{"release":{"id":"DR1","released_on":"2026-08-21","doi":null,"url":"https://spacecatalog.org/releases#dr1"},"epoch":{"requested":"now","label":"J2026.685","julian_year":2026.685,"time":"2026-09-08T05:24:17.348Z","years_from_j2000":26.685,"frame":"date","applied":"Proper motion, then precession and nutation. The catalogued J2000 position is carried along the great circle the object's own published motion puts it on, at a constant velocity, and the result is referred to the true equator and equinox of this instant. Those are separate things: the motion moves the object, and the rotation turns the grid under it by about fifty arcseconds a year, with nutation adding up to another seventeen.","excluded":"Parallax, the radial-velocity perspective term, aberration and refraction; each is below the accuracy of the catalogued positions themselves. An object with no published proper motion comes back where the catalogue has it rather than at a fabricated zero, and says so with a null pm_ra_mas_yr. A body with no fixed position is not propagated at all — its place comes from an ephemeris, which is what /api/v1/visible answers with."},"slug":"psr-j0952m0607","name":"PSR J0952-0607","class":"millisecond_pulsar","category":"neutron_star","object_type":"Millisecond pulsar","mag":null,"mag_band":null,"abs_mag":null,"abs_mag_band":null,"distance_ly":5675.120972271336,"distance_method":"dispersion measure through the YMW16 electron-density model","ra_deg":148.03467254166668,"dec_deg":-6.123191666666666,"epoch_ra_deg":148.370201,"epoch_dec_deg":-6.249115,"epoch_moved_arcsec":null,"pm_ra_mas_yr":null,"pm_dec_mas_yr":null,"orbits":null,"semi_major_axis_km":null,"periapsis_km":null,"mass_kg":null,"mass_msun":null,"constellation":"Sextans","discovered":"2017","featured":true,"url":"https://spacecatalog.org/object/psr-j0952m0607","radius_km":null,"radius_kind":null,"data_quality":null,"description":"Among the heaviest neutron stars measured, at roughly two and a third solar masses. It got there by stripping its companion: the star it is devouring is down to a few per cent of the Sun's mass, which is why objects like this are called black widows.","properties":{"associations":"GRS:4FGL_J0952.1-0607[aab+22],OPT:[bph+17]","binary_model":"ELL1","spin_period_s":0.0014137983550231202,"spin_period_derivative":4.773195983334601e-21,"characteristic_age_years":4692931798.916437,"dispersion_measure_pc_cm3":22.411533,"spin_down_luminosity_erg_s":6.668168830742757e+34,"surface_magnetic_field_gauss":83128194.42612727},"designations":[{"catalog":"ATNF","designation":"J0952-0607"},{"catalog":"ATNF","designation":"PSR J0952-0607"}],"source":{"id":"atnf","name":"ATNF Pulsar Catalogue (Manchester+ 2005)","url":"https://www.atnf.csiro.au/research/pulsar/psrcat","license":"Free to use with attribution; cite Manchester+ 2005 (2005AJ....129.1993M)"},"updated_at":"2026-09-02T19:50:56.720Z","attribution":"Data from SpaceCatalog.org. Individual records carry their source and license in `source`; attribution is required for CC-BY and CC-BY-SA rows."}