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 MBM12 OFF-CLOUD 41.3205 18.3346 40.61976 18.124407 44.482795 2.251416 157.33933963 -36.81758445 247.4802 53772.648599537 2006-02-06 15:33:59 53774.618275463 2006-02-08 14:50:19 501104010 75.3292 70 75.3372 75.3292 75.3372 75.3372 2 2 2 2 1 0 0 67.769 67.769 170.1159 1 PROCESSED 57532.9691550926 2016-05-24 23:15:35 54401 2007-10-28 00:00:00 53905.9757523148 2006-06-19 23:25:05 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011262 Suzaku will observe MBM 12, a nearby molecular cloud which shadows all but the most local soft X-ray emission. The goal of that observation is to measure the O VII and O VIII emission from the Local Hot Bubble, taking advantage of Suzaku's low energy sensitivity and low background. In light of this, we propose to observe the diffuse background near the MBM 12 position. This will: (1) Measure the O VII and O VIII emission from the Galactic disk and halo, after subtracting the local emission, and (2) confirm that this background emission does not contaminate the initial observation. The absolute measure of the strength of the O VII line, as well as the O VIII/O VII ratio, is essential to understanding the origin of the Galactic component to the 3/4 keV diffuse emission. GALACTIC DIFFUSE EMISSION 5 B RANDALL SMITH USA 1 AO1 THE ORIGIN OF THE GALACTIC DIFFUSE 3/4 KEV X-RAY BACKGROUND XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501104010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501104010'

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