DDOTI Closed for the Winter Break

22 December 2019

DDOTI has closed for the OAN winter break. Most of the other telescopes were closed on 14 December, but for the first time DDOTI, COATLI, and SAINT-EX stayed open longer under the care of a skeleton crew. We thank Ilse Plauchu and Rosa Becerra for technical support in this period.


DDOTI Observations of the LIGO/Virgo Source S190521g

21 May 2019

DDOTI observed a 14 by 21 degree region (294 square degrees) centered on the probability peak of the LIGO/Virgo source S190521g, a candidate binary black-hole merger. We detect no uncataloged sources with significant fading down to our 10-sigma limit of 18.7 magnitude. We reported our observations in a GCN Circular


DDOTI Observations of the LIGO/Virgo Source S190426c

28 April 2019

DDOTI observed a 460 square degrees centered on the probability peak of the LIGO/Virgo source S190426c, a candidate binary neutron-star merger. We reported our observations in a GCN Circular


DDOTI Observations of the LIGO/Virgo Source S190408an

9 April 2019

DDOTI observed an 11 by 7 degree region (70 square degrees) centered on the probability peak of the LIGO/Virgo source S190408an, a candidate binary black-hole merger. We reported our observations in a GCN Circular


DDOTI Installation of All Six Telescopes

21 March 2019

DDOTI has been observing with two telescopes since the summer of 2017. We have now installed the four remaining telescope to give a full complement of six telescopes. The additional telescopes are a major hardware contribution from the University of Maryland group lead by Nora Troya and Alexander Kutyrev.

The installation was carried out by Fernando Ángeles, Alejandro Farah, Diego González, Margarita Pereyra, and Alan Watson with help from the staff of the Observatorio Astronómico Nacional.

DDOTI with Six Telescopes

Fernando Ángeles (left) and Alan Watson (right) with all six telescopes.


DDOTI Observations and Possible Detection of GRB 190129B

30 January 2019

DDOTI observed the entire IPN error box of GRB 190129B and detected a faint, apparently fading source which we suggest is the afterglow. We reported our results in a GCN Circular