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 | G21.5-0.9 | 278.4038 | -10.5066 | 277.711815 | -10.545632 | 278.460388 | 12.687474 | 21.56207071 | -0.86897985 | 103.5553 | 54190.0674074074 | 2007-03-31 01:37:04 | 54191.7405671296 | 2007-04-01 17:46:25 | 502065020 | 53.5261 | 100 | 53.5261 | 53.551 | 0 | 53.5661 | 1 | 2 | 0 | 1 | 1 | 0 | 0 | 48.618 | 48.618 | 144.5418 | 0 | PROCESSED | 57538.0817013889 | 2016-05-30 01:57:39 | 54695 | 2008-08-17 00:00:00 | 54200.5054861111 | 2007-04-10 12:07:54 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021211 | We propose an observation of the supernova remnant (SNR) G21.5--0.9. This SNR has a centrally peaked X-ray morphology which coupled with its non-thermal emission, suggested that the SNR's central engine was an undetected pulsar. Last year, a radio pulsar associated with the remnant was discovered (Gupta et al. 2005; Camilo et al. 2006). These announcements concur on the period of the pulsar and its period derivative making it the second highest spin-down luminosity pulsar. Deep Chandra imaging uncovered the missing shell (Matheson & Safi-Harb, 2005). Recent INTEGRAL and SWIFT/BAT slew observations detected G21.5--0.9 at more than 10 and 8 sigma respectively. The proposed observation will be the first self-consistent broad-band timing and spectral analysis from soft to very hard X-ray. | GALACTIC DIFFUSE EMISSION | 5 | B | ILANA HARRUS | USA | 2 | AO2 | SUZAKU OBSERVATIONS OF THE SUPERNOVA REMNANT G21.5-0.9 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502065020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '502065020'
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