IR photometry of Alpha Per low-mass members (Lodieu+, 2005)

Bibcode
2005yCat..34360853L
Lodieu, N.; McCaughrean, M. J.; Barrado Y Navascues, D.; Bouvier, J.; Stauffer, J. R.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/436/853. Originally published in: 2005A&A...436..853L

Advertised on:
3
2005
Number of authors
5
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Optical detections in five different fields of view (A, C, E, K, and L) are matched with the near-infrared detections described in this paper. The central coordinates of the five optical fields-of-view are as follows: (see Stauffer et al. 1999ApJ...527..219S for more details): A : RA = 03:27:10.0 DE = +49:24:00.0 C : RA = 03:24:50.0 DE = +48:42:00.0 E : RA = 03:19:35.0 DE = +49:27:00.0 K : RA = 03:27:00.0 DE = +50:13:00.0 L : RA = 03:23:10.0 DE = +48:11:00.0 The objects matched between the optical and the near-infrared catalogues are gathered in table2.dat. Optical and near-infrared coordinates (J2000.0) are provided as well as magnitudes and their associated errors. The last column give the name of the object according to the IAU convention. (1 data file).
Type
Non-refereed
Photometry

It may interest you

  • Non-refereed
    New Robotic Telescope system progress towards critical design review
    The 4m class New Robotic Telescope (NRT) is an optical facility designed to revolutionize the rapid follow-up and classification of variable and transient objects. The project is at the stage where key systems are progressing through their detailed design phases, which presents a major engineering challenge for all project partners to manage design
    Copley, David et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..3WC
    Citations
    0
  • Non-refereed
    Phase diversity application on the EST MCAO testbench
    Phase Diversity (PD) is a technique widely used to measure and compensate for Non-Common Path Aberrations (NCPA) in optical systems. Beyond its traditional applications, PD has found further uses in solar astrophysics, where it enhances image quality by processing multiple images to correct residual aberrations. In this work, we introduce a
    Rodriguez-Linares, Nicolas et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13097E..5OR
    Citations
    0
  • Non-refereed
    First light of the upgraded Gregor Infrared Spectrograph
    For more than ten years, the Gregor Infrared Spectrograph (GRIS) has been the infrared spectropolarimeter on the Gregor telescope since its inauguration in 2012. The instrument mainly performs polarimetric observations of the wavelength regions at 1083 and 1565nm, which have high scientific potential. There, observers can find spectral lines that
    Quintero Noda, C. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..42Q
    Citations
    0