schmidt | Wash. M | ![]() |
αBoo, star |
SDSS | 1 | 18, 19, | Apache Point | 2788 | 2.5 m | g, r, i, ... | ≲46″ | stars |
20, 21 | ||||||||
PSFA14 | 1 | 22 | New Mexico Skies | 2200 | Dragonfly Array | r | 5.̋1–56.́8 | αLyr |
Notes.Column 1, PSF notation used in this paper; Col. 2, the PSF is
shown in this figure; Col. 3, references; Col. 4, observatory; Col. 5, altitude of the
observatory (m); Col. 6, telescope (/instrument); Col. 7, wavelength bandpass or line
that was used; Col. 8; radial extent of PSF measurements; and Col. 9, objects used to
measure the PSF (and symbols used in Fig. 1). The
object symbols are ♃
(Jupiter),
(the Moon), and ☉ (the
Sun).
Reference. (1) Redman & Shirley (1938); (2) van de Hulst (1948); (3) de Vaucouleurs (1958); (4) K71; (5) Kormendy (1973); (6) Piccirillo (1973); (7) Shectman (1974); (8) CV83; (9) Surma et al. (1990); (10) Uson et al. (1991), (11) Mackie (1992); (12) MBH94; (13) Michard (2002); (14) Gonzalez et al. (2005); (15) B07; (16) Sandin et al. (2008); (17) SHM09; (18) Zibetti et al. (2004); (19) J08; (20) Bergvall et al. (2010); (21) Tal & van Dokkum (2011); (22) Abraham & van Dokkum (2014).
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