A Search for the Optical Counterpart to the Magnetar CXOU J010043.1-721134

Bibcode
2008ApJ...680.1394D
DOI
10.1086/529017
Durant, M.; van Kerkwijk, M. H.
Bibliographical reference

The Astrophysical Journal, Volume 680, Issue 2, pp. 1394-1397.

Advertised on:
6
2008
Journal
The Astrophysical Journal
Number of authors
2
IAC number of authors
1
Citations
8
Refereed citations
8
Description
After our tentative detection of an optical counterpart to CXOU J010043.1-721134 from archival Hubble Space Telescope (HST) imaging, we have followed up with further images in four bands. Unfortunately, the source originally identified is not confirmed. We provide deep photometric limits in four bands and accurate photometry of field stars around the location of the magnetar.
Related projects
Black hole in outburst
Black holes, neutron stars, white dwarfs and their local environment
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only confirmation of the existence of stellar mass black holes via dynamical mass measurements, but also the best opportunity for probing high-gravity environments and the physics of accretion; the most
Montserrat
Armas Padilla
In progress
Type
Refereed
Stellar & Interstellar Physics (FEEI)
Pulsars

It may interest you

  • Refereed
    Copacabana: a probabilistic membership assignment method for galaxy clusters
    Cosmological analyses using galaxy clusters in optical/near-infrared photometric surveys require robust characterization of their galaxy content. Precisely determining which galaxies belong to a cluster is crucial. In this paper, we present the COlor Probabilistic Assignment of Clusters And BAyesiaNAnalysis (Copacabana) algorithm. Copacabana
    Esteves, J. H. et al.

    Advertised on:

    1
    2025
    Bibcode
    2025MNRAS.536..931E
    Citations
    1
  • Refereed
    Constraints on compact objects from the Dark Energy Survey 5-yr supernova sample
    Gravitational lensing magnification of Type Ia supernovae (SNe Ia) allows information to be obtained about the distribution of matter on small scales. In this paper, we derive limits on the fraction $\alpha$ of the total matter density in compact objects (which comprise stars, stellar remnants, small stellar groupings, and primordial black holes)
    Shah, P. et al.

    Advertised on:

    1
    2025
    Bibcode
    2025MNRAS.536..946S
    Citations
    0
  • Refereed
    Multiband Optical Variability of the Blazar 3C 454.3 on Diverse Timescales
    Due to its peculiar and highly variable nature, the blazar 3C 454.3 has been extensively monitored by the WEBT team. Here, we present for the first time these long-term optical flux and color variability results using data acquired in B, V, R, and I bands over a time span of about two decades. We include data from WEBT collaborators and public
    Dogra, Karan et al.

    Advertised on:

    1
    2025
    Bibcode
    2025ApJS..276....1D
    Citations
    0