Optical Spectroscopy of Swift J0732.5-1331

Bibcode
2006ATel..763....1T
Torres, M. A. P.; Steeghs, D.; Garcia, M. R.; McClintock, J. E.; Berlind, P.; Zhao, P.; Calkins, M.; Jonker, P. G.; Callanan, P. J.; Marsh, T.; Gaensicke, B. T.; Rodriguez-Gil, P.; Littlefair, S.; Dhillon, V.
Bibliographical reference

The Astronomer's Telegram, #763

Advertised on:
3
2006
Number of authors
14
IAC number of authors
0
Citations
6
Refereed citations
4
Description
In response to the detection of the X-ray source Swift J0732.5-1331 (ATEL #697, #735, #757, #760), we observed its optical counterpart with the Mt. Hopkins 1.5m telescope equipped with the FAST spectrograph. A total of 22 spectra covering 3480-7410 A were acquired between Jan 22 and Mar 1. A 3" slit provided 6 A FWHM resolution. In addition, on March 5 we acquired 2.3 hours of spectroscopy (14 spectra) with the 600 gpm grating and a 2 arcsec slit width (4490-4895 A; 2.4 A FWHM).
Type
Non-refereed

It may interest you

  • Non-refereed
    joshspeagle/dynesty: v3.0.0
    This is major release with several infrastructural changes that will make future development of dynesty easier, as well as significant speedups. The release also deprecated some rarely used options. Major refactor of the code that makes it easier to add new samplers. Major speedup of the uniform sampler when sampling in parallel You can now provide
    Koposov, Sergey et al.

    Advertised on:

    10
    2025
    Bibcode
    2025zndo..17268284K
    Citations
    1
  • Non-refereed
    (163) Erigone, (302) Clarissa, and (752) Sulamitis as seen with JWST's NIRSpec
    Primitive asteroids in the Main Belt possess one of the most pristine inventories of materials in the Solar System. Main Belt primitive asteroids are particularly interesting due to clear evidence of phyllosilicates, i.e., silicates that have encountered liquid water and undergone chemical alteration. Since asteroids are thought to be likely
    Harvison, Brittany et al.

    Advertised on:

    9
    2025
    Bibcode
    2025epsc.conf.1004H
    Citations
    0
  • Non-refereed
    NEOMIR: project statut of ESA's space-based infrared mission for NEO detection and early warning
    To warn about potential asteroid or comet impacts, we must first observe and discover these objects through dedicated NEO surveys. Most current and planned surveys are ground-based and use visible light, but they face limitations like weather dependency, limited sky visibility, difficulty detecting at low galactic latitudes, and inability to
    Conversi, Luca et al.

    Advertised on:

    9
    2025
    Bibcode
    2025epsc.conf.1329C
    Citations
    0