DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 PKS2155-304 329.7191 -30.2247 328.99529 -30.464273 321.189186 -16.770975 17.73226544 -52.24760927 254.1358 53704.7749884259 2005-11-30 18:35:59 53706.3613888889 2005-12-02 08:40:24 700012010 63.9114 80 63.9194 63.9114 63.9194 63.9166 2 2 2 2 1 0 0 58.0114 58.0114 137.0498 3 PROCESSED 57532.3797685185 2016-05-24 09:06:52 54247 2007-05-27 00:00:00 54038.8920138889 2006-10-30 21:24:30 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001100 Jets in blazars are believed to be a powerful site of particle acceleration. TeV emitting blazars are very important, because we can study very end of electron distribution near the maximum energy by using X-ray spectrum, because X-ray emission is believed to be due to synchrotron emission from the higher energy electron. Comparison of spectral index between X-ray and TeV gives us a crucial information on these source, because this is very sensitive to the particle injection and rapid cooling. In order to maximize the capability of sensitive hard X-ray observations of Suzaku, we propose reserved TOO observations for the next six months of PV phase from the TeV emitting blazars established by HESS, selected from five candidates. EXTRAGALACTIC COMPACT SOURCES 7 A TADAYUKI TAKAHASHI JAP 0 SWG-TOO RESERVED TOO OBSERVATIONS OF SELECTED TEV-BRIGHT BLAZARS XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700012010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '700012010'

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