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 3C454.3 343.4944 16.1419 342.876791 15.875412 351.363537 21.325671 86.11044475 -38.19108399 249.0674 54439.2068865741 2007-12-05 04:57:55 54440.1112731482 2007-12-06 02:40:14 902002010 39.8895 40 39.8895 39.8895 0 39.8895 2 2 0 2 1 0 0 38.0412 38.0412 78.1319 1 PROCESSED 57540.8195023148 2016-06-01 19:40:05 54431 2007-11-27 00:00:00 54448.1589351852 2007-12-14 03:48:52 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 027002 We propose a 40 ksec Suzaku ToO observation of 3C 454.3, which is exhibiting ultra-high flaring activity in GeV gamma-ray band. 3C454.3 is a quasar hosted blazar (QHB) located at z =0.86. Daily monitoring of AGILE records E>100 MeV flux of 2x10^(-6) photons/cm^2/s or even greater. At present (Nov.23, 2007) flux is still increasing in both GeV and R-band, and this high state is expected to continue for typical flaring time scale of 1 month. Note this level of giant flare is recorded only 4-times through the entire life of EGRET onboard CGRO (3C279,1407-076,0528+134,1622-297). We propose to take a 40 ksec snapshot X-ray spectrum that is simultaneous with AGILE and world-wide ground-based radio-to-optical telescopes. EXTRAGALACTIC COMPACT SOURCES 9 A SWG JAP 2 TOO SUZAKU TOO OBSERVATION OF GIANT FLARE IN 3C454.3 TRIGGERED BY AGILE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/902002010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '902002010'

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