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 W44_SOUTH 284.0546 1.2208 283.419443 1.15468 285.391807 23.913502 34.56340933 -0.50670684 73.0006 56756.507025463 2014-04-09 12:10:07 56757.3474074074 2014-04-10 08:20:16 508003020 32.3696 33 32.3776 32.3776 0 32.3696 3 2 0 2 1 0 0 29.5034 29.5034 72.5959 1 PROCESSED 57614.2259837963 2016-08-14 05:25:25 57193 2015-06-20 00:00:00 56825.6834027778 2014-06-17 16:24:06 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080012 W44 is a middle-aged supernova remnant (SNR) categorized to mixed-morphology SNR. We have observed the center region of W44 with Suzaku in the AO5 phase. The spectra are well reproduced by a thermal plasma in a recombining phase. While such plasmas have been found from several SNRs, the origin is still unclear. We also discover hard X-ray emission which shows an arc-like structure spatially-correlated with a radio continuum filament. No conventional model for particle acceleration could explain the mechanism of the hard X-ray emission. The entire plasma distribution of W44 will provide a clue to resolve the origins of the reombining plasma and the hard X-ray emission. We therefore require four pointing observations for totally 280 ks. GALACTIC DIFFUSE EMISSION 5 A HIROYUKI UCHIDA JAP 8 AO8 MAPPING THE SPATIAL DISTRIBUTION OF HARD AND SOFT X-RAYS IN W44 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/508003020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '508003020'

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

Go to top of this page ⏏