4C Array: Difference between revisions

Content deleted Content added
Lightbot (talk | contribs)
Delink non-obscure units. Conversions. Report bugs to Lightmouse
fix date
 
(14 intermediate revisions by 12 users not shown)
Line 1:
{{Short description|Radio telescope in Cambridge, England}}
{{Infobox Telescope
{{Use dmy dates|date=April 2022}}
| name = 4C Array
{{unreferenced|date=October 2015}}
| image =
{{Infobox Telescopetelescope}}
| caption =
The '''4C Array''' is a cylindrical paraboloid [[radio telescope]] at the [[Mullard Radio Astronomy Observatory]], near Cambridge, England. It is similar in design to the [[Molonglo Observatory Synthesis Telescope]]. It is 450 m long, 20 m wide, with a second, moveable element (now mostly removed; some of it is still visible, beyond [[Cambridge Optical Aperture Synthesis Telescope (COAST)|COAST]]).{{Citation needed|date=January 2024}} The first large aperture synthesis telescope ([[1958]]), it was also the first new instrument to be built at [[Lord's Bridge (Cambridgeshire)|Lord's Bridge]], after the [[Mullard Radio Astronomy Observatory|Observatory]] was moved there in [[1957]], and needed {{convert|64|km|mi|abbr=on}} of reflector wire (since removed).{{Citation needed|date=January 2024}} The 4C operated at 178  MHz (1.7 m), and located nearly 5000 sources of the [[Fourth Cambridge Survey|4C (4th Cambridge) catalogue]] published in [[1965]] and [[1966]], which helped establish the evolution of the radio galaxy population of the universe. The telescope is now inoperable.{{Citation needed|date=January 2024}}
| organization = [[Mullard Radio Astronomy Observatory]]
| ___location = [[Lord's Bridge]], nr. [[Cambridge]], [[England]]
| coords = {{coord|52.164147|N|0.033174|E|display=inline,title}}
| altitude =
| weather =
| wavelength = 1.7m
| built = 1958
| first_light =
| website =
| style = Cylindrical paraboloid
| diameter =
| angular_resolution =
| area =
| focal_length =
| mounting =
}}
The '''4C Array''' is a cylindrical paraboloid [[radio telescope]] at the [[Mullard Radio Astronomy Observatory]]. It is similar in design to the [[Molonglo Observatory Synthesis Telescope]]. It is 450 m long, 20 m wide, with a second, moveable element (now mostly removed; some of it is still visible, beyond [[Cambridge Optical Aperture Synthesis Telescope (COAST)|COAST]]). The first large aperture synthesis telescope ([[1958]]), it was also the first new instrument to be built at [[Lord's Bridge (Cambridgeshire)|Lord's Bridge]], after the [[Mullard Radio Astronomy Observatory|Observatory]] was moved there in [[1957]], and needed {{convert|64|km|mi|abbr=on}} of reflector wire (since removed). The 4C operated at 178 MHz (1.7 m), and located nearly 5000 sources of the [[Fourth Cambridge Survey|4C (4th Cambridge) catalogue]] published in [[1965]] and [[1966]], which helped establish the evolution of the radio galaxy population of the universe. The telescope is now inoperable.
 
It is flanked to the northwest by the [[Cosmic Anisotropy Telescope]] enclosure and to the south by the [[One-Mile Telescope|One-Mile]] and [[Half-Mile Telescope]]s.{{Citation needed|date=January 2024}}
 
[[File:cmglee Cambridge MRAO One Mile Half Mile 4C.jpg|thumb|250px|none|One antenna of the One-Mile Telescope (left), two of the Half-Mile Telescope (centre) and the remains of the 4C Array (right) in June 2014]]
 
== References ==
<references />
 
[[Category:Cavendish Laboratory]]
Line 28 ⟶ 16:
[[Category:Interferometric telescopes]]
[[Category:Astronomical observatories in England]]
 
 
{{observatory-stub}}