We will report the observations of TeV gamma ray flares from Markarian 501 using Telescope Array Prototype. The observation were carried out continuously from the end of March to the end of July in 1997. The energy spectrum, and the time variation of the gamma ray intensities are shown. The intensity has been changed by the order of magnitude in this period and the possible quasi periodic oscillation of 12.7days were discovered
The energy spectrum of the active galactic nucleus Markarian 501 has been determined from 0.3 to 10 ...
The γ-ray emission above $250 \mathrm{GeV}$ from the BL Lac object Markarian 421 was observed by the...
A TeV flare from the BL Lac object Mrk 421 was detected in May of 1994 by the Whipple Observatory ai...
During remarkable flaring activity in 1997 Markarian 501 was the brightest source in the sky at TeV ...
Markarian 501 is only the second extragalactic source to be detected with high statistical certainty...
Markarian 501, a nearby (z=0.033) X-ray selected BL Lacertae object, is a well established source of...
The HEGRA system of 4 Imaging Atmospheric Cherenkov Telescopes (IACTs) has been used since March 199...
Between March 16, 1997 and April 14, 1997, a high flux level of TeV gamma-rays was observed from Mkn...
We present the gamma-ray spectrum of the BL Lacertae object, Markarian 421, above 500 GeV during its...
The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been ex...
The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been ex...
Markarian 421 was the first extragalactic source to be detected with high statistical certainty at T...
We present multiwavelength observations of the BL Lacertae object Markarian 501 (Mrk 501) in 1997 be...
posterOptical astronomy is the study of the heavens as they emit light, or the visible portion of th...
We present here the detection of TeV gamma rays from the extragalactic source Markarian 421. Observa...
The energy spectrum of the active galactic nucleus Markarian 501 has been determined from 0.3 to 10 ...
The γ-ray emission above $250 \mathrm{GeV}$ from the BL Lac object Markarian 421 was observed by the...
A TeV flare from the BL Lac object Mrk 421 was detected in May of 1994 by the Whipple Observatory ai...
During remarkable flaring activity in 1997 Markarian 501 was the brightest source in the sky at TeV ...
Markarian 501 is only the second extragalactic source to be detected with high statistical certainty...
Markarian 501, a nearby (z=0.033) X-ray selected BL Lacertae object, is a well established source of...
The HEGRA system of 4 Imaging Atmospheric Cherenkov Telescopes (IACTs) has been used since March 199...
Between March 16, 1997 and April 14, 1997, a high flux level of TeV gamma-rays was observed from Mkn...
We present the gamma-ray spectrum of the BL Lacertae object, Markarian 421, above 500 GeV during its...
The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been ex...
The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been ex...
Markarian 421 was the first extragalactic source to be detected with high statistical certainty at T...
We present multiwavelength observations of the BL Lacertae object Markarian 501 (Mrk 501) in 1997 be...
posterOptical astronomy is the study of the heavens as they emit light, or the visible portion of th...
We present here the detection of TeV gamma rays from the extragalactic source Markarian 421. Observa...
The energy spectrum of the active galactic nucleus Markarian 501 has been determined from 0.3 to 10 ...
The γ-ray emission above $250 \mathrm{GeV}$ from the BL Lac object Markarian 421 was observed by the...
A TeV flare from the BL Lac object Mrk 421 was detected in May of 1994 by the Whipple Observatory ai...