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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
xtend_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
xtend_data_mode1
xtend_data_mode2
processing_count
remarks
1 201110010 NGC7212 331.75588 10.23109 331.13888 9.98655 337.63959 20.37779 70.41922 -35.37821 240.16305 60655.10838 2024-12-11 02:36:04 60656.80560 2024-12-12 19:20:04 71.075 220.000 71.075 67.269 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 67.269 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-12-21 08:50:44 2026-01-03 00:00:00 2024-12-22 08:50:44 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012190 The nearby (z~0.0266) Compton thick AGN NGC 7212 is, to our knowledge, the first AGN with a detection of vanadium via X-ray spectroscopy. Vanadium is a short-lived intermediate product of the spallation of iron by cosmic rays. Its presence in the narrow line region suggests ongoing strong cosmic ray feedback, and the likelihood that the energy range between 4.5 keV and iron K-alpha is likely to be dominated by more stable He-like and H-like products of spallation (such as titanium, chromium and manganese). Only XRISM has the sensitivity and resolution to measure these lines. This would have deep and consequential implications for the "hard continuum" between 2-6 keV. We will also model extended hot feedback in conjunction with archival Chandra data. NON-JET-DOMINATED AGN 2 B WALTER MAKSYM USA 1 NOR COSMIC RAY SPALLATION AND THE ENIGMATIC EXTENDED NARROW LINE REGION OF NGC 7212 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201110010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201110010'

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