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
|
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1 | MRK421 | 166.1418 | 38.2711 | 165.447021 | 38.540933 | 151.207571 | 29.566146 | 179.67525089 | 65.03258412 | 111.0988 | 54803.7278240741 | 2008-12-03 17:28:04 | 54805.9480324074 | 2008-12-05 22:45:10 | 703020010 | 101.3075 | 100 | 101.3315 | 101.3075 | 0 | 101.3315 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 65.5148 | 65.5148 | 191.7877 | 3 | PROCESSED | 57544.7029398148 | 2016-06-05 16:52:14 | 55188 | 2009-12-23 00:00:00 | 54818.7659837963 | 2008-12-18 18:23:01 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030119 | Mrk421 provides our best opportunity to understand the high-energy emission of blazar jets, because it has produced the largest observed flux. Suzaku HXD has proved that spectum upto 40 keV can be measured only with an exposure of 1 ks from Mrk 421. Hard X-ray region is very crucial to study particle acceleration in the jet, since it corresponds to high energy end of electron distribution. Cooling and Acceleration phenomena will appear in this energy band. Here we will propose to monitor Mrk 421 for 200 ks, in which we can expect at least four or five flares. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | TADAYUKI TAKAHASHI | JAP | 3 | AO3 | STUDY OF HARD X-RAY EVOLUTION FROM THE BRIGHTEST BLAZAR JET. | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703020010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703020010'
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