DARTS Astro

total 1

No. target_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 proposal_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 hxd_burst_num processing_status processing_end_time_mjd processing_end_time public_date_mjd public_date distribute_start_date_mjd distribute_start_date processing_version processing_quantity processing_software proposal_id proposal_abstract proposal_category proposal_category_code proposal_priority pi_name co_pi_name proposal_affiliated_country proposal_cycle_count observation_type proposal_title main_detector xis_injection_flag data_access_url ql_access_url ql_image_url
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://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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