# One file per cluster. Field reference: docs/data-format.md

name: SDSS J1029+2623
designations:
  - CXOGSG J102911.9+262338
  - 1RXS J102912.0+262338
ra: "10:29:11.90"
dec: "+26:23:38.00"
z: 0.588

models:
  - title: Napier et al. (2023b)
    refs: [2023ApJ...959..134N]
    availability: unknown
    tags: [time-delay-cosmography]
    note: |-
      Modelled with [SDSS J1004+4112](cluster:sdss-j1004p4112) and
      [SDSS J2222+2745](cluster:sdss-j2222p2745) for a time-delay H0 measurement.
  - title: Acebron et al. (2022b)
    refs: [2022ApJ...926...86A]
    availability: unknown
    note: |-
      The paper also studies the [multiply imaged quasar](transient:sdss-j1029p2623-agn).
  - title: Oguri et al. (2013)
    refs: [2013MNRAS.429..482O]
    availability: unknown
  - title: Oguri et al. (2012)
    refs: [2012MNRAS.420.3213O]
    availability: unknown
  - title: Kratzer et al. (2011)
    refs: [2011ApJ...728L..18K]
    data: [ground]
    availability: unknown
    note: |-
      Model fitted to resolved radio (VLA) positions and flux ratios of images B and C,
      adding a substructure of about 10^9 solar masses near image B to explain the flux anomaly.
  - title: Oguri et al. (2008)
    refs: [2008ApJ...676L...1O]
    data: [ground]
    availability: unknown
    tags: [parametric]
    note: Mass models that include the newly found third quasar image (a naked-cusp configuration).
