Calendar

Mag
15
lun
PROVA ORALE CONCORSO 2023RIC/OAPA/Stiles/Posizione01
Mag 15@10:00–17:15
Mag
22
lun
PROVA ORALE CONCORSO 2023RIC/OAPA/Stiles/Posizione02
Mag 22@10:00–13:00
Mag
24
mer
museo +sole scuola piazzi
Mag 24@9:00–13:00

rif Daricello

Mag
25
gio
PROVA ORLALE CONCORSO: 2023TEC/OAPA/Stiles/Posizione02
Mag 25@15:30–19:00
Mag
29
lun
PROVA ORALE CONCORSO: 2023TEC/OAPA/Stiles/Posizione01
Mag 29@15:30–19:00
Giu
5
lun
Visita ragazzi Malaspina ref Daricello
Giu 5@10:00–13:00

8 ragazzi + 3 accompagnatori

Giu
6
mar
visita museo piazzi
Giu 6@9:00–13:00

scuola piazzi 2 classi

Giu
7
mer
visita museo piazzi
Giu 7@9:00–13:00

scuola piazzi 2 classi

Giu
12
lun
PROVA ORALE CONCORSO FUNZIONARIO AMM.VO TD PNRR – COD.:2023INAFAMM-OAPA-PNRR-POSIZIONE01.
Giu 12 giorno intero
Giu
14
mer
Seminario: Maria Giovanna Dainotti (NAOJ)
Giu 14@15:00–16:30

Speaker: M. G. Dainotti (National Astronomical Observatory of Japan)
Title: The optical 2D and 3D correlation and their application as cosmological tool

Abstract: Gamma-ray bursts (GRBs) are fascinating events due to their
panchromatic nature. We study optical plateaus in GRB afterglows via
an extended search into archival data. We comprehensively analyze all
published GRBs with known redshifts and optical plateaus observed by
many ground-based telescopes (e.g., Subaru Telescope, RATIR) around
the world and several space-based observatories such as the Neil
Gehrels Swift Observatory. We fit 500 optical light curves, showing
the existence of the plateau in 179 cases. This sample is 75% larger
than the previous one, and it is the largest compilation so far of
optical plateaus. We discover the 3D fundamental plane relation at
optical wavelengths using this sample. This correlation is between the
rest-frame time at the end of the plateau emission, Topt * , its
optical luminosity, Lopt, and the peak in the optical prompt emission,
Lpeak,opt, thus resembling the three-dimensional (3D) X-ray
fundamental plane (the so-called 3D Dainotti relation). We correct our
sample for redshift evolution and selection effects, discovering that
this correlation is indeed intrinsic to GRB physics. We investigate
the rest-frame end-time distributions in X-rays and optical (Topt * ,
TX *), and conclude that the plateau is achromatic only when selection
biases are not considered. We also investigate 3D optical correlation
as a cosmological tool, finding that it is as efficacious as the X-ray
3D correlation.