Rosat All Sky Survey

Rosat All Sky Survey. Skyfield_source_number the number of the individual source in a given sky field observing sequence. Rass total (cts/s) exposure time (s) j2000 j2000d gal.

ROSAT AllSky Survey 3/4 keV from heasarc.gsfc.nasa.gov

Rass total (cts/s) exposure time (s) j2000 j2000d gal. The sources have a detection likelihood of at least 15 and contain at least 15 source photons. The main bcs, which was presented in ebeling et al.

Source: heasarc.gsfc.nasa.gov

Rosat operated for over eight years, finally shutting. At a brightness limit of 0.1 cts/s (8,547 sources) the catalogue represents a sky coverage of 92%.

Source: heasarc.gsfc.nasa.gov

Skyfield_source_number the number of the individual source in a given sky field observing sequence. In the paper, the quasar optical luminosity function (lf) at 0.04 < z <= 0.3 is computed and shown to.

Source: www-xray.ast.cam.ac.uk

At a brightness limit of 0.1 cts/s (8,547 sources) the catalogue represents a sky coverage of 92%. A different prefix ('rxs') was used in the published version of this paper.

The Main Bcs, Which Was Presented In Ebeling Et Al.

The sources have a detection likelihood of at least 15 and contain at least 15 source photons. Rass total (cts/s) exposure time (s) j2000 j2000d gal. In the rosat survey, the entire sky was mapped and sources were visible a hundred times fainter than in any previous survey.

(For Comparison, The Surface Of The Sun Is About 5,000 Kelvin.)

The temperatures of these sources ranged from about 100,000 kelvin to 20 million kelvin! The sources have a detection likelihood of at least 15 and contain at least 15 source photons. More information on the data from the gsfc rass mirror site at:

Rosat Operated For Over Eight Years, Finally Shutting.

The maps cover approximately 98 % of the sky in the 1/4 kev, 3/4 kev, and 1.5 kev bands, with an angular resolution of about 2 degrees and high sensitivity for low surface brightness extended. The angular resolution of the rosat telescope in combination with the pspc camera is approximately 1.8 '. Ra the right ascension of the first source assumed to be the radio counterpart of the rass source, in the selected equinox.

At A Brightness Limit Of 0.1 Cts/S (8,547 Sources) The Catalogue Represents A Sky Coverage Of 92%.

The skyfield_number represents the rass sequence id number of the sky field. Skyfield_source_number the number of the individual source in a given sky field observing sequence. A different prefix ('rxs') was used in the published version of this paper.

In The Paper, The Quasar Optical Luminosity Function (Lf) At 0.04 < Z <= 0.3 Is Computed And Shown To.

During its first year of operation it performed the first imaging survey of the whole sky in x.