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 W49B 287.7847 9.1153 287.186342 9.031642 290.654992 31.289584 43.2812159 -0.18378496 89.2674 54921.5302662037 2009-03-31 12:43:35 54923.0613425926 2009-04-02 01:28:20 504035010 61.7825 100 61.7905 61.7845 0 61.7825 3 3 0 3 1 0 0 55.1556 55.1556 132.2739 3 PROCESSED 57546.0146412037 2016-06-07 00:21:05 55324 2010-05-08 00:00:00 54949.4493287037 2009-04-28 10:47:02 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040075 Observation of the W49B supernova remnant for 100 ksec is proposed to detect Ti emission line at the 3 sigma confidence level. In order to reveal whether it is a remnant of Type Ia supernova or not, detailed measurement of the rare metal elements such as Cr, Mn, Ni, and Ti is essential. We determine the type by Ti to Cr, Mn to Cr, and Ni to Fe ratios. Furthermore, we investigate whether its plasma is in the overionized status or not. GALACTIC DIFFUSE EMISSION 5 B MIDORI OZAWA JAP 4 AO4 UNMASK THE NATURE OF W49B ! XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504035010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504035010'

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