JHK photometry of Vega-type and PMS stars (Eiroa+, 2001)

Bibcode
2000yCat..33650110E
Eiroa, C.; Garzon, F.; Alberdi, A.; de Winter, D.; Ferlet, R.; Grady, C. A.; Collier Cameron, A.; Davies, J. K.; Deeg, H. J.; Harris, A. W.; Horne, K.; Merin, B.; Miranda, L. F.; Montesinos, B.; Mora, A.; Oudmaijer, R.; Palacios, J.; Penny, A.; Quirrenbach, A.; Rauer, H.; Schneider, J.; Solano, E.; Tsapras, Y.; Wesselius, P. R.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/365/110. Originally published in: 2001A&A...365..110E

Advertised on:
10
2000
Number of authors
24
IAC number of authors
0
Citations
0
Refereed citations
0
Description
File table1.dat contains near-infrared JHK magnitudes of a sample of 18 Vega-like and post-T Tauri stars observed by the EXPORT collaboration. File table2.dat contains near-infrared JHK magnitudes of a sample of 4 pre-main sequence stars observed by EXPORT. The data were taken during four observing runs in the period May 1998 to January 1999. (3 data files).
Type
Non-refereed
Photometry

It may interest you

  • Non-refereed
    Workshop summary: Kaons@CERN 2023

    Kaon physics is at a turning point - while the rare-kaon experiments NA62 and KOTO are in full swing, the end of their lifetime is approaching and the future experimental landscape needs to be defined. With HIKE, KOTO-II and LHCb-Phase-II on the table and under scrutiny, it is a very good moment in time to take stock and contemplate about the

    Anzivino, G. et al.

    Advertised on:

    4
    2024
    Bibcode
    2024EPJC...84..377A
    Citations
    0
  • Non-refereed
    Nodal Precession of a Hot Jupiter Transiting the Edge of a Late A-Type Star TOI-1518

    TOI-1518b, a hot Jupiter around a late A-type star, is one of the few planetary systems that transit the edge of the stellar surface (the impact parameter b~0.9) among hot Jupiters around hot stars (Cabot et al. 2021). The host star's high rotation speed (Vsini s~85 km s -1) and the planet's nearly polar orbit (λ~120 deg) may cause a nodal

    Watanabe, Noriharu et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....561705W
    Citations
    0
  • Non-refereed
    Observational evidence of different formation mechanisms of Solar System-type architectures across spectral types

    Despite being the most abundant classes of known exoplanets, super-Earths and mini-Neptunes are absent in our Solar System, and the exact reason for this is still unknown. Some models suggest that cold-Jupiters play a major role in the formation of inner low-mass planets. This could explain the current architecture of our Solar System, and the

    Pinamonti, Matteo et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....560801P
    Citations
    0
Go back