HERO Project - High Energy Objects

HERO is new project (since 2008) organised by Variable Star and Exoplanet Section of CAS and is pointed to observing of selected high energy sources.

HERO is acronym and means High EneRgy Objects

HERO objects can be divided to two basic ranges. Stellar sources of high energy and Extragalactic sources.

Stellar sources:
Mostly binaries with compact component emitting x-rays and gamma-rays due to various reasons:

Cataclysmic Variables
Low Mass X-Ray Binaries, LMXRB
High Mass X-Ray Binaries, HMXRB
New types

Extragalactic sources:
Beside stellar sources (mentioned above) many high energy emmissions comes from cosmologic distancies:

Active Galactic Nuclei, AGN
Blasars and quasars
Gamma Ray Burst, GRB
Extragalactic supernovae
Luminous Blue Variables, LBV

Contact persons of the project:

Doc. RNDr. René Hudec, PhD., rhudec@asu.cas.cz (scientific leader)
Bc. Luboš Brát, brat@pod.snezkou.cz (technical staff)

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> Minima predictions <

> Transits predictions <

New minimas B.R.N.O.:

XZ Leo (F. Marchi)
RW Tau (f. marchi)
FW Her (M. Lehky)
UX CrB (M. Lehky)
KW Pup (M. Lehky)
V 785 Cas (L. Šmelcer)
V 785 Cas (L. Šmelcer)
V 785 Cas (L. Šmelcer)
GU Leo (J. Trnka)
AW Vir (L. Šmelcer)

New transits TRESCA:

WASP-12 b (F. Lomoz)
XO-4 b (J. Trnka)
WASP-14 b (R. Kocián)
HAT-P-3 b (D. Gary)
HAT-P-3 b (B. Tieman)
WASP-19 b (J. Colque)
WASP-12 b (G. Haagen)
HAT-P-13 b (B. Tieman)
HAT-P-12 b (B. Tieman)
GJ436 b (B. Tieman)

New data MEDUZA & HERO:

CCD:
L. Brát: V 407 Cyg,
M. Lehký: SN2004et Cyg, SN2003gd Psc, SN2002ap Psc, SN2001bg Cnc, DX And, YY Her, V 1329 Cyg, V 2274 Cyg, V 1548 Aql,

VIZ:
P. Dubovský: WY And, Z And, BB Aur, Eps Aur, NSV 16874 Aur, NSV 3171 Aur, Psi1 Aur, UU Aur, VW Aur, NSV 6696 Boo, V Boo, SY Cam, U Cam, XX Cam, BX Cas, KS Cas, NSV 332 Cas, NSV 650 Cas, Rho Cas, ST Cas,

Currently operating observers:
Observers on-line chat

No logged observers are currently operating.