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 | NGC3516 | 166.7299 | 72.5779 | 165.877553 | 72.848305 | 123.367172 | 57.997458 | 133.2179652 | 42.40001774 | 148.9366 | 53655.5813541667 | 2005-10-12 13:57:09 | 53658.3801388889 | 2005-10-15 09:07:24 | 100031010 | 134.4696 | 150 | 134.5096 | 134.5956 | 134.5096 | 134.4696 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 122.818 | 122.818 | 241.6848 | 0 | PROCESSED | 57527.6243634259 | 2016-05-19 14:59:05 | 54247 | 2007-05-27 00:00:00 | 54036.4704976852 | 2006-10-28 11:17:31 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000031 | NGC 3516 is one of the brightest Seyfert 1s seen in BAT currently visible to Suzaku. Recent BAT and RXTE observations show that this source is ~2-3 mCrb in the 2-10 keV band and ~4-5 mCrb in 15-100 keV. NGC 3516 is currently much brighter than when XMM observed it in 2000 (e.g., it has since returned to "typical" flux). This source's Fe K line and Compton reflection hump are both quite strong (e.g., as seen with SAX; R is ~1.8 in SAX data). | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | NGC 3516 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100031010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100031010'
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