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 | 3EGJ1234 1318_2 | 188.017 | -13.0869 | 187.367769 | -12.810986 | 192.545784 | -8.84065 | 295.65674578 | 49.51103665 | 109.9322 | 54081.9277777778 | 2006-12-12 22:16:00 | 54082.7766087963 | 2006-12-13 18:38:19 | 801032010 | 30.9427 | 30 | 30.9667 | 30.9587 | 0 | 30.9427 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 26.083 | 26.083 | 73.3339 | 1 | PROCESSED | 57536.3393055556 | 2016-05-28 08:08:36 | 54735 | 2008-09-26 00:00:00 | 54094.2665740741 | 2006-12-25 06:23:52 | 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/ver3.0/801032010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801032010'
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