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
|
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1 | W44_EAST | 284.1459 | 1.2991 | 283.51111 | 1.232548 | 285.500202 | 23.981686 | 34.67473844 | -0.5521979 | 254.9985 | 56583.3375231482 | 2013-10-18 08:06:02 | 56584.8897337963 | 2013-10-19 21:21:13 | 508004010 | 58.2965 | 60 | 58.3045 | 58.2965 | 0 | 58.3149 | 3 | 2 | 0 | 3 | 1 | 0 | 0 | 52.7276 | 52.7276 | 134.0958 | 2 | PROCESSED | 57613.0782407407 | 2016-08-13 01:52:40 | 57004 | 2014-12-13 00:00:00 | 56637.6520949074 | 2013-12-11 15:39:01 | 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/ver3.0/508004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '508004010'
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