G.A.R.R.A Grupo de Astrofísica Relativista y Radioastronomía Instituto Argentino de Radioastronomía (IAR) C.C. 5, C.P. 1894 Villa Elisa La Plata. Buenos Aires, Argentina

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On-line scientific data of GARRA

• Variability indices for gamma-ray sources. In this sets of tables we show the variability indices $\tau$ -mean, minimum, and maximum values- (Tompkins 1999) and $I$ (Torres, Pessah &Romero, 2001) for the variability of gamma-ray sources. Columns are: 1 and 2 -> EGRET source, 3-> I, 4 -> mean value of tau, 5->min. value and 6-> maximum value.

1. Pulsars
2. AGNs
3. Low-latitude unidentified sources
4. High-latitude unidentified sources

• Candidates to SNRs. In this table we show the galactic coordinates and the size, of 101 candidates to SNRs discovered using filtering techniques by several authors. For details see the paper: Low latitude gamma ray sources and the hypothesis of a black hole population [astro-ph/0007464], by Diego F. Torres, Gustavo E. Romero, J. Combi, Paula Benaglia, Brian Punsly & Heinz Andernach.

• Statistical variability of AGNs detected by EGRET. In this table we show  3EG Source
  [2] AGN Name
  [3] l
  [4] b
  [5] Spectral index <\gamma>
  [6] <F_\gamma> (\times 10^{-8} ph cm^{-2} s^{-1})
  [7] \sigma_{sd}
  [8] N_{vp}
  [9] Variability index \mu
  [10] Variability index I
  For details see the paper: Low latitude gamma ray sources and the hypothesis of a black hole population [astro-ph/0007464], by Diego F. Torres, Gustavo E. Romero, J. Combi, Paula Benaglia, Brian Punsly & Heinz Andernach.

• Possible radio counterparts of  40 EGRET sources without positional coincidences with any known galactic object. In this (very big!) table we show, for each source, the following columns: Survey |  Source name |  RA_J2000 |  err (s)  |  DEC_J2000  |  freq/MHz  |  flux/Jy  |  err/Jy   | comments. An etensive list of references is also provided. For details see the paper: Low latitude gamma ray sources and the hypothesis of a black hole population [astro-ph/0007464], by Diego F. Torres, Gustavo E. Romero, J. Combi, Paula Benaglia, Brian Punsly & Heinz Andernach.

• Statistical variability of all EGRET sources at low galactic latitudes. In this table we show two columns: the EGRET source name and the variability index I, as explained in the paper. For details see the paper: Low latitude gamma ray sources and the hypothesis of a black hole population [astro-ph/0007464], by Diego F. Torres, Gustavo E. Romero, J. Combi, Paula Benaglia, Brian Punsly & Heinz Andernach.

• Variability data for the optical outburst of AO 0235+164 detected on November 1999. See the paper Extreme ultranight variability in the BL Lacertae object AO 0235+164 by G.E. Romero, S.A. Cellone & J.A. Combi, published in Astronomy &. Astrophysics Letters 360, L47-L50 (2000).

1. Table V.tab
2. Table R.tab
3. Table VR.tab

• On-line tables from the paper Rapid variability of southern extragalactic radio sources, by G. E. Romero, P. Benaglia and J. A. Combi, The journal of Astronomical Data 3, (1997).

1. Table index.
2. Campaign I
3. Campaign II
4. Campaign III

• Distribution of the stars from OB Associations listed by de Zeeuw et al. (1999), as surface density plots (stars per 60 arcmin²). The Associations are: Cep OB6, Coll 121, Lac OB1, Per OB2, Per OB3, Tr 10, and UCL.

• Q/I-U/I planes for all the objects in the diferent campaigns from the paper Polarization microvariability of BL Lac objects , by I. Andruchow, G. E. Romero and S. A. Cellone. A&A., 442, 97 (2005)

1. RBLs type
2. XBLs type