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 3EGJ1234 1318_1 188.0173 -13.3363 187.367898 -13.060386 192.646727 -9.069223 295.70141073 49.26333697 109.7313 54081.3723032407 2006-12-12 08:56:07 54081.9273032407 2006-12-12 22:15:19 801031010 19.4098 20 19.4178 19.4178 0 19.4098 2 2 0 2 1 0 0 18.7228 18.7228 47.9499 1 PROCESSED 57536.3099768518 2016-05-28 07:26:22 54735 2008-09-26 00:00:00 54094.2359722222 2006-12-25 05:39:48 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010068 We propose observations around 3EG J1234 1318, which is one of the EGRET un-ID sources. From recent optical survey, it is found that the source is located around a large scale structure at z ?sim 0.1. We propose a scenario that the GeV source is originating from a large shock wave within the structure formation. The XIS and the HXD provides a probe for thermal shock plasma and non-thermal IC emission, respectively. This observation will solve some questions on EGRET un-ID sources. EXTRAGALACTIC DIFFUSE SOURCES 8 C TOMONORI TOTANI JAP 1 AO1 CONFIRMING GAMMA-RAY EMISSION FROM INTERGALACTIC SHOCKS: A NEW WINDOW TO STUDY THE COSMIC STRUCTURE FORMATION HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801031010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801031010'

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