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 | NGC 2110 | 88.0444 | -7.458 | 87.440268 | -7.468978 | 87.743148 | -30.884192 | 212.92660512 | -16.54877043 | 103.4188 | 53629.3796296296 | 2005-09-16 09:06:40 | 53631.8308333333 | 2005-09-18 19:56:24 | 100024010 | 101.7487 | 100 | 101.9265 | 103.7601 | 101.7487 | 102.1483 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 86.0433 | 86.0433 | 211.7558 | 4 | PROCESSED | 57527.4030324074 | 2016-05-19 09:40:22 | 54247 | 2007-05-27 00:00:00 | 54035.4624189815 | 2006-10-27 11:05:53 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000024 | The Narrow Emission Line Galaxy NGC 2110 was the brightest AGN in the initial BAT survey release (BAT flux of 2.1E-10 erg/cm2/sec) visible to Suzaku during Sept./Oct., and is still currently bright in BAT. A 2003 RXTE observation yielded F_2-10 keV = 4E-11 erg/cm2/sec. The source is currently almost 3 times brighter than during the SAX observations. The main goals are to measure the high energy cutoff and to place a strong limit on the presence of reflection. The Compton reflection hump is weak in SAX data (suggesting that the Fe K line originates in Compton-thin material). Determining the strength of the reflection component is critical for constraining the geometry of the accreting material. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Narrow Emission Line Galaxy NGC 2110 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100024010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100024010'
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