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 287.7843 9.1147 287.18594 9.031044 290.654435 31.289046 43.28050127 -0.18371216 82.0064 57128.6891203704 2015-04-16 16:32:20 57131.6619328704 2015-04-19 15:53:11 509001030 100.9959 400 100.9959 106.4207 0 106.3967 4 2 0 2 0 0 0 0 0 0 0 PROCESSED 57618.0043518518 2016-08-18 00:06:16 56748 2014-04-01 00:00:00 57220.3809722222 2015-07-17 09:08:36 3.0.22.44 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090007 W49B is an unique SNR which shows the radiative recombination continuum of He-like Fe. The plasma code of recombining plasma is very limited, due to a lack of accurate information of this plasma process. Since the transient time scale of the recombining plasma in laboratory is very short, useful information is hard to obtain. The recombination features of Fe are located in the energy band of 6-10 keV, where no other prominent structure is found. Therefore the spectrum of W49B in this energy band is ideal to study details of the recombining plasma. We hence propose 400-ksec observations on W49B. This deep observation will serve the fundamental data of the recombining plasma from the space plasma for the first time, which is key information for the future study of space plasma with ASTRO-H. GALACTIC DIFFUSE EMISSION 5 B KATSUJI KOYAMA JAP 9 AO9 DEEP OBSERVATIONS OF W49B XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509001030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509001030'

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