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'
Your request has been accepted.
The download will start soon automatically.